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

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract / Description of output

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 i_AB = 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
Pages (from-to)	1-15
Number of pages	15
Journal	Astronomy and Astrophysics
Volume	647
DOIs	https://doi.org/10.1051/0004-6361/202040059
Publication status	Published - 26 Mar 2021

Keywords / Materials (for Non-textual outputs)

astro-ph.GA
astro-ph.CO

Access to Document

10.1051/0004-6361/202040059

2101.07645v1Accepted author manuscript, 4.93 MB

https://arxiv.org/abs/2101.07645

Cite this

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, 1-15. Article A150. https://doi.org/10.1051/0004-6361/202040059

@article{5f0928742182411a8cfe0f8d2710f3f2,

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 = "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 = "16 pages, 13 figures, accepted for publication in Astronomy & Astrophysics",

year = "2021",

month = mar,

day = "26",

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

language = "English",

volume = "647",

pages = "1--15",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

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 and Astrophysics, vol. 647, A150, pp. 1-15. https://doi.org/10.1051/0004-6361/202040059

TY - JOUR

T1 - The VANDELS ESO public spectroscopic survey 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.

N1 - 16 pages, 13 figures, accepted for publication in Astronomy & Astrophysics

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 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 - 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

SP - 1

EP - 15

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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Keywords / Materials (for Non-textual outputs)

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