Calibration of the jet energy scale and resolution of small-radius jets using semileptonic $t\bar{t}$ events with the ATLAS detector
ATLAS Collaboration
TL;DR
This work presents a data-driven calibration of the hadronic JES and JER for small-radius jets using semileptonic tt̄ events in ATLAS, exploiting the W-boson mass lineshape from hadronic W decays. The forward-folding technique generates templates that encode JES/JER variations, which are then fitted to data to extract per-jet-bin correction factors in the central region (|η|<0.8) across jets with 20–200 GeV pT. Analyses are performed on Run 2 (2015–2018, √s=13 TeV) and Run 3 (2022–2023, √s=13.6 TeV) data, with comprehensive systematic studies covering lepton, jet, and modelling uncertainties. The results show JES corrections near unity (Run 3), but with Run 2 requiring a modest scale-down relative to simulation, while JER corrections remain compatible with unity. The approach yields uncertainties of about 0.9–1.7% on JES and 14–28% on JER (excluding first pT bin sensitivity) and will be combined with other in-situ calibrations to further enhance ATLAS jet performance for precision measurements, including top-quark analyses.
Abstract
A measurement of correction factors for the hadronic jet energy scale and resolution in the ATLAS detector is presented. These correction factors account for differences between simulated and observed data. They are obtained by analysing a selection of top quark events collected in proton-proton collisions by ATLAS between the years 2015 and 2018 at a centre-of-mass energy $\sqrt{s} = 13$ TeV as well as in 2022 and 2023 at $\sqrt{s} = 13.6$ TeV. The forward-folding technique is used to quantify the impact of different jet energy scale or resolution corrections on the reconstructed mass of the hadronically decaying $W$ boson from top-quark decays in simulation. The correction factors are extracted from a fit to the parameterised reconstructed $W$-boson mass distribution to data. The energy scale and resolution corrections are measured as a function of the jet transverse momentum between 20 GeV and 200 GeV and absolute pseudorapidity less than 0.8. The uncertainties in the energy scale range from about 0.93% to about 1.7% for jets between 35 and 200 GeV, while for the energy resolution the uncertainties range from about 14% to 28%. The method presented will be used in conjunction with other techniques to further improve ATLAS jet energy scale and resolution precision.
