JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies - I. Survey overview and first results

被引：33

作者：

Saintonge, Amelie ^{[1
]}

Wilson, Christine D. ^{[2
]}

Xiao, Ting ^{[3
,4
]}

Lin, Lihwai ^{[5
]}

Hwang, Ho Seong ^{[6
]}

Tosaki, Tomoka ^{[7
]}

Bureau, Martin ^{[8
]}

Cigan, Phillip J. ^{[9
]}

Clark, Christopher J. R. ^{[9
]}

Clements, David L. ^{[10
]}

De Looze, Ilse ^{[1
,11
]}

Dharmawardena, Thavisha ^{[5
,12
]}

Gao, Yang ^{[4
]}

Gear, Walter K. ^{[9
]}

Greenslade, Joshua ^{[10
]}

Lamperti, Isabella ^{[1
]}

Lee, Jong Chul ^{[13
]}

Li, Cheng ^{[14
,15
]}

Michalowski, Michal J. ^{[16
,17
]}

Mok, Angus ^{[2
]}

Pan, Hsi-An ^{[5
]}

Sansom, Anne E. ^{[18
]}

Sargent, Mark ^{[19
]}

Smith, Matthew W. L. ^{[9
]}

Williams, Thomas ^{[9
]}

Yang, Chentao ^{[20
,21
]}

Zhu, Ming ^{[33
]}

Accurso, Gioacchino ^{[1
]}

Barmby, Pauline ^{[22
,23
]}

Brinks, Elias ^{[24
]}

Bourne, Nathan ^{[1
,16
]}

Brown, Toby ^{[2
]}

Chung, Aeree ^{[25
]}

Chung, Eun Jung ^{[13
]}

Cibinel, Anna ^{[19
]}

Coppin, Kristen ^{[24
]}

Davies, Jonathan ^{[9
]}

Davis, Timothy A. ^{[9
]}

Eales, Steve ^{[9
]}

Fanciullo, Lapo ^{[5
]}

Fang, Taotao ^{[26
,27
]}

Gao, Yu ^{[20
,21
]}

Glass, David H. W. ^{[18
]}

Gomez, Haley L. ^{[9
]}

Greve, Thomas ^{[1
]}

He, Jinhua ^{[28
,29
,30
]}

Ho, Luis C. ^{[31
,32
]}

Huang, Feng ^{[26
,27
]}

Jeong, Hyunjin ^{[13
]}

Jiang, Xuejian ^{[20
,21
]}

机构：

[1] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[2] McMaster Univ, Dept Phys & Astron, Hamilton, ON L8S 4M1, Canada

[3] Zhejiang Univ, Dept Phys, Hangzhou 310027, Zhejiang, Peoples R China

[4] Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China

[5] Acad Sinica, Inst Astron & Astrophys, POB 23-141, Taipei 10617, Taiwan

[6] Korea Inst Adv Study, Sch Phys, 85 Hoegiro, Seoul 02455, South Korea

[7] Joetsu Univ Educ, Yamayashiki Machi, Niigata 9438512, Japan

[8] Univ Oxford, Subdept Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England

[9] Cardiff Univ, Sch Phys & Astron, Queens Bldg, Cardiff CF24 3AA, S Glam, Wales

[10] Imperial Coll, Blackett Lab, Dept Phys, London SW7 2AZ, England

[11] Univ Ghent, Sterrenkundig Observ, Krijgslaan 281 S9, B-9000 Ghent, Belgium

[12] Natl Cent Univ, 300 Zhongda Rd, Taoyuan 32001, Taiwan

[13] Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea

[14] Tsinghua Univ, Tsinghua Ctr Astrophys, Beijing 100084, Peoples R China

[15] Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China

[16] Univ Edinburgh, Royal Observ, Inst Astron, SUPA, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

[17] Adam Mickiewicz Univ, Fac Phys, Astron Observ Inst, Ul Sloneczna 36, PL-60286 Poznan, Poland

[18] Univ Cent Lancashire, Jeremiah Horrocks Inst, Preston PR1 2HE, Lancs, England

[19] Univ Sussex, Dept Phys & Astron, Ctr Astron, Brighton BN1 9QH, E Sussex, England

[20] Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China

[21] Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China

[22] Univ Western Ontario, Dept Phys & Astron, London, ON N6A 3K7, Canada

[23] Univ Western Ontario, Ctr Planetary Sci & Explorat, London, ON N6A 3K7, Canada

