Unraveling the Brown Dwarf Desert: Four New Discoveries and a Unifying, Period-Coded Picture

TL;DR

Four transiting brown dwarfs discovered by TESS and confirmed with high-precision RVs extend the long-period BD tail, with three systems having periods above $100$ days and subsolar host metallicities. A population-level comparison of BD eccentricities and host metallicities with long-period giant planets and low-mass stellar companions shows long-period BDs ($P>16$ d) resemble LMS binaries, while short-period BDs favor metal-rich hosts, implying a period-coded mixture of formation channels. Excluding six nearly circular objects in the $10< P le 16$ d range, the BD eccentricity signal is shown to be driven by a small subset, and full CTL tidal-evolution modeling demonstrates that modest initial eccentricities and plausible stellar dissipation can reproduce observed eccentricities within ~10 Gyr. The authors propose a framework where fragmentation dominates wide-separation BD formation, while metal-rich discs enable inward delivery and survival of short-period BDs; expanding the BD census and homogenizing host metallicities are crucial for testing this scenario.

Abstract

We present four newly validated transiting brown dwarfs identified through TESS photometry and confirmed with high-precision radial velocity measurements obtained from the FEROS and PLATOSpec spectrographs. Notably, three of these companions exhibit orbital periods exceeding 100 days, thereby expanding the sample of long-period transiting brown dwarfs from two to five systems. The host stars of long-period brown dwarfs show mild subsolar metallicity. These discoveries highlight the expansion of the metal-poor, long-period distribution and help us better understand the brown dwarf desert. In our comparative analysis of eccentricity and metallicity demographics, we utilize catalogues of long-period giant planets, brown dwarfs, and low-mass stellar companions. After accounting for tidal influences, the eccentricity distribution aligns with that of low-mass stellar binaries, presenting a different profile than that observed within the giant planet population. Additionally, the metallicity of the host stars reveals a noteworthy trend: short-period transiting brown dwarfs are predominantly associated with metal-rich stars, whereas long-period brown dwarfs are more often found around metal-poor stars, demonstrating statistical similarities to low-mass stellar hosts. This trend has also been previously observed in studies of hot and cold Jupiters and points to a period-coded mixture of channels. A natural explanation is that most brown dwarfs originate from fragmentation at wider separations, with long-period systems retaining this stellar-like imprint, while only those embedded in massive, long-lived, metal-rich protoplanetary discs are efficiently delivered and stabilised to short orbits.

Figures (1)

• Figure 1: SOAR contrast curve for Cousins $I$ band with a $6$^$\times 6$^$reconstructed image of the field. We conducted a spectroscopic follow-up campaign with the FEROS spectrograph Kaufer1999 installed at the ESO-MPG 2.2 m telescope at La Silla Observatory. Observations were performed with the simultaneous calibration technique, in conjunction with a ThAr calibration lamp. FEROS data were reduced, extracted, and analyzed with the Ceres pipeline Brahm2017, delivering RV and bisector span measurements. We summarize the spectroscopic observations in Table \ref{['table:RV_s']}. We conducted a spectroscopic follow-up campaign with the PLATOSpec spectrograph Kabath2025 installed at the ESO 1.52 m telescope at La Silla Observatory. PLATOSpec is a white pupil echelle spectrograph with spectral resolving power of R\,=\,70,000, covering the range of wavelengths from 380 to 700 nm. Observations were performed with the simultaneous calibration technique, in conjunction with a ThAr calibration lamp. PLATOSpec data were reduced, extracted, and analyzed with the Ceres pipeline Brahm2017, delivering RV and bisector span measurements. We summarize the spectroscopic observations in Table \ref{['table:RV_s']}. Summary of Radial Velocity Measurements TargetN$_{obs}$Median $\sigma_{RV}$Observations datesTIC,934489910162022 March 072022 October 31TIC,5205992635182020 December 042023 August 25TIC,1334466819172020 March 022022 April 15TIC,6392146825232025 February 042025 September 14 We achieved a high signal-to-noise ratio by co-adding all high-resolution FEROS spectra after correcting for radial velocity shifts. This combined spectrum was utilized to derive the stellar parameters of our sample using the Spectroscopy Made Easy (SME) radiative transfer code Valenti96Piskunov17, integrated into the iSpec framework Blanco14Blanco19. Additionally, we modeled the spectra using MARCS atmospheric models Gustafsson08 and employed version 5 of the GES atomic line list Heiter15. The iSpec software generates synthetic spectra and compares them with the observed spectrum, minimizing the chi-squared statistic through a nonlinear least-squares fitting algorithm (Levenberg-Marquardt) Markwardt09. For our analysis, we focused on the spectral region from 490 to 580 nm to ascertain the effective temperature (T_{\rm eff}), metallicity (\rm [Fe/H]), and projected stellar equatorial velocity (v\sin{i}). We applied the Bayesian parameter estimation code {\tt PARAM 1.5} DaSilva06Rodrigues14Rodrigues17 to derive the surface gravity (\log{g}) from PARSEC isochrones Bressan12, incorporating the spectral parameters obtained and available photometric data (see Table \ref{['tab1']}), along with {\it Gaia} DR3 parallax measurements. This iterative procedure was executed until convergence to the final parameter values was achieved, which are summarized in Table \ref{['table:stellar_par']}. To independently verify our derived stellar parameters, we modeled the spectral energy distribution (SED) with the Bayesian model averaging fitter, spectrAl eneRgy dIstribution bAyesian moDel averagiNg fittEr Vines22. We determined T_{\rm eff}, \log{g}, metallicity (\rm [Fe/H]), stellar luminosity, and radius by combining 3D dust Bayestar maps for interstellar extinction Green19 with two atmospheric models: Kurucz Kurucz93, and Ck04 Castelli2004. Our priors were informed by the results obtained from iSpec. The final derived parameters, presented in Table \ref{['table:stellar_par']}, align well with previously established values. The SEDs are illustrated in Fig.~\ref{['fig:SED']}, featuring the best-fitting Phoenix model Husser2013. To estimate the mass, radius, and age of the stars, we utilized MIST stellar evolutionary tracks Choi16 based on our stellar parameters and the available photometry. In Fig. \ref{['fig:isochrones']}, we overlay the luminosity and effective temperature of our stars with the MIST tracks. Spectral types were estimated using the latest version of the empirical spectral type-color sequence as proposed by Pecaut13. Luminosity vs. effective temperature for the stars in our sample. Curves represent MIST isochrones for ages: 0.1,Gyr (blue), 1.0,Gyr (orange), 3, Gyr (green), and 10.0,Gyr (yellow). Different line types represent different metallicities. The red point represents the positions of stars with their error bars. Stellar parameters of TOI-2458. TIC,9344899TIC,52059926TIC,13344668TIC,63921468$\rm T_{eff}$ (K)$5800 \pm 70$$4505 \pm 70$$4491 \pm 70$$6500 \pm 70$$[{\rm Fe/H}]$ (dex)$0.07 \pm 0.05$$-0.08 \pm 0.05$$-0.20 \pm 0.05$$-0.22 \pm 0.05$$\log{g}$ (cgs)$4.39 \pm 0.04$$4.62 \pm 0.02$$4.63 \pm 0.02$$3.85 \pm 0.02$$v_{\rm rot} \sin{i_\star}$ (km/s)$2.0 \pm 1.5$$1.5 \pm 1.5$$1.5 \pm 1.5$$11.0 \pm 1.5$$M_\star$ ($\rm \,{\rm M_\odot}$)$0.98 \pm 0.08$$0.73 \pm 0.04$$0.70 \pm 0.03$$1.52 \pm 0.05$$R_\star$ ($\rm \,{\rm R_\odot}$)$1.06 \pm 0.03$$0.72 \pm 0.02$$0.69 \pm 0.02$$2.35 \pm 0.05$ARIADNE analysis$\rm T_{eff} (K)$$5703 \pm 69$$4479 \pm 52$$4444 \pm 57$$6442 \pm 69$$[{\rm Fe/H}]$$0.10 \pm 0.10$$-0.07 \pm 0.10$$-0.18 \pm 0.10$$-0.22 \pm 0.10$$\log{g}$$4.38 \pm 0.04$$4.62 \pm 0.03$$4.63 \pm 0.03$$3.86 \pm 0.02$$L_\star$ (L$_{\odot}$)$1.08 \pm 0.07$$0.19 \pm 0.01$$0.17 \pm 0.01$$8.61 \pm 0.43$Other parametersSpectral typeG3VK4.5VK5VF5VAge (Gyr)$6.1_{-2.9}^{+4.1}$$8.2_{-5.5}^{+5.2}$$2.7_{-2.2}^{+7.8}$$2.1_{-0.2}^{+0.2}$ SED fits for the systems in our sample. The blue points with vertical error bars show the observed catalog fluxes and uncertainties from { Gaia}, TESS, Tycho-2, 2MASS, and WISE, while the horizontal error bars illustrate the width of the photometric band. For illustrative purposes, we overplot the best-matching Phoenix atmospheric model Husser2013. To differentiate the Doppler reflex motion from signals due to planetary candidates and stellar activity, we conducted a frequency analysis on the FEROS RVs and Bisector Inverse Slope (BIS) values derived from the Ceres pipeline. We computed Generalized Lomb-Scargle (GLS) periodograms Zechmeister09 for the time series data, establishing theoretical false alarm probabilities (FAP) at levels of 10\%, 1\%, and 0.1\%, as illustrated in Fig.~\ref{['fig:per']}. The periodogram revealed a significant signal for the TIC\,9344899 RVs, corresponding to periods of 8.6 days, aligning with the transiting planets identified through TESS photometry. Following the removal of this signal, the periodogram of the residual RVs exhibited no further significant signals, nor did the BIS periodogram reveal any noteworthy peaks. In the case of the TIC\,52059926 and TIC\,13344668 systems, the planetary candidates remain undetermined in period due to TESS only capturing a single transit for each system. Analysis of the RV periodograms unveiled significant peaks at longer periods of 176 days and 142 days. Although additional significant peaks were also observed at even longer periods, the joint transit and RV modeling discussed in the subsequent section clarified the true period values, as highlighted in Fig.~\ref{['fig:per']}. Notably, we detected a potential additional planet in the TIC\,52059926 system with a shorter period of 3.7 days, which is non-transiting. Nonetheless, further RV monitoring is essential to confirm this signal. This finding is particularly intriguing, as it could represent the first instance of a transiting brown dwarf having a less massive companion on the inner orbit. The modeling of both the transit light curves and radial velocity (RV) measurements was performed in a fully joint framework using the {\tt allesfitter} package Gunther21. This software integrates several specialized tools: {\tt ellc} for transit and RV modeling Maxted16, {\tt aflare} for stellar flare characterization Davenport14, {\tt dynesty} for nested sampling Speagle20, {\tt emcee} for Markov Chain Monte Carlo exploration Foreman13, and {\tt celerite} for Gaussian process (GP) modeling of correlated noise Foreman17. The flexibility of {\tt allesfitter} allows us to model a wide range of astrophysical effects, including multi-planet and multi-star systems, transit timing variations, phase curves, stellar activity, starspots, and flares, as well as a variety of systematic trends. Before the fit, the light curves were corrected for stellar variability following the procedure described in Section~\ref{['sec:TESS']}. A quadratic limb-darkening law parameterized by q_1 and q_2 was adopted. The joint fit included our FEROS/PLATOSpec RV measurements, reduced according to the method described in Section~\ref{['sec:observations']}. The resulting posteriors are summarized in Table~\ref{['tab:sec_fit']}, while Table~\ref{['tab:sec_der']} lists the final transit and physical parameters, derived using the results from Table~\ref{['tab:sec_fit']}. The corresponding model fits are shown in Fig.~\ref{['fig:transit_all']}, Fig.~\ref{['fig:transit']}, and Fig.~\ref{['fig:RVs']}. The population of known transiting brown dwarfs. We filtered out objects with large uncertainties in mass or radius. Star symbols highlight the positions of our systems. The plot is color-coded by orbital period. The mass-radius tracks from ... are utilized. Combining data from the TESS mission with ground-based spectroscopy, we successfully confirmed the substellar nature of four candidates orbiting K, G, and F-type stars. Our findings indicate that two brown dwarfs (BDs) are situated near the lower mass boundary for BDs, while the other two exhibit masses approximately 70\,M_{\rm J}. Notably, TIC~13344668b is characterized by substantial mass uncertainties due to RV sampling that did not capture the minimum phase near 0.0, leading to multiple viable eccentricity solutions. It is worth noting that TIC~63921468\,b has previously been identified as a transiting exoplanet candidate in the study conducted by Salinas25. Figure~\ref{['fig:mr']} illustrates the positions of our four companions (denoted by star symbols) within the brown-dwarf mass–radius diagram, overplotted against evolutionary tracks as presented by Baraffe2003 and the ATMO models Phillips2020 spanning 0.1, 1, 3, and 10~Gyr. For objects that are degenerate and undergoing cooling, the models indicate a weak dependence of radius on mass, ranging from approximately 0.8 to 1.1\,R_{\rm J} across the mass interval of approximately 15 to 80\,M_{\rm J}. Furthermore, there is a monotonic contraction that occurs with age as internal entropy is gradually radiated. In contrast to hot Jupiters, the inflation driven by irradiation is anticipated to be minimal at brown dwarf masses. Consequently, deviations from the model envelopes typically signal the presence of unusual physical phenomena (such as ongoing tidal interactions, compositional variations, or deuterium burning) or systematic errors in the derived stellar parameters. \textit{TIC~9344899\,b}, \textit{TIC~52059926\,b}, \textit{TIC~13344668\,b}, and \textit{TIC~63921468\,b} fall within the 1--10~Gyr model envelopes, following the canonical BD cooling sequence: at their measured masses, they cluster near \sim0.8--1.0\,R_{\rm J} with no compelling evidence for inflation. Their periods (color scale in Fig.~\ref{['fig:mr']}) span from short to long; the lack of radius excess at high equilibrium temperatures (TIC~9344899\,b) in this subset reinforces the view that stellar irradiation alone rarely produces large radius anomalies in the BD regime. \textit{TIC~9344899\,b} lies on the compact edge of the brown-dwarf mass–radius relation (Fig.~\ref{['fig:mr']}). At M\approx19\, M_{\rm J} its measured radius (R\approx0.82\, R _{\rm J}) sits below the solar-composition ATMO/Baraffe evolutionary tracks at 10,Gyr, which generally approach a slow contraction asymptote of \sim\,0.9–1.0\,R_{\rm J} in this mass regime. This places \textit{TIC~9344899\,b} in mild tension with standard isolated–cooling models for solar composition Baraffe2003Phillips2020. It is important to note that an underestimated radius may result from an imprecise dilution estimate, particularly given the crowded field surrounding the star. In our methodology (see Sec.~\ref{['sec:TESS']}), we employed the most reliable approach currently available, which has recently been utilized to correct the radii of numerous planets discovered by TESS Han2025. The numerous ground-based photometry unfortunately cannot be used to confirm the transit depth due to insufficient coverage of the out-of-transit baseline. A useful analogue is the recently validated transiting brown dwarf TOI-5422\,b (27.7_{-1.1}^{+1.4},M_{\rm J}, 0.815_{-0.021}^{+0.036},R_{\rm J}, P=5.38\,d), whose discovery team explicitly describe it as slightly “underluminous” with respect to substellar evolution models at an old age (8.2\pm2.4\,Gyr) Zhang2025. TOI-5422\,b demonstrates that short-period, old brown dwarfs with radii near \sim\,0.8\,R_{\rm J} do exist; \textit{TIC~9344899\,b} would extend this compact tail to \emph{lower} mass, where most grids predict somewhat larger radii. Physically, a slightly sub-model radius at fixed mass can be produced by (i) lower atmospheric/metallicity opacities that hasten cooling, or (ii) higher mean molecular weight (e.g., interior metal enrichment), each shrinking the radius by a few percent at Gyr ages. “Cold–start’’ initial entropies can also push toward smaller radii at early times, but for high-mass objects (\geq5-10\, M_{\rm J}) the hot–cold differences decay within \lesssim 10^8 yr and are negligible by Gyr ages Spiegel2012. The models used are based on standard, solar-composition, isolated-cooling grids that utilize a singular H/He equation of state along with specific opacity and cloud prescriptions. These foundational assumptions do not account for several factors that may introduce biases to the radii estimates at the few to ten percent level. Notable omissions include metallicity and cloud-dependent opacities, gradients in interior composition, and systematic discrepancies in the equation of state. Consequently, the actual lower envelope of radii may be somewhat more compact than the baseline predictions suggest. In particular, recent advancements in the dense H/He equation of state indicate slightly increased compressibility when compared to older datasets. This adjustment results in reduced adiabatic temperatures, accelerated cooling rates, and subsequently modestly smaller radii at fixed mass and age Chabrier2023. The ongoing integration of such refined physical models, together with improved opacity and cloud treatment as well as inclusion of composition effects, is anticipated to enhance the precision of the theoretical lower envelope and may alleviate the discrepancies observed in compact systems such as TIC 9344899\,b and TOI-5422\,b. Circularization timescale $\tau_e$ (Gyr, logarithmic color scale) as a function of the modified tidal quality factors of the brown dwarf and the star for TIC,9344899. Black contours mark $\tau_e=1,3$ Gyr (solid) and $10$ Gyr (dashed); the white contour indicates the system median age; the red curve shows the boundary where tides in the companion and in the star contribute equally ($\tau_{e,2}=\tau_{e,\star}$). Contours are nearly horizontal in both panels, indicating that $\tau_e$ is chiefly set by stellar dissipation over plausible $Q'_2$. Following Jackson2008, in the small–eccentricity limit the eccentricity damps approximately exponentially, \dot e \simeq -e/\tau_e, with \frac{1}{\tau_e} =\;\frac{63}{4}\, n\,\frac{M_\star}{M_2}\left(\frac{R_2}{a}\right)^{\!5}\frac{1}{Q'_2} \;+\;\frac{171}{16}\, n\,\frac{M_2}{M_\star}\left(\frac{R_\star}{a}\right)^{\!5}\frac{1}{Q'_\star}, where n=\sqrt{G(M_\star+M_2)/a^3} is the mean motion, Q'_2 and Q'_\star are the modified tidal quality factors of the companion and the star (Q'\equiv 3Q/2k_2, with k_2 the Love number), M_\star (M_2) and R_\star (R_2) are the stellar (companion) mass and radius, and a is the semi-major axis. It is often convenient to write the two contributions as separate timescales, \tau_{e,2}=\frac{4}{63}\, Q'_2\left(\frac{M_2}{M_\star}\right)\left(\frac{a}{R_2}\right)^{\!5}\frac{1}{n}, \qquad \tau_{e,\star}=\frac{16}{171}\, Q'_\star\left(\frac{M_\star}{M_2}\right)\left(\frac{a}{R_\star}\right)^{\!5}\frac{1}{n}, so that 1/\tau_e=1/\tau_{e,2}+1/\tau_{e,\star}. These expressions assume the equilibrium tide with constant phase lag, zero obliquities, and the small-e limit; \tau_e is the e-folding time, not the time to reach e=0. We evaluate the eccentricity–damping time \tau_e for our 8\,d system TIC\,9344899 over the plausible tidal quality factors (\log Q'_2\sim4.5\!-\!6.5 for BDs and \log Q'_\star\sim4\!-\!8 for stars; Heller2010Beatty2018Jackson2008Penev2012CollierCameron2018Vissapragada2022). TIC 9344899 system falls in a regime where \emph{stellar} tides dominate the eccentricity damping for most of the plausible Q' ranges; the decisive levers are the sizes and masses of the bodies. \textit{TIC~9344899\,b} orbits a near-solar host star with a radius of R_\star = 1.06\, R_\odot. It has a more compact companion with a radius of R_2 = 0.82\, R_{\rm J}, which is also located relatively far away, resulting in slower tidal interactions. The older age of TIC 9344899\,b, estimated at 6.1^{+4.1}_{-2.9} billion years, partly compensates for its weaker tidal effects. Read directly from the \tau_e maps in Fig. \ref{['fig:tides']}, the stellar Q'_\star threshold where \tau_e\simeq\,age is therefore \emph{similar}: \log_{10}Q'_\star\approx5.5. For solar-type stars, both population studies and theoretical models generally suggest a higher value of Q'_\star (indicating less dissipation) on the main sequence, which typically falls within the range of Q'_\star \sim 10^{5.5\text{–}6.5} Ogilvie2014. This implies that the circularization of orbits likely occurs more slowly than the median stellar age, unless the star exhibits unusually high dissipation or the system's age is at the upper end of the uncertainty range. Given these efficiencies, the system does not permit a sharp distinction between gentle (disk/in–situ) and impulsive (scattering/Kozai) pathways: the present low eccentricity is consistent with either, once plausible Q'_\star and ages are allowed. Targeted RV follow-up to search for outer perturbers would help to break this degeneracy. Recent work on transiting long-period companions has argued that brown dwarfs (BDs) with P>10\,d exhibit an eccentricity distribution similar to that of warm/hot giant planets A_New_BD_Mstar_2025. That conclusion rests on adopting P>10\,d as a practical boundary for "negligible tides" and then comparing the BD e distribution to that of giant planets (GTPs) and low-mass stars (LMSs). In what follows, we reproduce the P>10\,d cut for comparability, but we also examine the period-eccentricity structure of the BD sample and find that the apparent GTP-like e distribution is largely driven by a small subset of six systems at 10\!<\! P\!\le\!16\,d with very low eccentricities (see Fig. \ref{['fig:split']} and Fig. \ref{['fig:beta']}). Concretely, across four groups: GTPs, all BDs (P\geq10\,d), LMSs, and BDs with P\geq16\,d, we obtain (median e, 16–84\%): GTPs (0.294,,0.035–0.670), all BDs (0.250,,0.037–0.641), LMSs (0.312,,0.160–0.512), BD(P\geq16\,d) (0.329,,0.200–0.693). Two-sample tests show that most pairs are not distinguishable at current N, but a shape-sensitive Epps–Singleton test flags differences between GTPs and LMSs and between GTPs and BDs (P\geq16\,d), while GTPs vs “all BDs” is not rejected. Parametric cross-checks with single-Beta fits illustrate the same shift (GTPs: \alpha=0.75,\ \beta=1.44; BDs (P\geq16\,d): \alpha=1.81,\ \beta=2.59), albeit with mixed information-criterion support given small samples (weak \Delta AIC\,<0 for separate fits; \Delta BIC\,>0 favoring a pooled model at current N). Taken together, the simplest takeaway is: When short-period ($10$–$16$,d) low-$e$ BDs are set aside, the $P\geq16$,d BD population looks more LMS-like than GTP-like in eccentricity. Both the BD and LMS populations exhibit signs of bimodality; however, additional systems are needed for better statistical evaluation. We asked whether the low-eccentricity BD systems at P=10--16\,d exhibit any shared host or companion properties that would mark them as a distinct formation channel. They do not: the host masses, radii, and metallicities span wide ranges, and the companions likewise cover a broad swath in M_2, and mass ratio q. In particular, [Fe/H] and q show no significant offsets relative to longer-period BDs, and the only hint is a weak tendency toward lower M_2 and smaller R_2 at shorter periods (marginal at best). Lacking a clean demographic signature, the simplest explanation for their low eccentricities is \emph{partial tidal damping} at these separations. A common back-of-the-envelope is the small-e circularization time \tau_e evaluated at the present semi-major axis (e.g., constant-phase-lag scaling; Jackson2008). Scanning wide dissipation grids Q'_\star,Q'_2\in[10^4,10^8], we find that only two of six systems reach \tau_e<10,Gyr at the most dissipative edge (Q'_\star\sim10^4); for Q'_\star\ge10^5, all have \tau_e>10,Gyr. However, as expected, these small-e estimates may understate early damping, because tidal rates increase steeply at high e. We therefore integrated the standard constant-time-lag (CTL) equations for coupled star+BD tides with a pseudo-synchronous BD spin Hut1981Jackson2008. To set the initial orbit after an excitation phase, we adopted a constant-periastron start, which is a neutral, widely used way to connect high-e excitation to subsequent tidal cooling; once excitation ceases, tides act at the existing periastron distance r_p. For a modest e_0=0.25, we find for our 6 systems: Fast/likely: TOI-1406b and TOI-4776b have broad ranges of Q'\star in [10^4,10^6] with t_{\rm damp}(e_0\rightarrow e_{\rm obs})\lesssim5\,Gyr. Borderline: KOI-205b and TOI-5389Ab typically cool within \sim5\,Gyr near the more dissipative end Q'_\star\leq10^{4.5-4.75}. Slow: LHS,6343b and TOI-1278b need \gtrsim5–10\,Gyr unless Q'_\star is near 10^4. In our setup, the CTL damping rate gains a strong \emph{high-$e$} boost (through the Hut eccentricity functions) but suffers an a^{13/2} penalty from the inflated starting semi-major axis. For \emph{modest} excitation (e_0\!\sim\!0.25; a_0/a_{\rm now}=1/(1-e_0)=4/3), the high-e boost typically \emph{outweighs} the a^{13/2} penalty, so the full CTL time can be \emph{shorter} than the small-e \tau_e evaluated at today’s a. By contrast, for \emph{strong} excitation (e_0\!\gtrsim\!0.6; a_0/a_{\rm now}=2.5), the a^{13/2}\!\approx\!2.5^{6.5} and penalty dominates, making the CTL time \emph{longer} than the local small-e estimate and pushing several systems beyond a Hubble time. The fastest channels generally occur when stellar dissipation dominates (low Q'\star). Interestingly, our three companions with the weakest tidal interactions (TOI-5389\,Ab LHS\,6343\,b and TOI-1278\,b) are found around M-dwarf hosts. M-dwarfs being deeply convective, plausibly sit toward the more dissipative end Gallet2017. Within these ranges, tides can plausibly explain the low e for most—and potentially all—of the 10–16\,d systems if their post-excitation eccentricities were modest (e_0\sim0.2–0.3) and Q'\star is on the efficient side of empirically allowed values (especially for M dwarfs). Stronger initial excitation (e_0\gtrsim0.6) inflates a_0 (via a_0\propto1/(1-e_0)) and slows CTL damping roughly as a^{13/2}, pushing several systems beyond a Hubble time. \newline \textbf{Implication.} The GTP-like appearance of “BDs with P>10\,d” in prior work is largely set by the six low-e objects at 10–16\,d. Those systems do not share a clean demographic signature but do sit where tides are most effective; full CTL integrations show that modest post-excitation e_0 and efficient (but empirically plausible) stellar dissipation suffice for all of them. Beyond 16\,d, transiting BDs resemble LMS binaries, and our three new P!>!100\,d systems strengthen the LMS-like high-P tail. Eccentricity vs. period distribution of transiting brown dwarfs with periods above ten days separated by the 16-d period boundary. Eccentricity distributions for (a) giant planets, (b) all transiting brown dwarfs ($P>10$,d), (c) low-mass stellar companions, and (d) the BD subsample with $P>16$,d. Step histograms use uniform bins in $e$; solid curves show the single-Beta maximum-likelihood fit to each panel (annotated by $(\alpha,\beta)$). Sample sizes are indicated in the legends. BDs ($P>16$,d) resemble LMSs more than GTPs, with a higher, more concentrated mid-$e$ preference, whereas the all-BDs distribution is pulled toward the GTP-like shape by the short-period, low-$e$ objects. This visual comparison complements our statistical results (ES permutation $p=0.016$ for GTP vs. BD($>16$,d); non-separation of BD($>16$,d) from LMS at current $N$). The planet--metallicity correlation is well established for close-in giant planets Santos2004Fischer2005Petigura2018, while stellar-mass companions show no or even negative preference for metal-rich hosts Raghavan2010Moe2019. The goal of this section is to examine where brown dwarfs lie along this axis. We compared the host metallicity distributions of three groups: GTPs, BDs, and LMSs. Median host metallicities are (see Fig. \ref{['fig:met']}): \text{GTPs}:\ +0.14~{\rm dex},\quad \text{BDs}:\ -0.06~{\rm dex},\quad \text{LMSs}:\ +0.06~{\rm dex},\quad with interquartile ranges of roughly \simeq0.20--0.25\,dex per group. Multiple two-sample tests reject equality for GTPs vs.\ BDs (P{>}16\,d) at the p\!\sim\!10^{-2} level (KS p_{\rm adj}=0.037, CvM p_{\rm adj}=0.007, Epps--Singleton p_{\rm adj}=0.004, Anderson--Darling p_{\rm adj}=0.009). All other pairwise comparisons are consistent with equality at the current N. These metallicity patterns independently support our eccentricity-based conclusion that: \emph{long-period brown dwarfs resemble LMS companions more than giant planets}. Population plots in Vowell2025 show that most \emph{short-period} transiting BDs---both below and above the often-quoted 40\, M_{\rm J} division---cluster around metal-rich hosts, following the same overall planet--metallicity trend as hot/warm Jupiters. By contrast, \emph{long-period} BD hosts skew metal-poor and become indistinguishable from low-mass stellar (LMS) companions within present uncertainties. We also do not see any metallicity bifurcation at 40\, M_{\rm J} within the current sample size: both lower- and higher-mass short-period BDs are abundant around metal-rich stars, whereas at long periods both mass ranges shift toward more field-like, typically lower metallicities. This pattern points to a \emph{period-coded} mixture rather than a mass-coded one. Interestingly, an analogous period dependence is observed for the population of hot and cold Jupiters. Maldonado2018 used a large sample of stars and found that stars with hot Jupiters have higher metallicities than stars with cool, distant gas-giant planets, which they speculate as evidence for distinct formation channels for hot and cold Jupiters. In their scenario, planets in metal-poor discs either form farther out or form later and do not have time to migrate as far as planets in metal-rich systems. In the brown-dwarf regime, we intentionally avoid importing the same detailed conclusions, because such scenarios must be tuned separately for different seed mechanisms (core accretion for giant planets vs.\ fragmentation for BDs) and therefore add unnecessary complexity. By contrast, metallicity-dependent \emph{inward delivery and survival}---via more massive and longer-lived viscous discs in metal-rich systems---operates regardless of the initial formation channel. Metal-rich systems have longer-lived, more massive/viscous discs Yasui2009Ercolano2010, enabling disc-phase delivery and damping that yield a higher survival fraction of massive companions at small radii, whereas metal-poor systems disperse discs earlier, pushing inward delivery (if it occurs at all) into high-eccentricity, low-survival channels Dawson2018Fortney2021. This metallicity-dependent delivery–survival pipeline naturally explains the metal-rich excess among short-period companions without requiring a specific brown-dwarf formation channel. Long-period BDs, on the other hand, look more like a stellar-binary–style channel (core/disc fragmentation) in which host metallicity only weakly influences the companion rate. Population studies of binaries show that close-binary fractions do not increase with [Fe/H] in the way giant-planet frequencies do and can even anticorrelate Moe2019. Consistent with this, the eccentricity distribution of \emph{long-period} (10\!\lesssim\! P\!