The VANDELS ESO public spectroscopic survey

R. J. McLure, L. Pentericci, A. Cimatti, J. S. Dunlop, D. Elbaz, A. Fontana, K. Nandra, R. Amorin, M. Bolzonella, A. Bongiorno, A. C. Carnall, M. Castellano, M. Cirasuolo, O. Cucciati, F. Cullen, S. De Barros, S. L. Finkelstein, F. Fontanot, P. Franzetti, M. FumanaA. Gargiulo, B. Garilli, L. Guaita, W. G. Hartley, A. Iovino, M. J. Jarvis, S. Juneau, W. Karman, D. Maccagni, F. Marchi, E. Mármol-Queraltó, E. Pompei, L. Pozzetti, M. Scodeggio, V. Sommariva, M. Talia, O. Almaini, I. Balestra, S. Bardelli, E. F. Bell, N. Bourne, R. A.A. Bowler, M. Brusa, F. Buitrag, K. I. Caputi, P. Cassata, S. Charlot, A. Citro, G. Cresci, S. Cristiani, E. Curtis-Lake, M. Dickinson, G. G. Fazio, H. C. Ferguson, F. Fiore, M. Franco, J. P.U. Fynbo, A. Galametz, A. Georgakakis, M. Giavalisco, A. Grazian, N. P. Hathi, I. Jung, S. Kim, A. M. Koekemoer, Y. Khusanova, O. Le F'evre, J. M. Lotz, F. Mannucci, D. T. Maltby, K. Matsuoka, D. J. Mc Leod, Hernandez Mendez, J. Mendez-Abreu, M. Mignoli, M. Moresco, A. Mortlock, M. Nonino, M. Pannella, C. Papovich, P. Popesso, D. P. Rosario, M. Salvato, P. Santini, D. Schaerer, C. Schreiber, Daniel P Stark, L. A.M. Tasca, R. Thomas, T. Treu, E. Vanzella, V. Wild, C. C. Williams, G. Zamorani, E. Zucca

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

VANDELS is a uniquely deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO'sVery Large Telescope (VLT). The survey has obtained ultradeep optical (0.48 < ? < 1.0 μm) spectroscopy of ≃2100 galaxies within the redshift interval 1.0≤z≤ 7.0, over a total area of ≃0.2 deg2 centred on the CANDELS Ultra Deep Survey and Chandra Deep Field South fields. Based on accurate photometric redshift pre-selection, 85 per cent of the galaxies targeted by VANDELS were selected to be at z ≥ 3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to provide the high-signal-to-noise ratio spectra necessary to measure key physical properties such as stellar population ages, masses, metallicities, and outflow velocities from detailed absorption-line studies. Using integration times calculated to produce an approximately constant signal-tonoise ratio (20>tint >80 h), theVANDELS survey targeted: (a) bright star-forming galaxies at 2.4≤z≤5.5, (b) massive quiescent galaxies at 1.0≤z≤2.5, (c) fainter star-forming galaxies at 3.0≤z≤7.0, and (d) X-ray/Spitzer-selected active galactic nuclei and Herschel-detected galaxies. By targeting two extragalactic survey fields with superb multiwavelength imaging data, VANDELS will produce a unique legacy data set for exploring the physics underpinning high-redshift galaxy evolution. In this paper, we provide an overview of the VANDELS survey designed to support the science exploitation of the first ESO public data release, focusing on the scientific motivation, survey design, and target selection.

Original languageEnglish (US)
Pages (from-to)25-42
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume479
Issue number1
DOIs
StatePublished - Sep 1 2018

Fingerprint

European Southern Observatory
galaxies
survey design
field survey
targeting
stars
physics
exploitation
active galactic nuclei
spectrographs
public
telescopes
x rays

Keywords

  • Galaxies: evolution
  • Galaxies: high
  • Galaxies: star formation
  • Redshift
  • Surveys

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

McLure, R. J., Pentericci, L., Cimatti, A., Dunlop, J. S., Elbaz, D., Fontana, A., ... Zucca, E. (2018). The VANDELS ESO public spectroscopic survey. Monthly Notices of the Royal Astronomical Society, 479(1), 25-42. https://doi.org/10.1093/mnras/sty1213

