The VANDELS ESO public spectroscopic survey: Final Data Release of 2087 spectra and spectroscopic measurements

B. Garilli; R. McLure; L. Pentericci; P. Franzetti; A. Gargiulo; A. Carnall; O. Cucciati; A. Iovino; R. Amorin; M. Bolzonella; A. Bongiorno; M. Castellano; A. Cimatti; M. Cirasuolo; F. Cullen; J. Dunlop; D. Elbaz; S. Finkelstein; A. Fontana; F. Fontanot; M. Fumana; L. Guaita; W. Hartley; M. Jarvis; S. Juneau; D. Maccagni; D. McLeod; K. Nandra; E. Pompei; L. Pozzetti; M. Scodeggio; M. Talia; A. Calabro'; G. Cresci; J. P. U. Fynbo; N. P. Hathi; P. Hibon; A. M. Koekemoer; M. Magliocchetti; M. Salvato; G. Vietri; G. Zamorani; O. Almaini; I. Balestra; S. Bardelli; R. Begley; G. Brammer; E. F. Bell; R. A. A. Bowler; M. Brusa; F. Buitrago; C. Caputi; P. Cassata; S. Charlot; A. Citro; S. Cristiani; E. Curtis-Lake; M. Dickinson; G. Fazio; H. C. Ferguson; F. Fiore; M. Franco; A. Georgakakis; M. Giavalisco; A. Grazian; M. Hamadouche; I. Jung; S. Kim; Y. Khusanova; O. Le Fevre; M. Longhetti; J. Lotz; F. Mannucci; D. Maltby; K. Matsuoka; H. Mendez-Hernandez; J. Mendez-Abreu; M. Mignoli; M. Moresco; M. Nonino; M. Pannella; C. Papovich; P. Popesso; G. Roberts-Borsani; D. J. Rosario; A. Saldana-Lopez; P. Santini; A. Saxena; D. Schaerer; C. Schreiber; D. Stark; L. A. M. Tasca; R. Thomas; E. Vanzella; V. Wild; C. Williams; E. Zucca

doi:10.1051/0004-6361/202040059

The VANDELS ESO public spectroscopic survey: Final Data Release of 2087 spectra and spectroscopic measurements

B. Garilli, R. McLure, L. Pentericci, P. Franzetti, A. Gargiulo, A. Carnall, O. Cucciati, A. Iovino, R. Amorin, M. Bolzonella, A. Bongiorno, M. Castellano, A. Cimatti, M. Cirasuolo, F. Cullen, J. Dunlop, D. Elbaz, S. Finkelstein, A. Fontana, F. FontanotM. Fumana, L. Guaita, W. Hartley, M. Jarvis, S. Juneau, D. Maccagni, D. McLeod, K. Nandra, E. Pompei, L. Pozzetti, M. Scodeggio, M. Talia, A. Calabro', G. Cresci, J. P. U. Fynbo, N. P. Hathi, P. Hibon, A. M. Koekemoer, M. Magliocchetti, M. Salvato, G. Vietri, G. Zamorani, O. Almaini, I. Balestra, S. Bardelli, R. Begley, G. Brammer, E. F. Bell, R. A. A. Bowler, M. Brusa, F. Buitrago, C. Caputi, P. Cassata, S. Charlot, A. Citro, S. Cristiani, E. Curtis-Lake, M. Dickinson, G. Fazio, H. C. Ferguson, F. Fiore, M. Franco, A. Georgakakis, M. Giavalisco, A. Grazian, M. Hamadouche, I. Jung, S. Kim, Y. Khusanova, O. Le Fevre, M. Longhetti, J. Lotz, F. Mannucci, D. Maltby, K. Matsuoka, H. Mendez-Hernandez, J. Mendez-Abreu, M. Mignoli, M. Moresco, M. Nonino, M. Pannella, C. Papovich, P. Popesso, G. Roberts-Borsani, D. J. Rosario, A. Saldana-Lopez, P. Santini, A. Saxena, D. Schaerer, C. Schreiber, D. Stark, L. A. M. Tasca, R. Thomas, E. Vanzella, V. Wild, C. Williams, E. Zucca

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Abstract

VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We give 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{\AA} 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-IR photometry and physical parameters derived through SED fitting. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range 8.3<Log(M*/Msolar)

Original language	English
Article number	A150
Number of pages	15
Journal	Astronomy & Astrophysics
Volume	647
Early online date	26 Mar 2021
DOIs	https://doi.org/10.1051/0004-6361/202040059
Publication status	E-pub ahead of print - 26 Mar 2021

