中国科学院机构知识库网格
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ALMA 26 arcmin(2) Survey of GOODS-S at 1mm (ASAGAO): Near-infrared-dark Faint ALMA Sources

文献类型:期刊论文

AuthorYamaguchi, Yuki1; Kohno, Kotaro1,2; Hatsukade, Bunyo1; Wang, Tao1,3; Yoshimura, Yuki1; Ao, Yiping4,5; Caputi, Karina, I6; Dunlop, James S.7; Egami, Eiichi8; Espada, Daniel3,9
SourceASTROPHYSICAL JOURNAL
Issued Date2019-06-10
Volume878Issue:1Pages:8
ISSN0004-637X
Keywordgalaxies: evolution galaxies: high-redshift galaxies: star formation submillimeter: galaxies
DOI10.3847/1538-4357/ab0d22
Corresponding AuthorYamaguchi, Yuki(yyamaguchi@ioa.s.u-tokyo.ac.jp)
English AbstractWe report detections of two 1.2 mm continuum sources (S-1.2 mm similar to 0.6 mJy) without any counterparts in the deep H- and/or K-band image (i.e., K-band magnitude greater than or similar to 26 mag). These near-infrared-dark faint millimeter sources are uncovered by ASAGAO, a deep and wide-field (similar or equal to 26 arcmin(2)) Atacama Large Millimeter/submillimeter Array (ALMA) 1.2 mm survey. One has a red IRAC (3.6 and 4.5 mu m) counterpart, and the other has been independently detected at 850 and 870 mu m using SCUBA2 and ALMA Band 7, respectively. Their optical-to-radio spectral energy distributions indicate that they can lie at z greater than or similar to 3-5 and can be in the early phase of massive galaxy formation. Their contribution to the cosmic star formation rate density is estimated to be similar to 1 x 10(-3) M-circle dot yr(-1) Mpc(-3) if they lie somewhere in the redshift range of z similar to 3-5. This value can be consistent with, or greater than, that of bright submillimeter galaxies (S-870 mu m > 4.2 mJy) at z similar to 3-5. We also uncover three more candidate near-infrared-dark faint ALMA sources without any counterparts (S-1.2 mm similar to 0.45-0.86 mJy). These results show that an unbiased ALMA survey can reveal the dust-obscured star formation activities, which were missed in previous deep optical/near-infrared surveys.
WOS KeywordSPECTRAL ENERGY-DISTRIBUTION ; GALAXIES ; CAMERA ; IRAC
WOS Research AreaAstronomy & Astrophysics
Language英语
WOS IDWOS:000471729200011
PublisherIOP PUBLISHING LTD
源URL[http://libir.pmo.ac.cn/handle/332002/27493]  
Collection中国科学院紫金山天文台
Corresponding AuthorYamaguchi, Yuki
Affiliation1.Univ Tokyo, Grad Sch Sci, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan
2.Univ Tokyo, Res Ctr Early Universe, Grad Sch Sci, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan
3.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
4.Chinese Acad Sci, Purple Mt Observ, 8 Yuanhua Rd, Nanjing 210034, Jiangsu, Peoples R China
5.Chinese Acad Sci, Key Lab Radio Astron, 8 Yuanhua Rd, Nanjing 210034, Jiangsu, Peoples R China
6.Univ Groningen, Kapten Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands
7.Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland
8.Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA
9.Grad Univ Adv Studies, SOKENDAI, Dept Astron Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
10.Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
Recommended Citation
GB/T 7714
Yamaguchi, Yuki,Kohno, Kotaro,Hatsukade, Bunyo,et al. ALMA 26 arcmin(2) Survey of GOODS-S at 1mm (ASAGAO): Near-infrared-dark Faint ALMA Sources[J]. ASTROPHYSICAL JOURNAL,2019,878(1):8.
APA Yamaguchi, Yuki.,Kohno, Kotaro.,Hatsukade, Bunyo.,Wang, Tao.,Yoshimura, Yuki.,...&Yun, Min S..(2019).ALMA 26 arcmin(2) Survey of GOODS-S at 1mm (ASAGAO): Near-infrared-dark Faint ALMA Sources.ASTROPHYSICAL JOURNAL,878(1),8.
MLA Yamaguchi, Yuki,et al."ALMA 26 arcmin(2) Survey of GOODS-S at 1mm (ASAGAO): Near-infrared-dark Faint ALMA Sources".ASTROPHYSICAL JOURNAL 878.1(2019):8.

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