The VANDELS ESO public spectroscopic survey. / McLure, R. J.; Pentericci, L.; Cimatti, A.; Dunlop, J. S.; Elbaz, D.; Fontana, A.; Nandra, K.; Amorin, R.; Bolzonella, M.; Bongiorno, A.; Carnall, A. C.; Castellano, M.; Cirasuolo, M.; Cucciati, O.; Cullen, F.; De Barros, S.; Finkelstein, S. L.; Fontanot, F.; Franzetti, P.; Fumana, M.; Gargiulo, A.; Garilli, B.; Guaita, L.; Hartley, W. G.; Iovino, A.; Jarvis, M. J.; Juneau, S.; Karman, W.; Maccagni, D.; Marchi, F.; Mármol-Queraltó, E.; Pompei, E.; Pozzetti, L.; Scodeggio, M.; Sommariva, V.; Talia, M.; Almaini, O.; Balestra, I.; Bardelli, S.; Bell, E. F.; Bourne, N.; Bowler, R. A.A.; Brusa, M.; Buitrag, F.; Caputi, K. I.; Cassata, P.; Charlot, S.; Citro, A.; Cresci, G.; Cristiani, S.; Curtis-Lake, E.; Dickinson, M.; Fazio, G. G.; Ferguson, H. C.; Fiore, F.; Franco, M.; Fynbo, J. P.U.; Galametz, A.; Georgakakis, A.; Giavalisco, M.; Grazian, A.; Hathi, N. P.; Jung, I.; Kim, S.; Koekemoer, A. M.; Khusanova, Y.; Le F'evre, O.; Lotz, J. M.; Mannucci, F.; Maltby, D. T.; Matsuoka, K.; Mc Leod, D. J.; Mendez, Hernandez; Mendez-Abreu, J.; Mignoli, M.; Moresco, M.; Mortlock, A.; Nonino, M.; Pannella, M.; Papovich, C.; Popesso, P.; Rosario, D. P.; Salvato, M.; Santini, P.; Schaerer, D.; Schreiber, C.; Stark, Daniel P; Tasca, L. A.M.; Thomas, R.; Treu, T.; Vanzella, E.; Wild, V.; Williams, C. C.; Zamorani, G.; Zucca, E.

In: Monthly Notices of the Royal Astronomical Society, Vol. 479, No. 1, 01.09.2018, p. 25-42.