\lesssim\!10^3~d) transiting BDs is not planet-like: instead of peaking at e\simeq0 as warm Jupiters do, it is potentially bimodal, with one peak near e\simeq0.2 and a second near e\simeq0.7, quite resembling the distribution of close stellar binaries. Some fraction of the modest-eccentricity component may already be imprinted during disc dispersal: secular interactions between a companion inside an inner cavity and a massive, mildly eccentric outer disc can resonantly excite eccentricities even if the disc itself is only weakly eccentric Li2023. However, it is unlikely to be the sole origin of all eccentric systems. We therefore interpret the observed distribution more broadly as the superposition of (i) dynamically quieter systems—objects that migrated and circularised quiescently in or near the disc plane and/or experienced only mild secular evolution, yielding low to moderate eccentricities—and (ii) systems that were later excited to high eccentricities by binary-like secular processes (Kozai–Lidov cycles, scattering, or secular chaos in higher-order multiples) once the disc had dispersed. In this view, the short-period metallicity break is set primarily during the disc phase, by which companions are delivered to, and stabilised at, very short periods in metal-rich discs, whereas the bimodal eccentricity structure at longer periods mainly records subsequent, largely metallicity-insensitive binary-style secular evolution. Spin–orbit measurements of brown-dwarf systems provide a complementary constraint on the migration geometry. All transiting BDs with Rossiter–McLaughlin measurements are consistent with low projected obliquities, even when their orbits are substantially eccentric: TOI-2119~b (P\!=\!7.2~d, e\!\simeq\!0.3), TOI-2533~b (P\!\approx\!21~d, e\!\approx\!0.25), and HIP~33609~b (P\!=\!39~d, e\!=\!0.56) all exhibit aligned or nearly aligned orbits within current uncertainties Ferreira2024Doyle2025Vowell2025. This combination of a broad, binary-like eccentricity distribution and a narrow obliquity distribution points to eccentricity excitation that is predominantly \emph{coplanar} with the natal disc plane—such as secular interactions and scattering in hierarchically structured, but only mildly inclined, multiples. In this picture, most brown dwarfs inherit a disc-aligned configuration from their fragmentation and disc-interaction phase, with subsequent binary-style secular evolution broadening the eccentricity distribution without strongly tilting the orbital plane. Short-period transiting brown dwarfs are therefore most naturally explained by inward delivery rather than in\hbox{-}situ formation at few-day orbits. Gravitational instability (GI) and disc fragmentation (stellar-/disc-like formation) operate preferentially at larger distances (tens to hundreds of au), not at \lesssim 0.1~au where cooling is inefficient and irradiation is strong KratterLodato2016. Close binaries and BD companions at few-day periods are thus expected to have formed wider and then hardened/migrated inward through some combination of gas torques and multi-body dynamics Tokovinin2020CloseBinaries. Inward evolution need not proceed as a single, smooth Type-II track: hydrodynamic simulations show that migration, resonant capture, and planet–planet scattering can all operate while the gas disc is still present, and that interaction with the disc can circularise or stabilise surviving companions after the chaotic phase, reducing the incidence of ejections and leaving some companions on bound, moderately eccentric orbits that continue to migrate inward Moeckel2008Marzari2010. In this sense, even “high-eccentricity migration” channels can be disc-assisted when they operate during the gas phase, and the survival of a short-period BD is already contingent on the disc having enough mass and lifetime to both deliver and stabilise the companion. The metallicity dependence then enters most directly through the disc properties rather than through the subsequent dynamical heating. High-eccentricity migration channels that occur after disc dispersal (such as Kozai–Lidov cycles or secular chaos in stellar or BD multiples) play a role in shaping the overall brown dwarf desert. However, there is no compelling reason to expect these post-disc processes to be strongly influenced by metallicity. The relevant perturbers in these cases are typically other stars or substellar companions that formed through fragmentation; their occurrence rates do not increase with higher metallicity and may even anticorelate Moe2019. Consequently, while these channels can effectively broaden the distributions of semi-major axes and eccentricities, they do not inherently create a strong metallicity–period boundary on their own. By contrast, \emph{disc-driven migration and damping} of a high-mass companion tie short-period survival much more directly to the structure and lifetime of the protoplanetary gas disc, properties that are empirically and theoretically linked to metallicity, with low-metallicity environments showing systematically shorter disc lifetimes and lower gas masses Yasui2009KleyNelson2012. In this framework, the metal-rich excess of short-period BDs reflects the larger window, in high-metallicity discs, for any combination of disc-assisted migration and early dynamical excitation to bring brown dwarfs safely to few-day orbits. A recent \textit{TESS} timing analysis of transiting brown dwarfs reports \emph{no statistically significant transit-timing variations} attributable to additional companions Wang2025_ExoEchoBDTTV. Throughout, by TTVs we mean \emph{three-body} signals from nearby perturbers in or near resonance Agol2005Lithwick2012, not long-term tidal-decay drifts. This null detection is \emph{consistent} with inward, disc-driven delivery by a gap-opening, high-mass companion: such bodies push material away from their orbit and carve deep gaps, tending to deplete the immediate vicinity of long-lived, close neighbours where three-body TTVs would be most detectable KleyNelson2012. For context, early population studies found that hot Jupiters rarely show nearby companions/TTVs Steffen2012, with the few companion-rich systems likely tracing in-situ or very gentle migration channels that preserve neighbours Becker2015Almenara2016Canas2019_Kepler730Subjak2025_TOI2458. In our framework, \emph{short-period} BDs near the cavity should likewise rarely show close three-body TTVs, as found by Wang2025_ExoEchoBDTTV, whereas for \emph{long-period} transiting BDs the presence of both inner and outer gas during the nebular phase allows convergent migration and resonant neighbours in principle; such companions are, however, most plausibly relatively massive joint-gap neighbours, while low-mass near-resonant planets remain disfavoured by the BD’s wide gap and large chaotic zone. Altogether, the most straightforward conclusion is that metal-rich systems are over-efficient at disc-delivering and retaining massive companions close in (hence the metal-rich short-period tail), whereas metal-poor systems preferentially populate the long-period BD regime that follow-up is now uncovering. Finally, we point out several limitations in the current study. Metallicities come from heterogeneous spectroscopic pipelines and carry systematics, and small N makes many pairwise tests non-rejectable. The case would be strengthened by (i) a substantially larger long-period transiting BD and LMS sample, and (ii) homogenising the host stellar parameters used in future population-level analyses. Host [Fe/H] distributions for GTPs, LMSs, and BDs ($P>16$,d). BD hosts are more metal-poor than GTP hosts (multiple tests, Holm-adjusted $p\le0.04$) and are not separable from LMS hosts at current $N$, consistent with the LMS-like behavior seen in eccentricities. We report the discovery of four new transiting brown dwarfs, three of which exhibit orbital periods exceeding 100 days. Prior to this study, only two such long-period transiting brown dwarfs were known; thus, our findings effectively double the existing sample and enhance our understanding of the high-period tail of the population. Notably, all three long-period objects are found to orbit stars with subsolar metallicity, aligning with the broader trend observed for long-period brown dwarfs. In our analysis, we utilized catalogs of giant planets, brown dwarfs, and low-mass stellar companions with periods greater than 10 days to compare their eccentricity distributions. The inclusive dataset for all brown dwarfs with periods exceeding 10 days initially reflects the giant planet-like eccentricity distribution; however, this is influenced by six nearly circular objects within the 10 to 16-day period range. Upon excluding these objects, the sample of brown dwarfs with periods exceeding 16 days demonstrates a shift towards the regime of low-mass stars. We investigated whether the 10–16 d brown dwarfs exhibit distinct demographic characteristics. Our analysis indicates no significant differences in host metallicity [Fe/H], mass ratio q, or radii, suggesting that tidal interactions, rather than a unique formation process, are at play. The small-eccentricity circularization times calculated at their current semimajor axes appear prolonged. However, comprehensive circularization time law (CTL) integrations initiated from a moderate eccentricity (e_0 \sim 0.25) with a conservative constant-periastron initialization demonstrate that all six systems have the potential to achieve their observed eccentricities within approximately 10 billion years. Notably, this process may necessitate lower values of Q'_\star for certain systems. Therefore, it is plausible that mild tidal interactions contribute to the low eccentricities observed among these short-period brown dwarfs, thereby influencing the distribution of eccentricities. Host metallicities support the picture. Long-period brown dwarfs are predominantly found orbiting stars that exhibit significantly lower metallicity compared to long-period giant planet hosts. This observation aligns statistically with the characteristics of low-mass star hosts. In contrast, short-period brown dwarfs—regardless of whether they are below or above the frequently cited 40,M_{\rm J} threshold—are concentrated around metal-rich stars, reflecting the metallicity distribution observed in hot Jupiters. The lack of a distinct [Fe/H] bifurcation at 40,M_{\rm J} argues against a purely mass-coded split and instead favors a period-coded mixture. This conclusion is further substantiated by the analogous metallicity trends noted between hot and cold Jupiters. Metal-rich disks (more massive/viscous, longer-lived) preferentially deliver and retain massive companions at small radii, independent of whether the seeds formed via core accretion or fragmentation. In summary, our identification of three new brown dwarfs with periods greater than 100 days highlights the expansion of the metal-poor, long-period distribution, where these brown dwarfs exhibit characteristics akin to low-mass stellar binaries in terms of both the eccentricity distribution p(e) and [Fe/H]. Conversely, the short-period, metal-rich distribution likely reflects the influence of metallicity on inward migration and retention. Expanding the sample of transiting brown dwarfs and low-mass stars and homogenizing host metallicities will be critical for evaluating single- versus two-component models of p(e) and for clarifying the relative contributions of formation and migration processes in shaping the inner and outer boundaries of the brown dwarf desert. J.{S}. would like to acknowledge the support from GACR grant 23-06384O. A.J. acknowledges support from Fondecyt project 1251439. This work was supported by ANID Fondecyt n. 1251299 and Basal CATA FB210003. Funding for the TESS mission is provided by NASA's Science Mission Directorate. We acknowledge the use of public TESS data from pipelines at the TESS Science Office and at the TESS Science Processing Operations Center. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. This paper includes data collected by the TESS mission that are publicly available from the Mikulski Archive for Space Telescopes (MAST). This research has made use of the Exoplanet Follow-up Observation Program (ExoFOP; DOI: 10.26134/ExoFOP5) website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. This work makes use of observations from the LCOGT network. Part of the LCOGT telescope time was granted by NOIRLab through the Mid-Scale Innovations Program (MSIP). MSIP is funded by NSF. This work is based in part on data collected under the NGTS project at the ESO La Silla Paranal Observatory. The NGTS facility is operated by a consortium institutes with support from the UK Science and Technology Facilities Council (STFC) under projects ST/M001962/1, ST/S002642/1 and ST/W003163/1. This research has made use of the Simbad and Vizier databases, operated at the centre de Donn'ees Astronomiques de Strasbourg (CDS), and of NASA's Astrophysics Data System Bibliographic Services (ADS). This work has made use of data from the European Space Agency (ESA) mission { Gaia} (https://www.cosmos.esa.int/gaia), processed by the { Gaia} Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). 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B.}, title={Possible Solutions to the Radius Anomalies of Transiting Giant Planets}, journal={\apj}, keywords={Stars: Planetary Systems, Planets and Satellites: General, Astrophysics}, volume={661}, number={1}, pages={502-514}, doi={10.1086/514326}, archiveprefix={arXiv}, eprint={astro-ph/0612703}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2007ApJ...661..502B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Chabrier07, author={Chabrier, Gilles and Baraffe, Isabelle}, title={Heat Transport in Giant (Exo)planets: A New Perspective}, journal={\apjl}, keywords={Convection, Hydrodynamics, Stars: Planetary Systems, Planets and Satellites: General, Astrophysics}, volume={661}, number={1}, pages={L81-L84}, doi={10.1086/518473}, archiveprefix={arXiv}, eprint={astro-ph/0703755}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2007ApJ...661L..81C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Kurokawa15, author={Kurokawa, Hiroyuki and Inutsuka, Shu-ichiro}, title={On the Radius Anomaly of Hot Jupiters: Reexamination of the Possibility and Impact of Layered Convection}, journal={\apj}, keywords={planets and satellites: gaseous planets, planets and satellites: interiors, planets and satellites: physical evolution, Astrophysics - Earth and Planetary Astrophysics}, volume={815}, number={1}, eid={78}, pages={78}, doi={10.1088/0004-637X/815/1/78}, archiveprefix={arXiv}, eprint={1511.03063}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ApJ...815...78K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Youdin10, author={Youdin, Andrew N. and Mitchell, Jonathan L.}, title={The Mechanical Greenhouse: Burial of Heat by Turbulence in Hot Jupiter Atmospheres}, journal={\apj}, keywords={diffusion, opacity, planet-star interactions, planets and satellites: atmospheres, radiative transfer, turbulence, Astrophysics - Earth and Planetary Astrophysics}, volume={721}, number={2}, pages={1113-1126}, doi={10.1088/0004-637X/721/2/1113}, archiveprefix={arXiv}, eprint={1008.0645}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2010ApJ...721.1113Y}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Tremblin17, author={Tremblin, P. and Chabrier, G. and Mayne, N. J. and Amundsen, D. S. and Baraffe, I. and Debras, F. and Drummond, B. and Manners, J. and Fromang, S.}, title={Advection of Potential Temperature in the Atmosphere of Irradiated Exoplanets: A Robust Mechanism to Explain Radius Inflation}, journal={\apj}, keywords={atmospheric effects, methods: numerical, planets and satellites: general, Astrophysics - Earth and Planetary Astrophysics}, volume={841}, number={1}, eid={30}, pages={30}, doi={10.3847/1538-4357/aa6e57}, archiveprefix={arXiv}, eprint={1704.05440}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2017ApJ...841...30T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Batygin10, author={Batygin, Konstantin and Stevenson, David J.}, title={Inflating Hot Jupiters with Ohmic Dissipation}, journal={\apjl}, keywords={magnetohydrodynamics: MHD, methods: analytical, planets and satellites: interiors, Astrophysics - Earth and Planetary Astrophysics}, volume={714}, number={2}, pages={L238-L243}, doi={10.1088/2041-8205/714/2/L238}, archiveprefix={arXiv}, eprint={1002.3650}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2010ApJ...714L.238B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Perna10, author={Perna, Rosalba and Menou, Kristen and Rauscher, Emily}, title={Ohmic Dissipation in the Atmospheres of Hot Jupiters}, journal={\apj}, keywords={atmospheric effects, planets and satellites: general, planets and satellites: individual: HD9448b, Astrophysics - Earth and Planetary Astrophysics}, volume={724}, number={1}, pages={313-317}, doi={10.1088/0004-637X/724/1/313}, archiveprefix={arXiv}, eprint={1009.3273}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2010ApJ...724..313P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Wu13, author={Wu, Yanqin and Lithwick, Yoram}, title={Ohmic Heating Suspends, Not Reverses, the Cooling Contraction of Hot Jupiters}, journal={\apj}, keywords={planetary systems, planets and satellites: magnetic fields, planets and satellites: physical evolution, planet-star interactions, Astrophysics - Earth and Planetary Astrophysics}, volume={763}, number={1}, eid={13}, pages={13}, doi={10.1088/0004-637X/763/1/13}, archiveprefix={arXiv}, eprint={1202.0026}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2013ApJ...763...13W}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Ginzburg16, author={Ginzburg, Sivan and Sari, Re'em}, title={Extended Heat Deposition in Hot Jupiters: Application to Ohmic Heating}, journal={\apj}, keywords={planetary systems, planets and satellites: general, Astrophysics - Earth and Planetary Astrophysics}, volume={819}, number={2}, eid={116}, pages={116}, doi={10.3847/0004-637X/819/2/116}, archiveprefix={arXiv}, eprint={1511.00135}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2016ApJ...819..116G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Huang20, author={Huang, Chelsea X. and Vanderburg, Andrew and Pál, Andras and Sha, Lizhou and Yu, Liang and Fong, Willie and Fausnaugh, Michael and Shporer, Avi and Guerrero, Natalia and Vanderspek, Roland and Ricker, George}, title={Photometry of 10 Million Stars from the First Two Years of TESS Full Frame Images: Part I}, journal={Research Notes of the American Astronomical Society}, keywords={Space observatories, Astronomy data analysis, 1543, 1858, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={4}, number={11}, eid={204}, pages={204}, doi={10.3847/2515-5172/abca2e}, archiveprefix={arXiv}, eprint={2011.06459}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2020RNAAS...4..204H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Guerrero21, author={Guerrero, Natalia M. and Seager, S. and Huang, Chelsea X. and Vanderburg, Andrew and Garcia Soto, Aylin and Mireles, Ismael and Hesse, Katharine and Fong, William and Glidden, Ana and Shporer, Avi and Latham, David W. and Collins, Karen A. and Quinn, Samuel N. and Burt, Jennifer and Dragomir, Diana and Crossfield, Ian and Vanderspek, Roland and Fausnaugh, Michael and Burke, Christopher J. and Ricker, George and Daylan, Tansu and Essack, Zahra and Günther, Maximilian N. and Osborn, Hugh P. and Pepper, Joshua and Rowden, Pamela and Sha, Lizhou and Villanueva, Steven, Jr. and Yahalomi, Daniel A. and Yu, Liang and Ballard, Sarah and Batalha, Natalie M. and Berardo, David and Chontos, Ashley and Dittmann, Jason A. and Esquerdo, Gilbert A. and Mikal-Evans, Thomas and Jayaraman, Rahul and Krishnamurthy, Akshata and Louie, Dana R. and Mehrle, Nicholas and Niraula, Prajwal and Rackham, Benjamin V. and Rodriguez, Joseph E. and Rowden, Stephen J. L. and Sousa-Silva, Clara and Watanabe, David and Wong, Ian and Zhan, Zhuchang and Zivanovic, Goran and Christiansen, Jessie L. and Ciardi, David R. and Swain, Melanie A. and Lund, Michael B. and Mullally, Susan E. and Fleming, Scott W. and Rodriguez, David R. and Boyd, Patricia T. and Quintana, Elisa V. and Barclay, Thomas and Colón, Knicole D. and Rinehart, S. A. and Schlieder, Joshua E. and Clampin, Mark and Jenkins, Jon M. and Twicken, Joseph D. and Caldwell, Douglas A. and Coughlin, Jeffrey L. and Henze, Chris and Lissauer, Jack J. and Morris, Robert L. and Rose, Mark E. and Smith, Jeffrey C. and Tenenbaum, Peter and Ting, Eric B. and Wohler, Bill and Bakos, G. Á. and Bean, Jacob L. and Berta-Thompson, Zachory K. and Bieryla, Allyson and Bouma, Luke G. and Buchhave, Lars A. and Butler, Nathaniel and Charbonneau, David and Doty, John P. and Ge, Jian and Holman, Matthew J. and Howard, Andrew W. and Kaltenegger, Lisa and Kane, Stephen R. and Kjeldsen, Hans and Kreidberg, Laura and Lin, Douglas N. C. and Minsky, Charlotte and Narita, Norio and Paegert, Martin and Pál, András and Palle, Enric and Sasselov, Dimitar D. and Spencer, Alton and Sozzetti, Alessandro and Stassun, Keivan G. and Torres, Guillermo and Udry, Stephane and Winn, Joshua N.}, title={The TESS Objects of Interest Catalog from the TESS Prime Mission}, journal={\apjs}, keywords={Exoplanet catalogs, Exoplanets, Exoplanet astronomy, 488, 498, 486, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={254}, number={2}, eid={39}, pages={39}, doi={10.3847/1538-4365/abefe1}, archiveprefix={arXiv}, eprint={2103.12538}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021ApJS..254...39G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{Jenkins16, author={Jenkins, Jon M. and Twicken, Joseph D. and McCauliff, Sean and Campbell, Jennifer and Sanderfer, Dwight and Lung, David and Mansouri-Samani, Masoud and Girouard, Forrest and Tenenbaum, Peter and Klaus, Todd and Smith, Jeffrey C. and Caldwell, Douglas A. and Chacon, A. D. and Henze, Christopher and Heiges, Cory and Latham, David W. and Morgan, Edward and Swade, Daryl and Rinehart, Stephen and Vanderspek, Roland}, title={The TESS science processing operations center}, booktitle={Software and Cyberinfrastructure for Astronomy IV}, editor={Chiozzi, Gianluca and Guzman, Juan C.}, series={Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series}, volume={9913}, eid={99133E}, pages={99133E}, doi={10.1117/12.2233418}, adsurl={https://ui.adsabs.harvard.edu/abs/2016SPIE.9913E..3EJ}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Twicken18, author={Twicken, J. D. and Catanzarite, J. H. and Clarke, B. D. and Girouard, F. and Jenkins, J. M. and Klaus, T. C. and Li, J. and McCauliff, S. D. and Seader, S. E. and Tenenbaum, P. and Wohler, B. and Bryson, S. T. and Burke, C. J. and Caldwell, D. A. and Haas, M. R. and Henze, C. E. and Sanderfer, D. T.}, title={Kepler Data Validation I\mdashArchitecture, Diagnostic Tests, and Data Products for Vetting Transiting Planet Candidates}, journal={\pasp}, archiveprefix={arXiv}, eprint={1803.04526}, primaryclass={astro-ph.EP}, pages={064502}, doi={10.1088/1538-3873/aab694}, adsurl={http://adsabs.harvard.edu/abs/2018PASP..130f4502T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Barragan22, author={Barragán, Oscar and Aigrain, Suzanne and Rajpaul, Vinesh M. and Zicher, Norbert}, title={PYANETI - II. A multidimensional Gaussian process approach to analysing spectroscopic time-series}, journal={\mnras}, keywords={methods: numerical, techniques: photometry, techniques: spectroscopy, planets and satellites: general, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={509}, number={1}, pages={866-883}, doi={10.1093/mnras/stab2889}, archiveprefix={arXiv}, eprint={2109.14086}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022MNRAS.509..866B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Parviainen15, author={Parviainen, Hannu}, title={PYTRANSIT: fast and easy exoplanet transit modelling in PYTHON}, journal={\mnras}, keywords={methods: numerical, techniques: photometric, planets and satellites: general, Astrophysics - Earth and Planetary Astrophysics}, volume={450}, number={3}, pages={3233-3238}, doi={10.1093/mnras/stv894}, archiveprefix={arXiv}, eprint={1504.07433}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015MNRAS.450.3233P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Aller20, author={Aller, A. and Lillo-Box, J. and Jones, D. and Miranda, L. F. and Barceló Forteza, S.}, title={Planetary nebulae seen with TESS: Discovery of new binary central star candidates from Cycle 1}, journal={\aap}, keywords={planetary nebulae: general, techniques: photometric, binaries: general, Astrophysics - Solar and Stellar Astrophysics}, volume={635}, eid={A128}, pages={A128}, doi={10.1051/0004-6361/201937118}, archiveprefix={arXiv}, eprint={1911.09991}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2020A&A...635A.128A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Tokovinin08, author={Tokovinin, A. and Cantarutti, R.}, title={First Speckle Interferometry at SOAR Telescope with Electron-Multiplication CCD}, journal={\pasp}, volume={120}, number={864}, pages={170}, doi={10.1086/528809}, adsurl={https://ui.adsabs.harvard.edu/abs/2008PASP..120..170T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Tokovinin18, author={Tokovinin, Andrei}, title={Ten Years of Speckle Interferometry at SOAR}, journal={\pasp}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics}, volume={130}, number={985}, pages={035002}, doi={10.1088/1538-3873/aaa7d9}, archiveprefix={arXiv}, eprint={1801.04772}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2018PASP..130c5002T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Ziegler21, author={Ziegler, Carl and Tokovinin, Andrei and Latiolais, Madelyn and Briceño, César and Law, Nicholas and Mann, Andrew W.}, title={SOAR TESS Survey. II. The Impact of Stellar Companions on Planetary Populations}, journal={\aj}, keywords={Binary stars, Companion stars, Exoplanet astronomy, Exoplanet dynamics, Speckle interferometry, 154, 291, 486, 490, 1552, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={162}, number={5}, eid={192}, pages={192}, doi={10.3847/1538-3881/ac17f6}, archiveprefix={arXiv}, eprint={2103.12076}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021AJ....162..192Z}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Collins17, author={Collins, Karen A. and Kielkopf, John F. and Stassun, Keivan G. and Hessman, Frederic V.}, title={AstroImageJ: Image Processing and Photometric Extraction for Ultra-precise Astronomical Light Curves}, journal={\aj}, keywords={methods: data analysis, techniques: image processing, techniques: photometric, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={153}, number={2}, eid={77}, pages={77}, doi={10.3847/1538-3881/153/2/77}, archiveprefix={arXiv}, eprint={1701.04817}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2017AJ....153...77C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Blanco14, author={Blanco-Cuaresma, S. and Soubiran, C. and Heiter, U. and Jofré, P.}, title={Determining stellar atmospheric parameters and chemical abundances of FGK stars with iSpec}, journal={\aap}, keywords={stars: atmospheres, stars: abundances, methods: data analysis, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={569}, eid={A111}, pages={A111}, doi={10.1051/0004-6361/201423945}, archiveprefix={arXiv}, eprint={1407.2608}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2014A&A...569A.111B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Blanco19, author={Blanco-Cuaresma, Sergi}, title={Modern stellar spectroscopy caveats}, journal={\mnras}, keywords={techniques: spectroscopic, stars: abundances, stars: atmospheres, stars: fundamental parameters, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={486}, number={2}, pages={2075-2101}, doi={10.1093/mnras/stz549}, archiveprefix={arXiv}, eprint={1902.09558}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2075B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Dotter16, author={Dotter, Aaron}, title={MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the Construction of Stellar Isochrones}, journal={\apjs}, keywords={methods: numerical, stars: evolution, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={222}, number={1}, eid={8}, pages={8}, doi={10.3847/0067-0049/222/1/8}, archiveprefix={arXiv}, eprint={1601.05144}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2016ApJS..222....8D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Choi16, author={Choi, Jieun and Dotter, Aaron and Conroy, Charlie and Cantiello, Matteo and Paxton, Bill and Johnson, Benjamin D.}, title={Mesa Isochrones and Stellar Tracks (MIST). I. Solar-scaled Models}, journal={\apj}, keywords={stars: evolution, stars: general, stars: interiors, Astrophysics - Solar and Stellar Astrophysics}, volume={823}, number={2}, eid={102}, pages={102}, doi={10.3847/0004-637X/823/2/102}, archiveprefix={arXiv}, eprint={1604.08592}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2016ApJ...823..102C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Horch14, author={Horch, Elliott P. and Howell, Steve B. and Everett, Mark E. and Ciardi, David R.}, title={Most Sub-arcsecond Companions of Kepler Exoplanet Candidate Host Stars are Gravitationally Bound}, journal={\apj}, keywords={binaries: visual, planetary systems, stars: solar-type, techniques: high angular resolution, techniques: interferometric, techniques: photometric, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={795}, number={1}, eid={60}, pages={60}, doi={10.1088/0004-637X/795/1/60}, archiveprefix={arXiv}, eprint={1409.1249}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2014ApJ...795...60H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Matson18, author={Matson, Rachel A. and Howell, Steve B. and Horch, Elliott P. and Everett, Mark E.}, title={Stellar Companions of Exoplanet Host Stars in K2}, journal={\aj}, keywords={binaries: general, binaries: visual, planetary systems, techniques: high angular resolution, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={156}, number={1}, eid={31}, pages={31}, doi={10.3847/1538-3881/aac778}, archiveprefix={arXiv}, eprint={1805.08844}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2018AJ....156...31M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{ElBadry18, author={El-Badry, Kareem and Rix, Hans-Walter and Ting, Yuan-Sen and Weisz, Daniel R. and Bergemann, Maria and Cargile, Phillip and Conroy, Charlie and Eilers, Anna-Christina}, title={Signatures of unresolved binaries in stellar spectra: implications for spectral fitting}, journal={\mnras}, keywords={methods: data analysis, stars: abundances, binaries: spectroscopic, Galaxy: stellar content, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, volume={473}, number={4}, pages={5043-5049}, doi={10.1093/mnras/stx2758}, archiveprefix={arXiv}, eprint={1709.03983}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2018MNRAS.473.5043E}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Green19, author={Green, Gregory M. and Schlafly, Edward and Zucker, Catherine and Speagle, Joshua S. and Finkbeiner, Douglas}, title={A 3D Dust Map Based on Gaia, Pan-STARRS 1, and 2MASS}, journal={\apj}, keywords={Interstellar reddening, Interstellar dust extinction, Galaxy structure, Galaxy stellar content, Interstellar dust, 853, 837, 622, 621, 836, Astrophysics - Astrophysics of Galaxies}, volume={887}, number={1}, eid={93}, pages={93}, doi={10.3847/1538-4357/ab5362}, archiveprefix={arXiv}, eprint={1905.02734}, primaryclass={astro-ph.GA}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJ...887...93G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Green18, author={Green, Gregory M.}, title={dustmaps: A Python interface for maps of interstellar dust}, journal={The Journal of Open Source Software}, volume={3}, number={26}, pages={695}, doi={10.21105/joss.00695}, adsurl={https://ui.adsabs.harvard.edu/abs/2018JOSS....3..695G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Byrd95, title={A limited memory algorithm for bound constrained optimization}, abstract={An algorithm for solving large nonlinear optimization problems with simple bounds is described. It is based on the gradient projection method and uses a limited memory BFGS matrix to approximate the Hessian of the objective function. It is shown how to take advantage of the form of the limited memory approximation to implement the algorithm efficiently. The results of numerical tests on a set of large problems are reported.}, author={Byrd, Richard H. and Peihuang Lu and Jorge Nocedal and Ciyou Zhu}, year={1995}, doi={10.1137/0916069}, language={English}, volume={16}, pages={1190--1208}, journal={SIAM Journal of Scientific Computing}, issn={1064-8275}, publisher={Society for Industrial and Applied Mathematics Publications} }@article{Zhu97, author={Zhu, Ciyou and Byrd, Richard H. and Lu, Peihuang and Nocedal, Jorge}, title={Algorithm 778: L-BFGS-B: Fortran Subroutines for Large-Scale Bound-Constrained Optimization}, year={1997}, issue_date={Dec. 1997}, publisher={Association for Computing Machinery}, address={New York, NY, USA}, volume={23}, number={4}, issn={0098-3500}, url={https://doi.org/10.1145/279232.279236}, doi={10.1145/279232.279236}, abstract={L-BFGS-B is a limited-memory algorithm for solving large nonlinear optimization problems subject to simple bounds on the variables. It is intended for problems in which information on the Hessian matrix is difficult to obtain, or for large dense problems. L-BFGS-B can also be used for unconstrained problems and in this case performs similarly to its predessor, algorithm L-BFGS (Harwell routine VA15). The algorithm is implemented in Fortran 77.