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The VANDELS ESO public spectroscopic survey: final data release of 2087 spectra and spectroscopic measurements

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Nandra,  K.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Salvato,  M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Georgakakis,  A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Citation

Garilli, B., McLure, R., Pentericci, L., Franzetti, P., Gargiulo, A., Carnall, A., et al. (2021). The VANDELS ESO public spectroscopic survey: final data release of 2087 spectra and spectroscopic measurements. Astronomy and Astrophysics, 647: A150. doi:10.1051/0004-6361/202040059.


Cite as: http://hdl.handle.net/21.11116/0000-0008-FF57-8
Abstract
VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high-signal-to-noise ratio, medium-resolution spectra of galaxies at redshifts between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We provide a detailed description of sample selection, observations, and data reduction procedures. The final catalogue reaches a target selection completeness of 40% at iAB = 25. The high signal-to-noise ratio of the spectra (above 7 in 80% of the spectra) and the dispersion of 2.5 Å allowed us to measure redshifts with high precision, the redshift measurement success rate reaching almost 100%. Together with the redshift catalogue and the reduced spectra, we also provide optical mid-infrared photometry and physical parameters derived through fitting the spectral energy distribution. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range of 8.3 < Log(M*/M) < 11.7.