Multiwavelength properties of 850-μm selected sources from the North Ecliptic Pole SCUBA-2 survey

Author:

Shim Hyunjin1ORCID,Lee Dongseob1,Kim Yeonsik2,Scott Douglas3,Serjeant Stephen4ORCID,Ao Yiping56,Barrufet Laia78,Chapman Scott C39,Clements David L10ORCID,Conselice Christopher J11,Goto Tomotsugu12,Greve Thomas R131415,Hwang Ho Seong1617,Im Myungshin17ORCID,Jeong Woong-Seob18,Kim Helen K19,Kim Minjin2,Kim Seong Jin12ORCID,Kong Albert K H12ORCID,Koprowski Maciej P20,Malkan Matthew A19,Michałowski Michał J21,Pearson Chris4815ORCID,Seo Hyunjong18ORCID,Takagi Toshinobu22,Toba Yoshiki232425ORCID,White Glenn J48,Woo Jong-Hak16

Affiliation:

1. Department of Earth Science Education, Kyungpook National University , Daegu 41566, Republic of Korea

2. Department of Astronomy and Atmospheric Sciences, Kyungpook National University , Daegu 41566, Republic of Korea

3. Department of Physics and Astronomy, University of British Columbia , Vancouver, BC V6T 1Z1, Canada

4. School of Physical Sciences, The Open University , Milton Keynes, MK7 6AA, UK

5. Purple Mountain Observatory and Key Laboratory for Radio Astronomy, Chinese Academy of Sciences , Nanjing, 210033, China

6. School of Astronomy and Space Science, University of Science and Technology of China , Hefei, Anhui, 230026, China

7. Geneva Observatory, University of Geneva , 1290 Versoix, Switzerland

8. RAL Space, STFC Rutherford Appleton Laboratory , Didcot, Oxfordshire OX11 0QX, UK

9. Department of Physics and Atmospheric Science, Dalhouise University , Halifax NS B3H 4R2, Canada

10. Imperial College London , Blackett Lab., Prince Consort Road, London SW7 2AZ, UK

11. Department of Physics and Astronomy, University of Manchester , Manchester M13 9PL, UK

12. Institute of Astronomy, National Tsing Hua University , 101, Section 2. Kuang-Fu Road, Hsinchu 30013, Taiwan (R.O.C.)

13. Cosmic Dawn Center (DAWN), Technical University of Denmark , DK-2800 Kgs. Lyngby, Denmark

14. National Space Institute, DTU Space, Technical University of Denmark , Elektrovej 327, DK-2800 Kgs. Lyngby, Denmark

15. Department of Physics and Astronomy, University College London , Gower Street, London WC1E 6BT, UK

16. Astronomy Program, Department of Physics and Astronomy, Seoul National University , 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Republic of Korea

17. SNU Astronomy Research Center, Astronomy Program, Department of Physics and Astronomy, Seoul National University , Seoul 08826, Republic of Korea

18. Korea Astronomy and Space Science Institute , Daejeon 34055, Republic of Korea

19. Department of Physics and Astronomy, UCLA , Los Angeles, CA 90095-1547, USA

20. Institute of Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University , Grudziadzka 5, PL-87-100 Torun, Poland

21. Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University , ul. Słoneczna 36, PL-60-286 Poznań, Poland

22. Japan Science Forum , 3-2-1, Kandasurugadai, Chiyoda-ku, Tokyo 101-0062, Japan

23. Department of Astronomy, Kyoto University , Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502, Japan

24. Academia Sinica Institute of Astronomy and Astrophysics , 11F of Astronomy-Mathematics Building, AS/NTU, No.1, Section 4, Roosevelt Road, Taipei 10617, Taiwan

25. Research Center for Space and Cosmic Evolution, Ehime University , 2-5 Bunkyo-cho, Matsuyama, Ehime 790-8577, Japan

Abstract

ABSTRACT We present the multiwavelength counterparts of 850-$\mu$m selected submillimetre sources over a 2-deg2 field centred on the North Ecliptic Pole. In order to overcome the large beam size (15 arcsec) of the 850-$\mu$m images, deep optical to near-infrared (NIR) photometric data and arcsecond-resolution 20-cm images are used to identify counterparts of submillimetre sources. Among 647 sources, we identify 514 reliable counterparts for 449 sources (69 per cent in number), based either on probabilities of chance associations calculated from positional offsets or offsets combined with the optical-to-NIR colours. In the radio imaging, the fraction of 850-$\mu$m sources having multiple counterparts is 7 per cent. The photometric redshift, infrared luminosity, stellar mass, star formation rate (SFR), and the active galactic nucleus (AGN) contribution to the total infrared luminosity of the identified counterparts are investigated through spectral energy distribution fitting. The SMGs are infrared-luminous galaxies at an average 〈z〉 = 2.5 with log10(LIR/L⊙) = 11.5–13.5, with a mean stellar mass of log10(Mstar/M⊙) = 10.90 and SFR of $\mathrm{log}_{10} (\mathrm{SFR/M_\odot \, yr^{-1}})=2.34$. The submillimetre galaxies (SMGs) show twice as large SFR as galaxies on the star-forming main sequence, and about 40 per cent of the SMGs are classified as objects with bursty star formation. At z ≥ 4, the contribution of AGN luminosity to total luminosity for most SMGs is larger than 30 per cent. The FIR-to-radio correlation coefficient of SMGs is consistent with that of main-sequence galaxies at z ≃ 2.

Funder

NSFC

NRF

MSIT

National Science Centre

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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