}, journal={ACM Trans. Math. Softw.}, pages={550–560}, numpages={11}, keywords={large-scale optimization, limited-memory method, nonlinear optimization, variable metric method} }@article{Goodman10, author={Goodman, Jonathan and Weare, Jonathan}, title={Ensemble samplers with affine invariance}, journal={Communications in Applied Mathematics and Computational Science}, keywords={Markov chain Monte Carlo, affine invariance, ensemble samplers}, volume={5}, number={1}, pages={65-80}, doi={10.2140/camcos.2010.5.65}, adsurl={https://ui.adsabs.harvard.edu/abs/2010CAMCS...5...65G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Foreman13, author={Foreman-Mackey, Daniel and Hogg, David W. and Lang, Dustin and Goodman, Jonathan}, title={emcee: The MCMC Hammer}, journal={\pasp}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Computational Physics, Statistics - Computation}, volume={125}, number={925}, pages={306}, doi={10.1086/670067}, archiveprefix={arXiv}, eprint={1202.3665}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2013PASP..125..306F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Zechmeister09, author={Zechmeister, M. and Kürster, M.}, title={The generalised Lomb-Scargle periodogram. A new formalism for the floating-mean and Keplerian periodograms}, journal={\aap}, keywords={methods: data analysis, methods: analytical, methods: statistical, techniques: radial velocities, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={496}, number={2}, pages={577-584}, doi={10.1051/0004-6361:200811296}, archiveprefix={arXiv}, eprint={0901.2573}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2009A&A...496..577Z}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Gaia21, author={Gaia Collaboration and Brown, A. G. A. and Vallenari, A. and Prusti, T. and de Bruijne, J. H. J. and Babusiaux, C. and Biermann, M. and Creevey, O. L. and Evans, D. W. and Eyer, L. and Hutton, A. and Jansen, F. and Jordi, C. and Klioner, S. A. and Lammers, U. and Lindegren, L. and Luri, X. and Mignard, F. and Panem, C. and Pourbaix, D. and Randich, S. and Sartoretti, P. and Soubiran, C. and Walton, N. A. and Arenou, F. and Bailer-Jones, C. A. L. and Bastian, U. and Cropper, M. and Drimmel, R. and Katz, D. and Lattanzi, M. G. and van Leeuwen, F. and Bakker, J. and Cacciari, C. and Castañeda, J. and De Angeli, F. and Ducourant, C. and Fabricius, C. and Fouesneau, M. and Frémat, Y. and Guerra, R. and Guerrier, A. and Guiraud, J. and Jean-Antoine Piccolo, A. and Masana, E. and Messineo, R. and Mowlavi, N. and Nicolas, C. and Nienartowicz, K. and Pailler, F. and Panuzzo, P. and Riclet, F. and Roux, W. and Seabroke, G. M. and Sordo, R. and Tanga, P. and Thévenin, F. and Gracia-Abril, G. and Portell, J. and Teyssier, D. and Altmann, M. and Andrae, R. and Bellas-Velidis, I. and Benson, K. and Berthier, J. and Blomme, R. and Brugaletta, E. and Burgess, P. 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B. and Teixeira, R. and Thuillot, W. and Tonello, N. and Torra, F. and Torra, J. and Turon, C. and Unger, N. and Vaillant, M. and van Dillen, E. and Vanel, O. and Vecchiato, A. and Viala, Y. and Vicente, D. and Voutsinas, S. and Weiler, M. and Wevers, T. and Wyrzykowski, Ł. and Yoldas, A. and Yvard, P. and Zhao, H. and Zorec, J. and Zucker, S. and Zurbach, C. and Zwitter, T.}, title={Gaia Early Data Release 3. Summary of the contents and survey properties}, journal={\aap}, keywords={catalogs, astrometry, parallaxes, proper motions, techniques: photometric, techniques: radial velocities, Astrophysics - Astrophysics of Galaxies}, volume={649}, eid={A1}, pages={A1}, doi={10.1051/0004-6361/202039657}, archiveprefix={arXiv}, eprint={2012.01533}, primaryclass={astro-ph.GA}, adsurl={https://ui.adsabs.harvard.edu/abs/2021A&A...649A...1G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Stassun18, author={Stassun, Keivan G. and Oelkers, Ryan J. and Pepper, Joshua and Paegert, Martin and De Lee, Nathan and Torres, Guillermo and Latham, David W. and Charpinet, Stéphane and Dressing, Courtney D. and Huber, Daniel and Kane, Stephen R. and Lépine, Sébastien and Mann, Andrew and Muirhead, Philip S. and Rojas-Ayala, Bárbara and Silvotti, Roberto and Fleming, Scott W. and Levine, Al and Plavchan, Peter}, title={The TESS Input Catalog and Candidate Target List}, journal={\aj}, keywords={stars: fundamental parameters, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={156}, number={3}, eid={102}, pages={102}, doi={10.3847/1538-3881/aad050}, archiveprefix={arXiv}, eprint={1706.00495}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018AJ....156..102S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hog00, author={Høg, E. and Fabricius, C. and Makarov, V. V. and Bastian, U. and Schwekendiek, P. and Wicenec, A. and Urban, S. and Corbin, T. and Wycoff, G.}, title={Construction and verification of the Tycho-2 Catalogue}, journal={\aap}, keywords={ASTROMETRY, TECHNIQUES: PHOTOMETRIC, CATALOGS, METHODS: DATA ANALYSIS}, volume={357}, pages={367-386}, adsurl={https://ui.adsabs.harvard.edu/abs/2000A&A...357..367H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Cutri03, author={Cutri, R. M. and Skrutskie, M. F. and van Dyk, S. and Beichman, C. A. and Carpenter, J. M. and Chester, T. and Cambresy, L. and Evans, T. and Fowler, J. and Gizis, J. and Howard, E. and Huchra, J. and Jarrett, T. and Kopan, E. L. and Kirkpatrick, J. D. and Light, R. M. and Marsh, K. A. and McCallon, H. and Schneider, S. and Stiening, R. and Sykes, M. and Weinberg, M. and Wheaton, W. 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F. L.}, title={ellc: A fast, flexible light curve model for detached eclipsing binary stars and transiting exoplanets}, journal={\aap}, keywords={binaries: eclipsing, methods: data analysis, methods: numerical, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={591}, eid={A111}, pages={A111}, doi={10.1051/0004-6361/201628579}, archiveprefix={arXiv}, eprint={1603.08484}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2016A&A...591A.111M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Davenport14, author={Davenport, James R. A. and Hawley, Suzanne L. and Hebb, Leslie and Wisniewski, John P. and Kowalski, Adam F. and Johnson, Emily C. and Malatesta, Michael and Peraza, Jesus and Keil, Marcus and Silverberg, Steven M. and Jansen, Tiffany C. and Scheffler, Matthew S. and Berdis, Jodi R. and Larsen, Daniel M. and Hilton, Eric J.}, title={Kepler Flares. II. The Temporal Morphology of White-light Flares on GJ 1243}, journal={\apj}, keywords={stars: activity, stars: flare, stars: low-mass, Astrophysics - Solar and Stellar Astrophysics}, volume={797}, number={2}, eid={122}, pages={122}, doi={10.1088/0004-637X/797/2/122}, archiveprefix={arXiv}, eprint={1411.3723}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2014ApJ...797..122D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Speagle20, author={Speagle, Joshua S.}, title={DYNESTY: a dynamic nested sampling package for estimating Bayesian posteriors and evidences}, journal={\mnras}, keywords={methods: data analysis, methods: statistical, Astrophysics - Instrumentation and Methods for Astrophysics, Statistics - Computation}, volume={493}, number={3}, pages={3132-3158}, doi={10.1093/mnras/staa278}, archiveprefix={arXiv}, eprint={1904.02180}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2020MNRAS.493.3132S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Claret17, author={Claret, A.}, title={Limb and gravity-darkening coefficients for the TESS satellite at several metallicities, surface gravities, and microturbulent velocities}, journal={\aap}, keywords={planetary systems, stars: atmospheres, binaries: eclipsing, Astrophysics - Solar and Stellar Astrophysics}, volume={600}, eid={A30}, pages={A30}, doi={10.1051/0004-6361/201629705}, archiveprefix={arXiv}, eprint={1804.10295}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2017A&A...600A..30C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{David19, author={David, Trevor J. and Hillenbrand, Lynne A. and Gillen, Edward and Cody, Ann Marie and Howell, Steve B. and Isaacson, Howard T. and Livingston, John H.}, title={Age Determination in Upper Scorpius with Eclipsing Binaries}, journal={\apj}, keywords={binaries: eclipsing, binaries: spectroscopic, Hertzsprung–Russell and C–M diagrams, open clusters and associations: individual: Upper Scorpius, stars: evolution, stars: pre-main sequence, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={872}, number={2}, eid={161}, pages={161}, doi={10.3847/1538-4357/aafe09}, archiveprefix={arXiv}, eprint={1901.05532}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJ...872..161D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Zhou19, author={Zhou, G. and Bakos, G. Á. and Bayliss, D. and Bento, J. and Bhatti, W. and Brahm, R. and Csubry, Z. and Espinoza, N. and Hartman, J. D. and Henning, T. and Jordán, A. and Mancini, L. and Penev, K. and Rabus, M. and Sarkis, P. and Suc, V. and de Val-Borro, M. and Rodriguez, J. E. and Osip, D. and Kedziora-Chudczer, L. and Bailey, J. and Tinney, C. G. and Durkan, S. and Lázár, J. and Papp, I. and Sári, P.}, title={HATS-70b: A 13 MJ Brown Dwarf Transiting an A Star}, journal={\aj}, keywords={stars: individual: HATS-70, techniques: spectroscopic, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics}, volume={157}, number={1}, eid={31}, pages={31}, doi={10.3847/1538-3881/aaf1bb}, archiveprefix={arXiv}, eprint={1811.06925}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019AJ....157...31Z}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{JohnsKrull08, author={Johns-Krull, Christopher M. and McCullough, Peter R. and Burke, Christopher J. and Valenti, Jeff A. and Janes, K. A. and Heasley, J. N. and Prato, L. and Bissinger, R. and Fleenor, M. and Foote, C. N. and Garcia-Melendo, E. and Gary, B. L. and Howell, P. 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Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={163}, number={1}, eid={32}, pages={32}, doi={10.3847/1538-3881/ac365f}, archiveprefix={arXiv}, eprint={2111.03673}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022AJ....163...32D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Yang22, author={Yang, Fan and Wei, Xing}, title={Transit Timing Variation of XO-3b: Evidence for Tidal Evolution of Hot Jupiter with High Eccentricity}, journal={\pasp}, keywords={Exoplanet systems, Transit photometry, Transit timing variation method, Transit duration variation method, Tidal interaction, Exoplanet migration, Astrophysics - Earth and Planetary Astrophysics}, volume={134}, number={1032}, eid={024401}, pages={024401}, doi={10.1088/1538-3873/ac495a}, archiveprefix={arXiv}, eprint={2111.06551}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022PASP..134b4401Y}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Vissapragada22, author={Vissapragada, Shreyas and Chontos, Ashley and Greklek-McKeon, Michael and Knutson, Heather A. and Dai, Fei and Pérez González, Jorge and Grunblatt, Sam and Huber, Daniel and Saunders, Nicholas}, title={The Possible Tidal Demise of Kepler's First Planetary System}, journal={\apjl}, keywords={Exoplanet astronomy, Exoplanet evolution, Exoplanet dynamics, Exoplanet tides, Transits, Timing variation methods, Hot Jupiters, 486, 491, 490, 497, 1711, 1703, 753, Astrophysics - Earth and Planetary Astrophysics}, volume={941}, number={2}, eid={L31}, pages={L31}, doi={10.3847/2041-8213/aca47e}, archiveprefix={arXiv}, eprint={2212.09752}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022ApJ...941L..31V}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Espinoza19, author={Espinoza, Néstor and Kossakowski, Diana and Brahm, Rafael}, title={juliet: a versatile modelling tool for transiting and non-transiting exoplanetary systems}, journal={\mnras}, keywords={methods: data analysis, methods: statistical, techniques: photometric, techniques: radial velocities, planets and satellites: fundamental parameters, planets and satellites: individual: K2-140b, K2-32b, c, d, Astrophysics - Earth and Planetary Astrophysics}, year={2019}, month={Dec}, volume={490}, number={2}, pages={2262-2283}, doi={10.1093/mnras/stz2688}, archiveprefix={arXiv}, eprint={1812.08549}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019MNRAS.490.2262E}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Sullivan15, author={Sullivan, Peter W. and Winn, Joshua N. and Berta-Thompson, Zachory K. and Charbonneau, David and Deming, Drake and Dressing, Courtney D. and Latham, David W. and Levine, Alan M. and McCullough, Peter R. and Morton, Timothy and Ricker, George R. and Vanderspek, Roland and Woods, Deborah}, title={The Transiting Exoplanet Survey Satellite: Simulations of Planet Detections and Astrophysical False Positives}, journal={\apj}, keywords={planets and satellites: detection, space vehicles: instruments, surveys, Astrophysics - Earth and Planetary Astrophysics}, volume={809}, number={1}, eid={77}, pages={77}, doi={10.1088/0004-637X/809/1/77}, archiveprefix={arXiv}, eprint={1506.03845}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ApJ...809...77S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Charbonneau05, author={Charbonneau, David and Allen, Lori E. and Megeath, S. Thomas and Torres, Guillermo and Alonso, Roi and Brown, Timothy M. and Gilliland, Ronald L. and Latham, David W. and Mandushev, Georgi and O'Donovan, Francis T. and Sozzetti, Alessandro}, title={Detection of Thermal Emission from an Extrasolar Planet}, journal={\apj}, keywords={Stars: Binaries: Eclipsing, Infrared: Stars, Stars: Planetary Systems, Stars: Individual: Alphanumeric: TrES-1, Techniques: Photometric, Astrophysics}, volume={626}, number={1}, pages={523-529}, doi={10.1086/429991}, archiveprefix={arXiv}, eprint={astro-ph/0503457}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2005ApJ...626..523C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Jackson2008, author={Jackson, Brian and Greenberg, Richard and Barnes, Rory}, title={Tidal Evolution of Close-in Extrasolar Planets}, journal={\apj}, keywords={celestial mechanics, planetary systems: formation, planetary systems: protoplanetary disks, Astrophysics}, year={2008}, month={May}, volume={678}, number={2}, pages={1396-1406}, doi={10.1086/529187}, archiveprefix={arXiv}, eprint={0802.1543}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2008ApJ...678.1396J}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Goldreich66, author={Goldreich, Peter and Soter, Steven}, title={Q in the Solar System}, journal={\icarus}, year={1966}, month={Jan}, volume={5}, number={1}, pages={375-389}, doi={10.1016/0019-1035(66)90051-0}, adsurl={https://ui.adsabs.harvard.edu/abs/1966Icar....5..375G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Heller10, author={Heller, R. and Jackson, B. and Barnes, R. and Greenberg, R. and Homeier, D.}, title={Tidal effects on brown dwarfs: application to the eclipsing binary 2MASS J05352184-0546085. The anomalous temperature reversal in the context of tidal heating}, journal={\aap}, keywords={celestial mechanics, binaries: eclipsing, stars: evolution, stars: individual: 2MASSJ05352184-0546085, brown dwarfs, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, year={2010}, month={May}, volume={514}, eid={A22}, pages={A22}, doi={10.1051/0004-6361/200912826}, archiveprefix={arXiv}, eprint={1002.1246}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2010A&A...514A..22H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Beatty18, author={Beatty, Thomas G. and Morley, Caroline V. and Curtis, Jason L. and Burrows, Adam and Davenport, James R. A. and Montet, Benjamin T.}, title={A Significant Overluminosity in the Transiting Brown Dwarf CWW 89Ab}, journal={\aj}, keywords={brown dwarfs, open clusters and associations: individual: Ruprecht 147, NGC 6774, planets and satellites: atmospheres, stars: individual: CWW 89, EPIC 219388192, Astrophysics - Solar and Stellar Astrophysics}, year={2018}, month={Oct}, volume={156}, number={4}, eid={168}, pages={168}, doi={10.3847/1538-3881/aad697}, archiveprefix={arXiv}, eprint={1807.11500}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2018AJ....156..168B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Quinn14, author={Quinn, Samuel N. and White, Russel J. and Latham, David W. and Buchhave, Lars A. and Torres, Guillermo and Stefanik, Robert P. and Berlind, Perry and Bieryla, Allyson and Calkins, Michael C. and Esquerdo, Gilbert A. and Fűrész, Gabor and Geary, John C. and Szentgyorgyi, Andrew H.}, title={HD 285507b: An Eccentric Hot Jupiter in the Hyades Open Cluster}, journal={\apj}, keywords={open clusters and associations: individual: Hyades Melotte 25, planets and satellites: detection, planets and satellites: dynamical evolution and stability, planet-star interactions, stars: individual: HD 285507, Astrophysics - Earth and Planetary Astrophysics}, volume={787}, number={1}, eid={27}, pages={27}, doi={10.1088/0004-637X/787/1/27}, archiveprefix={arXiv}, eprint={1310.7328}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2014ApJ...787...27Q}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Penev12, author={Penev, Kaloyan and Jackson, Brian and Spada, Federico and Thom, Nicole}, title={Constraining Tidal Dissipation in Stars from the Destruction Rates of Exoplanets}, journal={\apj}, keywords={convection, planet-star interactions, stars: interiors, stars: rotation, stars: winds, outflows, turbulence, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={751}, number={2}, eid={96}, pages={96}, doi={10.1088/0004-637X/751/2/96}, archiveprefix={arXiv}, eprint={1205.1803}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012ApJ...751...96P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{CollierCameron2018, author={Collier Cameron, Andrew and Jardine, Moira}, title={Hierarchical Bayesian calibration of tidal orbit decay rates among hot Jupiters}, journal={\mnras}, keywords={methods: statistical, planets and satellites: dynamical evolution and stability, planetary systems, planet-star interactions, Astrophysics - Earth and Planetary Astrophysics}, year={2018}, month={May}, volume={476}, number={2}, pages={2542-2555}, doi={10.1093/mnras/sty292}, archiveprefix={arXiv}, eprint={1801.10561}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018MNRAS.476.2542C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Lainey2009, author={Lainey, Valéry and Arlot, Jean-Eudes and Karatekin, Özgür and van Hoolst, Tim}, title={Strong tidal dissipation in Io and Jupiter from astrometric observations}, journal={\nat}, year={2009}, month={Jun}, volume={459}, number={7249}, pages={957-959}, doi={10.1038/nature08108}, adsurl={https://ui.adsabs.harvard.edu/abs/2009Natur.459..957L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Coulombe23, author={Coulombe, Louis-Philippe and Benneke, Björn and Challener, Ryan and Piette, Anjali A. A. and Wiser, Lindsey S. and Mansfield, Megan and MacDonald, Ryan J. and Beltz, Hayley and Feinstein, Adina D. and Radica, Michael and Savel, Arjun B. and Dos Santos, Leonardo A. and Bean, Jacob L. and Parmentier, Vivien and Wong, Ian and Rauscher, Emily and Komacek, Thaddeus D. and Kempton, Eliza M. -R. and Tan, Xianyu and Hammond, Mark and Lewis, Neil T. and Line, Michael R. and Lee, Elspeth K. H. and Shivkumar, Hinna and Crossfield, Ian J. M. and Nixon, Matthew C. and Rackham, Benjamin V. and Wakeford, Hannah R. and Welbanks, Luis and Zhang, Xi and Batalha, Natalie M. and Berta-Thompson, Zachory K. and Changeat, Quentin and Désert, Jean-Michel and Espinoza, Néstor and Goyal, Jayesh M. and Harrington, Joseph and Knutson, Heather A. and Kreidberg, Laura and López-Morales, Mercedes and Shporer, Avi and Sing, David K. and Stevenson, Kevin B. and Aggarwal, Keshav and Ahrer, Eva-Maria and Alam, Munazza K. and Bell, Taylor J. and Blecic, Jasmina and Caceres, Claudio and Carter, Aarynn L. and Casewell, Sarah L. and Crouzet, Nicolas and Cubillos, Patricio E. and Decin, Leen and Fortney, Jonathan J. and Gibson, Neale P. and Heng, Kevin and Henning, Thomas and Iro, Nicolas and Kendrew, Sarah and Lagage, Pierre-Olivier and Leconte, Jérémy and Lendl, Monika and Lothringer, Joshua D. and Mancini, Luigi and Mikal-Evans, Thomas and Molaverdikhani, Karan and Nikolov, Nikolay K. and Ohno, Kazumasa and Palle, Enric and Piaulet, Caroline and Redfield, Seth and Roy, Pierre-Alexis and Tsai, Shang-Min and Venot, Olivia and Wheatley, Peter J.}, title={A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b}, journal={\nat}, keywords={Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={620}, number={7973}, pages={292-298}, doi={10.1038/s41586-023-06230-1}, archiveprefix={arXiv}, eprint={2301.08192}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023Natur.620..292C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Batalha19, author={Batalha, Natasha E. and Marley, Mark S. and Lewis, Nikole K. and Fortney, Jonathan J.}, title={Exoplanet Reflected-light Spectroscopy with PICASO}, journal={\apj}, keywords={planetary systems, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics}, volume={878}, number={1}, eid={70}, pages={70}, doi={10.3847/1538-4357/ab1b51}, archiveprefix={arXiv}, eprint={1904.09355}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJ...878...70B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Marley21, author={Marley, Mark S. and Saumon, Didier and Visscher, Channon and Lupu, Roxana and Freedman, Richard and Morley, Caroline and Fortney, Jonathan J. and Seay, Christopher and Smith, Adam J. R. W. and Teal, D. J. and Wang, Ruoyan}, title={The Sonora Brown Dwarf Atmosphere and Evolution Models. I. Model Description and Application to Cloudless Atmospheres in Rainout Chemical Equilibrium}, journal={\apj}, keywords={Brown dwarfs, T dwarfs, L dwarfs, L subdwarfs, T subdwarfs, Y dwarfs, Stellar atmospheres, 185, 1679, 894, 896, 1680, 1827, 1584, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={920}, number={2}, eid={85}, pages={85}, doi={10.3847/1538-4357/ac141d}, archiveprefix={arXiv}, eprint={2107.07434}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2021ApJ...920...85M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Husser2013, abstract={We present a new library of high-resolution synthetic spectra based on the stellar atmosphere code PHOENIX that can be used for a wide range of applications of spectral analysis and stellar parameter synthesis. The spherical mode of PHOENIX was used to create model atmospheres and to derive detailed synthetic stellar spectra from them. We present a new self-consistent way of describing micro-turbulence for our model atmospheres. The synthetic spectra cover the wavelength range from 500AA to 50.000AA with resolutions of R=500.000 in the optical and near IR, R=100.000 in the IR and a step size of 0.1AA in the UV. The parameter space covers 2.300K<=Teff<=12.000K, 0.0<=log(g)<=+6.0, -4.0<=[Fe/H]<=+1.0, and -0.2<=[alpha/Fe]<=+1.2. The library is a work in progress and we expect to extend it up to Teff=25.000 K.}, archiveprefix={arXiv}, arxivid={1303.5632}, author={Husser, Tim-Oliver and von Berg, Sebastian Wende - and Dreizler, Stefan and Homeier, Derek and Reiners, Ansgar and Barman, Travis and Hauschildt, Peter H}, doi={10.1051/0004-6361/201219058}, eprint={1303.5632}, issn={0004-6361}, journal={Astronomy & Astrophysics}, keywords={atmospheres,convection,late-type,stars}, pages={A6}, title={A new extensive library of PHOENIX stellar atmospheres and synthetic spectra}, url={http://arxiv.org/abs/1303.5632%0Ahttp://dx.doi.org/10.1051/0004-6361/201219058}, volume={553}, year={2013} }@article{Madhusudhan11, author={Madhusudhan, Nikku and Harrington, Joseph and Stevenson, Kevin B. and Nymeyer, Sarah and Campo, Christopher J. and Wheatley, Peter J. and Deming, Drake and Blecic, Jasmina and Hardy, Ryan A. and Lust, Nate B. and Anderson, David R. and Collier-Cameron, Andrew and Britt, Christopher B. T. and Bowman, William C. and Hebb, Leslie and Hellier, Coel and Maxted, Pierre F. L. and Pollacco, Don and West, Richard G.}, title={A high C/O ratio and weak thermal inversion in the atmosphere of exoplanet WASP-12b}, journal={\nat}, keywords={Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={469}, number={7328}, pages={64-67}, doi={10.1038/nature09602}, archiveprefix={arXiv}, eprint={1012.1603}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2011Natur.469...64M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Moses13, author={Moses, J. I. and Madhusudhan, N. and Visscher, C. and Freedman, R. S.}, title={Chemical Consequences of the C/O Ratio on Hot Jupiters: Examples from WASP-12b, CoRoT-2b, XO-1b, and HD 189733b}, journal={\apj}, keywords={planetary systems, planets and satellites: atmospheres, planets and satellites: composition, planets and satellites: individual: HD 189733b WASP-12b XO-1b CoRoT-2b, stars: individual: HD 189733 WASP-12 XO-1 CoRoT-2, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={763}, number={1}, eid={25}, pages={25}, doi={10.1088/0004-637X/763/1/25}, archiveprefix={arXiv}, eprint={1211.2996}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2013ApJ...763...25M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Line14, author={Line, Michael R. and Knutson, Heather and Wolf, Aaron S. and Yung, Yuk L.}, title={A Systematic Retrieval Analysis of Secondary Eclipse Spectra. II. A Uniform Analysis of Nine Planets and their C to O Ratios}, journal={\apj}, keywords={methods: statistical, planets and satellites: atmospheres, planets and satellites: composition, planets and satellites: gaseous planets, planets and satellites: individual: HD 189733b HD 149026b GJ436b WASP-12b WASP-19b WASP-43b TrES-2b TrES-3b, Astrophysics - Earth and Planetary Astrophysics}, volume={783}, number={2}, eid={70}, pages={70}, doi={10.1088/0004-637X/783/2/70}, archiveprefix={arXiv}, eprint={1309.6663}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2014ApJ...783...70L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Ahrer23, author={Ahrer, Eva-Maria and Stevenson, Kevin B. and Mansfield, Megan and Moran, Sarah E. and Brande, Jonathan and Morello, Giuseppe and Murray, Catriona A. and Nikolov, Nikolay K. and Petit dit de la Roche, Dominique J. M. and Schlawin, Everett and Wheatley, Peter J. and Zieba, Sebastian and Batalha, Natasha E. and Damiano, Mario and Goyal, Jayesh M. and Lendl, Monika and Lothringer, Joshua D. and Mukherjee, Sagnick and Ohno, Kazumasa and Batalha, Natalie M. and Battley, Matthew P. and Bean, Jacob L. and Beatty, Thomas G. and Benneke, Björn and Berta-Thompson, Zachory K. and Carter, Aarynn L. and Cubillos, Patricio E. and Daylan, Tansu and Espinoza, Néstor and Gao, Peter and Gibson, Neale P. and Gill, Samuel and Harrington, Joseph and Hu, Renyu and Kreidberg, Laura and Lewis, Nikole K. and Line, Michael R. and López-Morales, Mercedes and Parmentier, Vivien and Powell, Diana K. and Sing, David K. and Tsai, Shang-Min and Wakeford, Hannah R. and Welbanks, Luis and Alam, Munazza K. and Alderson, Lili and Allen, Natalie H. and Anderson, David R. and Barstow, Joanna K. and Bayliss, Daniel and Bell, Taylor J. and Blecic, Jasmina and Bryant, Edward M. and Burleigh, Matthew R. and Carone, Ludmila and Casewell, S. L. and Changeat, Quentin and Chubb, Katy L. and Crossfield, Ian J. M. and Crouzet, Nicolas and Decin, Leen and Désert, Jean-Michel and Feinstein, Adina D. and Flagg, Laura and Fortney, Jonathan J. and Gizis, John E. and Heng, Kevin and Iro, Nicolas and Kempton, Eliza M. -R. and Kendrew, Sarah and Kirk, James and Knutson, Heather A. and Komacek, Thaddeus D. and Lagage, Pierre-Olivier and Leconte, Jérémy and Lustig-Yaeger, Jacob and MacDonald, Ryan J. and Mancini, Luigi and May, E. M. and Mayne, N. J. and Miguel, Yamila and Mikal-Evans, Thomas and Molaverdikhani, Karan and Palle, Enric and Piaulet, Caroline and Rackham, Benjamin V. and Redfield, Seth and Rogers, Laura K. and Roy, Pierre-Alexis and Rustamkulov, Zafar and Shkolnik, Evgenya L. and Sotzen, Kristin S. and Taylor, Jake and Tremblin, P. and Tucker, Gregory S. and Turner, Jake D. and de Val-Borro, Miguel and Venot, Olivia and Zhang, Xi}, title={Early Release Science of the exoplanet WASP-39b with JWST NIRCam}, journal={\nat}, keywords={Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={614}, number={7949}, pages={653-658}, doi={10.1038/s41586-022-05590-4}, archiveprefix={arXiv}, eprint={2211.10489}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023Natur.614..653A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Arcangeli18, author={Arcangeli, Jacob and Désert, Jean-Michel and Line, Michael R. and Bean, Jacob L. and Parmentier, Vivien and Stevenson, Kevin B. and Kreidberg, Laura and Fortney, Jonathan J. and Mansfield, Megan and Showman, Adam P.}, title={H$^{-}$ Opacity and Water Dissociation in the Dayside Atmosphere of the Very Hot Gas Giant WASP-18b}, journal={\apjl}, keywords={planets and satellites: atmospheres, planets and satellites: gaseous planets, Astrophysics - Earth and Planetary Astrophysics}, volume={855}, number={2}, eid={L30}, pages={L30}, doi={10.3847/2041-8213/aab272}, archiveprefix={arXiv}, eprint={1801.02489}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018ApJ...855L..30A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@misc{Lightkurve18, author={Lightkurve Collaboration and Cardoso, J. V. d. M. and Hedges, C. and Gully-Santiago, M. and Saunders, N. and Cody, A. M. and Barclay, T. and Hall, O. and Sagear, S. and Turtelboom, E. and Zhang, J. and Tzanidakis, A. and Mighell, K. and Coughlin, J. and Bell, K. and Berta-Thompson, Z. and Williams, P. and Dotson, J. and Barentsen, G.}, title={Lightkurve: Kepler and TESS time series analysis in Python}, keywords={Software, NASA}, howpublished={Astrophysics Source Code Library}, archiveprefix={ascl}, eprint={1812.013}, adsurl={http://adsabs.harvard.edu/abs/2018ascl.soft12013L} }@misc{Morton15, author={Morton, Timothy D.}, title={isochrones: Stellar model grid package}, keywords={Software}, howpublished={Astrophysics Source Code Library, record ascl:1503.010}, eid={ascl:1503.010}, pages={ascl:1503.010}, archiveprefix={ascl}, eprint={1503.010}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ascl.soft03010M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@misc{Trifonov19, author={Trifonov, Trifon}, title={The Exo-Striker: Transit and radial velocity interactive fitting tool for orbital analysis and N-body simulations}, keywords={Software}, howpublished={Astrophysics Source Code Library, record ascl:1906.004}, eid={ascl:1906.004}, pages={ascl:1906.004}, archiveprefix={ascl}, eprint={1906.004}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ascl.soft06004T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@misc{Foreman17, author={Foreman-Mackey, Daniel and Agol, Eric and Ambikasaran, Sivaram and Angus, Ruth}, title={celerite: Scalable 1D Gaussian Processes in C++, Python, and Julia}, keywords={Software}, howpublished={Astrophysics Source Code Library, record ascl:1709.008}, eid={ascl:1709.008}, pages={ascl:1709.008}, archiveprefix={ascl}, eprint={1709.008}, adsurl={https://ui.adsabs.harvard.edu/abs/2017ascl.soft09008F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@misc{Jensen13, author={Jensen, Eric}, title={Tapir: A web interface for transit/eclipse observability}, keywords={Software}, eid={ascl:1306.007}, pages={ascl:1306.007}, archiveprefix={ascl}, eprint={1306.007}, adsurl={https://ui.adsabs.harvard.edu/abs/2013ascl.soft06007J}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{10.1111/j.1365-2966.2012.21382.x, author={Vanzi, L. and Chacon, J. and Helminiak, K. G. and Baffico, M. and Rivinius, T. and Štefl, S. and Baade, D. and Avila, G. and Guirao, C.