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. Calabrò; 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 Fèvre; 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. Calabrò, 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 Fèvre, 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 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.

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

Keywords

Galaxies: distances and redshifts
Galaxies: statistics
Galaxies: fundamental parameters
Cosmology: observations/surveys/catalogs

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10.1051/0004-6361/202040059

Garilli_2021_AA_VENDELS-ESO
Copyright © ESO 2021. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published 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 and Astrophysics, 647, Article A150. https://doi.org/10.1051/0004-6361/202040059

@article{36edf20d42e846159a6aa5fd3ca13f70,

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 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 {\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-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.",

keywords = "Galaxies: distances and redshifts, Galaxies: statistics, Galaxies: fundamental parameters, Cosmology: observations/surveys/catalogs",

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. Calabr{\`o} and G. Cresci and J.P.U. Fynbo and N.P. Hathi and P. Hibon and A.M. Koekemoer 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 E.F. Bell and R.A.A. Bowler 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 H.C. Ferguson 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 {Le F{\`e}vre}, O. 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 D.J. Rosario and A. Saldana-Lopez and P. Santini and A. Saxena and D. Schaerer and C. Schreiber and D. Stark and L.A.M. Tasca and R. Thomas and E. Vanzella and V. Wild and C. Williams and E. Zucca",

note = "This work has been partially funded by Premiale MITIC 2017 and INAF PRIN “Mainstream 2019”. A. C. acknowledges the support from grant PRIN MIUR 2017-20173ML3WW-001; R. A. acknowledges support from ANID FONDECYT Regular 1202007. FB acknowledges Junta de Castilla y Le{\'o}n and the European Regional Development Fund (ERDF) for financial support under grant BU229P18. M. M. and A. C. acknowledge support from the grants ASI n.I/023/12/0, ASI n.2018- 23-HH.0. M. M. acknowledges support from MIUR, PRIN 2017 (grant 20179ZF5KS). M. F. acknowledges support from the UK Science and Technology Facilities Council (STFC) (grant number ST/R000905/1). The TOPCAT software (Taylor 2005) has been widely use for this paper.",

year = "2021",

month = mar,

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

language = "English",

volume = "647",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP SCIENCES S A",

}

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, Calabrò, 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, Le Fèvre, O, 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 and 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 - Calabrò, 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 - Le Fèvre, O.

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.

N1 - This work has been partially funded by Premiale MITIC 2017 and INAF PRIN “Mainstream 2019”. A. C. acknowledges the support from grant PRIN MIUR 2017-20173ML3WW-001; R. A. acknowledges support from ANID FONDECYT Regular 1202007. FB acknowledges Junta de Castilla y León and the European Regional Development Fund (ERDF) for financial support under grant BU229P18. M. M. and A. C. acknowledge support from the grants ASI n.I/023/12/0, ASI n.2018- 23-HH.0. M. M. acknowledges support from MIUR, PRIN 2017 (grant 20179ZF5KS). M. F. acknowledges support from the UK Science and Technology Facilities Council (STFC) (grant number ST/R000905/1). The TOPCAT software (Taylor 2005) has been widely use for this paper.

PY - 2021/3

Y1 - 2021/3

N2 - 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.

AB - 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.

KW - Galaxies: distances and redshifts

KW - Galaxies: statistics

KW - Galaxies: fundamental parameters

KW - Cosmology: observations/surveys/catalogs

U2 - 10.1051/0004-6361/202040059

DO - 10.1051/0004-6361/202040059

M3 - Article

SN - 0004-6361

VL - 647

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A150

ER -

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

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