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We present the target list of solar-type stars to be observed inshort-cadence (2-min) for asteroseismology by the NASA Transiting ExoplanetSurvey Satellite (TESS) during its 2-year nominal survey mission. Thesolar-like Asteroseismic Target List (ATL) is comprised of bright, coolmain-sequence and subgiant stars and forms part of the larger target list ofthe TESS Asteroseismic Science Consortium (TASC). The ATL uses Gaia DR2 and theExtended Hipparcos Compilation (XHIP) to derive fundamental stellar properties,calculate detection probabilities and produce a rank-ordered target list. Weprovide a detailed description of how the ATL was produced and calculateexpected yields for solar-like oscillators based on the nominal photometricperformance by TESS. We also provide publicly available source code which canbe used to reproduce the ATL, thereby enabling comparisons of asteroseismicresults from TESS with predictions from synthetic stellar populations.

The Asteroseismic Target List (ATL) for solar-like oscillators observed in 2-minute cadence with the Transiting Exoplanet Survey Satellite (TESS)