Research output: Contribution to journalArticle

McLure, RJ, Pentericci, L, Cimatti, A, Dunlop, JS, Elbaz, D, Fontana, A, Nandra, K, Amorin, R, Bolzonella, M, Bongiorno, A, Carnall, AC, Castellano, M, Cirasuolo, M, Cucciati, O, Cullen, F, De Barros, S, Finkelstein, SL, Fontanot, F, Franzetti, P, Fumana, M, Gargiulo, A, Garilli, B, Guaita, L, Hartley, WG, Iovino, A, Jarvis, MJ, Juneau, S, Karman, W, Maccagni, D, Marchi, F, Mármol-Queraltó, E, Pompei, E, Pozzetti, L, Scodeggio, M, Sommariva, V, Talia, M, Almaini, O, Balestra, I, Bardelli, S, Bell, EF, Bourne, N, Bowler, RAA, Brusa, M, Buitrag, F, Caputi, KI, Cassata, P, Charlot, S, Citro, A, Cresci, G, Cristiani, S, Curtis-Lake, E, Dickinson, M, Fazio, GG, Ferguson, HC, Fiore, F, Franco, M, Fynbo, JPU, Galametz, A, Georgakakis, A, Giavalisco, M, Grazian, A, Hathi, NP, Jung, I, Kim, S, Koekemoer, AM, Khusanova, Y, Le F'evre, O, Lotz, JM, Mannucci, F, Maltby, DT, Matsuoka, K, Mc Leod, DJ, Mendez, H, Mendez-Abreu, J, Mignoli, M, Moresco, M, Mortlock, A, Nonino, M, Pannella, M, Papovich, C, Popesso, P, Rosario, DP, Salvato, M, Santini, P, Schaerer, D, Schreiber, C, Stark, DP, Tasca, LAM, Thomas, R, Treu, T, Vanzella, E, Wild, V, Williams, CC, Zamorani, G & Zucca, E 2018, 'The VANDELS ESO public spectroscopic survey', Monthly Notices of the Royal Astronomical Society, vol. 479, no. 1, pp. 25-42. https://doi.org/10.1093/mnras/sty1213
McLure RJ, Pentericci L, Cimatti A, Dunlop JS, Elbaz D, Fontana A et al. The VANDELS ESO public spectroscopic survey. Monthly Notices of the Royal Astronomical Society. 2018 Sep 1;479(1):25-42. https://doi.org/10.1093/mnras/sty1213
McLure, R. J. ; Pentericci, L. ; Cimatti, A. ; Dunlop, J. S. ; Elbaz, D. ; Fontana, A. ; Nandra, K. ; Amorin, R. ; Bolzonella, M. ; Bongiorno, A. ; Carnall, A. C. ; Castellano, M. ; Cirasuolo, M. ; Cucciati, O. ; Cullen, F. ; De Barros, S. ; Finkelstein, S. L. ; Fontanot, F. ; Franzetti, P. ; Fumana, M. ; Gargiulo, A. ; Garilli, B. ; Guaita, L. ; Hartley, W. G. ; Iovino, A. ; Jarvis, M. J. ; Juneau, S. ; Karman, W. ; Maccagni, D. ; Marchi, F. ; Mármol-Queraltó, E. ; Pompei, E. ; Pozzetti, L. ; Scodeggio, M. ; Sommariva, V. ; Talia, M. ; Almaini, O. ; Balestra, I. ; Bardelli, S. ; Bell, E. F. ; Bourne, N. ; Bowler, R. A.A. ; Brusa, M. ; Buitrag, F. ; Caputi, K. I. ; Cassata, P. ; Charlot, S. ; Citro, A. ; Cresci, G. ; Cristiani, S. ; Curtis-Lake, E. ; Dickinson, M. ; Fazio, G. G. ; Ferguson, H. C. ; Fiore, F. ; Franco, M. ; Fynbo, J. P.U. ; Galametz, A. ; Georgakakis, A. ; Giavalisco, M. ; Grazian, A. ; Hathi, N. P. ; Jung, I. ; Kim, S. ; Koekemoer, A. M. ; Khusanova, Y. ; Le F'evre, O. ; Lotz, J. M. ; Mannucci, F. ; Maltby, D. T. ; Matsuoka, K. ; Mc Leod, D. J. ; Mendez, Hernandez ; Mendez-Abreu, J. ; Mignoli, M. ; Moresco, M. ; Mortlock, A. ; Nonino, M. ; Pannella, M. ; Papovich, C. ; Popesso, P. ; Rosario, D. P. ; Salvato, M. ; Santini, P. ; Schaerer, D. ; Schreiber, C. ; Stark, Daniel P ; Tasca, L. A.M. ; Thomas, R. ; Treu, T. ; Vanzella, E. ; Wild, V. ; Williams, C. C. ; Zamorani, G. ; Zucca, E. / The VANDELS ESO public spectroscopic survey. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 479, No. 1. pp. 25-42.
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abstract = "VANDELS is a uniquely deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO'sVery Large Telescope (VLT). The survey has obtained ultradeep optical (0.48 < ? < 1.0 μm) spectroscopy of ≃2100 galaxies within the redshift interval 1.0≤z≤ 7.0, over a total area of ≃0.2 deg2 centred on the CANDELS Ultra Deep Survey and Chandra Deep Field South fields. Based on accurate photometric redshift pre-selection, 85 per cent of the galaxies targeted by VANDELS were selected to be at z ≥ 3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to provide the high-signal-to-noise ratio spectra necessary to measure key physical properties such as stellar population ages, masses, metallicities, and outflow velocities from detailed absorption-line studies. Using integration times calculated to produce an approximately constant signal-tonoise ratio (20>tint >80 h), theVANDELS survey targeted: (a) bright star-forming galaxies at 2.4≤z≤5.5, (b) massive quiescent galaxies at 1.0≤z≤2.5, (c) fainter star-forming galaxies at 3.0≤z≤7.0, and (d) X-ray/Spitzer-selected active galactic nuclei and Herschel-detected galaxies. By targeting two extragalactic survey fields with superb multiwavelength imaging data, VANDELS will produce a unique legacy data set for exploring the physics underpinning high-redshift galaxy evolution. In this paper, we provide an overview of the VANDELS survey designed to support the science exploitation of the first ESO public data release, focusing on the scientific motivation, survey design, and target selection.",
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T1 - The VANDELS ESO public spectroscopic survey

AU - McLure, R. J.

AU - Pentericci, L.

AU - Cimatti, A.

AU - Dunlop, J. S.

AU - Elbaz, D.

AU - Fontana, A.

AU - Nandra, K.

AU - Amorin, R.

AU - Bolzonella, M.

AU - Bongiorno, A.

AU - Carnall, A. C.

AU - Castellano, M.

AU - Cirasuolo, M.

AU - Cucciati, O.

AU - Cullen, F.

AU - De Barros, S.

AU - Finkelstein, S. L.

AU - Fontanot, F.

AU - Franzetti, P.

AU - Fumana, M.

AU - Gargiulo, A.

AU - Garilli, B.

AU - Guaita, L.

AU - Hartley, W. G.

AU - Iovino, A.

AU - Jarvis, M. J.

AU - Juneau, S.

AU - Karman, W.

AU - Maccagni, D.

AU - Marchi, F.

AU - Mármol-Queraltó, E.

AU - Pompei, E.

AU - Pozzetti, L.

AU - Scodeggio, M.

AU - Sommariva, V.

AU - Talia, M.

AU - Almaini, O.

AU - Balestra, I.

AU - Bardelli, S.

AU - Bell, E. F.

AU - Bourne, N.

AU - Bowler, R. A.A.

AU - Brusa, M.

AU - Buitrag, F.

