ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Source catalog and number counts
文献类型:期刊论文
作者 | Hatsukade, Bunyo1; Kohno, Kotaro1,2; Yamaguchi, Yuki1; Umehata, Hideki1,3; Ao, Yiping4,5; Aretxaga, Itziar6; Caputi, Karina I.7; Dunlop, James S.8; Egami, Eiichi9; Espada, Daniel10,11 |
刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN |
出版日期 | 2018-12-01 |
卷号 | 70期号:6页码:20 |
ISSN号 | 0004-6264 |
关键词 | cosmology: observations galaxies: evolution galaxies: formation galaxies: high-redshift submillimeter: galaxies |
DOI | 10.1093/pasj/psy104 |
通讯作者 | Hatsukade, Bunyo(hatsukade@ioa.s.u-tokyo.ac.jp) |
英文摘要 | We present the survey design, data reduction, construction of images, and source catalog of the Atacama Large Millimeter/submillimeter Array (ALMA) twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO). ASAGAO is a deep (1 sigma depth similar to 61 mu Jy beam(-1) for a 250 k lambda-tapered map with a synthesized beam size of 0.'' 51 x 0.'' 45) and wide area (26 arcmin(2)) survey on a contiguous field at 1.2 mm. By combining with ALMA archival data in the GOODS-South field, we obtained a deeper map in the same region (1 sigma size similar to 30 mu Jy beam(-1) for a deep region with a 250 k lambda-taper, and a synthesized beam size of 0.'' 59 x 0.'' 53), providing the largest sample of sources (25 sources at >= 5.0 sigma, 45 sources at >= 4.5 sigma) among ALMA blank-field surveys to date. The number counts shows that 52(-8)(+11)% of the extragalactic background light at 1.2 mm is resolved into discrete sources at S-1.2 mm > 135 mu Jy. We create infrared (IR) luminosity functions (LFs) in the redshift range of z = 1-3 from the ASAGAO sources with K-s-band counterparts, and constrain the faintest luminosity of the LF at 2.0 < z < 3.0. The LFs are consistent with previous results based on other ALMA and SCUBA-2 observations, which suggest a positive luminosity evolution and negative density evolution with increasing redshift. We find that obscured star-formation of sources with IR luminosities of log (L-IR/L-circle dot) greater than or similar to 11.8 account for approximate to 60%-90% of the z similar to 2 cosmic star-formation rate density. |
WOS关键词 | DEGREE EXTRAGALACTIC SURVEY ; COSMOLOGY LEGACY SURVEY ; OBSCURED STAR-FORMATION ; SPECTROSCOPIC SURVEY ; LUMINOSITY FUNCTION ; SUBMILLIMETER MAPS ; REDSHIFT SURVEY ; SIMPLE-MODEL ; FIELD ; GALAXIES |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000456072300007 |
源URL | [http://libir.pmo.ac.cn/handle/332002/19954] |
专题 | 中国科学院紫金山天文台 |
通讯作者 | Hatsukade, Bunyo |
作者单位 | 1.Univ Tokyo, Grad Sch Sci, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan 2.Univ Tokyo, Res Ctr Early Universe, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan 3.RIKEN, Cluster Pioneering Res, 2-1 Hirosawa, Wako, Saitama 3510198, 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.INAOE, Luis Enrique Erro 1, Puebla, Mexico 7.Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands 8.Univ Edinburgh, Royal Observ, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland 9.Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85721 USA 10.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan |
推荐引用方式 GB/T 7714 | Hatsukade, Bunyo,Kohno, Kotaro,Yamaguchi, Yuki,et al. ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Source catalog and number counts[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2018,70(6):20. |
APA | Hatsukade, Bunyo.,Kohno, Kotaro.,Yamaguchi, Yuki.,Umehata, Hideki.,Ao, Yiping.,...&Yun, Min S..(2018).ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Source catalog and number counts.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,70(6),20. |
MLA | Hatsukade, Bunyo,et al."ALMA twenty-six arcmin(2) survey of GOODS-S at one millimeter (ASAGAO): Source catalog and number counts".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 70.6(2018):20. |
入库方式: OAI收割
来源:紫金山天文台
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