}, title={PUCHEROS: a cost-effective solution for high-resolution spectroscopy with small telescopes}, journal={Monthly Notices of the Royal Astronomical Society}, volume={424}, number={4}, pages={2770-2777}, year={2012}, month={08}, abstract={We present PUCHEROS, the high-resolution echelle spectrograph, developed at the Center of Astro-Engineering of Pontificia Universidad Catolica de Chile to provide an effective tool for research and teaching of astronomy. The instrument is fed by a single-channel optical fibre and it covers the visible range from 390 to 730 nm in one shot, reaching a spectral resolution of about 20 000. In the era of extremely large telescopes our instrument aims to exploit the capabilities offered by small telescopes in a cost-effective way, covering the observing needs of a community of astronomers, in Chile and elsewhere, which do not necessarily need large collecting areas for their research. In particular the instrument is well suited for long-term spectroscopic monitoring of bright variable and transient targets down to a V magnitude of about 10. We describe the instrument and present a number of text case examples of observations obtained during commissioning and early science.}, issn={0035-8711}, doi={10.1111/j.1365-2966.2012.21382.x}, url={https://doi.org/10.1111/j.1365-2966.2012.21382.x}, eprint={https://academic.oup.com/mnras/article-pdf/424/4/2770/18708930/424-4-2770.pdf} }@article{2017PASP..129c4002B, author={Brahm, Rafael and Jordán, Andrés and Espinoza, Néstor}, title={CERES: A Set of Automated Routines for Echelle Spectra}, journal={\pasp}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={129}, number={973}, pages={034002}, doi={10.1088/1538-3873/aa5455}, archiveprefix={arXiv}, eprint={1609.02279}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2017PASP..129c4002B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Ma2014, author={Ma, B. and Ge, J.}, title={Statistical properties of brown dwarf companions: implications for different formation mechanisms}, journal={\mnras}, archiveprefix={arXiv}, eprint={1303.6442}, primaryclass={astro-ph.EP}, keywords={techniques: radial velocities, catalogues, brown dwarfs, stars: formation}, pages={2781-2789}, doi={10.1093/mnras/stu134}, adsurl={https://ui.adsabs.harvard.edu/abs/2014MNRAS.439.2781M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fulton15, author={Fulton, Benjamin J. and Collins, Karen A. and Gaudi, B. Scott and Stassun, Keivan G. and Pepper, Joshua and Beatty, Thomas G. and Siverd, Robert J. and Penev, Kaloyan and Howard, Andrew W. and Baranec, Christoph and Corfini, Giorgio and Eastman, Jason D. and Gregorio, Joao and Law, Nicholas M. and Lund, Michael B. and Oberst, Thomas E. and Penny, Matthew T. and Riddle, Reed and Rodriguez, Joseph E. and Stevens, Daniel J. and Zambelli, Roberto and Ziegler, Carl and Bieryla, Allyson and D'Ago, Giuseppe and DePoy, Darren L. and Jensen, Eric L. N. and Kielkopf, John F. and Latham, David W. and Manner, Mark and Marshall, Jennifer and McLeod, Kim K. and Reed, Phillip A.}, title={KELT-8b: A Highly Inflated Transiting Hot Jupiter and a New Technique for Extracting High-precision Radial Velocities from Noisy Spectra}, journal={\apj}, keywords={planetary systems, stars: individual: HD 343246, Astrophysics - Earth and Planetary Astrophysics}, volume={810}, number={1}, eid={30}, pages={30}, doi={10.1088/0004-637X/810/1/30}, archiveprefix={arXiv}, eprint={1505.06738}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ApJ...810...30F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Yee23, author={Yee, Samuel W. and Winn, Joshua N. and Hartman, Joel D. and Bouma, Luke G. and Zhou, George and Quinn, Samuel N. and Latham, David W. and Bieryla, Allyson and Rodriguez, Joseph E. and Collins, Karen A. and Alfaro, Owen and Barkaoui, Khalid and Beard, Corey and Belinski, Alexander A. and Benkhaldoun, Zouhair and Benni, Paul and Bernacki, Krzysztof and Boyle, Andrew W. and Butler, R. Paul and Caldwell, Douglas A. and Chontos, Ashley and Christiansen, Jessie L. and Ciardi, David R. and Collins, Kevin I. and Conti, Dennis M. and Crane, Jeffrey D. and Daylan, Tansu and Dressing, Courtney D. and Eastman, Jason D. and Essack, Zahra and Evans, Phil and Everett, Mark E. and Fajardo-Acosta, Sergio and Forés-Toribio, Raquel and Furlan, Elise and Ghachoui, Mourad and Gillon, Michaël and Hellier, Coel and Helm, Ian and Howard, Andrew W. and Howell, Steve B. and Isaacson, Howard and Jehin, Emmanuel and Jenkins, Jon M. and Jensen, Eric L. N. and Kielkopf, John F. and Laloum, Didier and Leonhardes-Barboza, Naunet and Lewin, Pablo and Logsdon, Sarah E. and Lubin, Jack and Lund, Michael B. and MacDougall, Mason G. and Mann, Andrew W. and Maslennikova, Natalia A. and Massey, Bob and McLeod, Kim K. and Muñoz, Jose A. and Newman, Patrick and Orlov, Valeri and Plavchan, Peter and Popowicz, Adam and Pozuelos, Francisco J. and Pritchard, Tyler A. and Radford, Don J. and Reefe, Michael and Ricker, George R. and Rudat, Alexander and Safonov, Boris S. and Schwarz, Richard P. and Schweiker, Heidi and Scott, Nicholas J. and Seager, S. and Shectman, Stephen A. and Stockdale, Chris and Tan, Thiam-Guan and Teske, Johanna K. and Thomas, Neil B. and Timmermans, Mathilde and Vanderspek, Roland and Vermilion, David and Watanabe, David and Weiss, Lauren M. and West, Richard G. and Van Zandt, Judah and Zejmo, Michal and Ziegler, Carl}, title={The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets}, journal={\apjs}, keywords={Exoplanets, Hot Jupiters, Radial velocity, Exoplanet detection methods, Transit photometry, 498, 753, 1332, 489, 1709, Astrophysics - Earth and Planetary Astrophysics}, volume={265}, number={1}, eid={1}, pages={1}, doi={10.3847/1538-4365/aca286}, archiveprefix={arXiv}, eprint={2210.15473}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023ApJS..265....1Y}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Sestovic18, author={Sestovic, Marko and Demory, Brice-Olivier and Queloz, Didier}, title={Investigating hot-Jupiter inflated radii with hierarchical Bayesian modelling}, journal={\aap}, keywords={planets and satellites: fundamental parameters, planets and satellites: atmospheres, methods: statistical, Astrophysics - Earth and Planetary Astrophysics}, volume={616}, eid={A76}, pages={A76}, doi={10.1051/0004-6361/201731454}, archiveprefix={arXiv}, eprint={1804.03075}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018A&A...616A..76S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Anderson11, author={Anderson, D. R. and Smith, A. M. S. and Lanotte, A. A. and Barman, T. S. and Collier Cameron, A. and Campo, C. J. and Gillon, M. and Harrington, J. and Hellier, C. and Maxted, P. F. L. and Queloz, D. and Triaud, A. H. M. J. and Wheatley, P. J.}, title={Thermal emission at 4.5 and 8 $\mu$m of WASP-17b, an extremely large planet in a slightly eccentric orbit}, journal={\mnras}, keywords={methods: data analysis, techniques: photometric, occultations, planets and satellites: atmospheres, planets and satellites: individual: WASP-17b, stars: individual: WASP-17, Astrophysics - Earth and Planetary Astrophysics}, volume={416}, number={3}, pages={2108-2122}, doi={10.1111/j.1365-2966.2011.19182.x}, archiveprefix={arXiv}, eprint={1101.5620}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2011MNRAS.416.2108A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Almenara15, author={Almenara, J. M. and Damiani, C. and Bouchy, F. and Havel, M. and Bruno, G. and Hébrard, G. and Diaz, R. F. and Deleuil, M. and Barros, S. C. C. and Boisse, I. and Bonomo, A. S. and Montagnier, G. and Santerne, A.}, title={SOPHIE velocimetry of Kepler transit candidates. XV. KOI-614b, KOI-206b, and KOI-680b: a massive warm Jupiter orbiting a G0 metallic dwarf and two highly inflated planets with a distant companion around evolved F-type stars}, journal={\aap}, keywords={planetary systems, techniques: photometric, techniques: radial velocities, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics}, volume={575}, eid={A71}, pages={A71}, doi={10.1051/0004-6361/201424291}, archiveprefix={arXiv}, eprint={1501.01486}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015A&A...575A..71A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Bowler23, author={Bowler, Brendan P. and Tran, Quang H. and Zhang, Zhoujian and Morgan, Marvin and Ashok, Katelyn B. and Blunt, Sarah and Bryan, Marta L. and Evans, Analis E. and Franson, Kyle and Huber, Daniel and Nagpal, Vighnesh and Wu, Ya-Lin and Zhou, Yifan}, title={Rotation Periods, Inclinations, and Obliquities of Cool Stars Hosting Directly Imaged Substellar Companions: Spin-Orbit Misalignments Are Common}, journal={\aj}, keywords={Brown dwarfs, Extrasolar gaseous giant planets, Planet formation, Stellar rotation, 185, 509, 1241, 1629, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={165}, number={4}, eid={164}, pages={164}, doi={10.3847/1538-3881/acbd34}, archiveprefix={arXiv}, eprint={2301.04692}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023AJ....165..164B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Masuda20, author={Masuda, Kento and Winn, Joshua N.}, title={On the Inference of a Star's Inclination Angle from its Rotation Velocity and Projected Rotation Velocity}, journal={\aj}, keywords={Exoplanet astronomy, Stellar rotation, Astrostatistics, 486, 1629, 1882, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={159}, number={3}, eid={81}, pages={81}, doi={10.3847/1538-3881/ab65be}, archiveprefix={arXiv}, eprint={2001.04973}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2020AJ....159...81M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Bailey19, author={Bailey, Avery and Goodman, Jeremy}, title={Understanding WASP-12b}, journal={\mnras}, keywords={planets and satellites: dynamical evolution and stability, planets and satellites: individual: WASP-12b, planet-star interactions, stars: individual: WASP-12, Astrophysics - Earth and Planetary Astrophysics}, volume={482}, number={2}, pages={1872-1882}, doi={10.1093/mnras/sty2805}, archiveprefix={arXiv}, eprint={1808.00052}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.1872B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Yee20, author={Yee, Samuel W. and Winn, Joshua N. and Knutson, Heather A. and Patra, Kishore C. and Vissapragada, Shreyas and Zhang, Michael M. and Holman, Matthew J. and Shporer, Avi and Wright, Jason T.}, title={The Orbit of WASP-12b Is Decaying}, journal={\apjl}, keywords={Hot Jupiters, Exoplanets, Transit photometry, 753, 498, 1709, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={888}, number={1}, eid={L5}, pages={L5}, doi={10.3847/2041-8213/ab5c16}, archiveprefix={arXiv}, eprint={1911.09131}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2020ApJ...888L...5Y}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Crossfield12, author={Crossfield, Ian J. M. and Barman, Travis and Hansen, Brad M. S. and Tanaka, Ichi and Kodama, Tadayuki}, title={Re-evaluating WASP-12b: Strong Emission at 2.315 $\mu$m, Deeper Occultations, and an Isothermal Atmosphere}, journal={\apj}, keywords={eclipses, infrared: planetary systems, stars: individual: WASP-12 Bergfors-6, techniques: photometric, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={760}, number={2}, eid={140}, pages={140}, doi={10.1088/0004-637X/760/2/140}, archiveprefix={arXiv}, eprint={1210.4836}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012ApJ...760..140C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hut80, author={Hut, P.}, title={Stability of tidal equilibrium}, journal={\aap}, keywords={Binary Stars, Celestial Mechanics, Dynamic Stability, Stellar Evolution, Stellar Oscillations, Stellar Rotation, Angular Momentum, Equilibrium, Orbital Elements, X Ray Sources, Astronomy}, volume={92}, number={1-2}, pages={167-170}, adsurl={https://ui.adsabs.harvard.edu/abs/1980A&A....92..167H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Changeat22, author={Changeat, Q. and Edwards, B. and Al-Refaie, A. F. and Tsiaras, A. and Skinner, J. W. and Cho, J. Y. K. and Yip, K. H. and Anisman, L. and Ikoma, M. and Bieger, M. F. and Venot, O. and Shibata, S. and Waldmann, I. P. and Tinetti, G.}, title={Five Key Exoplanet Questions Answered via the Analysis of 25 Hot-Jupiter Atmospheres in Eclipse}, journal={\apjs}, keywords={Exoplanet atmospheres, Bayesian statistics, Surveys, Hubble Space Telescope, Astronomy data reduction, 487, 1900, 1671, 761, 1861, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={260}, number={1}, eid={3}, pages={3}, doi={10.3847/1538-4365/ac5cc2}, archiveprefix={arXiv}, eprint={2204.11729}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022ApJS..260....3C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Kreidberg18, author={Kreidberg, Laura and Line, Michael R. and Parmentier, Vivien and Stevenson, Kevin B. and Louden, Tom and Bonnefoy, Mickäel and Faherty, Jacqueline K. and Henry, Gregory W. and Williamson, Michael H. and Stassun, Keivan and Beatty, Thomas G. and Bean, Jacob L. and Fortney, Jonathan J. and Showman, Adam P. and Désert, Jean-Michel and Arcangeli, Jacob}, title={Global Climate and Atmospheric Composition of the Ultra-hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations}, journal={\aj}, keywords={planets and satellites: atmospheres, planets and satellites: gaseous planets, planets and satellites: individual: WASP-103b, Astrophysics - Earth and Planetary Astrophysics}, volume={156}, number={1}, eid={17}, pages={17}, doi={10.3847/1538-3881/aac3df}, archiveprefix={arXiv}, eprint={1805.00029}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018AJ....156...17K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mansfield18, author={Mansfield, Megan and Bean, Jacob L. and Line, Michael R. and Parmentier, Vivien and Kreidberg, Laura and Désert, Jean-Michel and Fortney, Jonathan J. and Stevenson, Kevin B. and Arcangeli, Jacob and Dragomir, Diana}, title={An HST/WFC3 Thermal Emission Spectrum of the Hot Jupiter HAT-P-7b}, journal={\aj}, keywords={planets and satellites: atmospheres, planets and satellites: gaseous planets, planets and satellites: individual: HAT-P-7b, Astrophysics - Earth and Planetary Astrophysics}, volume={156}, number={1}, eid={10}, pages={10}, doi={10.3847/1538-3881/aac497}, archiveprefix={arXiv}, eprint={1805.00424}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018AJ....156...10M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Arcangeli19, author={Arcangeli, Jacob and Désert, Jean-Michel and Parmentier, Vivien and Stevenson, Kevin B. and Bean, Jacob L. and Line, Michael R. and Kreidberg, Laura and Fortney, Jonathan J. and Showman, Adam P.}, title={Climate of an ultra hot Jupiter. Spectroscopic phase curve of WASP-18b with HST/WFC3}, journal={\aap}, keywords={planets and satellites: atmospheres, Astrophysics - Earth and Planetary Astrophysics}, volume={625}, eid={A136}, pages={A136}, doi={10.1051/0004-6361/201834891}, archiveprefix={arXiv}, eprint={1904.02069}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019A&A...625A.136A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Enoch12, author={Enoch, B. and Collier Cameron, A. and Horne, K.}, title={Factors affecting the radii of close-in transiting exoplanets}, journal={\aap}, keywords={methods: statistical, planetary systems, planets and satellites: general, planets and satellites: physical evolution, Astrophysics - Earth and Planetary Astrophysics}, volume={540}, eid={A99}, pages={A99}, doi={10.1051/0004-6361/201117317}, archiveprefix={arXiv}, eprint={1202.6199}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012A&A...540A..99E}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Sarkis21, author={Sarkis, P. and Mordasini, C. and Henning, Th. and Marleau, G. D. and Mollière, P.}, title={Evidence of three mechanisms explaining the radius anomaly of hot Jupiters}, journal={\aap}, keywords={planets and satellites: gaseous planets, planets and satellites: interiors, planets and satellites: physical evolution, Astrophysics - Earth and Planetary Astrophysics}, volume={645}, eid={A79}, pages={A79}, doi={10.1051/0004-6361/202038361}, archiveprefix={arXiv}, eprint={2009.04291}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021A&A...645A..79S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Showman02, author={Showman, A. P. and Guillot, T.}, title={Atmospheric circulation and tides of "51 Pegasus b-like" planets}, journal={\aap}, keywords={PLANETS AND SATELLITES: GENERAL, STARS: PLANETARY SYSTEMS, Astrophysics}, volume={385}, pages={166-180}, doi={10.1051/0004-6361:20020101}, archiveprefix={arXiv}, eprint={astro-ph/0202236}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2002A&A...385..166S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Huang12, author={Huang, Xu and Cumming, Andrew}, title={Ohmic Dissipation in the Interiors of Hot Jupiters}, journal={\apj}, keywords={magnetohydrodynamics: MHD, planets and satellites: atmospheres, planets and satellites: interiors, planets and satellites: magnetic fields, Astrophysics - Earth and Planetary Astrophysics}, volume={757}, number={1}, eid={47}, pages={47}, doi={10.1088/0004-637X/757/1/47}, archiveprefix={arXiv}, eprint={1207.3278}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012ApJ...757...47H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Arras06, author={Arras, Phil and Bildsten, Lars}, title={Thermal Structure and Radius Evolution of Irradiated Gas Giant Planets}, journal={\apj}, keywords={Stars: Planetary Systems, Planets and Satellites: General, Astrophysics}, volume={650}, number={1}, pages={394-407}, doi={10.1086/506011}, archiveprefix={arXiv}, eprint={astro-ph/0601317}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2006ApJ...650..394A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Marleau14, author={Marleau, G. -D. and Cumming, A.}, title={Constraining the initial entropy of directly detected exoplanets}, journal={\mnras}, keywords={techniques: imaging spectroscopy, planets and satellites: fundamental parameters, planets and satellites: gaseous planets, stars: individual: $\beta$ Pictoris, stars: individual: 2MASSWJ 1207334-393254, stars: individual: HR 8799, Astrophysics - Earth and Planetary Astrophysics}, volume={437}, number={2}, pages={1378-1399}, doi={10.1093/mnras/stt1967}, archiveprefix={arXiv}, eprint={1302.1517}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2014MNRAS.437.1378M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Molliere15, author={Mollière, P. and van Boekel, R. and Dullemond, C. and Henning, Th. and Mordasini, C.}, title={Model Atmospheres of Irradiated Exoplanets: The Influence of Stellar Parameters, Metallicity, and the C/O Ratio}, journal={\apj}, keywords={methods: numerical, planets and satellites: atmospheres, radiative transfer, Astrophysics - Earth and Planetary Astrophysics}, volume={813}, number={1}, eid={47}, pages={47}, doi={10.1088/0004-637X/813/1/47}, archiveprefix={arXiv}, eprint={1509.07523}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ApJ...813...47M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Oberg11, author={Öberg, Karin I. and Murray-Clay, Ruth and Bergin, Edwin A.}, title={The Effects of Snowlines on C/O in Planetary Atmospheres}, journal={\apjl}, keywords={astrochemistry, circumstellar matter, molecular processes, planetary systems, planet-disk interactions, planets and satellites: atmospheres, Astrophysics - Astrophysics of Galaxies}, volume={743}, number={1}, eid={L16}, pages={L16}, doi={10.1088/2041-8205/743/1/L16}, archiveprefix={arXiv}, eprint={1110.5567}, primaryclass={astro-ph.GA}, adsurl={https://ui.adsabs.harvard.edu/abs/2011ApJ...743L..16O}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Molliere22, author={Mollière, Paul and Molyarova, Tamara and Bitsch, Bertram and Henning, Thomas and Schneider, Aaron and Kreidberg, Laura and Eistrup, Christian and Burn, Remo and Nasedkin, Evert and Semenov, Dmitry and Mordasini, Christoph and Schlecker, Martin and Schwarz, Kamber R. and Lacour, Sylvestre and Nowak, Mathias and Schulik, Matthäus}, title={Interpreting the Atmospheric Composition of Exoplanets: Sensitivity to Planet Formation Assumptions}, journal={\apj}, keywords={Exoplanet atmospheric composition, Exoplanet formation, 2021, 492, Astrophysics - Earth and Planetary Astrophysics}, volume={934}, number={1}, eid={74}, pages={74}, doi={10.3847/1538-4357/ac6a56}, archiveprefix={arXiv}, eprint={2204.13714}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022ApJ...934...74M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Yan23, author={Yan, F. and Nortmann, L. and Reiners, A. and Piskunov, N. and Hatzes, A. and Seemann, U. and Shulyak, D. and Lavail, A. and Rains, A. D. and Cont, D. and Rengel, M. and Lesjak, F. and Nagel, E. and Kochukhov, O. and Czesla, S. and Boldt-Christmas, L. and Heiter, U. and Smoker, J. V. and Rodler, F. and Bristow, P. and Dorn, R. J. and Jung, Y. and Marquart, T. and Stempels, E.}, title={CRIRES$^{+}$ detection of CO emissions lines and temperature inversions on the dayside of WASP-18b and WASP-76b}, journal={\aap}, keywords={planets and satellites: atmospheres, techniques: spectroscopic, planets and satellites: individual: WASP-18b, planets and satellites: individual: WASP-76b, Astrophysics - Earth and Planetary Astrophysics}, volume={672}, eid={A107}, pages={A107}, doi={10.1051/0004-6361/202245371}, archiveprefix={arXiv}, eprint={2302.08736}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023A&A...672A.107Y}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hatzes15, author={Hatzes, Artie P. and Rauer, Heike}, title={A Definition for Giant Planets Based on the Mass-Density Relationship}, journal={\apjl}, keywords={brown dwarfs, planets and satellites: fundamental parameters, stars: low-mass, Astrophysics - Earth and Planetary Astrophysics}, volume={810}, number={2}, eid={L25}, pages={L25}, doi={10.1088/2041-8205/810/2/L25}, archiveprefix={arXiv}, eprint={1506.05097}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ApJ...810L..25H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Subjak23, author={Šubjak, J. and Lodieu, N. and Kabáth, P. and Boffin, H. M. J. and Nowak, G. and Grundahl, F. and Béjar, V. J. S. and Zapatero Osorio, M. R. and Antoci, V.}, title={Search for planets around stars with wide brown dwarfs}, journal={\aap}, keywords={techniques: spectroscopic, techniques: radial velocities, techniques: photometric, planets and satellites: detection, planetary systems, brown dwarfs, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={671}, eid={A10}, pages={A10}, doi={10.1051/0004-6361/202244238}, archiveprefix={arXiv}, eprint={2212.03757}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023A&A...671A..10S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Stumpe2012, author={Stumpe, Martin C. and Smith, Jeffrey C. and Van Cleve, Jeffrey E. and Twicken, Joseph D. and Barclay, Thomas S. and Fanelli, Michael N. and Girouard, Forrest R. and Jenkins, Jon M. and Kolodziejczak, Jeffery J. and McCauliff, Sean D. and Morris, Robert L.}, title={Kepler Presearch Data Conditioning I—Architecture and Algorithms for Error Correction in Kepler Light Curves}, journal={\pasp}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics, Statistics - Applications}, year={2012}, month={Sep}, volume={124}, number={919}, pages={985}, doi={10.1086/667698}, archiveprefix={arXiv}, eprint={1203.1382}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2012PASP..124..985S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Stumpe2014, author={Stumpe, M. C. and Smith, J. C. and Catanzarite, J. H. and Van Cleve, J. E. and Jenkins, J. M. and Twicken, J. D. and Girouard, F. R.}, title={Multiscale Systematic Error Correction via Wavelet-Based Bandsplitting in Kepler Data}, journal={\pasp}, pages={100}, doi={10.1086/674989}, adsurl={http://adsabs.harvard.edu/abs/2014PASP..126..100S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Smith12, author={Smith, J. C. and Stumpe, M. C. and Van Cleve, J. E. and Jenkins, J. M. and Barclay, T. S. and Fanelli, M. N. and Girouard, F. R. and Kolodziejczak, J. J. and McCauliff, S. D. and Morris, R. L. and Twicken, J. D.}, title={Kepler Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction}, journal={\pasp}, archiveprefix={arXiv}, eprint={1203.1383}, primaryclass={astro-ph.IM}, pages={1000}, doi={10.1086/667697}, adsurl={http://adsabs.harvard.edu/abs/2012PASP..124.1000S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Skrutskie06, author={Skrutskie, M. F. and Cutri, R. M. and Stiening, R. and Weinberg, M. D. and Schneider, S. and Carpenter, J. M. and Beichman, C. and Capps, R. and Chester, T. and Elias, J. and Huchra, J. and Liebert, J. and Lonsdale, C. and Monet, D. G. and Price, S. and Seitzer, P. and Jarrett, T. and Kirkpatrick, J. D. and Gizis, J. E. and Howard, E. and Evans, T. and Fowler, J. and Fullmer, L. and Hurt, R. and Light, R. and Kopan, E. L. and Marsh, K. A. and McCallon, H. L. and Tam, R. and Van Dyk, S. and Wheelock, S.}, title={The Two Micron All Sky Survey (2MASS)}, journal={\aj}, keywords={Catalogs, Infrared: General, Surveys}, volume={131}, number={2}, pages={1163-1183}, doi={10.1086/498708}, adsurl={https://ui.adsabs.harvard.edu/abs/2006AJ....131.1163S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Leggett92, author={Leggett, S. K.}, title={Infrared Colors of Low-Mass Stars}, journal={\apjs}, keywords={Infrared Photometry, Red Dwarf Stars, Stellar Mass, Stellar Spectrophotometry, Color-Color Diagram, Metallicity, Stellar Color, Stellar Spectra, Stellar Temperature, Ubv Spectra, Astrophysics, STARS: ABUNDANCES, STARS: FUNDAMENTAL PARAMETERS, STARS: LOW-MASS, BROWN DWARFS}, volume={82}, pages={351}, doi={10.1086/191720}, adsurl={https://ui.adsabs.harvard.edu/abs/1992ApJS...82..351L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Bensby03, author={Bensby, T. and Feltzing, S. and Lundström, I.}, title={Elemental abundance trends in the Galactic thin and thick disks as traced by nearby F and G dwarf stars}, journal={\aap}, keywords={stars: fundamental parameters, stars: abundances, Galaxy: disk, Galaxy: formation, Galaxy: abundances, Galaxy: kinematics and dynamics}, volume={410}, pages={527-551}, doi={10.1051/0004-6361:20031213}, adsurl={https://ui.adsabs.harvard.edu/abs/2003A&A...410..527B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fuhrmann98, author={Fuhrmann, Klaus}, title={Nearby stars of the Galactic disk and halo}, journal={\aap}, keywords={STARS: DISTANCES, STARS: FUNDAMENTAL PARAMETERS, STARS: LATE-TYPE, GALAXY: EVOLUTION}, volume={338}, pages={161-183}, adsurl={https://ui.adsabs.harvard.edu/abs/1998A&A...338..161F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Steinmetz20, author={Steinmetz, Matthias and Guiglion, Guillaume and McMillan, Paul J. and Matijevič, Gal and Enke, Harry and Kordopatis, Georges and Zwitter, Tomaž and Valentini, Marica and Chiappini, Cristina and Casagrande, Luca and Wojno, Jennifer and Anguiano, Borja and Bienaymé, Olivier and Bijaoui, Albert and Binney, James and Burton, Donna and Cass, Paul and de Laverny, Patrick and Fiegert, Kristin and Freeman, Kenneth and Fulbright, Jon P. and Gibson, Brad K. and Gilmore, Gerard and Grebel, Eva K. and Helmi, Amina and Kunder, Andrea and Munari, Ulisse and Navarro, Julio F. and Parker, Quentin and Ruchti, Gregory R. and Recio-Blanco, Alejandra and Reid, Warren and Seabroke, George M. and Siviero, Alessandro and Siebert, Arnaud and Stupar, Milorad and Watson, Fred and Williams, Mary E. K. and Wyse, Rosemary F. G. and Anders, Friedrich and Antoja, Teresa and Birko, Danijela and Bland-Hawthorn, Joss and Bossini, Diego and Garcıa, Rafael A. and Carrillo, Ismael and Chaplin, William J. and Elsworth, Yvonne and Famaey, Benoit and Gerhard, Ortwin and Jofre, Paula and Just, Andreas and Mathur, Savita and Miglio, Andrea and Minchev, Ivan and Monari, Giacomo and Mosser, Benoit and Ritter, Andreas and Rodrigues, Thaise S. and Scholz, Ralf-Dieter and Sharma, Sanjib and Sysoliatina, Kseniia and RAVE Collaboration}, title={The Sixth Data Release of the Radial Velocity Experiment (RAVE). II. Stellar Atmospheric Parameters, Chemical Abundances, and Distances}, journal={\aj}, keywords={Surveys, Sky surveys, Milky Way Galaxy, Milky Way dynamics, Galaxy stellar content, Stellar populations, Catalogs, 1671, 1464, 1054, 1051, 621, 1622, 205, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, volume={160}, number={2}, eid={83}, pages={83}, doi={10.3847/1538-3881/ab9ab8}, archiveprefix={arXiv}, eprint={2002.04512}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2020AJ....160...83S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hirsch17, author={Hirsch, Lea A. and Ciardi, David R. and Howard, Andrew W. and Everett, Mark E. and Furlan, Elise and Saylors, Mindy and Horch, Elliott P. and Howell, Steve B. and Teske, Johanna and Marcy, Geoffrey W.}, title={Assessing the Effect of Stellar Companions from High-resolution Imaging of Kepler Objects of Interest}, journal={\aj}, keywords={binaries: visual, planets and satellites: detection, planets and satellites: fundamental parameters, techniques: high angular resolution, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics}, volume={153}, number={3}, eid={117}, pages={117}, doi={10.3847/1538-3881/153/3/117}, archiveprefix={arXiv}, eprint={1701.06577}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2017AJ....153..117H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mandushev05, author={Mandushev, Georgi and Torres, Guillermo and Latham, David W. and Charbonneau, David and Alonso, Roi and White, Russel J. and Stefanik, Robert P. and Dunham, Edward W. and Brown, Timothy M. and O'Donovan, Francis T.}, title={The Challenge of Wide-Field Transit Surveys: The Case of GSC 01944-02289}, journal={\apj}, keywords={Stars: Binaries: Eclipsing, Line: Profiles, Stars: Planetary Systems, Techniques: Photometric, Techniques: Radial Velocities, Astrophysics}, volume={621}, number={2}, pages={1061-1071}, doi={10.1086/427727}, archiveprefix={arXiv}, eprint={astro-ph/0501554}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2005ApJ...621.1061M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Zucker94, author={Zucker, S. and Mazeh, T.}, title={Study of Spectroscopic Binaries with TODCOR. I. A New Two-dimensional Correlation Algorithm to Derive the Radial Velocities of the Two Components}, journal={\apj}, keywords={Algorithms, Binary Stars, Cross Correlation, Radial Velocity, Two Dimensional Models, Doppler Effect, Fast Fourier Transformations, Astrophysics, STARS: BINARIES: CLOSE, TECHNIQUES: RADIAL VELOCITIES}, volume={420}, pages={806}, doi={10.1086/173605}, adsurl={https://ui.adsabs.harvard.edu/abs/1994ApJ...420..806Z}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Brown13, author={Brown, T. M. and Baliber, N. and Bianco, F. B. and Bowman, M. and Burleson, B. and Conway, P. and Crellin, M. and Depagne, É. and De Vera, J. and Dilday, B. and Dragomir, D. and Dubberley, M. and Eastman, J. D. and Elphick, M. and Falarski, M. and Foale, S. and Ford, M. and Fulton, B. J. and Garza, J. and Gomez, E. L. and Graham, M. and Greene, R. and Haldeman, B. and Hawkins, E. and Haworth, B. and Haynes, R. and Hidas, M. and Hjelstrom, A. E. and Howell, D. A. and Hygelund, J. and Lister, T. A. and Lobdill, R. and Martinez, J. and Mullins, D. S. and Norbury, M. and Parrent, J. and Paulson, R. and Petry, D. L. and Pickles, A. and Posner, V. and Rosing, W. E. and Ross, R. and Sand, D. J. and Saunders, E. S. and Shobbrook, J. and Shporer, A. and Street, R. A. and Thomas, D. and Tsapras, Y. and Tufts, J. R. and Valenti, S. and Vander Horst, K. and Walker, Z. and White, G. and Willis, M.}, title={Las Cumbres Observatory Global Telescope Network}, journal={\pasp}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics}, volume={125}, number={931}, pages={1031}, doi={10.1086/673168}, archiveprefix={arXiv}, eprint={1305.2437}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2013PASP..125.1031B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{McCully18, author={McCully, Curtis and Volgenau, Nikolaus H. and Harbeck, Daniel-Rolf and Lister, Tim A. and Saunders, Eric S. and Turner, Monica L. and Siiverd, Robert J. and Bowman, Mark}, title={Real-time processing of the imaging data from the network of Las Cumbres Observatory Telescopes using BANZAI}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics}, booktitle={Software and Cyberinfrastructure for Astronomy V}, editor={Guzman, Juan C. and Ibsen, Jorge}, series={Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series}, volume={10707}, eid={107070K}, pages={107070K}, doi={10.1117/12.2314340}, archiveprefix={arXiv}, eprint={1811.04163}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2018SPIE10707E..0KM}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Allard2012, abstract={Within the next few years, GAIA and several instruments aiming at imag- ing extrasolar planets will see first light. In parallel, low mass planets are being searched around red dwarfs which offer more favourable conditions, both for radial velocity de- tection and transit studies, than solar-type stars. Authors of the model atmosphere code which has allowed the detection of water vapour in the atmosphere of Hot Jupiters re- view recent advancement in modelling the stellar to substellar transition. The revised solar oxygen abundances and cloud model allow for the first time to reproduce the pho- tometric and spectroscopic properties of this transition. Also presented are highlight results of a model atmosphere grid for stars, brown dwarfs and extrasolar planets.