Keywords

astro-ph.GA
astro-ph.CO

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© ESO 2021. The original publication is available at https://doi.org/10.1051/0004-6361/202040059.
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Garilli, B., McLure, R., Pentericci, L., Franzetti, P., Gargiulo, A., Carnall, A., Cucciati, O., Iovino, A., Amorin, R., Bolzonella, M., Bongiorno, A., Castellano, M., Cimatti, A., Cirasuolo, M., Cullen, F., Dunlop, J., Elbaz, D., Finkelstein, S., Fontana, A., ... Zucca, E. (2021). The VANDELS ESO public spectroscopic survey: Final Data Release of 2087 spectra and spectroscopic measurements. Astronomy & Astrophysics, 647, Article A150. Advance online publication. https://doi.org/10.1051/0004-6361/202040059

@article{04f46e1bdacd40d2b8aae9683e2c4156,

title = "The VANDELS ESO public spectroscopic survey: Final Data Release of 2087 spectra and spectroscopic measurements",

abstract = " VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We give 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\{\textbackslash{}AA\} 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-IR photometry and physical parameters derived through SED fitting. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range 8.3",

keywords = "astro-ph.GA, astro-ph.CO",

author = "B. Garilli and R. McLure and L. Pentericci and P. Franzetti and A. Gargiulo and A. Carnall and O. Cucciati and A. Iovino and R. Amorin and M. Bolzonella and A. Bongiorno and M. Castellano and A. Cimatti and M. Cirasuolo and F. Cullen and J. Dunlop and D. Elbaz and S. Finkelstein and A. Fontana and F. Fontanot and M. Fumana and L. Guaita and W. Hartley and M. Jarvis and S. Juneau and D. Maccagni and D. McLeod and K. Nandra and E. Pompei and L. Pozzetti and M. Scodeggio and M. Talia and A. Calabro' and G. Cresci and Fynbo, \{J. P. U.\} and Hathi, \{N. P.\} and P. Hibon and Koekemoer, \{A. M.\} and M. Magliocchetti and M. Salvato and G. Vietri and G. Zamorani and O. Almaini and I. Balestra and S. Bardelli and R. Begley and G. Brammer and Bell, \{E. F.\} and Bowler, \{R. A. A.\} and M. Brusa and F. Buitrago and C. Caputi and P. Cassata and S. Charlot and A. Citro and S. Cristiani and E. Curtis-Lake and M. Dickinson and G. Fazio and Ferguson, \{H. C.\} and F. Fiore and M. Franco and A. Georgakakis and M. Giavalisco and A. Grazian and M. Hamadouche and I. Jung and S. Kim and Y. Khusanova and Fevre, \{O. Le\} and M. Longhetti and J. Lotz and F. Mannucci and D. Maltby and K. Matsuoka and H. Mendez-Hernandez and J. Mendez-Abreu and M. Mignoli and M. Moresco and M. Nonino and M. Pannella and C. Papovich and P. Popesso and G. Roberts-Borsani and Rosario, \{D. J.\} and A. Saldana-Lopez and P. Santini and A. Saxena and D. Schaerer and C. Schreiber and D. Stark and Tasca, \{L. A. M.\} and R. Thomas and E. Vanzella and V. Wild and C. Williams and E. Zucca",

note = "{\textcopyright} ESO 2021. The original publication is available at https://doi.org/10.1051/0004-6361/202040059 ",

year = "2021",

month = mar,

day = "26",

doi = "10.1051/0004-6361/202040059",

language = "English",

volume = "647",

journal = "Astronomy \& Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

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Garilli, B, McLure, R, Pentericci, L, Franzetti, P, Gargiulo, A, Carnall, A, Cucciati, O, Iovino, A, Amorin, R, Bolzonella, M, Bongiorno, A, Castellano, M, Cimatti, A, Cirasuolo, M, Cullen, F, Dunlop, J, Elbaz, D, Finkelstein, S, Fontana, A, Fontanot, F, Fumana, M, Guaita, L, Hartley, W, Jarvis, M, Juneau, S, Maccagni, D, McLeod, D, Nandra, K, Pompei, E, Pozzetti, L, Scodeggio, M, Talia, M, Calabro', A, Cresci, G, Fynbo, JPU, Hathi, NP, Hibon, P, Koekemoer, AM, Magliocchetti, M, Salvato, M, Vietri, G, Zamorani, G, Almaini, O, Balestra, I, Bardelli, S, Begley, R, Brammer, G, Bell, EF, Bowler, RAA, Brusa, M, Buitrago, F, Caputi, C, Cassata, P, Charlot, S, Citro, A, Cristiani, S, Curtis-Lake, E, Dickinson, M, Fazio, G, Ferguson, HC, Fiore, F, Franco, M, Georgakakis, A, Giavalisco, M, Grazian, A, Hamadouche, M, Jung, I, Kim, S, Khusanova, Y, Fevre, OL, Longhetti, M, Lotz, J, Mannucci, F, Maltby, D, Matsuoka, K, Mendez-Hernandez, H, Mendez-Abreu, J, Mignoli, M, Moresco, M, Nonino, M, Pannella, M, Papovich, C, Popesso, P, Roberts-Borsani, G, Rosario, DJ, Saldana-Lopez, A, Santini, P, Saxena, A, Schaerer, D, Schreiber, C, Stark, D, Tasca, LAM, Thomas, R, Vanzella, E, Wild, V, Williams, C & Zucca, E 2021, 'The VANDELS ESO public spectroscopic survey: Final Data Release of 2087 spectra and spectroscopic measurements', Astronomy & Astrophysics, vol. 647, A150. https://doi.org/10.1051/0004-6361/202040059

