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

被引：69

作者：

Garilli, B. ^{[1
]}

McLure, R. ^{[2
]}

Pentericci, L. ^{[3
]}

Franzetti, P. ^{[1
]}

Gargiulo, A. ^{[1
]}

Carnall, A. ^{[2
]}

Cucciati, O. ^{[4
]}

Iovino, A. ^{[5
]}

Amorin, R. ^{[6
,7
]}

Bolzonella, M. ^{[4
]}

Bongiorno, A. ^{[3
]}

Castellano, M. ^{[3
]}

Cimatti, A. ^{[8
,9
]}

Cirasuolo, M. ^{[10
]}

Cullen, F. ^{[2
]}

Dunlop, J. ^{[2
]}

Elbaz, D. ^{[12
]}

Finkelstein, S. ^{[13
]}

Fontana, A. ^{[3
]}

Fontanot, F. ^{[14
,48
]}

Fumana, M. ^{[1
]}

Guaita, L. ^{[15
]}

Hartley, W. ^{[16
]}

Jarvis, M. ^{[17
]}

Juneau, S. ^{[54
]}

Maccagni, D. ^{[1
]}

McLeod, D. ^{[2
]}

Nandra, K. ^{[18
]}

Pompei, E. ^{[19
]}

Pozzetti, L. ^{[4
]}

Scodeggio, M. ^{[1
]}

Talia, M. ^{[4
,8
]}

Calabro, A. ^{[3
]}

Cresci, G. ^{[9
]}

Fynbo, J. P. U. ^{[20
]}

Hathi, N. P. ^{[21
]}

Hibon, P. ^{[19
]}

Koekemoer, A. M. ^{[21
]}

Magliocchetti, M. ^{[22
]}

Salvato, M. ^{[18
]}

Vietri, G. ^{[1
]}

Zamorani, G. ^{[4
]}

Almaini, O. ^{[23
]}

Balestra, I. ^{[24
]}

Bardelli, S. ^{[5
]}

Begley, R. ^{[2
]}

Brammer, G. ^{[20
]}

Bell, E. F. ^{[25
]}

Bowler, R. A. A. ^{[17
]}

Brusa, M. ^{[8
]}

机构：

[1] INAF Ist Astrofis Spaziale & Fis Cosm Milano, Via A Corti 12, I-20133 Milan, Italy

[2] Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland

[3] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy

[4] INAF Osservatorio Astrofis & Sci Spazio Bologna, Via Gobetti 93-3, I-40129 Bologna, Italy

[5] INAF Osservatorio Astronomico Brera, Via Brera 28, I-20122 Milan, Italy

[6] Univ La Serena, Inst Invest Multidisciplinar Ciencia & Tecnol, La Serena 1305, Chile

[7] Univ La Serena, Dept Astron, Ave Juan Cisternas 1200, La Serena, Chile

[8] Univ Bologna, Dept Phys & Astron Augusto Righi DIFA, Via Gobetti 93-2, I-40129 Bologna, Italy

[9] INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50157 Florence, Italy

[10] European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany

[11] Univ Geneva, Observ Geneve, 51 Ch Maillettes, CH-1290 Versoix, Switzerland

[12] CEA DSM Irfu, CNRS, Lab AIM Paris Saclay, Gif Sur Yvette, France

[13] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA

[14] INAF Astron Observ Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy

[15] Univ Diego Port, Fac Ingn, Nucleo Astron, Ave Ejercito 441, Santiago, Chile

[16] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[17] Univ Oxford, Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England

[18] Max Planck Inst Extraterr Phys, Giessenbach Str 1, D-85748 Garching, Germany

[19] European Southern Observ, Ave Alonso de Cordova 3107, Santiago 19001, Chile

[20] Univ Copenhagen, Niels Bohr Inst, Cosm Dawn Ctr, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

[21] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[22] INAF Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00133 Rome, Italy

[23] Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England

[24] Univ Observ Munich, Scheinerstr 1, D-81679 Munich, Germany

[25] Univ Michigan, Dept Astron, 311 West Hall,1085 South Univ Ave, Ann Arbor, MI 48109 USA

[26] Univ Lisbon, OAL, Inst Astrofis & Ciencias Espaco, P-1349018 Lisbon, Portugal

[27] Univ Lisbon, Fac Ciencias, Dept Fis, Edificio C8,Campo Grande 1749-016, P-1749016 Campo Grande, MS, Portugal

[28] Univ Groningen, Kapteyn Astron Inst, Postbus 800, NL-9700 Groningen, Netherlands

[29] Dipartimento Fis & Astron Galileo Galilei DFA, Vicolo Osservatorio,3, Padua, Italy

[30] Univ Paris 06, CNRS, Inst Astrophys Paris, 98 Bis Blvd Arago, F-75014 Paris, France

[31] Natl Opt Astron Observ, 950 North Cherry Ave, Tucson, AZ 85719 USA

[32] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 20138 USA

[33] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

[34] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA

[35] INAF Osservatorio Astron Padova, Vicolo Osservatorio,5, I-35122 Padua, Italy

[36] Pontificia Univ Catolica Chile, Inst Astrofis, Avda Vicuna Mackenna 4860, Santiago, Chile

[37] Aix Marseille Univ, CNRS, Lab Astrophys Marseille, UMR 7326, F-13388 Marseille, France

[38] Univ Valparaiso, Fac Ciencias, Inst Fis & Astron, Valparaiso 1111, Chile

[39] Inst Astrofis Canarias, Calle Via Lactea S-N, Tenerife 38205, Spain

[40] Univ La Laguna, Dept Astrofis, Tenerife 38200, Spain

[41] Ludwig Maximilians Univ Munchen, Fac Phys, Scheinerstr 1, D-81679 Munich, Germany

[42] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA

[43] Excellence Cluster, Boltzmannstr 2, D-85748 Garching, Germany

[44] Univ Durham, Dept Phys, South Rd, Durham DH1 3LE, England

[45] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[46] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA

[47] Univ St Andrews, SUPA, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland

[48] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy

[49] Univ Valladolid, Dept Fis Teor Atom & Opt, Valladolid 47011, Spain

[50] Goddard Space Flight Ctr, Astrophys Sci Div, Greenbelt, MD 20771 USA

来源：

ASTRONOMY & ASTROPHYSICS | 2021年 / 647卷

基金：

英国科学技术设施理事会;

关键词：

galaxies: distances and redshifts; galaxies: statistics; galaxies: fundamental parameters; cosmology: observations; surveys; catalogs; STAR-FORMING GALAXIES; X-RAY-PROPERTIES; VLT DEEP SURVEY; REDSHIFT SURVEY; QUIESCENT GALAXIES; DATA-REDUCTION; STELLAR; I; EVOLUTION; SELECTION;

D O I：

10.1051/0004-6361/202040059

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 angstrom 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-circle dot) < 11.7.

引用

页数：15

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