}, author={Allard, F. and Homeier, D. and Freytag, B.}, doi={10.1098/rsta.2011.0269}, issn={1364503X}, journal={Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences}, keywords={Brown dwarfs,CO5BOLD,Opacities,Stars,Very-low-mass stars}, number={1968}, pages={2765--2777}, title={Models of very-low-mass stars, brown dwarfs and exoplanets}, volume={370}, year={2012} }@article{Kurucz93, author={Kurucz, Robert}, title={ATLAS9 Stellar Atmosphere Programs and 2 km/s grid.}, journal={ATLAS9 Stellar Atmosphere Programs and 2 km/s grid. Kurucz CD-ROM No. 13. Cambridge}, year={1993}, month={Jan}, volume={13}, adsurl={https://ui.adsabs.harvard.edu/abs/1993KurCD..13.....K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{Castelli2004, author={Castelli, F. and Kurucz, R. L.}, title={New Grids of ATLAS9 Model Atmospheres}, keywords={Astrophysics}, booktitle={Modelling of Stellar Atmospheres}, year={2003}, editor={Piskunov, N. and Weiss, W. W. and Gray, D. F.}, volume={210}, month={jan}, pages={A20}, series={}, archiveprefix={arXiv}, eprint={astro-ph/0405087}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2003IAUS..210P.A20C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Vines22, author={Vines, Jose I. and Jenkins, James S.}, title={ARIADNE: Measuring accurate and precise stellar parameters through SED fitting}, journal={\mnras}, keywords={stars:atmospheres, methods:data analysis, stars:fundamental parameters, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, doi={10.1093/mnras/stac956}, archiveprefix={arXiv}, eprint={2204.03769}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2022MNRAS.tmp..920V}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Noyes84, author={Noyes, R. W. and Hartmann, L. W. and Baliunas, S. L. and Duncan, D. K. and Vaughan, A. H.}, title={Rotation, convection, and magnetic activity in lower main-sequence stars.}, journal={\apj}, keywords={Magnetic Stars, Main Sequence Stars, Stellar Activity, Stellar Magnetic Fields, Stellar Rotation, Chromosphere, Convection, Late Stars, Magnetoactivity, Astrophysics}, volume={279}, pages={763-777}, doi={10.1086/161945}, adsurl={https://ui.adsabs.harvard.edu/abs/1984ApJ...279..763N}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mittag13, author={Mittag, M. and Schmitt, J. H. M. M. and Schröder, K. -P.}, title={Ca II H+K fluxes from S-indices of large samples: a reliable and consistent conversion based on PHOENIX model atmospheres}, journal={\aap}, keywords={stars: atmospheres, stars: activity, stars: chromospheres, stars: late-type, stars: solar-type}, volume={549}, eid={A117}, pages={A117}, doi={10.1051/0004-6361/201219868}, adsurl={https://ui.adsabs.harvard.edu/abs/2013A&A...549A.117M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mamajek:2008, author={Mamajek, Eric E. and Hillenbrand, Lynne A.}, title={Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics}, journal={\apj}, keywords={stars: activity, stars: chromospheres, stars: coronae, stars: fundamental parameters, stars: rotation, X-rays: stars, Astrophysics}, volume={687}, number={2}, pages={1264-1293}, doi={10.1086/591785}, archiveprefix={arXiv}, eprint={0807.1686}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2008ApJ...687.1264M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mentuch08, author={Mentuch, Erin and Brandeker, Alexis and van Kerkwijk, Marten H. and Jayawardhana, Ray and Hauschildt, Peter H.}, title={Lithium Depletion of Nearby Young Stellar Associations}, journal={\apj}, keywords={line: profiles, open clusters and associations: individual: $\eta$ Chamaeleontis TW Hydrae $\beta$ Pictoris Tucanae-Horologium AB Doradus, stars: abundances, stars: pre-main sequence, Astrophysics}, volume={689}, number={2}, pages={1127-1140}, doi={10.1086/592764}, archiveprefix={arXiv}, eprint={0808.3584}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2008ApJ...689.1127M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Soderblom93, author={Soderblom, David R. and Jones, Burton F. and Balachandran, Suchitra and Stauffer, John R. and Duncan, Douglas K. and Fedele, Stephen B. and Hudon, J. D.}, title={The Evolution of the Lithium Abundances of Solar-Type Stars. III. The Pleiades}, journal={\aj}, keywords={Abundance, F Stars, G Stars, K Stars, Lithium, Star Clusters, Stellar Evolution, Color-Magnitude Diagram, Spectral Line Width, Starspots, Stellar Atmospheres, Stellar Rotation, Stellar Spectra, Astrophysics, STARS: ABUNDANCES, OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: PLEIADES}, volume={106}, pages={1059}, doi={10.1086/116704}, adsurl={https://ui.adsabs.harvard.edu/abs/1993AJ....106.1059S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Jones97, author={Jones, Burton F. and Fischer, Debra and Shetrone, Matthew and Soderblom, David R.}, title={The Evolution of the Lithium Abundances of Solar-Type Stars.VII.M34 (NGC 1039) and the Role of Rotation in Lithium Depletion}, journal={\aj}, volume={114}, pages={352-362}, doi={10.1086/118479}, adsurl={https://ui.adsabs.harvard.edu/abs/1997AJ....114..352J}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Soderblom1993, author={Soderblom, David R. and Pilachowski, Catherine A. and Fedele, Stephen B. and Jones, Burton F.}, title={The Evolution of the Lithium Abundances of Solar-Type Stars. II. the Ursa Major Group}, journal={\aj}, keywords={Abundance, Lithium, Main Sequence Stars, Stellar Composition, Dwarf Stars, G Stars, K Stars, Stellar Evolution, Astrophysics, STARS: ABUNDANCES}, volume={105}, pages={2299}, doi={10.1086/116608}, adsurl={https://ui.adsabs.harvard.edu/abs/1993AJ....105.2299S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Soderblom993, author={Soderblom, David R. and Fedele, Stephen B. and Jones, Burton F. and Stauffer, John R. and Prosser, Charles F.}, title={The Evolution of the Lithium Abundances of Solar-Type Stars. IV. Praesepe}, journal={\aj}, keywords={Abundance, F Stars, G Stars, Lithium, Star Clusters, Stellar Evolution, Binary Stars, Color-Magnitude Diagram, Spectral Line Width, Stellar Composition, Stellar Spectrophotometry, Stellar Temperature, Astrophysics, OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: PRAESEPE, STARS: ABUNDANCES}, volume={106}, pages={1080}, doi={10.1086/116705}, adsurl={https://ui.adsabs.harvard.edu/abs/1993AJ....106.1080S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Soderblom90, author={Soderblom, D. R. and Oey, M. S. and Johnson, D. R. H. and Stone, R. P. S.}, title={The Evolution of the Lithium Abundances of Solar-Type Stars. I. The Hyades and Coma Berenices Clusters}, journal={\aj}, keywords={Lithium, Star Clusters, Stellar Evolution, Abundance, Chemical Composition, High Resolution, Signal To Noise Ratios, Astrophysics, STARS: ABUNDANCES}, volume={99}, pages={595}, doi={10.1086/115353}, adsurl={https://ui.adsabs.harvard.edu/abs/1990AJ.....99..595S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Jones99, author={Jones, Burton F. and Fischer, Debra and Soderblom, David R.}, title={The Evolution of the Lithium Abundances of Solar-Type Stars. VIII. M67 (NGC 2682)}, journal={\aj}, keywords={GALAXY: OPEN CLUSTERS AND ASSOCIATIONS: GENERAL, STARS: ABUNDANCES, STARS: EVOLUTION, STARS: LATE-TYPE, STARS: ROTATION}, volume={117}, number={1}, pages={330-338}, doi={10.1086/300664}, adsurl={https://ui.adsabs.harvard.edu/abs/1999AJ....117..330J}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Godoy21, author={Godoy-Rivera, Diego and Pinsonneault, Marc H. and Rebull, Luisa M.}, title={Stellar Rotation in the Gaia Era: Revised Open Clusters' Sequences}, journal={\apjs}, keywords={1160, 1567, 1581, 1629, 2050, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={257}, number={2}, eid={46}, pages={46}, doi={10.3847/1538-4365/ac2058}, archiveprefix={arXiv}, eprint={2101.01183}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2021ApJS..257...46G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Curtis19, author={Curtis, Jason Lee and Agüeros, Marcel A. and Douglas, Stephanie T. and Meibom, Søren}, title={A Temporary Epoch of Stalled Spin-down for Low-mass Stars: Insights from NGC 6811 with Gaia and Kepler}, journal={\apj}, keywords={open clusters and associations: individual: NGC 6811, Pleiades, Praesepe, stars: evolution, stars: rotation, stars: solar-type, Astrophysics - Solar and Stellar Astrophysics}, volume={879}, number={1}, eid={49}, pages={49}, doi={10.3847/1538-4357/ab2393}, archiveprefix={arXiv}, eprint={1905.06869}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJ...879...49C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Gaia2018, author={Gaia Collaboration and Babusiaux, C. and van Leeuwen, F. and Barstow, M. A. and Jordi, C. and Vallenari, A. and Bossini, D. and Bressan, A. and Cantat-Gaudin, T. and van Leeuwen, M. and Brown, A. G. A. and Prusti, T. and de Bruijne, J. H. J. and Bailer-Jones, C. A. L. and Biermann, M. and Evans, D. W. and Eyer, L. and Jansen, F. and Klioner, S. A. and Lammers, U. and Lindegren, L. and Luri, X. and Mignard, F. and Panem, C. and Pourbaix, D. and Randich, S. and Sartoretti, P. and Siddiqui, H. I. and Soubiran, C. and Walton, N. A. and Arenou, F. and Bastian, U. and Cropper, M. and Drimmel, R. and Katz, D. and Lattanzi, M. G. and Bakker, J. and Cacciari, C. and Castañeda, J. and Chaoul, L. and Cheek, N. and De Angeli, F. and Fabricius, C. and Guerra, R. and Holl, B. and Masana, E. and Messineo, R. and Mowlavi, N. and Nienartowicz, K. and Panuzzo, P. and Portell, J. and Riello, M. and Seabroke, G. M. and Tanga, P. and Thévenin, F. and Gracia-Abril, G. and Comoretto, G. and Garcia-Reinaldos, M. and Teyssier, D. and Altmann, M. and Andrae, R. and Audard, M. and Bellas-Velidis, I. and Benson, K. and Berthier, J. and Blomme, R. and Burgess, P. and Busso, G. and Carry, B. and Cellino, A. and Clementini, G. and Clotet, M. and Creevey, O. and Davidson, M. and De Ridder, J. and Delchambre, L. and Dell'Oro, A. and Ducourant, C. and Fernández-Hernández, J. and Fouesneau, M. and Frémat, Y. and Galluccio, L. and Garcıa-Torres, M. and González-Núñez, J. and González-Vidal, J. J. and Gosset, E. and Guy, L. P. and Halbwachs, J. -L. and Hambly, N. C. and Harrison, D. L. and Hernández, J. and Hestroffer, D. and Hodgkin, S. T. and Hutton, A. and Jasniewicz, G. and Jean-Antoine-Piccolo, A. and Jordan, S. and Korn, A. J. and Krone-Martins, A. and Lanzafame, A. C. and Lebzelter, T. and Löffler, W. and Manteiga, M. and Marrese, P. M. and Martın-Fleitas, J. M. and Moitinho, A. and Mora, A. and Muinonen, K. and Osinde, J. and Pancino, E. and Pauwels, T. and Petit, J. -M. and Recio-Blanco, A. and Richards, P. J. and Rimoldini, L. and Robin, A. C. and Sarro, L. M. and Siopis, C. and Smith, M. and Sozzetti, A. and Süveges, M. and Torra, J. and van Reeven, W. and Abbas, U. and Abreu Aramburu, A. and Accart, S. and Aerts, C. and Altavilla, G. and Álvarez, M. A. and Alvarez, R. and Alves, J. and Anderson, R. I. and Andrei, A. H. and Anglada Varela, E. and Antiche, E. and Antoja, T. and Arcay, B. and Astraatmadja, T. L. and Bach, N. and Baker, S. G. and Balaguer-Núñez, L. and Balm, P. and Barache, C. and Barata, C. and Barbato, D. and Barblan, F. and Barklem, P. S. and Barrado, D. and Barros, M. and Bartholomé Muñoz, L. and Bassilana, J. -L. and Becciani, U. and Bellazzini, M. and Berihuete, A. and Bertone, S. and Bianchi, L. and Bienaymé, O. and Blanco-Cuaresma, S. and Boch, T. and Boeche, C. and Bombrun, A. and Borrachero, R. and Bouquillon, S. and Bourda, G. and Bragaglia, A. and Bramante, L. and Breddels, M. A. and Brouillet, N. and Brüsemeister, T. and Brugaletta, E. and Bucciarelli, B. and Burlacu, A. and Busonero, D. and Butkevich, A. G. and Buzzi, R. and Caffau, E. and Cancelliere, R. and Cannizzaro, G. and Carballo, R. and Carlucci, T. and Carrasco, J. M. and Casamiquela, L. and Castellani, M. and Castro-Ginard, A. and Charlot, P. and Chemin, L. and Chiavassa, A. and Cocozza, G. and Costigan, G. and Cowell, S. and Crifo, F. and Crosta, M. and Crowley, C. and Cuypers, J. and Dafonte, C. and Damerdji, Y. and Dapergolas, A. and David, P. and David, M. and de Laverny, P. and De Luise, F. and De March, R. and de Martino, D. and de Souza, R. and de Torres, A. and Debosscher, J. and del Pozo, E. and Delbo, M. and Delgado, A. and Delgado, H. E. and Diakite, S. and Diener, C. and Distefano, E. and Dolding, C. and Drazinos, P. and Durán, J. and Edvardsson, B. and Enke, H. and Eriksson, K. and Esquej, P. and Eynard Bontemps, G. and Fabre, C. and Fabrizio, M. and Faigler, S. and Falcão, A. 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Paul}, title={The HARPS-TERRA Project. I. Description of the Algorithms, Performance, and New Measurements on a Few Remarkable Stars Observed by HARPS}, journal={\apjs}, keywords={methods: data analysis, planetary systems, stars: individual: Tau Ceti HD 85512 Barnard's star Proxima Kapteyn's star GJ676A Epsilon Eridani HD 69830, techniques: radial velocities, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={200}, number={2}, eid={15}, pages={15}, doi={10.1088/0067-0049/200/2/15}, archiveprefix={arXiv}, eprint={1202.2570}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012ApJS..200...15A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mayor03, author={Mayor, M. and Pepe, F. and Queloz, D. and Bouchy, F. and Rupprecht, G. and Lo Curto, G. and Avila, G. and Benz, W. and Bertaux, J. -L. and Bonfils, X. and Dall, Th. and Dekker, H. and Delabre, B. and Eckert, W. and Fleury, M. and Gilliotte, A. and Gojak, D. and Guzman, J. 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N.}, title={Exoplanet Transits and Occultations}, booktitle={Exoplanets}, editor={Seager, S.}, pages={55-77}, adsurl={https://ui.adsabs.harvard.edu/abs/2010exop.book...55W}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fossati17, author={Fossati, L. and Erkaev, N. V. and Lammer, H. and Cubillos, P. E. and Odert, P. and Juvan, I. and Kislyakova, K. G. and Lendl, M. and Kubyshkina, D. and Bauer, S. J.}, title={Aeronomical constraints to the minimum mass and maximum radius of hot low-mass planets}, journal={\aap}, keywords={planets and satellites: atmospheres, planets and satellites: fundamental parameters, planets and satellites: gaseous planets, Astrophysics - Earth and Planetary Astrophysics}, volume={598}, eid={A90}, pages={A90}, doi={10.1051/0004-6361/201629716}, archiveprefix={arXiv}, eprint={1612.05624}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2017A&A...598A..90F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{pyaneti, author={Barragán, O. and Gandolfi, D. and Antoniciello, G.}, title={PYANETI: a fast and powerful software suite for multiplanet radial velocity and transit fitting}, journal={\mnras}, keywords={methods: numerical, techniques: photometric, techniques: spectroscopic, planets and satellites: general, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Data Analysis, Statistics and Probability}, volume={482}, pages={1017-1030}, doi={10.1093/mnras/sty2472}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/#abs/2019MNRAS.482.1017B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Georgieva21, author={Georgieva, I. 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D. and Vanderspek, R. and Van Eylen, V. and Winn, J. N.}, title={Hot planets around cool stars - two short-period mini-Neptunes transiting the late K-dwarf TOI-1260}, journal={\mnras}, keywords={techniques: photometric, techniques: radial velocities, planets and satellites: atmospheres, planets and satellites: individual: TOI-1260b, c, planets and satellites: composition, stars: low-mass, planetary systems, Astrophysics - Earth and Planetary Astrophysics}, volume={505}, number={4}, pages={4684-4701}, doi={10.1093/mnras/stab1464}, archiveprefix={arXiv}, eprint={2104.05653}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021MNRAS.505.4684G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Demory13, author={Demory, Brice-Olivier and Torres, Guillermo and Neves, Vasco and Rogers, Leslie and Gillon, Michaël and Horch, Elliott and Sullivan, Peter and Bonfils, Xavier and Delfosse, Xavier and Forveille, Thierry and Lovis, Christophe and Mayor, Michel and Santos, Nuno and Seager, Sara and Smalley, Barry and Udry, Stephane}, title={Spitzer Observations of GJ 3470 b: A Very Low-density Neptune-size Planet Orbiting a Metal-rich M Dwarf}, journal={\apj}, keywords={planetary systems, stars: individual: GJ 3470, techniques: photometric, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics}, volume={768}, number={2}, eid={154}, pages={154}, doi={10.1088/0004-637X/768/2/154}, archiveprefix={arXiv}, eprint={1301.6555}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2013ApJ...768..154D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Benneke19, author={Benneke, Björn and Knutson, Heather A. and Lothringer, Joshua and Crossfield, Ian J. 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M. and Nagel, E. and Yan, F. and Alonso-Floriano, F. J. and Amado, P. J. and Chen, G. and Cifuentes, C. and Cortés-Contreras, M. and Czesla, S. and Molaverdikhani, K. and Montes, D. and Passegger, V. M. and Quirrenbach, A. and Reiners, A. and Ribas, I. and Sánchez-López, A. and Schweitzer, A. and Stangret, M. and Zapatero Osorio, M. R. and Zechmeister, M.}, title={A He I upper atmosphere around the warm Neptune GJ 3470 b}, journal={\aap}, keywords={planetary systems, planets and satellites: atmospheres, planet-star interactions, planets and satellites: general, planets and satellites: individual: GJ 3470b, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={638}, eid={A61}, pages={A61}, doi={10.1051/0004-6361/202037719}, archiveprefix={arXiv}, eprint={2004.12812}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2020A&A...638A..61P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Wilson22, author={Wilson, Thomas G. and Goffo, Elisa and Alibert, Yann and Gandolfi, Davide and Bonfanti, Andrea and Persson, Carina M. and Collier Cameron, Andrew and Fridlund, Malcolm and Fossati, Luca and Korth, Judith and Benz, Willy and Deline, Adrien and Florén, Hans-Gustav and Guterman, Pascal and Adibekyan, Vardan and Hooton, Matthew J. and Hoyer, Sergio and Leleu, Adrien and Mustill, Alexander James and Salmon, Sébastien and Sousa, Sérgio G. and Suarez, Olga and Abe, Lyu and Agabi, Abdelkrim and Alonso, Roi and Anglada, Guillem and Asquier, Joel and Bárczy, Tamas and Barrado Navascues, David and Barros, Susana C. C. and Baumjohann, Wolfgang and Beck, Mathias and Beck, Thomas and Billot, Nicolas and Bonfils, Xavier and Brandeker, Alexis and Broeg, Christopher and Bryant, Edward M. and Burleigh, Matthew R. and Buttu, Marco and Cabrera, Juan and Charnoz, Sébastien and Ciardi, David R. and Cloutier, Ryan and Cochran, William D. and Collins, Karen A. and Colón, Knicole D. and Crouzet, Nicolas and Csizmadia, Szilard and Davies, Melvyn B. and Deleuil, Magali and Delrez, Laetitia and Demangeon, Olivier and Demory, Brice-Olivier and Dragomir, Diana and Dransfield, Georgina and Ehrenreich, David and Erikson, Anders and Fortier, Andrea and Gan, Tianjun and Gill, Samuel and Gillon, Michaël and Gnilka, Crystal L. and Grieves, Nolan and Grziwa, Sascha and Güdel, Manuel and Guillot, Tristan and Haldemann, Jonas and Heng, Kevin and Horne, Keith and Howell, Steve B. and Isaak, Kate G. and Jenkins, Jon M. and Jensen, Eric L. N. and Kiss, Laszlo and Lacedelli, Gaia and Lam, Kristine and Laskar, Jacques and Latham, David W. and Lecavelier des Etangs, Alain and Lendl, Monika and Lester, Kathryn V. and Levine, Alan M. and Livingston, John and Lovis, Christophe and Luque, Rafael and Magrin, Demetrio and Marie-Sainte, Wenceslas and Maxted, Pierre F. L. and Mayo, Andrew W. and McLean, Brian and Mecina, Marko and Mékarnia, Djamel and Nascimbeni, Valerio and Nielsen, Louise D. and Olofsson, Göran and Osborn, Hugh P. and Osborne, Hannah L. M. and Ottensamer, Roland and Pagano, Isabella and Pallé, Enric and Peter, Gisbert and Piotto, Giampaolo and Pollacco, Don and Queloz, Didier and Ragazzoni, Roberto and Rando, Nicola and Rauer, Heike and Redfield, Seth and Ribas, Ignasi and Ricker, George R. and Rieder, Martin and Santos, Nuno C. and Scandariato, Gaetano and Schmider, François-Xavier and Schwarz, Richard P. and Scott, Nicholas J. and Seager, Sara and Ségransan, Damien and Serrano, Luisa Maria and Simon, Attila E. and Smith, Alexis M. S. and Steller, Manfred and Stockdale, Chris and Szabó, Gyula and Thomas, Nicolas and Ting, Eric B. and Triaud, Amaury H. M. J. and Udry, Stéphane and Van Eylen, Vincent and Van Grootel, Valérie and Vanderspek, Roland K. and Viotto, Valentina and Walton, Nicholas and Winn, Joshua N.}, title={A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS}, journal={\mnras}, keywords={techniques: photometric, techniques: radial velocities, planets and satellites: composition, planets and satellites: detection, planets and satellites: interiors, stars: individual: TOI-1064 (TIC 79748331, Gaia EDR3 6683371847364921088), Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={511}, number={1}, pages={1043-1071}, doi={10.1093/mnras/stab3799}, archiveprefix={arXiv}, eprint={2201.03570}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022MNRAS.511.1043W}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Baumeister23, author={Baumeister, Philipp and Tosi, Nicola}, title={ExoMDN: Rapid characterization of exoplanet interior structures with mixture density networks★}, journal={\aap}, keywords={planets and satellites: interiors, planets and satellites: composition, methods: numerical, methods: statistical, Astrophysics - Earth and Planetary Astrophysics, Computer Science - Machine Learning}, volume={676}, eid={A106}, pages={A106}, doi={10.1051/0004-6361/202346216}, archiveprefix={arXiv}, eprint={2306.09002}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023A&A...676A.106B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Baumeister20, author={Baumeister, Philipp and Padovan, Sebastiano and Tosi, Nicola and Montavon, Grégoire and Nettelmann, Nadine and MacKenzie, Jasmine and Godolt, Mareike}, title={Machine-learning Inference of the Interior Structure of Low-mass Exoplanets}, journal={\apj}, keywords={Exoplanet structure, Exoplanets, Neural networks, Planetary interior, Computational methods, Planetary theory, 495, 498, 1933, 1248, 1965, 1258, Astrophysics - Earth and Planetary Astrophysics}, volume={889}, number={1}, eid={42}, pages={42}, doi={10.3847/1538-4357/ab5d32}, archiveprefix={arXiv}, eprint={1911.12745}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2020ApJ...889...42B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{MacKenzie23, author={MacKenzie, Jasmine and Grenfell, John Lee and Baumeister, Philipp and Tosi, Nicola and Cabrera, Juan and Rauer, Heike}, title={Effect of improved atmospheric opacities in modelling sub-Neptunes. A case study for GJ 1214 b}, journal={\aap}, keywords={planets and satellites: individual: GJ 1214 b, planets and satellites: atmospheres, planets and satellites: composition, planets and satellites: fundamental parameters, planets and satellites: interiors}, volume={671}, eid={A65}, pages={A65}, doi={10.1051/0004-6361/202141784}, adsurl={https://ui.adsabs.harvard.edu/abs/2023A&A...671A..65M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Csizmadia19, author={Csizmadia, Sz. and Hellard, H. and Smith, A. M. S.}, title={An estimate of the k$_{2}$ Love number of WASP-18Ab from its radial velocity measurements}, journal={\aap}, keywords={techniques: radial velocities, planets and satellites: interiors, planets and satellites: individual: WASP-18b, methods: data analysis, Astrophysics - Earth and Planetary Astrophysics}, volume={623}, eid={A45}, pages={A45}, doi={10.1051/0004-6361/201834376}, archiveprefix={arXiv}, eprint={1812.04463}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019A&A...623A..45C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Akinsanmi19, author={Akinsanmi, B. and Barros, S. C. C. and Santos, N. C. and Correia, A. C. M. and Maxted, P. F. L. and Boué, G. and Laskar, J.}, title={Detectability of shape deformation in short-period exoplanets}, journal={\aap}, keywords={methods: analytical, techniques: photometric, planets and satellites: interiors, Astrophysics - Earth and Planetary Astrophysics}, volume={621}, eid={A117}, pages={A117}, doi={10.1051/0004-6361/201834215}, archiveprefix={arXiv}, eprint={1812.04538}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019A&A...621A.117A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Dorn15, author={Dorn, Caroline and Khan, Amir and Heng, Kevin and Connolly, James A. D. and Alibert, Yann and Benz, Willy and Tackley, Paul}, title={Can we constrain the interior structure of rocky exoplanets from mass and radius measurements?}, journal={\aap}, keywords={planets and satellites: terrestrial planets, planets and satellites: interiors, Astrophysics - Earth and Planetary Astrophysics}, volume={577}, eid={A83}, pages={A83}, doi={10.1051/0004-6361/201424915}, archiveprefix={arXiv}, eprint={1502.03605}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015A&A...577A..83D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fares09, author={Fares, R. and Donati, J. -F. and Moutou, C. and Bohlender, D. and Catala, C. and Deleuil, M. and Shkolnik, E. and Collier Cameron, A. and Jardine, M. M. and Walker, G. A. H.}, title={Magnetic cycles of the planet-hosting star $\tau$ Bootis - II. A second magnetic polarity reversal}, journal={\mnras}, keywords={stars: activity, stars: individual: $\tau$ Boo, stars: magnetic fields, planetary systems, Astrophysics - Solar and Stellar Astrophysics}, volume={398}, number={3}, pages={1383-1391}, doi={10.1111/j.1365-2966.2009.15303.x}, archiveprefix={arXiv}, eprint={0906.4515}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2009MNRAS.398.1383F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Carone07, author={Carone, Ludmila and Pätzold, Martin}, title={Constraints on the tidal dissipation factor of a main sequence star: The case of OGLE-TR-56b}, journal={\planss}, volume={55}, number={5}, pages={643-650}, doi={10.1016/j.pss.2006.05.044}, adsurl={https://ui.adsabs.harvard.edu/abs/2007P&SS...55..643C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Jackson09, author={Jackson, Brian and Barnes, Rory and Greenberg, Richard}, title={Observational Evidence for Tidal Destruction of Exoplanets}, journal={\apj}, keywords={planetary systems: formation, planetary systems: protoplanetary disks, Astrophysics - Earth and Planetary Astrophysics}, volume={698}, number={2}, pages={1357-1366}, doi={10.1088/0004-637X/698/2/1357}, archiveprefix={arXiv}, eprint={0904.1170}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2009ApJ...698.1357J}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Oetjens20, author={Oetjens, A. and Carone, L. and Bergemann, M. and Serenelli, A.}, title={The influence of planetary engulfment on stellar rotation in metal-poor main-sequence stars}, journal={\aap}, keywords={planet-star interactions, stars: rotation, stars: low-mass, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={643}, eid={A34}, pages={A34}, doi={10.1051/0004-6361/202038653}, archiveprefix={arXiv}, eprint={2009.03624}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2020A&A...643A..34O}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fleming19, author={Fleming, David P. and Barnes, Rory and Davenport, James R. A. and Luger, Rodrigo}, title={Rotation Period Evolution in Low-mass Binary Stars: The Impact of Tidal Torques and Magnetic Braking}, journal={\apj}, keywords={binaries: close, stars: evolution, stars: kinematics and dynamics, stars: rotation, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={881}, number={2}, eid={88}, pages={88}, doi={10.3847/1538-4357/ab2ed2}, archiveprefix={arXiv}, eprint={1903.05686}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJ...881...88F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Santos19, author={Santos, A. R. G. and Garcıa, R. A. and Mathur, S. and Bugnet, L. and van Saders, J. L. and Metcalfe, T. S. and Simonian, G. V. A. and Pinsonneault, M. H.}, title={Surface Rotation and Photometric Activity for Kepler Targets. I. M and K Main-sequence Stars}, journal={\apjs}, keywords={methods: data analysis, stars: activity, stars: low-mass, stars: rotation, starspots, techniques: photometric, Astrophysics - Solar and Stellar Astrophysics}, volume={244}, number={1}, eid={21}, pages={21}, doi={10.3847/1538-4365/ab3b56}, archiveprefix={arXiv}, eprint={1908.05222}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJS..244...21S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Baliunas97, author={Baliunas, Sallie L. and Henry, Gregory W. and Donahue, Robert A. and Fekel, Francis C. and Soon, Willie H.}, title={Properties of Sun-like Stars with Planets: $\rho$$^{1}$ Cancri, $\tau$ Bootis, and $\upsilon$ Andromedae}, journal={\apjl}, keywords={STARS: ACTIVITY, STARS: PLANETARY SYSTEMS, STARS: LATE-TYPE, TECHNIQUES: PHOTOMETRIC, TECHNIQUES: SPECTROSCOPIC, Stars: Planetary Systems, Stars: Activity, Stars: Late-Type, Techniques: Photometric-- Techniques: Spectroscopic}, volume={474}, number={2}, pages={L119-L122}, doi={10.1086/310442}, adsurl={https://ui.adsabs.harvard.edu/abs/1997ApJ...474L.119B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mengel16, author={Mengel, M. W. and Fares, R. and Marsden, S. C. and Carter, B. D. and Jeffers, S. V. and Petit, P. and Donati, J. -F. and Folsom, C. P. and BCool Collaboration}, title={The evolving magnetic topology of $\tau$ Bo}, journal={\mnras}, keywords={magnetic fields, techniques: polarimetric, stars: activity, stars: imaging, stars: individual: $\tau$ Boo, planetary systems, Astrophysics - Solar and Stellar Astrophysics}, volume={459}, number={4}, pages={4325-4342}, doi={10.1093/mnras/stw828}, archiveprefix={arXiv}, eprint={1604.02501}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2016MNRAS.459.4325M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mittag17, author={Mittag, M. and Robrade, J. and Schmitt, J. H. M. M. and Hempelmann, A. and González-Pérez, J. N. and Schröder, K. -P.}, title={Four-month chromospheric and coronal activity cycle in $\tau$ Bo}, journal={\aap}, keywords={stars: activity, stars: chromospheres, stars: late-type, stars: individual: $\tau$ Boo}, volume={600}, eid={A119}, pages={A119}, doi={10.1051/0004-6361/201629156}, adsurl={https://ui.adsabs.harvard.edu/abs/2017A&A...600A.119M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mittag19, author={Mittag, M. and Schmitt, J. H. M. M. and Hempelmann, A. and Schröder, K. -P.}, title={Discovery of short-term activity cycles in F-type stars}, journal={\aap}, keywords={stars: activity, stars: atmospheres, stars: chromospheres, stars: late-type}, volume={621}, eid={A136}, pages={A136}, doi={10.1051/0004-6361/201834319}, adsurl={https://ui.adsabs.harvard.edu/abs/2019A&A...621A.136M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Loutrel11, author={Loutrel, N. P. and Luhman, K. L. and Lowrance, P. J. and Bochanski, J. J.}, title={Discovery of a Companion at the L/T Transition with the Wide-field Infrared Survey Explorer}, journal={\apj}, keywords={binaries: visual, brown dwarfs, infrared: stars, proper motions, stars: individual: HD 46588 2MASS J06462756+7935045 WISEP J064627.10+793457.8, Astrophysics - Astrophysics of Galaxies}, volume={739}, number={2}, eid={81}, pages={81}, doi={10.1088/0004-637X/739/2/81}, archiveprefix={arXiv}, eprint={1107.1812}, primaryclass={astro-ph.GA}, adsurl={https://ui.adsabs.harvard.edu/abs/2011ApJ...739...81L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Seach22, author={Seach, J. M. and Marsden, S. C. and Carter, B. D. and Evensberget, D. and Folsom, C. P. and Neiner, C. and Mengel, M. W.