van Houdt, JoshaJoshavan HoudtVAN DER WEL, ARJENARJENVAN DER WELBezanson, RachelRachelBezansonFranx, MarijnMarijnFranxd'Eugenio, FrancescoFrancescod'EugenioBarisic, IvanaIvanaBarisicBell, Eric F.Eric F.BellGALLAZZI, Anna RitaAnna RitaGALLAZZIde Graaff, AnnaAnnade GraaffMaseda, Michael V.Michael V.MasedaPacifici, CamillaCamillaPacificivan de Sande, JesseJessevan de SandeSobral, DavidDavidSobralStraatman, CarolineCarolineStraatmanWu, Po-FengPo-FengWu2022-03-182022-03-1820210004-637Xhttp://hdl.handle.net/20.500.12386/31697We present spatially resolved stellar kinematics for 797 z = 0.6-1 galaxies selected from the LEGA-C survey and construct axisymmetric Jeans models to quantify their dynamical mass and degree of rotational support. The survey is K <SUB> s </SUB>-band selected, irrespective of color or morphological type, and allows for a first assessment of the stellar dynamical structure of the general L* galaxy population at large look-back time. Using light profiles from Hubble Space Telescope imaging as a tracer, our approach corrects for observational effects (seeing convolution and slit geometry), and uses well-informed priors on inclination, anisotropy, and a non-luminous mass component. Tabulated data include total mass estimates in a series of spherical apertures (1, 5, and 10 kpc; 1 × and 2 × R <SUB>e</SUB>), as well as rotational velocities, velocity dispersions, and anisotropy. We show that almost all star-forming galaxies and ~50% of quiescent galaxies are rotation dominated, with deprojected V/σ ~ 1-2. Revealing the complexity in galaxy evolution, we find that the most massive star-forming galaxies are among the most rotation dominated, and the most massive quiescent galaxies among the least rotation-dominated galaxies. These measurements set a new benchmark for studying galaxy evolution, using stellar dynamical structure for galaxies at large look-back time. Together with the additional information on stellar population properties from the LEGA-C spectra, the dynamical mass and V/σ measurements presented here create new avenues for studying galaxy evolution at large look-back time.STAMPAenArticle10.3847/1538-4357/ac1f292-s2.0-85121761204https://iopscience.iop.org/article/10.3847/1538-4357/ac1f29https://api.elsevier.com/content/abstract/scopus_id/851217612042021ApJ...923...11VFIS/05 - ASTRONOMIA E ASTROFISICA