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.

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 & ASTROPHYSICS, 647, 1-15 [10.1051/0004-6361/202040059].

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

Cimatti A.
Membro del Collaboration Group
;
Talia M.;Brusa M.;Moresco M.;
2021

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.
2021
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 & ASTROPHYSICS, 647, 1-15 [10.1051/0004-6361/202040059].
Garilli B.; McLure R.; Pentericci L.; Franzetti P.; Gargiulo A.; Carnall A.; Cucciati O.; Iovino A.; Amorin R.; Bolzonella M.; Bongiorno A.; Castellan...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/869248
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