}, title={The magnetic fields and stellar winds of the mature late F-stars: $\beta$ Virginis and $\theta$ Draconis}, journal={\mnras}, keywords={stars: magnetic field, stars: solar-type, stars: activity, stars: winds, outflows}, volume={509}, number={4}, pages={5117-5141}, doi={10.1093/mnras/stab3289}, adsurl={https://ui.adsabs.harvard.edu/abs/2022MNRAS.509.5117S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fulton17, author={Fulton, Benjamin J. and Petigura, Erik A. and Howard, Andrew W. and Isaacson, Howard and Marcy, Geoffrey W. and Cargile, Phillip A. and Hebb, Leslie and Weiss, Lauren M. and Johnson, John Asher and Morton, Timothy D. and Sinukoff, Evan and Crossfield, Ian J. M. and Hirsch, Lea A.}, title={The California-Kepler Survey. III. 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I. Method, formation tracks, and mass-distance distribution}, journal={\aap}, keywords={stars: planetary systems, stars: planetary systems: formation, stars: planetary systems: protoplanetary disks, planets and satellites: formation, solar system: formation, methods: numerical, Astrophysics - Earth and Planetary Astrophysics}, volume={501}, number={3}, pages={1139-1160}, doi={10.1051/0004-6361/200810301}, archiveprefix={arXiv}, eprint={0904.2524}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2009A&A...501.1139M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Batygin16, author={Batygin, Konstantin and Bodenheimer, Peter H. and Laughlin, Gregory P.}, title={In Situ Formation and Dynamical Evolution of Hot Jupiter Systems}, journal={\apj}, keywords={planets and satellites: dynamical evolution and stability, planets and satellites: formation, Astrophysics - Earth and Planetary Astrophysics}, volume={829}, number={2}, eid={114}, pages={114}, doi={10.3847/0004-637X/829/2/114}, archiveprefix={arXiv}, eprint={1511.09157}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2016ApJ...829..114B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mulders15, author={Mulders, Gijs D. and Pascucci, Ilaria and Apai, Dániel}, title={A Stellar-mass-dependent Drop in Planet Occurrence Rates}, journal={\apj}, keywords={planetary systems, planet-star interactions, planets and satellites: formation, protoplanetary disks, stars: low-mass, Astrophysics - Earth and Planetary Astrophysics}, volume={798}, number={2}, eid={112}, pages={112}, doi={10.1088/0004-637X/798/2/112}, archiveprefix={arXiv}, eprint={1406.7356}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ApJ...798..112M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Winn15, author={Winn, Joshua N. and Fabrycky, Daniel C.}, title={The Occurrence and Architecture of Exoplanetary Systems}, journal={\araa}, keywords={Astrophysics - Earth and Planetary Astrophysics}, volume={53}, pages={409-447}, doi={10.1146/annurev-astro-082214-122246}, archiveprefix={arXiv}, eprint={1410.4199}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ARA&A..53..409W}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Knutson14, author={Knutson, Heather A. and Fulton, Benjamin J. and Montet, Benjamin T. and Kao, Melodie and Ngo, Henry and Howard, Andrew W. and Crepp, Justin R. and Hinkley, Sasha and Bakos, Gaspar Á. and Batygin, Konstantin and Johnson, John Asher and Morton, Timothy D. and Muirhead, Philip S.}, title={Friends of Hot Jupiters. 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C.}, title={Orbital migration of the planetary companion of 51 Pegasi to its present location}, journal={\nat}, volume={380}, number={6575}, pages={606-607}, doi={10.1038/380606a0}, adsurl={https://ui.adsabs.harvard.edu/abs/1996Natur.380..606L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Pollack96, author={Pollack, James B. and Hubickyj, Olenka and Bodenheimer, Peter and Lissauer, Jack J. and Podolak, Morris and Greenzweig, Yuval}, title={Formation of the Giant Planets by Concurrent Accretion of Solids and Gas}, journal={\icarus}, volume={124}, number={1}, pages={62-85}, doi={10.1006/icar.1996.0190}, adsurl={https://ui.adsabs.harvard.edu/abs/1996Icar..124...62P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Boss97, author={Boss, A. 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P.}, title={Planet-Disk Interaction and Orbital Evolution}, journal={\araa}, keywords={Astrophysics - Earth and Planetary Astrophysics}, volume={50}, pages={211-249}, doi={10.1146/annurev-astro-081811-125523}, archiveprefix={arXiv}, eprint={1203.1184}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012ARA&A..50..211K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Rafikov06, author={Rafikov, Roman R.}, title={Atmospheres of Protoplanetary Cores: Critical Mass for Nucleated Instability}, journal={\apj}, keywords={Stars: Planetary Systems: Protoplanetary Disks, Planets and Satellites: Formation, Solar System: Formation, Astrophysics}, volume={648}, number={1}, pages={666-682}, doi={10.1086/505695}, archiveprefix={arXiv}, eprint={astro-ph/0405507}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2006ApJ...648..666R}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Howard10, author={Howard, Andrew W. and Marcy, Geoffrey W. and Johnson, John Asher and Fischer, Debra A. and Wright, Jason T. and Isaacson, Howard and Valenti, Jeff A. and Anderson, Jay and Lin, Doug N. C. and Ida, Shigeru}, title={The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters}, journal={Science}, keywords={ASTRONOMY, Astrophysics - Earth and Planetary Astrophysics}, volume={330}, number={6004}, pages={653}, doi={10.1126/science.1194854}, archiveprefix={arXiv}, eprint={1011.0143}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2010Sci...330..653H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Batalha13, author={Batalha, Natalie M. and Rowe, Jason F. and Bryson, Stephen T. and Barclay, Thomas and Burke, Christopher J. and Caldwell, Douglas A. and Christiansen, Jessie L. and Mullally, Fergal and Thompson, Susan E. and Brown, Timothy M. and Dupree, Andrea K. and Fabrycky, Daniel C. and Ford, Eric B. and Fortney, Jonathan J. and Gilliland, Ronald L. and Isaacson, Howard and Latham, David W. and Marcy, Geoffrey W. and Quinn, Samuel N. and Ragozzine, Darin and Shporer, Avi and Borucki, William J. and Ciardi, David R. and Gautier, Thomas N., III and Haas, Michael R. and Jenkins, Jon M. and Koch, David G. and Lissauer, Jack J. and Rapin, William and Basri, Gibor S. and Boss, Alan P. and Buchhave, Lars A. and Carter, Joshua A. and Charbonneau, David and Christensen-Dalsgaard, Joergen and Clarke, Bruce D. and Cochran, William D. and Demory, Brice-Olivier and Desert, Jean-Michel and Devore, Edna and Doyle, Laurance R. and Esquerdo, Gilbert A. and Everett, Mark and Fressin, Francois and Geary, John C. and Girouard, Forrest R. and Gould, Alan and Hall, Jennifer R. and Holman, Matthew J. and Howard, Andrew W. and Howell, Steve B. and Ibrahim, Khadeejah A. and Kinemuchi, Karen and Kjeldsen, Hans and Klaus, Todd C. and Li, Jie and Lucas, Philip W. and Meibom, Søren and Morris, Robert L. and Prša, Andrej and Quintana, Elisa and Sanderfer, Dwight T. and Sasselov, Dimitar and Seader, Shawn E. and Smith, Jeffrey C. and Steffen, Jason H. and Still, Martin and Stumpe, Martin C. and Tarter, Jill C. and Tenenbaum, Peter and Torres, Guillermo and Twicken, Joseph D. and Uddin, Kamal and Van Cleve, Jeffrey and Walkowicz, Lucianne and Welsh, William F.}, title={Planetary Candidates Observed by Kepler. III. Analysis of the First 16 Months of Data}, journal={\apjs}, keywords={catalogs, eclipses, planetary systems, space vehicles, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics}, volume={204}, number={2}, eid={24}, pages={24}, doi={10.1088/0067-0049/204/2/24}, archiveprefix={arXiv}, eprint={1202.5852}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2013ApJS..204...24B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Dressing13, author={Dressing, Courtney D. and Charbonneau, David}, title={The Occurrence Rate of Small Planets around Small Stars}, journal={\apj}, keywords={catalogs, methods: data analysis, planetary systems, stars: low-mass, surveys, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={767}, number={1}, eid={95}, pages={95}, doi={10.1088/0004-637X/767/1/95}, archiveprefix={arXiv}, eprint={1302.1647}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2013ApJ...767...95D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Petigura13, author={Petigura, Erik A. and Howard, Andrew W. and Marcy, Geoffrey W.}, title={Prevalence of Earth-size planets orbiting Sun-like stars}, journal={Proceedings of the National Academy of Science}, keywords={extrasolar planets, astrobiology, Astrophysics - Earth and Planetary Astrophysics}, volume={110}, number={48}, pages={19273-19278}, doi={10.1073/pnas.1319909110}, archiveprefix={arXiv}, eprint={1311.6806}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2013PNAS..11019273P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Becker15, author={Becker, Juliette C. and Vanderburg, Andrew and Adams, Fred C. and Rappaport, Saul A. and Schwengeler, Hans Martin}, title={WASP-47: A Hot Jupiter System with Two Additional Planets Discovered by K2}, journal={\apjl}, keywords={planets and satellites: detection, planets and satellites: dynamical evolution and stability, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics}, volume={812}, number={2}, eid={L18}, pages={L18}, doi={10.1088/2041-8205/812/2/L18}, archiveprefix={arXiv}, eprint={1508.02411}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ApJ...812L..18B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Canas19, author={Cañas, Caleb I. and Wang, Songhu and Mahadevan, Suvrath and Bender, Chad F. and De Lee, Nathan and Fleming, Scott W. and Garcıa-Hernández, D. A. and Hearty, Fred R. and Majewski, Steven R. and Roman-Lopes, Alexandre and Schneider, Donald P. and Stassun, Keivan G.}, title={Kepler-730: A Hot Jupiter System with a Close-in, Transiting, Earth-sized Planet}, journal={\apjl}, keywords={methods: statistical, planetary systems, techniques: photometric, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics}, volume={870}, number={2}, eid={L17}, pages={L17}, doi={10.3847/2041-8213/aafa1e}, archiveprefix={arXiv}, eprint={1812.08358}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJ...870L..17C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Huang2020, author={Huang, Chelsea X. and Quinn, Samuel N. and Vanderburg, Andrew and Becker, Juliette and Rodriguez, Joseph E. and Pozuelos, Francisco J. and Gandolfi, Davide and Zhou, George and Mann, Andrew W. and Collins, Karen A. and Crossfield, Ian and Barkaoui, Khalid and Collins, Kevin I. and Fridlund, Malcolm and Gillon, Michaël and Gonzales, Erica J. and Günther, Maximilian N. and Henry, Todd J. and Howell, Steve B. and James, Hodari-Sadiki and Jao, Wei-Chun and Jehin, Emmanuël and Jensen, Eric L. N. and Kane, Stephen R. and Lissauer, Jack J. and Matthews, Elisabeth and Matson, Rachel A. and Paredes, Leonardo A. and Schlieder, Joshua E. and Stassun, Keivan G. and Shporer, Avi and Sha, Lizhou and Tan, Thiam-Guan and Georgieva, Iskra and Mathur, Savita and Palle, Enric and Persson, Carina M. and Van Eylen, Vincent and Ricker, George R. and Vanderspek, Roland K. and Latham, David W. and Winn, Joshua N. and Seager, S. and Jenkins, Jon M. and Burke, Christopher J. and Goeke, Robert F. and Rinehart, Stephen and Rose, Mark E. and Ting, Eric B. and Torres, Guillermo and Wong, Ian}, title={TESS Spots a Hot Jupiter with an Inner Transiting Neptune}, journal={\apjl}, keywords={Exoplanet astronomy, Extrasolar gaseous giant planets, Extrasolar rocky planets, Exoplanets, Hot Jupiters, 486, 509, 511, 498, 753, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={892}, number={1}, eid={L7}, pages={L7}, doi={10.3847/2041-8213/ab7302}, archiveprefix={arXiv}, eprint={2003.10852}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2020ApJ...892L...7H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Korth23, author={Korth, J. and Gandolfi, D. and Šubjak, J. and Howard, S. and Ataiee, S. and Collins, K. A. and Quinn, S. N. and Mustill, A. J. and Guillot, T. and Lodieu, N. and Smith, A. M. S. and Esposito, M. and Rodler, F. and Muresan, A. and Abe, L. and Albrecht, S. H. and Alqasim, A. and Barkaoui, K. and Beck, P. G. and Burke, C. J. and Butler, R. P. and Conti, D. M. and Collins, K. I. and Crane, J. D. and Dai, F. and Deeg, H. J. and Evans, P. and Grziwa, S. and Hatzes, A. P. and Hirano, T. and Horne, K. and Huang, C. X. and Jenkins, J. M. and Kabáth, P. and Kielkopf, J. F. and Knudstrup, E. and Latham, D. W. and Livingston, J. and Luque, R. and Mathur, S. and Murgas, F. and Osborne, H. L. M. and Palle, E. and Persson, C. M. and Rodriguez, J. E. and Rose, M. and Rowden, P. and Schwarz, R. P. and Seager, S. and Serrano, L. M. and Sha, L. and Shectman, S. A. and Shporer, A. and Srdoc, G. and Stockdale, C. and Tan, T. -G. and Teske, J. K. and Van Eylen, V. and Vanderburg, A. and Vanderspek, R. and Wang, S. X. and Winn, J. N.}, title={TOI-1130: A photodynamical analysis of a hot Jupiter in resonance with an inner low-mass planet}, journal={\aap}, keywords={planetary systems, planets and satellites: individual: TOI-1130, techniques: photometric, techniques: radial velocities, Astrophysics - Earth and Planetary Astrophysics}, volume={675}, eid={A115}, pages={A115}, doi={10.1051/0004-6361/202244617}, archiveprefix={arXiv}, eprint={2305.15565}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023A&A...675A.115K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hord22, author={Hord, Benjamin J. and Colón, Knicole D. and Berger, Travis A. and Kostov, Veselin and Silverstein, Michele L. and Stassun, Keivan G. and Lissauer, Jack J. and Collins, Karen A. and Schwarz, Richard P. and Sefako, Ramotholo and Ziegler, Carl and Briceño, César and Law, Nicholas and Mann, Andrew W. and Ricker, George R. and Latham, David W. and Seager, S. and Winn, Joshua N. and Jenkins, Jon M. and Bouma, Luke G. and Falk, Ben and Torres, Guillermo and Twicken, Joseph D. and Vanderburg, Andrew}, title={The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 b}, journal={\aj}, keywords={Exoplanet astronomy, Exoplanet systems, Exoplanets, Hot Jupiters, Extrasolar gaseous planets, Transit photometry, 486, 484, 498, 753, 2172, 1709, Astrophysics - Earth and Planetary Astrophysics}, volume={164}, number={1}, eid={13}, pages={13}, doi={10.3847/1538-3881/ac6f57}, archiveprefix={arXiv}, eprint={2205.02501}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022AJ....164...13H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Sha23, author={Sha, Lizhou and Vanderburg, Andrew M. and Huang, Chelsea X. and Armstrong, David J. and Brahm, Rafael and Giacalone, Steven and Wood, Mackenna L. and Collins, Karen A. and Nielsen, Louise D. and Hobson, Melissa J. and Ziegler, Carl and Howell, Steve B. and Torres-Miranda, Pascal and Mann, Andrew W. and Zhou, George and Delgado-Mena, Elisa and Rojas, Felipe I. and Abe, Lyu and Trifonov, Trifon and Adibekyan, Vardan and Sousa, Sérgio G. and Fajardo-Acosta, Sergio B. and Guillot, Tristan and Howard, Saburo and Littlefield, Colin and Hawthorn, Faith and Schmider, François-Xavier and Eberhardt, Jan and Tan, Thiam-Guan and Osborn, Ares and Schwarz, Richard P. and Strøm, Paul and Jordán, Andrés and Wang, Gavin and Henning, Thomas and Massey, Bob and Law, Nicholas and Stockdale, Chris and Furlan, Elise and Srdoc, Gregor and Wheatley, Peter J. and Barrado Navascués, David and Lissauer, Jack J. and Stassun, Keivan G. and Ricker, George R. and Vanderspek, Roland K. and Latham, David W. and Winn, Joshua N. and Seager, Sara and Jenkins, Jon M. and Barclay, Thomas and Bouma, Luke G. and Christiansen, Jessie L. and Guerrero, Natalia and Rose, Mark E.}, title={TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system}, journal={\mnras}, keywords={techniques: photometric, techniques: radial velocities, planets and satellites: detection, planets and satellites: formation, planets and satellites: gaseous planets, stars: individual: TOI-2000 (TIC 371188886), Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={524}, number={1}, pages={1113-1138}, doi={10.1093/mnras/stad1666}, archiveprefix={arXiv}, eprint={2209.14396}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023MNRAS.524.1113S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hebrard20, author={Hébrard, G. and Dıaz, R. F. and Correia, A. C. M. and Collier Cameron, A. and Laskar, J. and Pollacco, D. and Almenara, J. -M. and Anderson, D. R. and Barros, S. C. C. and Boisse, I. and Bonomo, A. S. and Bouchy, F. and Boué, G. and Boumis, P. and Brown, D. J. A. and Dalal, S. and Deleuil, M. and Demangeon, O. D. S. and Doyle, A. P. and Haswell, C. A. and Hellier, C. and Osborn, H. and Kiefer, F. and Kolb, U. C. and Lam, K. and Lecavelier des Étangs, A. and Lopez, T. and Martin-Lagarde, M. and Maxted, P. and McCormac, J. and Nielsen, L. D. and Pallé, E. and Prieto-Arranz, J. and Queloz, D. and Santerne, A. and Smalley, B. and Turner, O. and Udry, S. and Verilhac, D. and West, R. and Wheatley, P. J. and Wilson, P. A.}, title={Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets}, journal={\aap}, keywords={planetary systems, techniques: radial velocities, techniques: photometric, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics}, volume={640}, eid={A32}, pages={A32}, doi={10.1051/0004-6361/202038296}, archiveprefix={arXiv}, eprint={2004.14645}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2020A&A...640A..32H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{Scott18, author={Scott, Nicholas J. and Howell, Steve B.}, title={NESSI and 'Alopeke: two new dual-channel speckle imaging instruments}, booktitle={Optical and Infrared Interferometry and Imaging VI}, editor={Creech-Eakman, Michelle J. and Tuthill, Peter G. and Mérand, Antoine}, series={Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series}, volume={10701}, eid={107010G}, pages={107010G}, doi={10.1117/12.2311539}, adsurl={https://ui.adsabs.harvard.edu/abs/2018SPIE10701E..0GS}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Howell11, author={Howell, Steve B. and Everett, Mark E. and Sherry, William and Horch, Elliott and Ciardi, David R.}, title={Speckle Camera Observations for the NASA Kepler Mission Follow-up Program}, journal={\aj}, keywords={instrumentation: high angular resolution, planets and satellites: general, techniques: photometric}, volume={142}, number={1}, eid={19}, pages={19}, doi={10.1088/0004-6256/142/1/19}, adsurl={https://ui.adsabs.harvard.edu/abs/2011AJ....142...19H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hayward01, author={Hayward, T. L. and Brandl, B. and Pirger, B. and Blacken, C. and Gull, G. E. and Schoenwald, J. and Houck, J. R.}, title={PHARO: A Near-Infrared Camera for the Palomar Adaptive Optics System}, journal={\pasp}, keywords={Instrumentation: Adaptive Optics}, volume={113}, number={779}, pages={105-118}, doi={10.1086/317969}, adsurl={https://ui.adsabs.harvard.edu/abs/2001PASP..113..105H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Rodrigues14, author={Rodrigues, Thaıse S. and Girardi, Léo and Miglio, Andrea and Bossini, Diego and Bovy, Jo and Epstein, Courtney and Pinsonneault, Marc H. and Stello, Dennis and Zasowski, Gail and Allende Prieto, Carlos and Chaplin, William J. and Hekker, Saskia and Johnson, Jennifer A. and Mészáros, Szabolcs and Mosser, Benoıt and Anders, Friedrich and Basu, Sarbani and Beers, Timothy C. and Chiappini, Cristina and da Costa, Luiz A. N. and Elsworth, Yvonne and Garcıa, Rafael A. and Garcıa Pérez, Ana E. and Hearty, Fred R. and Maia, Marcio A. 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A. and Piskunov, N.}, title={Spectroscopy made easy: A new tool for fitting observations with synthetic spectra.}, journal={\aaps}, keywords={RADIATIVE TRANSFER, METHODS: NUMERICAL, TECHNIQUES: SPECTROSCOPIC, STARS: FUNDAMENTAL PARAMETERS, SUN: FUNDAMENTAL PARAMETERS, ATOMIC DATA}, volume={118}, pages={595-603}, adsurl={https://ui.adsabs.harvard.edu/abs/1996A&AS..118..595V}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Piskunov17, author={Piskunov, Nikolai and Valenti, Jeff A.}, title={Spectroscopy Made Easy: Evolution}, journal={\aap}, keywords={stars: abundances, radiative transfer, stars: fundamental parameters, stars: atmospheres, techniques: spectroscopic, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={597}, eid={A16}, pages={A16}, doi={10.1051/0004-6361/201629124}, archiveprefix={arXiv}, eprint={1606.06073}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2017A&A...597A..16P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Gustafsson08, author={Gustafsson, B. and Edvardsson, B. and Eriksson, K. and Jørgensen, U. G. and Nordlund, Å. and Plez, B.}, title={A grid of MARCS model atmospheres for late-type stars. I. Methods and general properties}, journal={\aap}, keywords={stars: atmospheres, Sun: abundances, stars: fundamental parameters, stars: general, stars: late-type, stars: supergiants, Astrophysics}, volume={486}, number={3}, pages={951-970}, doi={10.1051/0004-6361:200809724}, archiveprefix={arXiv}, eprint={0805.0554}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2008A&A...486..951G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Heiter15, author={Heiter, U. and Lind, K. and Asplund, M. and Barklem, P. S. and Bergemann, M. and Magrini, L. and Masseron, T. and Mikolaitis, Š. and Pickering, J. C. and Ruffoni, M. P.}, title={Atomic and molecular data for optical stellar spectroscopy}, journal={\physscr}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={90}, number={5}, eid={054010}, pages={054010}, doi={10.1088/0031-8949/90/5/054010}, archiveprefix={arXiv}, eprint={1506.06697}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2015PhyS...90e4010H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{Markwardt09, author={Markwardt, C. B.}, title={Non-linear Least-squares Fitting in IDL with MPFIT}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics}, booktitle={Astronomical Data Analysis Software and Systems XVIII}, editor={Bohlender, D. A. and Durand, D. and Dowler, P.}, series={Astronomical Society of the Pacific Conference Series}, volume={411}, pages={251}, archiveprefix={arXiv}, eprint={0902.2850}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2009ASPC..411..251M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{DaSilva06, author={da Silva, L. and Girardi, L. and Pasquini, L. and Setiawan, J. and von der Lühe, O. and de Medeiros, J. R. and Hatzes, A. and Döllinger, M. P. and Weiss, A.}, title={Basic physical parameters of a selected sample of evolved stars}, journal={\aap}, keywords={stars: fundamental parameters, stars: evolution, stars: oscillations, Hertzsprung-Russell (HR) and C-M diagrams, stars: late-type, stars: luminosity function, mass function, Astrophysics}, volume={458}, number={2}, pages={609-623}, doi={10.1051/0004-6361:20065105}, archiveprefix={arXiv}, eprint={astro-ph/0608160}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2006A&A...458..609D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Pecaut13, author={Pecaut, Mark J. and Mamajek, Eric E.}, title={Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars}, journal={\apjs}, keywords={open clusters and associations: individual: $\eta$ Cha cluster TW Hydra Association $\beta$ Pic Moving Group Tucana-Horologium Association, stars: fundamental parameters, stars: pre-main sequence, Astrophysics - Solar and Stellar Astrophysics}, volume={208}, number={1}, eid={9}, pages={9}, doi={10.1088/0067-0049/208/1/9}, archiveprefix={arXiv}, eprint={1307.2657}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2013ApJS..208....9P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Yee17, author={Yee, Samuel W. and Petigura, Erik A. and von Braun, Kaspar}, title={Precision Stellar Characterization of FGKM Stars using an Empirical Spectral Library}, journal={\apj}, keywords={techniques: spectroscopic, Astrophysics - Solar and Stellar Astrophysics}, volume={836}, number={1}, eid={77}, pages={77}, doi={10.3847/1538-4357/836/1/77}, archiveprefix={arXiv}, eprint={1701.00922}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2017ApJ...836...77Y}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Deming15, author={Deming, Drake and Knutson, Heather and Kammer, Joshua and Fulton, Benjamin J. and Ingalls, James and Carey, Sean and Burrows, Adam and Fortney, Jonathan J. and Todorov, Kamen and Agol, Eric and Cowan, Nicolas and Desert, Jean-Michel and Fraine, Jonathan and Langton, Jonathan and Morley, Caroline and Showman, Adam P.}, title={Spitzer Secondary Eclipses of the Dense, Modestly-irradiated, Giant Exoplanet HAT-P-20b Using Pixel-level Decorrelation}, journal={\apj}, keywords={eclipses, infrared: planetary systems, planetary systems, planets and satellites: atmospheres, Astrophysics - Earth and Planetary Astrophysics}, volume={805}, number={2}, eid={132}, pages={132}, doi={10.1088/0004-637X/805/2/132}, archiveprefix={arXiv}, eprint={1411.7404}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015ApJ...805..132D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Barnes16, author={Barnes, Sydney A. and Weingrill, Joerg and Fritzewski, Dario and Strassmeier, Klaus G. and Platais, Imants}, title={Rotation Periods for Cool Stars in the 4 Gyr old Open Cluster M67, The Solar-Stellar Connection, and the Applicability of Gyrochronology to at least Solar Age}, journal={\apj}, keywords={open clusters and associations: individual: M67, NGC 2682, stars: activity, stars: evolution, stars: rotation, stars: solar-type, starspots, Astrophysics - Solar and Stellar Astrophysics}, volume={823}, number={1}, eid={16}, pages={16}, doi={10.3847/0004-637X/823/1/16}, archiveprefix={arXiv}, eprint={1603.09179}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2016ApJ...823...16B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Curtis20, author={Curtis, Jason Lee and Agüeros, Marcel A. and Matt, Sean P. and Covey, Kevin R. and Douglas, Stephanie T. and Angus, Ruth and Saar, Steven H. and Cody, Ann Marie and Vanderburg, Andrew and Law, Nicholas M. and Kraus, Adam L. and Latham, David W. and Baranec, Christoph and Riddle, Reed and Ziegler, Carl and Lund, Mikkel N. and Torres, Guillermo and Meibom, Søren and Aguirre, Victor Silva and Wright, Jason T.}, title={When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147}, journal={\apj}, keywords={Open star clusters, Stellar evolution, Stellar ages, Stellar rotation, 1160, 1599, 1581, 1629, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies}, volume={904}, number={2}, eid={140}, pages={140}, doi={10.3847/1538-4357/abbf58}, archiveprefix={arXiv}, eprint={2010.02272}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2020ApJ...904..140C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Trotta08, author={Trotta, Roberto}, title={Bayes in the sky: Bayesian inference and model selection in cosmology}, journal={Contemporary Physics}, keywords={Astrophysics}, volume={49}, number={2}, pages={71-104}, doi={10.1080/00107510802066753}, archiveprefix={arXiv}, eprint={0803.4089}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2008ConPh..49...71T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Lovis2007, author={Lovis, C. and Pepe, F.}, title={A new list of thorium and argon spectral lines in the visible}, journal={\aap}, keywords={atomic data, techniques: spectroscopic, atlases, catalogs, Astrophysics}, volume={468}, number={3}, pages={1115-1121}, doi={10.1051/0004-6361:20077249}, archiveprefix={arXiv}, eprint={astro-ph/0703412}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2007A&A...468.1115L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Zechmeister2018, author={Zechmeister, M. and Reiners, A. and Amado, P. J. and Azzaro, M. and Bauer, F. F. and Béjar, V. J. S. and Caballero, J. A. and Guenther, E. W. and Hagen, H. -J. and Jeffers, S. V. and Kaminski, A. and Kürster, M. and Launhardt, R. and Montes, D. and Morales, J. C. and Quirrenbach, A. and Reffert, S. and Ribas, I. and Seifert, W. and Tal-Or, L. and Wolthoff, V.}, title={Spectrum radial velocity analyser (SERVAL). High-precision radial velocities and two alternative spectral indicators}, journal={\aap}, keywords={methods: data analysis, techniques: radial velocities, techniques: spectroscopic, planets and satellites: detection, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={609}, eid={A12}, pages={A12}, doi={10.1051/0004-6361/201731483}, archiveprefix={arXiv}, eprint={1710.10114}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2018A&A...609A..12Z}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Tejada21, author={Tejada Arevalo, Roberto A. and Winn, Joshua N. and Anderson, Kassandra R.}, title={Further Evidence for Tidal Spin-up of Hot Jupiter Host Stars}, journal={\apj}, keywords={Tidal interaction, Stellar rotation, Hot Jupiters, Dynamical evolution, Stellar ages, Extrasolar gaseous giant planets, 1699, 1629, 753, 421, 1581, 509, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={919}, number={2}, eid={138}, pages={138}, doi={10.3847/1538-4357/ac1429}, archiveprefix={arXiv}, eprint={2107.05759}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021ApJ...919..138T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Benbakoura19, author={Benbakoura, M. and Réville, V. and Brun, A. S. and Le Poncin-Lafitte, C. and Mathis, S.}, title={Evolution of star-planet systems under magnetic braking and tidal interaction}, journal={\aap}, keywords={stars: evolution, stars: solar-type, stars: low-mass, stars: rotation, planet-star interactions, planetary systems, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={621}, eid={A124}, pages={A124}, doi={10.1051/0004-6361/201833314}, archiveprefix={arXiv}, eprint={1811.06354}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2019A&A...621A.124B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Zeng19, author={Zeng, Li and Jacobsen, Stein B. and Sasselov, Dimitar D. and Petaev, Michail I. and Vanderburg, Andrew and Lopez-Morales, Mercedes and Perez-Mercader, Juan and Mattsson, Thomas R. and Li, Gongjie and Heising, Matthew Z. and Bonomo, Aldo S. and Damasso, Mario and Berger, Travis A. and Cao, Hao and Levi, Amit and Wordsworth, Robin D.}, title={Growth model interpretation of planet size distribution}, journal={Proceedings of the National Academy of Science}, keywords={Astrophysics - Earth and Planetary Astrophysics, Physics - Geophysics}, volume={116}, number={20}, pages={9723-9728}, doi={10.1073/pnas.1812905116}, archiveprefix={arXiv}, eprint={1906.04253}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019PNAS..116.9723Z}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{cruzsaenz14, author={Cruz-Saenz de Miera, F. and Chavez, M. and Bertone, E. and Vega, O.}, title={Searching for infrared excesses in Sun-like stars observed by WISE}, journal={\mnras}, keywords={circumstellar matter, infrared: stars, Astrophysics - Solar and Stellar Astrophysics}, volume={437}, number={1}, pages={391-396}, doi={10.1093/mnras/stt1888}, archiveprefix={arXiv}, eprint={1310.2640}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2014MNRAS.437..391C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{siegler07, author={Siegler, Nick and Muzerolle, James and Young, Erick T. and Rieke, George H. and Mamajek, Eric E. and Trilling, David E. and Gorlova, Nadya and Su, Kate Y. L.}, title={Spitzer 24 $\mu$m Observations of Open Cluster IC 2391 and Debris Disk Evolution of FGK Stars}, journal={\apj}, keywords={Infrared: Stars, Galaxy: Open Clusters and Associations: Individual: Alphanumeric: IC 2391, Stars: Planetary Systems: Protoplanetary Disks, Astrophysics}, volume={654}, number={1}, pages={580-594}, doi={10.1086/509042}, archiveprefix={arXiv}, eprint={astro-ph/0609141}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2007ApJ...654..580S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{gaspar09, author={Gáspár, A. and Rieke, G. H. and Su, K. Y. L. and Balog, Z. and Trilling, D. and Muzzerole, J. and Apai, D. and Kelly, B. C.