Van Der Wel ABezanson RD'Eugenio FStraatman CFranx MVan Houdt JMaseda M.VGallazzi APO-FENG WUPacifici CBarisic IBrammer G.BMunoz-Mateos J.CVervalcke SZibetti SSobral DDe Graaff ACalhau JKaushal YMuzzin ABell E.FVan Dokkum P.G.2022-11-112022-11-11202100670049https://www.scopus.com/inward/record.uri?eid=2-s2.0-85117616691&doi=10.3847%2f1538-4365%2fac1356&partnerID=40&md5=f0071853d83f5d2dc1deb130adc877b4https://scholars.lib.ntu.edu.tw/handle/123456789/624902We 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, Ks -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 s -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. © 2021. The American Astronomical Society. All rights reserved..FITS filejournal article10.3847/1538-4365/ac13562-s2.0-85117616691