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The ALMA Spectroscopic Survey in the HUDF: A Search for [C ii] Emitters at 6 ≤ z ≤ 8

文献类型:期刊论文

作者Uzgil,Bade D.12,13; Oesch,Pascal A.14,15; Walter,Fabian13,16; Aravena,Manuel17; Boogaard,Leindert18; Carilli,Chris13; Decarli,Roberto19; Díaz-Santos,Tanio17,20,21; Fudamoto,Yoshi14; Inami,Hanae1
刊名The Astrophysical Journal
出版日期2021-05-01
卷号912期号:1
ISSN号0004-637X
关键词High-redshift galaxies Interstellar medium
DOI10.3847/1538-4357/abe86b
英文摘要Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Band 6 scan (212–272 GHz) covers potential [C ii] emission in galaxies at 6 ≤ z ≤ 8 throughout a 2.9 arcmin2 area. By selecting on known Lyα emitters (LAEs) and photometric dropout galaxies in the field, we perform targeted searches down to a 5σ [C ii] luminosity depth L[C II] ~ 2.0 × 108 L⊙, corresponding roughly to star formation rates (SFRs) of 10–20 M⊙ yr?1 when applying a locally calibrated conversion for star-forming galaxies, yielding zero detections. While the majority of galaxies in this sample are characterized by lower SFRs, the resulting upper limits on [C ii] luminosity in these sources are consistent with the current literature sample of targeted ALMA observations of z = 6–7 LAEs and Lyman-break galaxies (LBGs), as well as the locally calibrated relations between L[C ii] and SFR—with the exception of a single [C ii]-deficient, UV-luminous LBG. We also perform a blind search for [C ii]-bright galaxies that may have been missed by optical selections, resulting in an upper limit on the cumulative number density of [C ii] sources with L[C II] > 2.0 × 108 L⊙ (5σ) to be less than 1.8 × 10?4 Mpc?3 (90% confidence level). At this luminosity depth and volume coverage, we present an observed evolution of the [C ii] luminosity function from z = 6–8 to z ~ 0 by comparing the ASPECS measurement to literature results at lower redshift.
语种英语
出版者The American Astronomical Society
WOS记录号IOP:0004-637X-912-1-ABE86B
源URL[http://ir.bao.ac.cn/handle/114a11/58210]  
专题中国科学院国家天文台
通讯作者Uzgil,Bade D.
作者单位1.Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan
2.Joint ALMA Observatory—ESO, Av. Alonso de Córdova, 3104, Santiago, Chile
3.National Radio Astronomy Observatory, 520 Edgemont Rd, Charlottesville, VA 22903, USA
4.Sorbonne Université, UPMC Université Paris 6 & CNRS, UMR 7095, Institut d’Astrophysique de Paris, 98b boulevard Arago, F-75014 Paris, France
5.Laboratoire AIM, CEA/DSM-CNRS-Université Paris, France
6.Las Campanas Observatory, Carnegie Institution of Washington, Casilla 601, La Serena, Chile
7.Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, VIC 3122, Australia
8.European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748, Garching, Germany
9.Max-Planck-Institut für Radioastronomie, Auf dem Hügel 71, D-53121 Bonn, Germany
10.Max-Planck-Institut für Astronomie, K?nigstuhl 17, D-69117 Heidelberg, Germany
推荐引用方式
GB/T 7714
Uzgil,Bade D.,Oesch,Pascal A.,Walter,Fabian,et al. The ALMA Spectroscopic Survey in the HUDF: A Search for [C ii] Emitters at 6 ≤ z ≤ 8[J]. The Astrophysical Journal,2021,912(1).
APA Uzgil,Bade D..,Oesch,Pascal A..,Walter,Fabian.,Aravena,Manuel.,Boogaard,Leindert.,...&Weiss,Axel.(2021).The ALMA Spectroscopic Survey in the HUDF: A Search for [C ii] Emitters at 6 ≤ z ≤ 8.The Astrophysical Journal,912(1).
MLA Uzgil,Bade D.,et al."The ALMA Spectroscopic Survey in the HUDF: A Search for [C ii] Emitters at 6 ≤ z ≤ 8".The Astrophysical Journal 912.1(2021).

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来源:国家天文台

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