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 |
DOI | 10.3847/1538-4357/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). |
入库方式: OAI收割
来源:国家天文台
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