[24] Univ Hertfordshire, Ctr Astrophys Res, Coll Lane, Hatfield AL10 9AB, Herts, England

[25] Yonsei Univ, Dept Astron, 50 Yonsei Ro, Seoul 03722, South Korea

[26] Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China

[27] Xiamen Univ, Inst Theoret Phys & Astrophys, Xiamen 361005, Peoples R China

[28] Chinese Acad Sci, Yunnan Observ, Key Lab Struct & Evolut Celestial Objects, POB 110, Kunming 650011, Yunnan, Peoples R China

[29] CASSACA, Camino El Observ 1515, Santiago, Chile

[30] Univ Chile, Dept Astron, Casilla 36-D, Santiago, Chile

[31] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China

[32] Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China

[33] Natl Astron Observ China, 20A Datun Rd, Beijing 100012, Peoples R China

[34] Natl Astron Observ Japan, Subaru Telescope, 650 North Aohoku Pl, Hilo, HI 96720 USA

[35] Univ Sci & Technol China, Dept Astron, Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China

[36] Univ Durham, Dept Phys, Inst Computat Cosmol, South Rd, Durham DH1 3LE, England

[37] Northwestern Univ, CIERA, 2145 Sheridan Rd, Evanston, IL 60201 USA

[38] Northwestern Univ, Dept Phys & Astron, 2145 Sheridan Rd, Evanston, IL 60201 USA

[39] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England

[40] Haverford Coll, Dept Phys & Astron, 370 Lancaster Ave, Haverford, PA 19041 USA

[41] Johns Hopkins Univ, Bloomberg Ctr, Dept Phys, Astron, 3400 N Charles St, Baltimore, MD 21218 USA

[42] Oberlin Coll, Dept Phys, Oberlin, OH 44074 USA

[43] Open Univ, Sch Phys Sci, Walton Hall, Milton Keynes MK7 6AA, Bucks, England

[44] Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210093, Jiangsu, Peoples R China

[45] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China

[46] Kyungpook Natl Univ, Dept Earth Sci Educ, 80 Daehak Ro, Daegu 41556, South Korea

[47] Royal Mil Coll Canada, Dept Phys, POB 17000, Kingston, ON K7K 7B4, Canada

[48] East Asian Observ, 660 North AOhoku Pl, Hilo, HI 96720 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2018年 / 481卷 / 03期

基金：

美国国家科学基金会; 英国科学技术设施理事会; 加拿大创新基金会; 欧盟地平线“2020”; 美国安德鲁·梅隆基金会; 加拿大自然科学与工程研究理事会; 欧洲研究理事会; 国家重点研发计划; 美国国家航空航天局;

关键词：

ISM: general; galaxies: evolution; galaxies: ISM; galaxies: photmetry; ARECIBO SDSS SURVEY; DIGITAL SKY SURVEY; STAR-FORMATION; ABSORPTION-COEFFICIENT; DATA RELEASE; TEMPERATURE-DEPENDENCE; PHYSICAL-PROPERTIES; INFRARED-EMISSION; MASSIVE GALAXIES; HERSCHEL-ATLAS;

D O I：

10.1093/mnras/sty2499

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

JINGLE is a new JCMT legacy survey designed to systematically study the cold interstellar medium of galaxies in the local Universe. As part of the survey we perform 850 mu m continuum measurements with SCUBA-2 for a representative sample of 193 Herschel-selected galaxies withM(*) > 10(9) M-circle dot, as well as integrated CO(2-1) line fluxes with RxA3m for a subset of 90 of these galaxies. The sample is selected from fields covered by the Herschel-ATLAS survey that are also targeted by the MaNGA optical integral-field spectroscopic survey. The new JCMT observations combined with the multiwavelength ancillary data will allow for the robust characterization of the properties of dust in the nearby Universe, and the benchmarking of scaling relations between dust, gas, and global galaxy properties. In this paper we give an overview of the survey objectives and details about the sample selection and JCMT observations, present a consistent 30-band UV-to-FIR photometric catalogue with derived properties, and introduce the JINGLE Main Data Release. Science highlights include the non-linearity of the relation between 850 mu m luminosity and CO line luminosity (log LCO(2-1) = 1.372 logL(850)-1.376), and the serendipitous discovery of candidate z > 6 galaxies.

引用

页码：3497 / 3519

页数：23

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