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We present the second data release of the Large Early Galaxy AstrophysicsCensus (LEGA-C), an ESO 130-night public spectroscopic survey conducted withVIMOS on the Very Large Telescope. We release 1988 spectra with typicalcontinuum S / N ~= 20 /Angstrom of galaxies at 0.6 ~< z ~< 1.0, each observedfor ~20 hours and fully reduced with a custom-built pipeline. We also release acatalog with spectroscopic redshifts, emission line fluxes, Lick/IDS indices,and observed stellar and gas velocity dispersions that are spatially integratedquantities including both rotational motions and genuine dispersion. Toillustrate the new parameter space in the intermediate redshift regime probedby LEGA-C we explore relationships between dynamical and stellar populationproperties. The star-forming galaxies typically have observed stellar velocitydispersions of ~150 km/s and strong Hdelta absorption (Hd_A ~ 5 Angstrom),while passive galaxies have higher observed stellar velocity dispersions ~200km/s and weak Hdelta absortion (Hd_A ~ 0 Angstrom). Strong [O III]5007 / Hbetaratios tend to occur mostly for galaxies with weak Hd_A or galaxies with higherobserved velocity dispersion. Beyond these broad trends, we find a largediversity of possible combinations of rest-frame colors, absorption linestrengths and emission line detections, illustrating the utility ofspectroscopic measurements to more accurately understand galaxy evolution. Bymaking the spectra and value-added catalogs publicly available we encourage thecommunity to take advantage of this very substantial investment in telescopetime provided by ESO.

the astrophysical journal. supplement series/astrophysical journal. supplement series

The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release II:  dynamical and stellar population properties of z ~< 1 galaxies in the COSMOS  field