TY - JOUR

T1 - The VANDELS ESO public spectroscopic survey

T2 - Final Data Release of 2087 spectra and spectroscopic measurements

AU - Garilli, B.

AU - McLure, R.

AU - Pentericci, L.

AU - Franzetti, P.

AU - Gargiulo, A.

AU - Carnall, A.

AU - Cucciati, O.

AU - Iovino, A.

AU - Amorin, R.

AU - Bolzonella, M.

AU - Bongiorno, A.

AU - Castellano, M.

AU - Cimatti, A.

AU - Cirasuolo, M.

AU - Cullen, F.

AU - Dunlop, J.

AU - Elbaz, D.

AU - Finkelstein, S.

AU - Fontana, A.

AU - Fontanot, F.

AU - Fumana, M.

AU - Guaita, L.

AU - Hartley, W.

AU - Jarvis, M.

AU - Juneau, S.

AU - Maccagni, D.

AU - McLeod, D.

AU - Nandra, K.

AU - Pompei, E.

AU - Pozzetti, L.

AU - Scodeggio, M.

AU - Talia, M.

AU - Calabro', A.

AU - Cresci, G.

AU - Fynbo, J. P. U.

AU - Hathi, N. P.

AU - Hibon, P.

AU - Koekemoer, A. M.

AU - Magliocchetti, M.

AU - Salvato, M.

AU - Vietri, G.

AU - Zamorani, G.

AU - Almaini, O.

AU - Balestra, I.

AU - Bardelli, S.

AU - Begley, R.

AU - Brammer, G.

AU - Bell, E. F.

AU - Bowler, R. A. A.

AU - Brusa, M.

AU - Buitrago, F.

AU - Caputi, C.

AU - Cassata, P.

AU - Charlot, S.

AU - Citro, A.

AU - Cristiani, S.

AU - Curtis-Lake, E.

AU - Dickinson, M.

AU - Fazio, G.

AU - Ferguson, H. C.

AU - Fiore, F.

AU - Franco, M.

AU - Georgakakis, A.

AU - Giavalisco, M.

AU - Grazian, A.

AU - Hamadouche, M.

AU - Jung, I.

AU - Kim, S.

AU - Khusanova, Y.

AU - Fevre, O. Le

AU - Longhetti, M.

AU - Lotz, J.

AU - Mannucci, F.

AU - Maltby, D.

AU - Matsuoka, K.

AU - Mendez-Hernandez, H.

AU - Mendez-Abreu, J.

AU - Mignoli, M.

AU - Moresco, M.

AU - Nonino, M.

AU - Pannella, M.

AU - Papovich, C.

AU - Popesso, P.

AU - Roberts-Borsani, G.

AU - Rosario, D. J.

AU - Saldana-Lopez, A.

AU - Santini, P.

AU - Saxena, A.

AU - Schaerer, D.

AU - Schreiber, C.

AU - Stark, D.

AU - Tasca, L. A. M.

AU - Thomas, R.

AU - Vanzella, E.

AU - Wild, V.

AU - Williams, C.

AU - Zucca, E.

PY - 2021/3/26

Y1 - 2021/3/26

N2 - VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We give 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{\AA} 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-IR photometry and physical parameters derived through SED fitting. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range 8.3

AB - VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we present the final Public Data Release of the VANDELS Survey, comprising 2087 redshift measurements. We give 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{\AA} 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-IR photometry and physical parameters derived through SED fitting. The observed galaxy sample comprises both passive and star forming galaxies covering a stellar mass range 8.3

KW - astro-ph.GA

KW - astro-ph.CO

U2 - 10.1051/0004-6361/202040059

DO - 10.1051/0004-6361/202040059

M3 - Article

SN - 0004-6361

VL - 647

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A150

ER -

The VANDELS ESO public spectroscopic survey: Final Data Release of 2087 spectra and spectroscopic measurements

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