AU - Caputi, K. I.

AU - Cassata, P.

AU - Charlot, S.

AU - Citro, A.

AU - Cresci, G.

AU - Cristiani, S.

AU - Curtis-Lake, E.

AU - Dickinson, M.

AU - Fazio, G. G.

AU - Ferguson, H. C.

AU - Fiore, F.

AU - Franco, M.

AU - Fynbo, J. P.U.

AU - Galametz, A.

AU - Georgakakis, A.

AU - Giavalisco, M.

AU - Grazian, A.

AU - Hathi, N. P.

AU - Jung, I.

AU - Kim, S.

AU - Koekemoer, A. M.

AU - Khusanova, Y.

AU - Le F'evre, O.

AU - Lotz, J. M.

AU - Mannucci, F.

AU - Maltby, D. T.

AU - Matsuoka, K.

AU - Mc Leod, D. J.

AU - Mendez, Hernandez

AU - Mendez-Abreu, J.

AU - Mignoli, M.

AU - Moresco, M.

AU - Mortlock, A.

AU - Nonino, M.

AU - Pannella, M.

AU - Papovich, C.

AU - Popesso, P.

AU - Rosario, D. P.

AU - Salvato, M.

AU - Santini, P.

AU - Schaerer, D.

AU - Schreiber, C.

AU - Stark, Daniel P

AU - Tasca, L. A.M.

AU - Thomas, R.

AU - Treu, T.

AU - Vanzella, E.

AU - Wild, V.

AU - Williams, C. C.

AU - Zamorani, G.

AU - Zucca, E.

PY - 2018/9/1

Y1 - 2018/9/1

N2 - VANDELS is a uniquely deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO'sVery Large Telescope (VLT). The survey has obtained ultradeep optical (0.48 < ? < 1.0 μm) spectroscopy of ≃2100 galaxies within the redshift interval 1.0≤z≤ 7.0, over a total area of ≃0.2 deg2 centred on the CANDELS Ultra Deep Survey and Chandra Deep Field South fields. Based on accurate photometric redshift pre-selection, 85 per cent of the galaxies targeted by VANDELS were selected to be at z ≥ 3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to provide the high-signal-to-noise ratio spectra necessary to measure key physical properties such as stellar population ages, masses, metallicities, and outflow velocities from detailed absorption-line studies. Using integration times calculated to produce an approximately constant signal-tonoise ratio (20>tint >80 h), theVANDELS survey targeted: (a) bright star-forming galaxies at 2.4≤z≤5.5, (b) massive quiescent galaxies at 1.0≤z≤2.5, (c) fainter star-forming galaxies at 3.0≤z≤7.0, and (d) X-ray/Spitzer-selected active galactic nuclei and Herschel-detected galaxies. By targeting two extragalactic survey fields with superb multiwavelength imaging data, VANDELS will produce a unique legacy data set for exploring the physics underpinning high-redshift galaxy evolution. In this paper, we provide an overview of the VANDELS survey designed to support the science exploitation of the first ESO public data release, focusing on the scientific motivation, survey design, and target selection.

AB - VANDELS is a uniquely deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO'sVery Large Telescope (VLT). The survey has obtained ultradeep optical (0.48 < ? < 1.0 μm) spectroscopy of ≃2100 galaxies within the redshift interval 1.0≤z≤ 7.0, over a total area of ≃0.2 deg2 centred on the CANDELS Ultra Deep Survey and Chandra Deep Field South fields. Based on accurate photometric redshift pre-selection, 85 per cent of the galaxies targeted by VANDELS were selected to be at z ≥ 3. Exploiting the red sensitivity of the refurbished VIMOS spectrograph, the fundamental aim of the survey is to provide the high-signal-to-noise ratio spectra necessary to measure key physical properties such as stellar population ages, masses, metallicities, and outflow velocities from detailed absorption-line studies. Using integration times calculated to produce an approximately constant signal-tonoise ratio (20>tint >80 h), theVANDELS survey targeted: (a) bright star-forming galaxies at 2.4≤z≤5.5, (b) massive quiescent galaxies at 1.0≤z≤2.5, (c) fainter star-forming galaxies at 3.0≤z≤7.0, and (d) X-ray/Spitzer-selected active galactic nuclei and Herschel-detected galaxies. By targeting two extragalactic survey fields with superb multiwavelength imaging data, VANDELS will produce a unique legacy data set for exploring the physics underpinning high-redshift galaxy evolution. In this paper, we provide an overview of the VANDELS survey designed to support the science exploitation of the first ESO public data release, focusing on the scientific motivation, survey design, and target selection.

KW - Galaxies: evolution

KW - Galaxies: high

KW - Galaxies: star formation

KW - Redshift

KW - Surveys

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JF - Monthly Notices of the Royal Astronomical Society

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