}, title={The Low Level of Debris Disk Activity at the Time of the Late Heavy Bombardment: A Spitzer Study of Praesepe}, journal={\apj}, keywords={circumstellar matter, infrared: stars, open clusters and associations: individual: Praesepe M44 NGC 2632 Beehive, planetary systems: formation, stars: evolution, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={697}, number={2}, pages={1578-1596}, doi={10.1088/0004-637X/697/2/1578}, archiveprefix={arXiv}, eprint={0903.4193}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2009ApJ...697.1578G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{mizuki24, author={Mizuki, Toshiyuki and Momose, Munetake and Aizawa, Masataka and Kobayashi, Hiroshi}, title={Frequencies of Warm Debris Disks Based on Point Source Catalogs of Spitzer, WISE, and Gaia}, journal={\aj}, keywords={Debris disks, Infrared excess, Spectral energy distribution, Catalogs, Main sequence stars, Space observatories, Gaia, 363, 788, 2129, 205, 1000, 1543, 2360, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={167}, number={6}, eid={275}, pages={275}, doi={10.3847/1538-3881/ad3df8}, archiveprefix={arXiv}, eprint={2404.03907}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2024AJ....167..275M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{greaves04, author={Greaves, J. S. and Wyatt, M. C. and Holland, W. S. and Dent, W. R. F.}, title={The debris disc around $\tau$ Ceti: a massive analogue to the Kuiper Belt}, journal={\mnras}, keywords={Kuiper Belt: circumstellar matter: planetary systems: formation: planetary systems: protoplanetary discs: infrared: stars}, volume={351}, number={3}, pages={L54-L58}, doi={10.1111/j.1365-2966.2004.07957.x}, adsurl={https://ui.adsabs.harvard.edu/abs/2004MNRAS.351L..54G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{wyatt08, author={Wyatt, M. C.}, title={Evolution of debris disks.}, journal={\araa}, volume={46}, pages={339-383}, doi={10.1146/annurev.astro.45.051806.110525}, adsurl={https://ui.adsabs.harvard.edu/abs/2008ARA&A..46..339W}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{mustillwyatt09, author={Mustill, Alexander J. and Wyatt, Mark C.}, title={Debris disc stirring by secular perturbations from giant planets}, journal={\mnras}, keywords={circumstellar matter, planetary systems: formation, stars: individual: ɛ Eridani, stars: individual: Fomalhaut, planetary systems: protoplanetary discs, Astrophysics - Earth and Planetary Astrophysics}, volume={399}, number={3}, pages={1403-1414}, doi={10.1111/j.1365-2966.2009.15360.x}, archiveprefix={arXiv}, eprint={0907.1389}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2009MNRAS.399.1403M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Trilling08, author={Trilling, D. E. and Bryden, G. and Beichman, C. A. and Rieke, G. H. and Su, K. Y. L. and Stansberry, J. A. and Blaylock, M. and Stapelfeldt, K. R. and Beeman, J. W. and Haller, E. E.}, title={Debris Disks around Sun-like Stars}, journal={\apj}, keywords={circumstellar matter, infrared: stars, planetary systems: formation, Astrophysics}, volume={674}, number={2}, pages={1086-1105}, doi={10.1086/525514}, archiveprefix={arXiv}, eprint={0710.5498}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2008ApJ...674.1086T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Poon21, author={Poon, Sanson T. S. and Nelson, Richard P. and Coleman, Gavin A. L.}, title={In situ formation of hot Jupiters with companion super-Earths}, journal={\mnras}, keywords={planets and satellites: composition, planets and satellites: dynamical evolution and stability, planets and satellites: formation, planets and satellites: gaseous planets, planets and satellites: terrestrial planets, planet-disc interactions, Astrophysics - Earth and Planetary Astrophysics}, volume={505}, number={2}, pages={2500-2516}, doi={10.1093/mnras/stab1466}, archiveprefix={arXiv}, eprint={2105.08553}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021MNRAS.505.2500P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hasegawa19, author={Hasegawa, Yasuhiro and Yu, Tze Yeung Mathew and Hansen, Bradley M. S.}, title={Close-in giant-planet formation via in-situ gas accretion and their natal disk properties}, journal={\aap}, keywords={accretion, accretion disks, magnetic fields, turbulence, protoplanetary disks, planets and satellites: formation, planets and satellites: gaseous planets, Astrophysics - Earth and Planetary Astrophysics}, volume={629}, eid={L1}, pages={L1}, doi={10.1051/0004-6361/201936138}, archiveprefix={arXiv}, eprint={1908.00647}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019A&A...629L...1H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Ahuir21, author={Ahuir, J. and Strugarek, A. and Brun, A. -S. and Mathis, S.}, title={Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population}, journal={\aap}, keywords={planet-star interactions, stars: evolution, stars: solar-type, stars: rotation, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={650}, eid={A126}, pages={A126}, doi={10.1051/0004-6361/202040173}, archiveprefix={arXiv}, eprint={2104.01004}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021A&A...650A.126A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Jenkins02, author={Jenkins, Jon M.}, title={The Impact of Solar-like Variability on the Detectability of Transiting Terrestrial Planets}, journal={\apj}, keywords={Methods: Data Analysis, Stars: Planetary Systems, Techniques: Photometric}, volume={575}, number={1}, pages={493-505}, doi={10.1086/341136}, adsurl={https://ui.adsabs.harvard.edu/abs/2002ApJ...575..493J}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{Jenkins10, author={Jenkins, Jon M. and Chandrasekaran, Hema and McCauliff, Sean D. and Caldwell, Douglas A. and Tenenbaum, Peter and Li, Jie and Klaus, Todd C. and Cote, Miles T. and Middour, Christopher}, title={Transiting planet search in the Kepler pipeline}, booktitle={Software and Cyberinfrastructure for Astronomy}, editor={Radziwill, Nicole M. and Bridger, Alan}, series={Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series}, volume={7740}, eid={77400D}, pages={77400D}, doi={10.1117/12.856764}, adsurl={https://ui.adsabs.harvard.edu/abs/2010SPIE.7740E..0DJ}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@misc{Jenkins20, author={Jenkins, Jon M. and Tenenbaum, Peter and Seader, Shawn and Burke, Christopher J. and McCauliff, Sean D. and Smith, Jeffrey C. and Twicken, Joseph D. and Chandrasekaran, Hema}, title={Kepler Data Processing Handbook: Transiting Planet Search}, keywords={Kepler}, howpublished={Kepler Science Document KSCI-19081-003, id. 9. Edited by Jon M. Jenkins.}, eid={9}, pages={9}, adsurl={https://ui.adsabs.harvard.edu/abs/2020ksci.rept....9J}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Li19, author={Li, Jie and Tenenbaum, Peter and Twicken, Joseph D. and Burke, Christopher J. and Jenkins, Jon M. and Quintana, Elisa V. and Rowe, Jason F. and Seader, Shawn E.}, title={Kepler Data Validation II-Transit Model Fitting and Multiple-planet Search}, journal={\pasp}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={131}, number={996}, pages={024506}, doi={10.1088/1538-3873/aaf44d}, archiveprefix={arXiv}, eprint={1812.00103}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2019PASP..131b4506L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Dungee22, author={Dungee, Ryan and van Saders, Jennifer and Gaidos, Eric and Chun, Mark and Garcıa, Rafael A. and Magnier, Eugene A. and Mathur, Savita and Santos, Ângela R. G.}, title={A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67}, journal={\apj}, keywords={Open star clusters, Stellar evolution, Stellar ages, Stellar rotation, 1160, 1599, 1581, 1629, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies}, volume={938}, number={2}, eid={118}, pages={118}, doi={10.3847/1538-4357/ac90be}, archiveprefix={arXiv}, eprint={2211.01377}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2022ApJ...938..118D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Brown:2013, author={Brown, T. M. and Baliber, N. and Bianco, F. B. and Bowman, M. and Burleson, B. and Conway, P. and Crellin, M. and Depagne, É. and De Vera, J. and Dilday, B. and Dragomir, D. and Dubberley, M. and Eastman, J. D. and Elphick, M. and Falarski, M. and Foale, S. and Ford, M. and Fulton, B. J. and Garza, J. and Gomez, E. L. and Graham, M. and Greene, R. and Haldeman, B. and Hawkins, E. and Haworth, B. and Haynes, R. and Hidas, M. and Hjelstrom, A. E. and Howell, D. A. and Hygelund, J. and Lister, T. A. and Lobdill, R. and Martinez, J. and Mullins, D. S. and Norbury, M. and Parrent, J. and Paulson, R. and Petry, D. L. and Pickles, A. and Posner, V. and Rosing, W. E. and Ross, R. and Sand, D. J. and Saunders, E. S. and Shobbrook, J. and Shporer, A. and Street, R. A. and Thomas, D. and Tsapras, Y. and Tufts, J. R. and Valenti, S. and Vander Horst, K. and Walker, Z. and White, G. and Willis, M.}, title={Las Cumbres Observatory Global Telescope Network}, journal={\pasp}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics}, volume={125}, number={931}, pages={1031}, doi={10.1086/673168}, archiveprefix={arXiv}, eprint={1305.2437}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2013PASP..125.1031B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@misc{Jensen:2013, author={Jensen, E.}, title={Tapir: A web interface for transit/eclipse observability}, howpublished={Astrophysics Source Code Library}, archiveprefix={ascl}, eprint={1306.007}, adsurl={http://adsabs.harvard.edu/abs/2013ascl.soft06007J}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Collins:2017, author={Collins, K. A. and Kielkopf, J. F. and Stassun, K. G. and Hessman, F. V.}, title={AstroImageJ: Image Processing and Photometric Extraction for Ultra-precise Astronomical Light Curves}, journal={\aj}, archiveprefix={arXiv}, eprint={1601.02622}, primaryclass={astro-ph.IM}, keywords={methods: data analysis, techniques: image processing, techniques: photometric}, eid={77}, pages={77}, doi={10.3847/1538-3881/153/2/77}, adsurl={http://adsabs.harvard.edu/abs/2017AJ....153...77C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{McCully:2018, author={McCully, Curtis and Volgenau, Nikolaus H. and Harbeck, Daniel-Rolf and Lister, Tim A. and Saunders, Eric S. and Turner, Monica L. and Siiverd, Robert J. and Bowman, Mark}, title={Real-time processing of the imaging data from the network of Las Cumbres Observatory Telescopes using BANZAI}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics}, booktitle={\procspie}, year={2018}, series={Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series}, volume={10707}, month={Jul}, eid={107070K}, pages={107070K}, doi={10.1117/12.2314340}, archiveprefix={arXiv}, eprint={1811.04163}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2018SPIE10707E..0KM}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hedges21, author={Hedges, Christina and Hughes, Alex and Zhou, George and David, Trevor J. and Becker, Juliette and Giacalone, Steven and Vanderburg, Andrew and Rodriguez, Joseph E. and Bieryla, Allyson and Wirth, Christopher and Atherton, Shaun and Fetherolf, Tara and Collins, Karen A. and Price-Whelan, Adrian M. and Bedell, Megan and Quinn, Samuel N. and Gan, Tianjun and Ricker, George R. and Latham, David W. and Vanderspek, Roland K. and Seager, Sara and Winn, Joshua N. and Jenkins, Jon M. and Kielkopf, John F. and Schwarz, Richard P. and Dressing, Courtney D. and Gonzales, Erica J. and Crossfield, Ian J. M. and Matthews, Elisabeth C. and Jensen, Eric L. N. and Furlan, Elise and Gnilka, Crystal L. and Howell, Steve B. and Lester, Kathryn V. and Scott, Nicholas J. and Feliz, Dax L. and Lund, Michael B. and Siverd, Robert J. and Stevens, Daniel J. and Narita, N. and Fukui, A. and Murgas, F. and Palle, Enric and Sutton, Phil J. and Stassun, Keivan G. and Bouma, Luke G. and Vezie, Michael and Villaseñor, Jesus Noel and Quintana, Elisa V. and Smith, Jeffrey C.}, title={TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up}, journal={\aj}, keywords={Exoplanets, Transits, Time series analysis, 498, 1711, 1916, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={162}, number={2}, eid={54}, pages={54}, doi={10.3847/1538-3881/ac06cd}, archiveprefix={arXiv}, eprint={2111.01311}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021AJ....162...54H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Ricker15, author={Ricker, George R. and Winn, Joshua N. and Vanderspek, Roland and Latham, David W. and Bakos, Gáspár Á. and Bean, Jacob L. and Berta-Thompson, Zachory K. and Brown, Timothy M. and Buchhave, Lars and Butler, Nathaniel R. and Butler, R. Paul and Chaplin, William J. and Charbonneau, David and Christensen-Dalsgaard, Jørgen and Clampin, Mark and Deming, Drake and Doty, John and De Lee, Nathan and Dressing, Courtney and Dunham, Edward W. and Endl, Michael and Fressin, Francois and Ge, Jian and Henning, Thomas and Holman, Matthew J. and Howard, Andrew W. and Ida, Shigeru and Jenkins, Jon M. and Jernigan, Garrett and Johnson, John Asher and Kaltenegger, Lisa and Kawai, Nobuyuki and Kjeldsen, Hans and Laughlin, Gregory and Levine, Alan M. and Lin, Douglas and Lissauer, Jack J. and MacQueen, Phillip and Marcy, Geoffrey and McCullough, Peter R. and Morton, Timothy D. and Narita, Norio and Paegert, Martin and Palle, Enric and Pepe, Francesco and Pepper, Joshua and Quirrenbach, Andreas and Rinehart, Stephen A. and Sasselov, Dimitar and Sato, Bun'ei and Seager, Sara and Sozzetti, Alessandro and Stassun, Keivan G. and Sullivan, Peter and Szentgyorgyi, Andrew and Torres, Guillermo and Udry, Stephane and Villasenor, Joel}, title={Transiting Exoplanet Survey Satellite (TESS)}, journal={Journal of Astronomical Telescopes, Instruments, and Systems}, volume={1}, eid={014003}, pages={014003}, doi={10.1117/1.JATIS.1.1.014003}, adsurl={https://ui.adsabs.harvard.edu/abs/2015JATIS...1a4003R}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Barros17, author={Barros, S. C. C. and Gosselin, H. and Lillo-Box, J. and Bayliss, D. and Delgado Mena, E. and Brugger, B. and Santerne, A. and Armstrong, D. J. and Adibekyan, V. and Armstrong, J. D. and Barrado, D. and Bento, J. and Boisse, I. and Bonomo, A. S. and Bouchy, F. and Brown, D. J. A. and Cochran, W. D. and Collier Cameron, A. and Deleuil, M. and Demangeon, O. and Dıaz, R. F. and Doyle, A. and Dumusque, X. and Ehrenreich, D. and Espinoza, N. and Faedi, F. and Faria, J. P. and Figueira, P. and Foxell, E. and Hébrard, G. and Hojjatpanah, S. and Jackman, J. and Lendl, M. and Ligi, R. and Lovis, C. and Melo, C. and Mousis, O. and Neal, J. J. and Osborn, H. P. and Pollacco, D. and Santos, N. C. and Sefako, R. and Shporer, A. and Sousa, S. G. and Triaud, A. H. M. J. and Udry, S. and Vigan, A. and Wyttenbach, A.}, title={Precise masses for the transiting planetary system HD 106315 with HARPS}, journal={\aap}, keywords={planets and satellites: detection, planets and satellites: fundamental parameters, planets and satellites: composition, stars: individual: HD 106315, techniques: radial velocities, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics}, volume={608}, eid={A25}, pages={A25}, doi={10.1051/0004-6361/201731276}, archiveprefix={arXiv}, eprint={1709.00865}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2017A&A...608A..25B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{celerite2, author={Foreman-Mackey, D.}, title={Scalable Backpropagation for Gaussian Processes using Celerite}, journal={Research Notes of the American Astronomical Society}, pages={31}, doi={10.3847/2515-5172/aaaf6c}, adsurl={http://adsabs.harvard.edu/abs/2018RNAAS...2a..31F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Gillen20, author={Gillen, Edward and Briegal, Joshua T. and Hodgkin, Simon T. and Foreman-Mackey, Daniel and Van Leeuwen, Floor and Jackman, James A. G. and McCormac, James and West, Richard G. and Queloz, Didier and Bayliss, Daniel and Goad, Michael R. and Watson, Christopher A. and Wheatley, Peter J. and Belardi, Claudia and Burleigh, Matthew R. and Casewell, Sarah L. and Jenkins, James S. and Raynard, Liam and Smith, Alexis M. S. and Tilbrook, Rosanna H. and Vines, Jose I.}, title={NGTS clusters survey - I. Rotation in the young benchmark open cluster Blanco 1}, journal={\mnras}, keywords={stars: rotation, stars: variables: general, binaries: general, open clusters and associations: individual: Blanco 1, Astrophysics - Solar and Stellar Astrophysics}, volume={492}, number={1}, pages={1008-1024}, doi={10.1093/mnras/stz3251}, archiveprefix={arXiv}, eprint={1911.09705}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2020MNRAS.492.1008G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{David2019, author={David, Trevor J. and Petigura, Erik A. and Luger, Rodrigo and Foreman-Mackey, Daniel and Livingston, John H. and Mamajek, Eric E. and Hillenbrand, Lynne A.}, title={Four Newborn Planets Transiting the Young Solar Analog V1298 Tau}, journal={\apjl}, keywords={Exoplanets, Exoplanet astronomy, Exoplanet evolution, Transit photometry, Planetary system formation, Weak-line T Tauri stars, Young star clusters, 498, 486, 491, 1709, 1257, 1795, 1833, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={885}, number={1}, eid={L12}, pages={L12}, doi={10.3847/2041-8213/ab4c99}, archiveprefix={arXiv}, eprint={1910.04563}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJ...885L..12D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Lovis11, author={Lovis, C. and Dumusque, X. and Santos, N. C. and Bouchy, F. and Mayor, M. and Pepe, F. and Queloz, D. and Ségransan, D. and Udry, S.}, title={The HARPS search for southern extra-solar planets. XXXI. Magnetic activity cycles in solar-type stars: statistics and impact on precise radial velocities}, journal={arXiv e-prints}, keywords={Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, eid={arXiv:1107.5325}, pages={arXiv:1107.5325}, doi={10.48550/arXiv.1107.5325}, archiveprefix={arXiv}, eprint={1107.5325}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2011arXiv1107.5325L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Mascareno15, author={Suárez Mascareño, A. and Rebolo, R. and González Hernández, J. I. and Esposito, M.}, title={Rotation periods of late-type dwarf stars from time series high-resolution spectroscopy of chromospheric indicators}, journal={\mnras}, keywords={stars: activity, stars: chromospheres, planetary systems, stars: rotation, starspots, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={452}, number={3}, pages={2745-2756}, doi={10.1093/mnras/stv1441}, archiveprefix={arXiv}, eprint={1506.08039}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015MNRAS.452.2745S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Panichi_Gozdziewski_Turchetti-2017MNRAS.468..469P, author={Panichi, Federico and Goździewski, Krzyszof and Turchetti, Giorgio}, title={The reversibility error method (REM): a new, dynamical fast indicator for planetary dynamics}, journal={\mnras}, keywords={methods: numerical, celestial mechanics, stars: individual: Kepler-26, stars: individual: Kepler-29, stars: individual: Kepler-36, planetary systems, Astrophysics - Earth and Planetary Astrophysics}, volume={468}, number={1}, pages={469-491}, doi={10.1093/mnras/stx374}, archiveprefix={arXiv}, eprint={1703.10596}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2017MNRAS.468..469P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Rein_Liu-2012A&A...537A.128R, author={Rein, H. and Liu, S. -F.}, title={REBOUND: an open-source multi-purpose N-body code for collisional dynamics}, journal={\aap}, keywords={methods: numerical, planets and satellites: rings, protoplanetary disks, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Mathematics - Dynamical Systems, Physics - Computational Physics}, volume={537}, eid={A128}, pages={A128}, doi={10.1051/0004-6361/201118085}, archiveprefix={arXiv}, eprint={1110.4876}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012A&A...537A.128R}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Rein_Spiegel-2015MNRAS.446.1424R, author={Rein, Hanno and Spiegel, David S.}, title={IAS15: a fast, adaptive, high-order integrator for gravitational dynamics, accurate to machine precision over a billion orbits}, journal={\mnras}, keywords={gravitation, methods: numerical, planets and satellites: dynamical evolution and stability, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics, Mathematics - Numerical Analysis}, volume={446}, number={2}, pages={1424-1437}, doi={10.1093/mnras/stu2164}, archiveprefix={arXiv}, eprint={1409.4779}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2015MNRAS.446.1424R}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Raymond-2008ApJ...687L.107R, author={Raymond, Sean N. and Barnes, Rory and Armitage, Philip J. and Gorelick, Noel}, title={Mean Motion Resonances from Planet-Planet Scattering}, journal={\apjl}, keywords={planetary systems: formation, methods: N-body simulations, Astrophysics}, volume={687}, number={2}, pages={L107}, doi={10.1086/593301}, archiveprefix={arXiv}, eprint={0809.3449}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2008ApJ...687L.107R}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Naoz2013, author={Naoz, Smadar and Farr, Will M. and Lithwick, Yoram and Rasio, Frederic A. and Teyssandier, Jean}, title={Secular dynamics in hierarchical three-body systems}, journal={\mnras}, keywords={minor planets, asteroids: general, planets and satellites: dynamical evolution and stability, binaries: close, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={431}, number={3}, pages={2155-2171}, doi={10.1093/mnras/stt302}, archiveprefix={arXiv}, eprint={1107.2414}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2013MNRAS.431.2155N}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{Nobili1986, author={Nobili, Anna and Roxburgh, Ian W.}, title={Simulation of General Relativistic Corrections in Longterm Numerical Integrations of Planetary Orbits}, keywords={Celestial Mechanics, Computational Astrophysics, Numerical Integration, Orbital Mechanics, Planetary Orbits, Relativistic Effects, Gravitational Effects, Newton Theory, Orbit Perturbation, Planet Ephemerides, Astrophysics}, booktitle={Relativity in Celestial Mechanics and Astrometry. High Precision Dynamical Theories and Observational Verifications}, editor={Kovalevsky, Jean and Brumberg, V. A.}, series={IAU Symposium}, volume={114}, pages={105}, adsurl={https://ui.adsabs.harvard.edu/abs/1986IAUS..114..105N}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@book{Shevchenko2017, author={Shevchenko, Ivan I.}, title={The Lidov-Kozai Effect - Applications in Exoplanet Research and Dynamical Astronomy}, publisher={Springer}, volume={441}, doi={10.1007/978-3-319-43522-0}, adsurl={https://ui.adsabs.harvard.edu/abs/2017ASSL..441.....S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@inproceedings{2024tsc3.confE..17R, author={Rapetti, David and Jenkins, Jon and Twicken, Joseph and Caldwell, Douglas}, title={Comparing and Automatically Optimizing the Performance of Systematic Error Correctors for TESS Light Curves}, keywords={Data Analysis Techniques, Exoplanets, TESS mission, Systematic Error Corrections, Corrected Light Curves, Zenodo community tsc3}, booktitle={TESS Science Conference III}, eid={17}, pages={17}, doi={10.5281/zenodo.13756103}, adsurl={https://ui.adsabs.harvard.edu/abs/2024tsc3.confE..17R}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@unpublished{rapetti, author={Rapetti, David and others}, year={in prep.} }@article{Castro-Gonzalez24, title={TOI-5005 b: A super-Neptune in the savanna near the ridge}, author={Castro-González, A and Lillo-Box, J and Armstrong, DJ and Acuña, L and Aguichine, A and Bourrier, V and Gandhi, S and Sousa, SG and Delgado-Mena, E and Moya, A and others}, journal={Astronomy & Astrophysics}, volume={691}, pages={A233}, year={2024}, publisher={EDP Sciences} }@software{Bell22, author={Bell, Keaton J. and Higgins, Michael E.}, title={TESS_PRF: Display the TESS pixel response function}, howpublished={Astrophysics Source Code Library, record ascl:2207.008}, eid={ascl:2207.008}, adsurl={https://ui.adsabs.harvard.edu/abs/2022ascl.soft07008B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Baraffe2002, author={Baraffe, I. and Chabrier, G. and Allard, F. and Hauschildt, P. H.}, title={Evolutionary models for low-mass stars and brown dwarfs: Uncertainties and limits at very young ages}, journal={\aap}, eprint={astro-ph/0111385}, keywords={STARS: LOW-MASS, BROWN DWARFS, STARS: EVOLUTION, STARS: PRE-MAIN SEQUENCE}, pages={563-572}, doi={10.1051/0004-6361:20011638}, adsurl={https://ui.adsabs.harvard.edu/abs/2002A%26A...382..563B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Spiegel2011, author={Spiegel, D. S. and Burrows, A. and Milsom, J. A.}, title={The Deuterium-burning Mass Limit for Brown Dwarfs and Giant Planets}, journal={\apj}, archiveprefix={arXiv}, eprint={1008.5150}, primaryclass={astro-ph.EP}, keywords={brown dwarfs, radiative transfer, stars: low-mass, stars: evolution}, eid={57}, pages={57}, doi={10.1088/0004-637X/727/1/57}, adsurl={https://ui.adsabs.harvard.edu/abs/2011ApJ...727...57S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Persson2019, author={Persson, Carina M. and Csizmadia, Szilárd and Mustill, Alexander J. and Fridlund, Malcolm and Hatzes, Artie P. and Nowak, Grzegorz and Georgieva, Iskra and Gandolfi, Davide and Davies, Melvyn B. and Livingston, John H. and Palle, Enric and Montañes Rodrıguez, Pilar and Endl, Michael and Hirano, Teruyuki and Prieto-Arranz, Jorge and Korth, Judith and Grziwa, Sascha and Esposito, Massimiliano and Albrecht, Simon and Johnson, Marshall C. and Barragán, Oscar and Parviainen, Hannu and Van Eylen, Vincent and Alonso Sobrino, Roi and Beck, Paul G. and Cabrera, Juan and Carleo, Ilaria and Cochran, William D. and Dai, Fei and Deeg, Hans J. and de Leon, Jerome P. and Eigmüller, Philipp and Erikson, Anders and Fukui, Akai and González-Cuesta, Lucıa and Guenther, Eike W. and Hidalgo, Diego and Hjorth, Maria and Kabath, Petr and Knudstrup, Emil and Kusakabe, Nobuhiko and Lam, Kristine W. F. and Lund, Mikkel N. and Luque, Rafael and Mathur, Savita and Murgas, Felipe and Narita, Norio and Nespral, David and Niraula, Prajwal and Olofsson, A. O. Henrik and Pätzold, Martin and Rauer, Heike and Redfield, Seth and Ribas, Ignasi and Skarka, Marek and Smith, Alexis M. S. and Subjak, Jan and Tamura, Motohide}, title={Greening of the brown-dwarf desert. EPIC 212036875b: a 51 M$_{J}$ object in a 5-day orbit around an F7 V star}, journal={\aap}, keywords={planetary systems, stars: fundamental parameters, stars: individual: EPIC 212036875, techniques: photometric, techniques: radial velocities, Astrophysics - Earth and Planetary Astrophysics}, volume={628}, eid={A64}, pages={A64}, doi={10.1051/0004-6361/201935505}, archiveprefix={arXiv}, eprint={1906.05048}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2019A&A...628A..64P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Subjak2020, author={Šubjak, Ján and Sharma, Rishikesh and Carmichael, Theron W. and Johnson, Marshall C. and Gonzales, Erica J. and Matthews, Elisabeth and Boffin, Henri M. J. and Brahm, Rafael and Chaturvedi, Priyanka and Chakraborty, Abhijit and Ciardi, David R. and Collins, Karen A. and Esposito, Massimiliano and Fridlund, Malcolm and Gan, Tianjun and Gandolfi, Davide and Garcıa, Rafael A. and Guenther, Eike and Hatzes, Artie and Latham, David W. and Mathis, Stéphane and Mathur, Savita and Persson, Carina M. and Relles, Howard M. and Schlieder, Joshua E. and Barclay, Thomas and Dressing, Courtney D. and Crossfield, Ian and Howard, Andrew W. and Rodler, Florian and Zhou, George and Quinn, Samuel N. and Esquerdo, Gilbert A. and Calkins, Michael L. and Berlind, Perry and Stassun, Keivan G. and Blažek, Martin and Skarka, Marek and Špoková, Magdalena and Žák, Jiřı and Albrecht, Simon and Sobrino, Roi Alonso and Beck, Paul and Cabrera, Juan and Carleo, Ilaria and Cochran, William D. and Csizmadia, Szilard and Dai, Fei and Deeg, Hans J. and de Leon, Jerome P. and Eigmüller, Philipp and Endl, Michael and Erikson, Anders and Fukui, Akihiko and Georgieva, Iskra and González-Cuesta, Lucıa and Grziwa, Sascha and Hidalgo, Diego and Hirano, Teruyuki and Hjorth, Maria and Knudstrup, Emil and Korth, Judith and Lam, Kristine W. F. and Livingston, John H. and Lund, Mikkel N. and Luque, Rafael and Montanes Rodrıguez, Pilar and Murgas, Felipe and Narita, Norio and Nespral, David and Niraula, Prajwal and Nowak, Grzegorz and Pallé, Enric and Pätzold, Martin and Prieto-Arranz, Jorge and Rauer, Heike and Redfield, Seth and Ribas, Ignasi and Smith, Alexis M. S. and Van Eylen, Vincent and Kabáth, Petr}, title={TOI-503: The First Known Brown-dwarf Am-star Binary from the TESS Mission}, journal={\aj}, keywords={Brown dwarfs, Stellar ages, Am stars, Spectroscopy, Transit photometry, Radial velocity, Stellar rotation, Stellar astronomy, 185, 1581, 33, 1558, 1709, 1332, 1629, 1583, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={159}, number={4}, eid={151}, pages={151}, doi={10.3847/1538-3881/ab7245}, archiveprefix={arXiv}, eprint={1909.07984}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2020AJ....159..151S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Carmichael2022, author={Carmichael, Theron W. and Irwin, Jonathan M. and Murgas, Felipe and Pallé, Enric and Stassun, Keivan G. and Bartnik, Matthew and Collins, Karen A. and de Leon, Jerome and Esparza-Borges, Emma and Fedewa, Jeremy and Fong, William and Fukui, Akihiko and Jenkins, Jon M. and Kagetani, Taiki and Latham, David W. and Lund, Michael B. and Mann, Andrew W. and Moldovan, Dan and Morgan, Edward H. and Narita, Norio and Painter, Shane and Parviainen, Hannu and Quintana, Elisa V. and Ricker, George R. and Schulte, Jack and Schwarz, Richard P. and Seager, Sara and Sokolovsky, Kirill and Twicken, Joseph D. and Winn, Joshua N.}, title={TOI-2119: a transiting brown dwarf orbiting an active M-dwarf from NASA's TESS mission}, journal={\mnras}, keywords={techniques: photometric, techniques: radial velocities, techniques: spectroscopic, (stars:) brown dwarfs, stars: low-mass, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={514}, number={4}, pages={4944-4957}, doi={10.1093/mnras/stac1666}, archiveprefix={arXiv}, eprint={2202.08842}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2022MNRAS.514.4944C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Vowell2025, author={Vowell, Noah and Dong, Jiayin and Rodriguez, Joseph E. and Bieryla, Allyson and Zhou, George and Carmichael, Theron W. and Giacalone, Steven and Crane, Jeffrey D. and Shectman, Stephen A. and Teske, Johanna}, title={The OATMEAL Survey. III. An Aligned Transiting Warm Brown Dwarf and Evidence for Quiescent Brown Dwarf Migration}, journal={arXiv e-prints}, keywords={Earth and Planetary Astrophysics, Solar and Stellar Astrophysics}, eid={arXiv:2510.00105}, pages={arXiv:2510.00105}, doi={10.48550/arXiv.2510.00105}, archiveprefix={arXiv}, eprint={2510.00105}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2025arXiv251000105V}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Subjak2024, author={Šubjak, Ján and Latham, David W. and Quinn, Samuel N. and Berlind, Perry and Calkins, Michael L. and Esquerdo, Gilbert A. and Brahm, Rafael and Caballero, José A. and Collins, Karen A. and Guenther, Eike and Janık, Jan and Kabáth, Petr and Schwarz, Richard P. and Tan, Thiam-Guan and Vanzi, Leonardo and Zambelli, Roberto and Ziegler, Carl and Jenkins, Jon M. and Mireles, Ismael and Seager, Sara and Shporer, Avi and Striegel, Stephanie and Winn, Joshua N.