The ALPINE-ALMA [CII] survey Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6

被引：175

作者：

Le Fevre, O. ^{[1
]}

Bethermin, M. ^{[1
]}

Faisst, A. ^{[2
]}

Jones, G. C. ^{[15
,16
]}

Capak, P. ^{[2
,27
,28
]}

Cassata, P. ^{[4
,5
]}

Silverman, J. D. ^{[6
,32
]}

Schaerer, D. ^{[7
,8
]}

Yan, L. ^{[23
]}

Amorin, R. ^{[12
,13
]}

Bardelli, S. ^{[11
]}

Boquien, M. ^{[14
]}

Cimatti, A. ^{[9
,10
]}

Dessauges-Zavadsky, M. ^{[7
]}

Giavalisco, M. ^{[17
]}

Hathi, N. P. ^{[17
]}

Fudamoto, Y. ^{[7
,25
]}

Fujimoto, S. ^{[25
,26
]}

Ginolfi, M. ^{[7
]}

Gruppioni, C. ^{[11
]}

Hemmati, S. ^{[28
]}

Ibar, E. ^{[20
]}

Koekemoer, A. ^{[17
]}

Khusanova, Y. ^{[1
]}

Lagache, G. ^{[1
]}

Lemaux, B. C. ^{[3
]}

Loiacono, F. ^{[9
,11
]}

Maiolino, R. ^{[15
,16
]}

Mancini, C. ^{[4
,5
]}

Narayanan, D. ^{[27
,30
,31
]}

Morselli, L. ^{[4
]}

Mendez-Hernandez, Hugo ^{[20
]}

Oesch, P. A. ^{[7
]}

Pozzi, F. ^{[9
]}

Romano, M. ^{[4
]}

Riechers, D. ^{[22
,29
]}

Scoville, N. ^{[33
]}

Talia, M. ^{[9
,11
]}

Tasca, L. A. M. ^{[1
]}

Thomas, R. ^{[18
]}

Toft, S. ^{[27
,28
]}

Vallini, L. ^{[21
]}

Vergani, D. ^{[11
]}

Walter, F. ^{[23
]}

Zamorani, G. ^{[11
]}

Zucca, E. ^{[11
,19
,24
]}

机构：

[1] Aix Marseille Univ, CNRS, LAM Lab Astrophys Marseille, CNES, F-13013 Marseille, France

[2] CALTECH, IPAC, 1200 East Calif Blvd, Pasadena, CA 91125 USA

[3] Univ Calif Davis, Dept Phys, One Shields Ave, Davis, CA 95616 USA

[4] Univ Padua, Dipartimento Fis & Astron, Vicolo Osservatorio 3, I-35122 Padua, Italy

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

[6] Univ Tokyo, WPI, Kavli Inst Phys & Math Universe, Kashiwa, Chiba 2778583, Japan

[7] Univ Geneva, Dept Astron, Ch Maillettes 51, CH-1290 Versoix, Switzerland

[8] Univ Toulouse, CNRS, Inst Rech Astrophys & Planetol IRAP, UPS OMP, 14 Ave E Belin, F-31400 Toulouse, France

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

[10] Osserv Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy

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

[12] Univ La Serena, Inst Invest Multidisciplinar Ciencia & Tecnol, Raul Bitran 1305, La Serena, Chile

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

[14] Univ Antofagasta, Ctr Astron CITEVA, Ave Angamos 601, Antofagasta, Chile

[15] Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England

[16] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

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

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

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

[20] Univ Valparaiso, Inst Fis & Astron, Avda Gran Bretana 1111, Valparaiso, Chile

[21] Leiden Univ, Leiden Observ, POB 9500, NL-2300 RA Leiden, Netherlands

[22] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[23] CALTECH, Dept Astron, 1200 E Calif Blvd,MC 249-17, Pasadena, CA 91125 USA

[24] Waseda Univ, Dept Phys, Waseda Res Inst Sci & Engn Tokyo, Tokyo, Japan

[25] Waseda Univ, Res Inst Sci & Engn, Shinjuku Ku, 3-4-1 Okubo, Tokyo 1698555, Japan

[26] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan

[27] Cosm Dawn Ctr DAWN, Copenhagen, Denmark

[28] Univ Copenhagen, Niels Bohr Inst, Lyngbyvej 2, DK-2100 Copenhagen, Denmark

[29] Cornell Univ, Dept Astron, Space Sci Bldg, Ithaca, NY 14853 USA

[30] Univ Florida, Dept Astron, Bryant Space Sci Ctr 211, Gainesville, FL 32611 USA

[31] Univ Florida, Informat Inst, 432 Newell Dr,CISE Bldg E251, Gainesville, FL 32611 USA

[32] Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan

[33] CALTECH, Cahill Ctr Astrophys, 1216 East Calif Blvd, Pasadena, CA 91125 USA

来源：

ASTRONOMY & ASTROPHYSICS | 2020年 / 643卷

基金：

欧洲研究理事会; 美国国家科学基金会; 英国科学技术设施理事会; 新加坡国家研究基金会; 欧盟地平线“2020”;

关键词：

galaxies: evolution; galaxies: star formation; galaxies: formation; EVOLUTION SURVEY COSMOS; C II EMISSION; MAIN-SEQUENCE; BILLION YEARS; BLACK-HOLES; COOL GAS; REDSHIFT; SIMULATIONS; FIELD; FRAMEWORK;

D O I：

10.1051/0004-6361/201936965

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) features 118 galaxies observed in the [CII]-158 mu m line and far infrared (FIR) continuum emission during the period of rapid mass assembly, right after the end of the HI reionization, at redshifts of 4< z< 6. We present the survey science goals, the observational strategy, and the sample selection of the 118 galaxies observed with ALMA, with an average beam minor axis of about 0.85 '', or similar to 5 kpc at the median redshift of the survey. The properties of the sample are described, including spectroscopic redshifts derived from the UV-rest frame, stellar masses, and star-formation rates obtained from a spectral energy distribution (SED) fitting. The observed properties derived from the ALMA data are presented and discussed in terms of the overall detection rate in [CII] and FIR continuum, with the observed signal-to-noise distribution. The sample is representative of the SFG population in the main sequence at these redshifts. The overall detection rate in [CII] is 64% for a signal-to-noise ratio (S/N) threshold larger than 3.5 corresponding to a 95% purity (40% detection rate for S/N> 5). Based on a visual inspection of the [CII] data cubes together with the large wealth of ancillary data, we find a surprisingly wide range of galaxy types, including 40% that are mergers, 20% extended and dispersion-dominated, 13% compact, and 11% rotating discs, with the remaining 16% too faint to be classified. This diversity indicates that a wide array of physical processes must be at work at this epoch, first and foremost, those of galaxy mergers. This paper sets a reference sample for the gas distribution in normal SFGs at 4< z< 6, a key epoch in galaxy assembly, which is ideally suited for studies with future facilities, such as the James Webb Space Telescope (JWST) and the Extremely Large Telescopes (ELTs).

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页数：19

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The ALPINE-ALMA [CII] survey Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 &lt; z &lt; 6

The ALPINE-ALMA [CII] survey Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6