Straatman, Caroline M. S.Caroline M. S.StraatmanVAN DER WEL, ARJENARJENVAN DER WELBezanson, RachelRachelBezansonPacifici, CamillaCamillaPacificiGALLAZZI, Anna RitaAnna RitaGALLAZZIWu, Po-FengPo-FengWuNoeske, KaiKaiNoeskeBarišić, IvanaIvanaBarišićBell, Eric F.Eric F.BellBrammer, Gabriel B.Gabriel B.BrammerCalhau, JoãoJoãoCalhauChauke, PriscillaPriscillaChaukeFranx, MarijnMarijnFranxvan Houdt, JoshaJoshavan HoudtLabbé, IvoIvoLabbéMaseda, Michael V.Michael V.MasedaMuñoz-Mateos, Juan C.Juan C.Muñoz-MateosMuzzin, AdamAdamMuzzinvan de Sande, JesseJessevan de SandeSobral, DavidDavidSobralSpilker, Justin S.Justin S.Spilker2020-10-232020-10-2320180067-0049http://hdl.handle.net/20.500.12386/27960We present the second data release of the Large Early Galaxy Astrophysics Census (LEGA-C), an ESO 130-night public spectroscopic survey conducted with VIMOS on the Very Large Telescope. We release 1988 spectra with typical continuum S/N ≃ 20 Å<SUP>-1</SUP> of galaxies at 0.6 ≲ z ≲ 1.0, each observed for ∼20 hr and fully reduced with a custom-built pipeline. We also release a catalog with spectroscopic redshifts, emission-line fluxes, Lick/IDS indices, and observed stellar and gas velocity dispersions that are spatially integrated quantities, including both rotational motions and genuine dispersion. To illustrate the new parameter space in the intermediate-redshift regime probed by LEGA-C, we explore relationships between dynamical and stellar population properties. The star-forming galaxies typically have observed stellar velocity dispersions of ∼150 km s<SUP>-1</SUP> and strong Hδ absorption (Hδ <SUB>A</SUB> ∼ 5 Å), while passive galaxies have higher observed stellar velocity dispersions (∼200 km s<SUP>-1</SUP>) and weak Hδ absorption (Hδ <SUB>A</SUB> ∼ 0 Å). Strong [O III]5007/Hβ ratios tend to occur mostly for galaxies with weak Hδ <SUB>A</SUB> or galaxies with higher observed velocity dispersion. Beyond these broad trends, we find a diversity of possible combinations of rest-frame colors, absorption-line strengths, and emission-line detections, illustrating the utility of spectroscopic measurements to more accurately understand galaxy evolution. By making the spectra and value-added catalogs publicly available we encourage the community to take advantage of this very substantial investment in telescope time provided by ESO.STAMPAenArticle10.3847/1538-4365/aae37a2-s2.0-85059154473000452524600005https://iopscience.iop.org/article/10.3847/1538-4365/aae37a2018ApJS..239...27SFIS/05 - ASTRONOMIA E ASTROFISICA