}, title={Evolution of BD-14 3065b (TOI-4987b) from giant planet to brown dwarf as possible evidence of deuterium burning at old stellar ages}, journal={\aap}, keywords={techniques: photometric, techniques: radial velocities, techniques: spectroscopic, planets and satellites: gaseous planets, brown dwarfs, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={688}, eid={A120}, pages={A120}, doi={10.1051/0004-6361/202349028}, archiveprefix={arXiv}, eprint={2403.12311}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2024A&A...688A.120S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Kunimoto2022, author={Kunimoto, Michelle and Daylan, Tansu and Guerrero, Natalia and Fong, William and Bryson, Steve and Ricker, George R. and Fausnaugh, Michael and Huang, Chelsea X. and Sha, Lizhou and Shporer, Avi and Vanderburg, Andrew and Vanderspek, Roland K. and Yu, Liang}, title={The TESS Faint-star Search: 1617 TOIs from the TESS Primary Mission}, journal={\apjs}, keywords={Exoplanets, Exoplanet detection methods, Transit photometry, Time series analysis, 498, 489, 1709, 1916, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, volume={259}, number={2}, eid={33}, pages={33}, doi={10.3847/1538-4365/ac5688}, archiveprefix={arXiv}, eprint={2112.02176}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022ApJS..259...33K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fausnaugh2020, author={Fausnaugh, Michael M. and Burke, Christopher J. and Ricker, George R. and Vanderspek, Roland}, title={Calibrated Full-frame Images for the TESS Quick Look Pipeline}, journal={Research Notes of the American Astronomical Society}, keywords={Astronomy data reduction, Astronomy data analysis, 1861, 1858}, volume={4}, number={12}, eid={251}, pages={251}, doi={10.3847/2515-5172/abd63a}, adsurl={https://ui.adsabs.harvard.edu/abs/2020RNAAS...4..251F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{kunimoto2021, author={Kunimoto, Michelle and Huang, Chelsea and Tey, Evan and Fong, Willie and Hesse, Katharine and Shporer, Avi and Guerrero, Natalia and Fausnaugh, Michael and Vanderspek, Roland and Ricker, George}, title={Quick-look Pipeline Lightcurves for 9.1 Million Stars Observed over the First Year of the TESS Extended Mission}, journal={Research Notes of the American Astronomical Society}, keywords={Light curves, Transit photometry, Exoplanets, 918, 1709, 498, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={5}, number={10}, eid={234}, pages={234}, doi={10.3847/2515-5172/ac2ef0}, archiveprefix={arXiv}, eprint={2110.05542}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021RNAAS...5..234K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Kaufer1999, author={Kaufer, A. and Stahl, O. and Tubbesing, S. and Nørregaard, P. and Avila, G. and Francois, P. and Pasquini, L. and Pizzella, A.}, title={Commissioning FEROS, the new high-resolution spectrograph at La-Silla.}, journal={The Messenger}, keywords={Spectrographs: Data Processing}, volume={95}, pages={8-12}, adsurl={https://ui.adsabs.harvard.edu/abs/1999Msngr..95....8K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Brahm2017, author={Brahm, Rafael and Jordán, Andrés and Espinoza, Néstor}, title={CERES: A Set of Automated Routines for Echelle Spectra}, journal={\pasp}, keywords={Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={129}, number={973}, pages={034002}, doi={10.1088/1538-3873/aa5455}, archiveprefix={arXiv}, eprint={1609.02279}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2017PASP..129c4002B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Kabath2025, author={Kabáth, P. and Skarka, M. and Hatzes, A. and Guenther, E. and Vanzi, L. and Brahm, R. and Janık, J. and Pintr, P. and Gajdoš, P. and Lipták, J. and Žák, J. and Boffin, H. M. J. and Antonucci, L. and Avila, G. and Balkóová, Z. and Ball, M. E. and Flores, M. and Fuentes, A. and Fuchs, J. and Greimel, R. and Gajardo, A. and Ivanov, V. D. and Köhler, J. and Leitzinger, M. and Moravčık, T. and Nečásek, J. and Neubert, R. J. U. and Odert, P. and Olguin, G. and Tala Pinto, M. and Roth, M. and Řezba, L. and Schaffenroth, V. and Sigwarth, M. and Srba, J. and Suárez, A. and Škoda, P. and Šubjak, J. and Václavık, J. and Veselý, M. and Veselý, R. and Vıtková, M. and Winkler, J. U. and Zummer, M. and Ždárská, E.}, title={PLATOSpec: a precise spectrograph in support of space missions}, journal={arXiv e-prints}, keywords={Instrumentation and Methods for Astrophysics}, eid={arXiv:2510.11961}, pages={arXiv:2510.11961}, archiveprefix={arXiv}, eprint={2510.11961}, primaryclass={astro-ph.IM}, adsurl={https://ui.adsabs.harvard.edu/abs/2025arXiv251011961K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Baraffe2003, author={Baraffe, I. and Chabrier, G. and Barman, T. S. and Allard, F. and Hauschildt, P. H.}, title={Evolutionary models for cool brown dwarfs and extrasolar giant planets. The case of HD 209458}, journal={\aap}, keywords={planetary systems, stars: brown dwarfs, stars: evolution, stars: individual (HD 209458), Astrophysics}, volume={402}, pages={701-712}, doi={10.1051/0004-6361:20030252}, archiveprefix={arXiv}, eprint={astro-ph/0302293}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2003A&A...402..701B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Phillips2020, author={Phillips, M. W. and Tremblin, P. and Baraffe, I. and Chabrier, G. and Allard, N. F. and Spiegelman, F. and Goyal, J. M. and Drummond, B. and Hébrard, E.}, title={A new set of atmosphere and evolution models for cool T-Y brown dwarfs and giant exoplanets}, journal={\aap}, keywords={brown dwarfs, planets and satellites: atmospheres, stars: evolution, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={637}, eid={A38}, pages={A38}, doi={10.1051/0004-6361/201937381}, archiveprefix={arXiv}, eprint={2003.13717}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2020A&A...637A..38P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Zhang2025, author={Zhang, Elina Y. and Carmichael, Theron W. and Huber, Daniel and Stassun, Keivan G. and Fukui, Akihiko and Narita, Norio and Murgas, Felipe and Palle, Enric and Latham, David W. and Calkins, Michael L. and Seager, Sara and Winn, Joshua N. and Vezie, Michael and Hounsell, Rebekah and Osborn, Hugh P. and Caldwell, Douglas A. and Jenkins, Jon M.}, title={An Oasis in the Brown Dwarf Desert: Confirmation of Two Low-mass Transiting Brown Dwarfs Discovered by TESS}, journal={arXiv e-prints}, keywords={Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, eid={arXiv:2503.05115}, pages={arXiv:2503.05115}, doi={10.48550/arXiv.2503.05115}, archiveprefix={arXiv}, eprint={2503.05115}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2025arXiv250305115Z}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Spiegel2012, author={Spiegel, David S. and Burrows, Adam}, title={Spectral and Photometric Diagnostics of Giant Planet Formation Scenarios}, journal={\apj}, keywords={brown dwarfs, radiative transfer, stars: evolution, stars: low-mass, Astrophysics - Earth and Planetary Astrophysics}, volume={745}, number={2}, eid={174}, pages={174}, doi={10.1088/0004-637X/745/2/174}, archiveprefix={arXiv}, eprint={1108.5172}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012ApJ...745..174S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Chabrier2023, author={Chabrier, Gilles and Baraffe, Isabelle and Phillips, Mark and Debras, Florian}, title={Impact of a new H/He equation of state on the evolution of massive brown dwarfs. New determination of the hydrogen burning limit}, journal={\aap}, keywords={dense matter, equation of state, stars: low-mass, brown dwarfs, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies}, volume={671}, eid={A119}, pages={A119}, doi={10.1051/0004-6361/202243832}, archiveprefix={arXiv}, eprint={2212.07153}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2023A&A...671A.119C}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{toi2525, author={Trifonov, Trifon and Brahm, Rafael and Jordán, Andrés and Hartogh, Christian and Henning, Thomas and Hobson, Melissa J. and Schlecker, Martin and Howard, Saburo and Reichardt, Finja and Espinoza, Nestor and Lee, Man Hoi and Nesvorny, David and Rojas, Felipe I. and Barkaoui, Khalid and Kossakowski, Diana and Boyle, Gavin and Dreizler, Stefan and Kürster, Martin and Heller, René and Guillot, Tristan and Triaud, Amaury H. 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M. J. and Crouzet, Nicolas and Dransfield, Georgina and Cloutier, Ryan and Barkaoui, Khalid and Schwarz, Rick P. and Stockdale, Chris and Harris, Mallory and Mireles, Ismael and Evans, Phil and Mann, Andrew W. and Ziegler, Carl and Dragomir, Diana and Villanueva, Steven and Mordasini, Christoph and Ricker, George and Vanderspek, Roland and Latham, David W. and Seager, Sara and Winn, Joshua N. and Jenkins, Jon M. and Vezie, Michael and Youngblood, Allison and Daylan, Tansu and Collins, Karen A. and Caldwell, Douglas A. and Ciardi, David R. and Palle, Enric and Murgas, Felipe}, title={Three Long-period Transiting Giant Planets from TESS}, journal={\aj}, keywords={Exoplanets, Extrasolar gaseous giant planets, Radial velocity, Transit photometry, 498, 509, 1332, 1709, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={165}, number={6}, eid={227}, pages={227}, doi={10.3847/1538-3881/accadd}, archiveprefix={arXiv}, eprint={2304.02139}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023AJ....165..227B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Heller2010, author={Heller, R. and Jackson, B. and Barnes, R. and Greenberg, R. and Homeier, D.}, title={Tidal effects on brown dwarfs: application to the eclipsing binary 2MASS J05352184-0546085. The anomalous temperature reversal in the context of tidal heating}, journal={\aap}, keywords={celestial mechanics, binaries: eclipsing, stars: evolution, stars: individual: 2MASSJ05352184-0546085, brown dwarfs, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={514}, eid={A22}, pages={A22}, doi={10.1051/0004-6361/200912826}, archiveprefix={arXiv}, eprint={1002.1246}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2010A&A...514A..22H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Beatty2018, author={Beatty, Thomas G. and Morley, Caroline V. and Curtis, Jason L. and Burrows, Adam and Davenport, James R. A. and Montet, Benjamin T.}, title={A Significant Overluminosity in the Transiting Brown Dwarf CWW 89Ab}, journal={\aj}, keywords={brown dwarfs, open clusters and associations: individual: Ruprecht 147, NGC 6774, planets and satellites: atmospheres, stars: individual: CWW 89, EPIC 219388192, Astrophysics - Solar and Stellar Astrophysics}, volume={156}, number={4}, eid={168}, pages={168}, doi={10.3847/1538-3881/aad697}, archiveprefix={arXiv}, eprint={1807.11500}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2018AJ....156..168B}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Penev2012, author={Penev, Kaloyan and Jackson, Brian and Spada, Federico and Thom, Nicole}, title={Constraining Tidal Dissipation in Stars from the Destruction Rates of Exoplanets}, journal={\apj}, keywords={convection, planet-star interactions, stars: interiors, stars: rotation, stars: winds, outflows, turbulence, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={751}, number={2}, eid={96}, pages={96}, doi={10.1088/0004-637X/751/2/96}, archiveprefix={arXiv}, eprint={1205.1803}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2012ApJ...751...96P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Vissapragada2022, author={Vissapragada, Shreyas and Chontos, Ashley and Greklek-McKeon, Michael and Knutson, Heather A. and Dai, Fei and Pérez González, Jorge and Grunblatt, Sam and Huber, Daniel and Saunders, Nicholas}, title={The Possible Tidal Demise of Kepler's First Planetary System}, journal={\apjl}, keywords={Exoplanet astronomy, Exoplanet evolution, Exoplanet dynamics, Exoplanet tides, Transits, Timing variation methods, Hot Jupiters, 486, 491, 490, 497, 1711, 1703, 753, Astrophysics - Earth and Planetary Astrophysics}, volume={941}, number={2}, eid={L31}, pages={L31}, doi={10.3847/2041-8213/aca47e}, archiveprefix={arXiv}, eprint={2212.09752}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2022ApJ...941L..31V}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Ogilvie2014, author={Ogilvie, Gordon I.}, title={Tidal Dissipation in Stars and Giant Planets}, journal={\araa}, keywords={Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={52}, pages={171-210}, doi={10.1146/annurev-astro-081913-035941}, archiveprefix={arXiv}, eprint={1406.2207}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2014ARA&A..52..171O}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{A_New_BD_Mstar_2025, author={Gan, Tianjun and Cadieux, Charles and Ida, Shigeru and Wang, Sharon X. and Mao, Shude and Lin, Zitao and Stassun, Keivan G. and Burgasser, Adam J. and Howell, Steve B. and Clark, Catherine A. and Strakhov, Ivan A. and Benni, Paul and Ricker, George R. and Vanderspek, Roland and Latham, David W. and Seager, Sara and Winn, Joshua N. and Jenkins, Jon M. and Arnold, Luc and Artigau, Étienne and Charbonneau, David and Collins, Karen A. and Cook, Neil J. and de Beurs, Zoë L. and Deveny, Sarah J. and Doty, John P. and Doyon, René and Littlefield, Colin and Pritchard, Tyler and Ross, Gabrielle and Shporer, Avi and Theissen, Christopher R. and Tofflemire, Benjamin M. and Vanderburg, Andrew and Watanabe, David}, title={A New Brown Dwarf Orbiting an M Star and an Investigation of the Eccentricity Distribution of Transiting Long-period Brown Dwarfs}, journal={\apjl}, keywords={Brown dwarfs, Eccentricity, Low mass stars, Binary stars, Extrasolar gaseous giant planets, Astrostatistics, Transit photometry, Radial velocity, 185, 441, 2050, 154, 509, 1882, 1709, 1332, Earth and Planetary Astrophysics, Solar and Stellar Astrophysics}, volume={988}, number={2}, eid={L78}, pages={L78}, doi={10.3847/2041-8213/adef55}, archiveprefix={arXiv}, eprint={2507.09461}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2025ApJ...988L..78G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Hut1981, author={Hut, P.}, title={Tidal evolution in close binary systems.}, journal={\aap}, keywords={Binary Stars, Celestial Mechanics, Stellar Evolution, Stellar Models, Tides, Two Body Problem, Angular Momentum, Companion Stars, Conservation Laws, Energy Dissipation, Equilibrium Equations, Gravitational Effects, Perturbation Theory, Stellar Rotation, Synchronism, X Ray Stars, Astrophysics}, volume={99}, pages={126-140}, adsurl={https://ui.adsabs.harvard.edu/abs/1981A&A....99..126H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Santos2004, author={Santos, N. C. and Israelian, G. and Mayor, M.}, title={Spectroscopic [Fe/H] for 98 extra-solar planet-host stars. Exploring the probability of planet formation}, journal={\aap}, keywords={stars: abundances, stars: fundamental parameters, stars: planetary systems, stars: planetary systems: formation, stars: chemically peculiar, Astrophysics}, volume={415}, pages={1153-1166}, doi={10.1051/0004-6361:20034469}, archiveprefix={arXiv}, eprint={astro-ph/0311541}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2004A&A...415.1153S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fischer2005, author={Fischer, Debra A. and Valenti, Jeff}, title={The Planet-Metallicity Correlation}, journal={\apj}, keywords={Stars: Planetary Systems, Stars: Abundances, Stars: Fundamental Parameters}, volume={622}, number={2}, pages={1102-1117}, doi={10.1086/428383}, adsurl={https://ui.adsabs.harvard.edu/abs/2005ApJ...622.1102F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Petigura2018, author={Petigura, Erik A. and Marcy, Geoffrey W. and Winn, Joshua N. and Weiss, Lauren M. and Fulton, Benjamin J. and Howard, Andrew W. and Sinukoff, Evan and Isaacson, Howard and Morton, Timothy D. and Johnson, John Asher}, title={The California-Kepler Survey. IV. Metal-rich Stars Host a Greater Diversity of Planets}, journal={\aj}, keywords={methods: statistical, planets and satellites: formation, planets and satellites: general, stars: abundances, stars: fundamental parameters, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics}, volume={155}, number={2}, eid={89}, pages={89}, doi={10.3847/1538-3881/aaa54c}, archiveprefix={arXiv}, eprint={1712.04042}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018AJ....155...89P}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Raghavan2010, author={Raghavan, Deepak and McAlister, Harold A. and Henry, Todd J. and Latham, David W. and Marcy, Geoffrey W. and Mason, Brian D. and Gies, Douglas R. and White, Russel J. and ten Brummelaar, Theo A.}, title={A Survey of Stellar Families: Multiplicity of Solar-type Stars}, journal={\apjs}, keywords={binaries: general, planetary systems, stars: solar-type, stars: statistics, surveys, Astrophysics - Solar and Stellar Astrophysics}, volume={190}, number={1}, pages={1-42}, doi={10.1088/0067-0049/190/1/1}, archiveprefix={arXiv}, eprint={1007.0414}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2010ApJS..190....1R}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Moe2019, author={Moe, Maxwell and Kratter, Kaitlin M. and Badenes, Carles}, title={The Close Binary Fraction of Solar-type Stars Is Strongly Anticorrelated with Metallicity}, journal={\apj}, keywords={binaries: close, binaries: eclipsing, binaries: spectroscopic, stars: abundances, stars: formation, stars: solar-type, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies}, volume={875}, number={1}, eid={61}, pages={61}, doi={10.3847/1538-4357/ab0d88}, archiveprefix={arXiv}, eprint={1808.02116}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2019ApJ...875...61M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Maldonado2018, author={Maldonado, J. and Villaver, E. and Eiroa, C.}, title={Chemical fingerprints of hot Jupiter planet formation}, journal={\aap}, keywords={techniques: spectroscopic, stars: abundances, stars: late-type, planetary systems, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={612}, eid={A93}, pages={A93}, doi={10.1051/0004-6361/201732001}, archiveprefix={arXiv}, eprint={1712.01035}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018A&A...612A..93M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Yasui2009, author={Yasui, Chikako and Kobayashi, Naoto and Tokunaga, Alan T. and Saito, Masao and Tokoku, Chihiro}, title={The Lifetime of Protoplanetary Disks in a Low-metallicity Environment}, journal={\apj}, keywords={infrared: stars, open clusters and associations: individual: Digel Cloud 2, planetary systems: protoplanetary disks, stars: formation, stars: pre-main sequence, Astrophysics - Solar and Stellar Astrophysics}, volume={705}, number={1}, pages={54-63}, doi={10.1088/0004-637X/705/1/54}, archiveprefix={arXiv}, eprint={0908.4026}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2009ApJ...705...54Y}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Dawson2018, author={Dawson, Rebekah I. and Johnson, John Asher}, title={Origins of Hot Jupiters}, journal={\araa}, keywords={Astrophysics - Earth and Planetary Astrophysics}, volume={56}, pages={175-221}, doi={10.1146/annurev-astro-081817-051853}, archiveprefix={arXiv}, eprint={1801.06117}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2018ARA&A..56..175D}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Fortney2021, author={Fortney, Jonathan J. and Dawson, Rebekah I. and Komacek, Thaddeus D.}, title={Hot Jupiters: Origins, Structure, Atmospheres}, journal={Journal of Geophysical Research (Planets)}, keywords={Astrophysics - Earth and Planetary Astrophysics}, volume={126}, number={3}, eid={e06629}, pages={e06629}, doi={10.1029/2020JE006629}, archiveprefix={arXiv}, eprint={2102.05064}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2021JGRE..12606629F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Salinas25, author={Salinas, Helem and Brahm, Rafael and Olmschenk, Greg and Barry, Richard K. and Pichara, Karim and Ishitani Silva, Stela and Araujo, Vladimir}, title={Exoplanet transit candidate identification in TESS full-frame images via a transformer-based algorithm}, journal={\mnras}, keywords={Earth and Planetary Astrophysics, Astrophysics of Galaxies, Instrumentation and Methods for Astrophysics, Artificial Intelligence}, volume={538}, number={3}, pages={2031-2049}, doi={10.1093/mnras/staf347}, archiveprefix={arXiv}, eprint={2502.07542}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2025MNRAS.538.2031S}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Wang2025_ExoEchoBDTTV, author={Wang, Wenqin and Ma, Xinyue and Chen, Zhangliang and Yu, Cong and Liu, Shangfei and Ma, Bo}, title={Exoplanet Ephemerides Change Observations (ExoEcho). II. 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M. and Dıaz, R. F. and Bonfils, X. and Udry, S.}, title={Absolute densities, masses, and radii of the WASP-47 system determined dynamically}, journal={\aap}, keywords={stars: individual: WASP-47, planetary systems, techniques: photometric, techniques: radial velocities, Astrophysics - Earth and Planetary Astrophysics}, volume={595}, eid={L5}, pages={L5}, doi={10.1051/0004-6361/201629770}, archiveprefix={arXiv}, eprint={1610.09533}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2016A&A...595L...5A}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Canas2019_Kepler730, author={Cañas, Caleb I. and Wang, Songhu and Mahadevan, Suvrath and Bender, Chad F. and De Lee, Nathan and Fleming, Scott W. and Garcıa-Hernández, D. 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Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={54}, pages={271-311}, doi={10.1146/annurev-astro-081915-023307}, archiveprefix={arXiv}, eprint={1603.01280}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2016ARA&A..54..271K}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Tokovinin2020CloseBinaries, author={Tokovinin, Andrei and Moe, Maxwell}, title={Formation of close binaries by disc fragmentation and migration, and its statistical modelling}, journal={\mnras}, keywords={binaries: close, binaries: general, binaries: spectroscopic, stars: formation, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics}, volume={491}, number={4}, pages={5158-5171}, doi={10.1093/mnras/stz3299}, archiveprefix={arXiv}, eprint={1910.01522}, primaryclass={astro-ph.SR}, adsurl={https://ui.adsabs.harvard.edu/abs/2020MNRAS.491.5158T}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Han2025, author={Han, Te and Robertson, Paul and Brandt, Timothy D. and Kanodia, Shubham and Cañas, Caleb and Shporer, Avi and Ricker, George and Beard, Corey}, title={Hundreds of TESS Exoplanets Might Be Larger than We Thought}, journal={\apjl}, keywords={Exoplanets, Light curves, Transits, 498, 918, 1711, Earth and Planetary Astrophysics, Instrumentation and Methods for Astrophysics}, volume={988}, number={1}, eid={L4}, pages={L4}, doi={10.3847/2041-8213/ade794}, archiveprefix={arXiv}, eprint={2506.19985}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2025ApJ...988L...4H}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Wheatley2018, author={Wheatley, Peter J. and West, Richard G. and Goad, Michael R. and Jenkins, James S. and Pollacco, Don L. and Queloz, Didier and Rauer, Heike and Udry, Stéphane and Watson, Christopher A. and Chazelas, Bruno and Eigmüller, Philipp and Lambert, Gregory and Genolet, Ludovic and McCormac, James and Walker, Simon and Armstrong, David J. and Bayliss, Daniel and Bento, Joao and Bouchy, François and Burleigh, Matthew R. and Cabrera, Juan and Casewell, Sarah L. and Chaushev, Alexander and Chote, Paul and Csizmadia, Szilárd and Erikson, Anders and Faedi, Francesca and Foxell, Emma and Gänsicke, Boris T. and Gillen, Edward and Grange, Andrew and Günther, Maximilian N. and Hodgkin, Simon T. and Jackman, James and Jordán, Andrés and Louden, Tom and Metrailler, Lionel and Moyano, Maximiliano and Nielsen, Louise D. and Osborn, Hugh P. and Poppenhaeger, Katja and Raddi, Roberto and Raynard, Liam and Smith, Alexis M. 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The Aligned Orbit of TOI-2533 b, a Transiting Brown Dwarf Orbiting an F8-type Star}, journal={\aj}, keywords={Brown dwarfs, Exoplanet dynamics, Exoplanet formation, Exoplanet evolution, Planetary alignment, Star-planet interactions, Binary stars, Close binary stars, 185, 490, 492, 491, 1243, 2177, 154, 254, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={168}, number={4}, eid={145}, pages={145}, doi={10.3847/1538-3881/ad6b7f}, archiveprefix={arXiv}, eprint={2408.00725}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2024AJ....168..145F}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Li2023, author={Li, Jiaru and Lai, Dong}, title={Resonant Excitation of Planetary Eccentricity due to a Dispersing Eccentric Protoplanetary Disk: A New Mechanism of Generating Large Planetary Eccentricities}, journal={\apj}, keywords={Hydrodynamics, Protoplanetary disks, Celestial mechanics, Exoplanet dynamics, 1963, 1300, 211, 490, Astrophysics - Earth and Planetary Astrophysics}, volume={956}, number={1}, eid={17}, pages={17}, doi={10.3847/1538-4357/aced89}, archiveprefix={arXiv}, eprint={2211.07305}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2023ApJ...956...17L}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Moeckel2008, author={Moeckel, Nickolas and Raymond, Sean N. and Armitage, Philip J.}, title={Extrasolar Planet Eccentricities from Scattering in the Presence of Residual Gas Disks}, journal={\apj}, keywords={accretion, accretion disks, planetary systems: formation, planetary systems: protoplanetary disks, planets and satellites: formation, scattering, Astrophysics}, volume={688}, number={2}, pages={1361-1367}, doi={10.1086/592286}, archiveprefix={arXiv}, eprint={0807.4186}, primaryclass={astro-ph}, adsurl={https://ui.adsabs.harvard.edu/abs/2008ApJ...688.1361M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Marzari2010, author={Marzari, F. and Baruteau, C. and Scholl, H.}, title={Planet-planet scattering in circumstellar gas disks}, journal={\aap}, keywords={planets and satellites: formation, protoplanetary disks, planetary systems}, volume={514}, eid={L4}, pages={L4}, doi={10.1051/0004-6361/201014716}, adsurl={https://ui.adsabs.harvard.edu/abs/2010A&A...514L...4M}, adsnote={Provided by the SAO/NASA Astrophysics Data System} }@article{Gallet2017, author={Gallet, F. and Bolmont, E. and Mathis, S. and Charbonnel, C. and Amard, L.}, title={Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets. I. From the PMS to the RGB at solar metallicity}, journal={\aap}, keywords={hydrodynamics, waves, planet-star interactions, stars: evolution, stars: rotation, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, volume={604}, eid={A112}, pages={A112}, doi={10.1051/0004-6361/201730661}, archiveprefix={arXiv}, eprint={1705.10164}, primaryclass={astro-ph.EP}, adsurl={https://ui.adsabs.harvard.edu/abs/2017A&A...604A.112G}, adsnote={Provided by the SAO/NASA Astrophysics Data System} } TESS LCs for stars in our sample downloaded with the { lightkurve} tool. Gray points represent the TESS observations, while red lines correspond to the out-of-transit GP models created with { citlalicue} to capture the variability in the LC. Datasets were divided by these models, leading to a flattened TESS LC (blue points) with the transit model (orange line). Green triangles indicate the positions of transits. Top: Heatmap illustrating the percentage of the flux from stars in our sample that falls within each pixel of the TESS TPF image using { Gaia} DR2/DR3 catalogs. Bottom: Pie chart representing the flux from the target and nearby stars inside the photometric aperture. Generalized Lomb-Scargle periodograms of FEROS RVs of stars in our sample from top to bottom: (a) TIC,9344899 RVs, (b) TIC,9344899 RVs minus transiting planet signal, (c) TIC,52059926 RVs, (d) TIC,52059926 RVs minus planet signal, (e) TIC,13344668 RVs, (f) TIC,13344668 RVs minus planet signal. The vertical red lines highlight the orbital period of the companions. Horizontal dashed lines show the theoretical FAP levels of 10%, 1%, and 0.1% for each panel. Fitted parameters from the { allesfitter} analysis. ParameterTIC 9344899TIC 52059926TIC 13344668TIC 63921468UnitFitted parameters$R_b / R_\star$$0.0792\pm0.0027$$0.1376_{-0.0065}^{+0.0052}$$0.1414_{-0.0068}^{+0.0059}$$0.03626_{-0.00073}^{+0.00087}$$(R_\star + R_b) / a_b$$0.0652_{-0.0022}^{+0.0028}$$0.00683_{-0.00023}^{+0.00027}$$0.00738_{-0.00023}^{+0.00026}$$0.01920_{-0.00043}^{+0.00047}$$\cos{i_b}$$0.0183_{-0.011}^{+0.0097}$$0.0055_{-0.0018}^{+0.0012}$$0.0085_{-0.0046}^{+0.0022}$$0.01633\pm0.00079$$T_{0;b}^a$$2163.6472_{-0.0012}^{+0.0012}$$1350.1844_{-0.0016}^{+0.0017}$$1445.0473_{-0.0010}^{+0.0015}$$1400.5143_{-0.0087}^{+0.0034}$$\mathrm{BJD}$$P_b$$8.5821566_{-0.0000072}^{+0.0000072}$$175.532\pm0.097$$141.77_{-0.63}^{+0.72}$$131.331\pm0.010$$\mathrm{d}$$K_b$$1.915\pm0.030$$0.862\pm0.027$$4.8_{-1.9}^{+2.5}$$2.0222_{-0.011}^{+0.0099}$$\mathrm{km\,s^{-1}}$$\sqrt{e_b} \cos{\omega_b}$$0.035_{-0.12}^{+0.090}$$-0.228\pm0.040$$-0.65_{-0.11}^{+0.17}$$-0.2723_{-0.0088}^{+0.0095}$$\sqrt{e_b} \sin{\omega_b}$$0.134_{-0.10}^{+0.060}$$0.676_{-0.022}^{+0.020}$$0.551_{-0.092}^{+0.084}$$0.3213\pm0.0084$$q_{1; \mathrm{TESS}}$$0.29_{-0.21}^{+0.39}$$0.62_{-0.29}^{+0.26}$$0.35_{-0.28}^{+0.41}$$0.19_{-0.12}^{+0.18}$$q_{2; \mathrm{TESS}}$$0.22_{-0.16}^{+0.33}$$0.48\pm0.28$$0.27_{-0.20}^{+0.35}$$0.43_{-0.30}^{+0.36}$$\ln{\sigma_\mathrm{TESS}}$$-6.846_{-0.033}^{+0.035}$$-6.53_{-0.12}^{+0.13}$$-6.64_{-0.13}^{+0.15}$$-8.776\pm0.077$$\ln{ \mathrm{rel. flux.} }$$\ln{\sigma_\mathrm{jitter; FEROS}}$$-2.66_{-0.28}^{+0.32}$$-2.42_{-0.13}^{+0.14}$$-1.70_{-0.17}^{+0.18}$$-4.19_{-4.5}^{+0.63}$$\ln{ \mathrm{km/s} }$ {a -- BJD - 2,457,000} Derived parameters from the { allesfitter} analysis. ParameterTIC 9344899TIC 52059926TIC 13344668TIC 63921468Derived parametersHost radius over semi-major axis; $R_\star/a_\mathrm{b}$$0.0604_{-0.0020}^{+0.0026}$$0.00601_{-0.00019}^{+0.00023}$$0.00647_{-0.00020}^{+0.00023}$$0.01853_{-0.00042}^{+0.00045}$Semi-major axis over host radius; $a_\mathrm{b}/R_\star$$16.55_{-0.67}^{+0.57}$$166.4_{-6.0}^{+5.4}$$154.6_{-5.3}^{+4.9}$$54.0\pm1.3$Companion radius over semi-major axis b; $R_\mathrm{b}/a_\mathrm{b}$$0.00478_{-0.00022}^{+0.00029}$$0.000825\pm0.000054$$0.000913_{-0.000051}^{+0.000056}$$0.000672_{-0.000022}^{+0.000025}$Companion radius; $R_\mathrm{b}$ ($\mathrm{R_{\oplus}}$)$9.16\pm0.40$$10.71_{-0.57}^{+0.52}$$10.32\pm0.57$$9.30_{-0.27}^{+0.30}$Companion radius; $R_\mathrm{b}$ ($\mathrm{R_{jup}}$)$0.817\pm0.036$$0.955_{-0.051}^{+0.047}$$0.921\pm0.051$$0.830_{-0.024}^{+0.027}$Semi-major axis; $a_\mathrm{b}$ ($\mathrm{R_{\odot}}$)$17.52_{-0.86}^{+0.80}$$118.8\pm5.4$$103.4\pm4.6$$126.7\pm4.1$Semi-major axis; $a_\mathrm{b}$ (AU)$0.0815_{-0.0040}^{+0.0037}$$0.553\pm0.025$$0.481\pm0.022$$0.589\pm0.019$Inclination; $i_\mathrm{b}$ (deg)$88.95_{-0.56}^{+0.63}$$89.685_{-0.071}^{+0.11}$$89.51_{-0.13}^{+0.27}$$89.064\pm0.046$Eccentricity; $e_\mathrm{b}$$0.029_{-0.018}^{+0.021}$$0.510\pm0.026$$0.747_{-0.13}^{+0.062}$$0.1773\pm0.0051$Argument of periastron; $w_\mathrm{b}$ (deg)$80._{-33}^{+72}$$108.6\pm3.4$$139.5_{-12}^{+9.5}$$130.3\pm1.5$Mass ratio; $q_\mathrm{b}$$0.01890_{-0.00090}^{+0.0010}$$0.0221_{-0.0012}^{+0.0013}$$0.094_{-0.028}^{+0.038}$$0.0425_{-0.0014}^{+0.0015}$Companion mass; $M_\mathrm{b}$ ($\mathrm{M_{\oplus}}$)$6170_{-580}^{+610}$$5380_{-370}^{+390}$$21500_{-6500}^{+8800}$$21510\pm1000$Companion mass; $M_\mathrm{b}$ ($\mathrm{M_{jup}}$)$19.4_{-1.8}^{+1.9}$$16.9_{-1.1}^{+1.2}$$68_{-20.}^{+28}$$67.7\pm3.3$Companion mass; $M_\mathrm{b}$ ($\mathrm{M_{\odot}}$)$0.0185_{-0.0017}^{+0.0018}$$0.0162_{-0.0011}^{+0.0012}$$0.065_{-0.020}^{+0.026}$$0.0646\pm0.0031$Impact parameter; $b_\mathrm{tra;b}$$0.30_{-0.18}^{+0.15}$$0.460_{-0.16}^{+0.100}$$0.41\pm0.25$$0.750_{-0.021}^{+0.023}$Total transit duration; $T_\mathrm{tot;b}$ (h)$4.00_{-0.10}^{+0.12}$$4.87_{-0.14}^{+0.16}$$3.36_{-0.22}^{+0.28}$$11.56_{-0.34}^{+0.20}$Host density from orbit; $\rho_\mathrm{\star;b}$ (cgs)$1.16_{-0.14}^{+0.12}$$2.83\pm0.30$$3.47\pm0.34$$0.172\pm0.012$Companion density; $\rho_\mathrm{b}$ (cgs)$44.1_{-7.0}^{+8.4}$$24.1_{-3.6}^{+4.8}$$111_{-42}^{+51}$$147_{-16}^{+18}$Companion surface gravity; $g_\mathrm{b}$ (cgs)$71000_{-8000}^{+7200}$$45100_{-5400}^{+6500}$$199000_{-71000}^{+76000}$$244000\pm17000$Equilibrium temperature; $T_\mathrm{eq;b}$ (K)$^1$$923_{-19}^{+22}$$229.6_{-5.1}^{+5.5}$$237.7_{-5.2}^{+5.6}$$572.4\pm9.3$Transit depth (undil.); $\delta_\mathrm{tr; undil; b; TESS}$ (ppt)$7.10_{-0.34}^{+0.36}$$22.94_{-0.81}^{+0.90}$$22.50_{-0.86}^{+0.82}$$1.316_{-0.049}^{+0.055}$Transit depth (dil.); $\delta_\mathrm{tr; dil; b; TESS}$ (ppt)$3.52_{-0.17}^{+0.18}$$22.94_{-0.81}^{+0.90}$$22.50_{-0.86}^{+0.82}$$1.316_{-0.049}^{+0.055}$ {1 -- computed assuming zero albedo} All phased LCs for TIC,9344899. The gray points represent TESS data, and the blue points are TESS binned data in the phase curve with a bin width of 24 minutes in phase. The red lines represent the best transit models. The phased LCs fitted with { allesfitter} as described in Section \ref{['sec:RVs']}. The gray points represent TESS data, and the blue points are TESS binned data in the phase curve with a bin width of 24 minutes in phase. The red lines represent the best transit models. The radial velocity curves fitted with the { allesfitter} as described in Section \ref{['sec:RVs']}. The red lines represent the best RV models. $