VAN DER WEL, ARJENARJENVAN DER WELBezanson, RachelRachelBezansonD'Eugenio, FrancescoFrancescoD'EugenioStraatman, CarolineCarolineStraatmanFranx, MarijnMarijnFranxvan Houdt, JoshaJoshavan HoudtMaseda, Michael V.Michael V.MasedaGALLAZZI, Anna RitaAnna RitaGALLAZZIWu, Po-FengPo-FengWuPacifici, CamillaCamillaPacificiBarisic, IvanaIvanaBarisicBrammer, Gabriel B.Gabriel B.BrammerMunoz-Mateos, Juan CarlosJuan CarlosMunoz-MateosVervalcke, SarahSarahVervalckeZIBETTI, StefanoStefanoZIBETTISobral, DavidDavidSobralde Graaff, AnnaAnnade GraaffCalhau, JoaoJoaoCalhauKaushal, YashaYashaKaushalMuzzin, AdamAdamMuzzinBell, Eric F.Eric F.Bellvan Dokkum, Pieter G.Pieter G.van Dokkum2022-03-182022-03-1820210067-0049http://hdl.handle.net/20.500.12386/31696We present the third and final data release of the Large Early Galaxy Astrophysics Census (LEGA-C), an ESO/Very Large Telescope public spectroscopic survey targeting 0.6 < z < 1.0, K<SUB>s</SUB>-selected galaxies. The data release contains 3528 spectra with measured stellar velocity dispersions and stellar population properties, a 25-fold increase in sample size compared to previous work. This K<SUB>s</SUB>-selected sample probes the galaxy population down to ~0.3L*, for all colors and morphological types. Along with the spectra, we publish a value-added catalog with stellar and ionized gas velocity dispersions, stellar absorption line indices, emission-line fluxes, and equivalent widths, complemented with structural parameters measured from Hubble Space Telescope Advanced Camera for Surveys imaging. With its combination of high precision and large sample size, LEGA-C provides a new benchmark for galaxy evolution studies.STAMPAenArticle10.3847/1538-4365/ac13562-s2.0-85117616691https://iopscience.iop.org/article/10.3847/1538-4365/ac1356https://api.elsevier.com/content/abstract/scopus_id/851176166912021ApJS..256...44VFIS/05 - ASTRONOMIA E ASTROFISICA