Abstract

Abstract We 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.

Highlights

  • The successful tenure of ESO’s VLT/VIMOS spectrograph (Le Fèvre et al 2003) was completed by the implementation of the two most recent Public SpectroscopicSurveys: LEGA-C (van der Wel et al 2016; Straatman et al 2018) and VANDELS (McLure et al 2018; Pentericci et al 2018)

  • We present the third and final data release of the Large Early Galaxy Astrophysics Census (LEGAC), an ESO/VLT 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

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Summary

Sterrenkundig

10 European Southern Observatory, Karl-Schwarzchild Straße 2, D-85748 Garching bei Munchen, Germany. 13 Departamento de Astrofısica, Universidad de La Laguna, E-38206 La Laguna, Spain. 14 Department of Physics and Astronomy, York University, 4700 Keele St., Toronto, Ontario, M3J 1P3, Canada. 15 Department of Astronomy, University of Michigan, 1085 South University Ave., Ann Arbor, MI 48109, USA. 16 Astronomy Department, Yale University, 52 Hillhouse Ave, New Haven, CT 06511, USA

INTRODUCTION
The LEGA-C Survey
Custom LEGA-C pipeline
Telluric Absorption
Flux Calibration
Hubble Space Telescope Imaging
Redshifts
Stellar and Ionized Gas Kinematics
Emission Line Fluxes and Equivalent Widths
Absorption Line Indices
Spectra
The spectra and catalog are available on this website: https:
Catalog
COMPLETENESS
PHOTOMETRY AND FITTING THE SPECTRAL ENERGY DISTRIBUTION
UNCERTAINTIES IN SPECTRAL PROPERTIES
Findings
UltraVista Original ZP
Full Text
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