Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71Herscheltargets

Author:

Hagimoto M1ORCID,Bakx T J L C12ORCID,Serjeant S3ORCID,Bendo G J4ORCID,Urquhart S A3,Eales S5,Harrington K C6ORCID,Tamura Y1ORCID,Umehata H17,Berta S8,Cooray A R9,Cox P10,De Zotti G11ORCID,Lehnert M D12,Riechers D A13,Scott D14,Temi P15,van der Werf P P16,Yang C17,Amvrosiadis A18,Andreani P M19ORCID,Baker A J2021,Beelen A22ORCID,Borsato E23,Buat V22ORCID,Butler K M16,Dannerbauer H2425,Dunne L5,Dye S26ORCID,Enia A F M2728ORCID,Fan L293031,Gavazzi R1032,González-Nuevo J3334,Harris A I35,Herrera C N8,Hughes D H36,Ismail D22,Ivison R J19ORCID,Jones B13ORCID,Kohno K3738ORCID,Krips M8,Lagache G22,Marchetti L3940ORCID,Massardi M4041,Messias H642ORCID,Negrello M5,Neri R8,Omont A10,Perez-Fournon I2425,Sedgwick C3,Smith M W L5ORCID,Stanley F10,Verma A43,Vlahakis C44,Ward B5,Weiner C3,Weiß A45,Young A J20

Affiliation:

1. Department of Physics, Graduate School of Science, Nagoya University , Nagoya, Aichi 464-8602, Japan

2. National Astronomical Observatory of Japan , 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan

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

4. UK ALMA Regional Centre Node, Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester , Oxford Road, Manchester M13 9PL, UK

5. School of Physics and Astronomy, Cardiff University , The Parade, Cardiff CF24 3AA, UK

6. European Southern Observatory , Alonso de Córdova 3107, Vitacura, Casilla 19001, Santiago de Chile, Chile

7. Institute for Advanced Research, Nagoya University , Furocho, Chikusa, Nagoya 464-8602, Japan

8. Institut de Radioastronomie Millimétrique (IRAM) , 300 Rue de la Piscine, F-38400 Saint-Martin-d’Hères, France

9. Department of Physics & Astronomy, University of California , Irvine, 4129 Reines Hall, Irvine, CA 92697, USA

10. Institut d’Astrophysique de Paris, Sorbonne Université,UPMC Université Paris 6 and CNRS , UMR 7095, 98 bis boulevard Arago, F-75014 Paris, France

11. INAF – Osservatorio Astronomico di Padova , Vicolo dell’Osservatorio 5, I-35122 Padova, Italy

12. Centre de Recherche Astrophysique de Lyon, ENS de Lyon, Université Lyon 1, CNRS, UMR5574 , F-69230 Saint-Genis-Laval, France

13. I. Physikalisches Institut, Universität zu Köln , Zülpicher Strasse 77, D-50937 Köln, Germany

14. Department of Physics and Astronomy, University of British Columbia , 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada

15. Astrophysics Branch, NASA–Ames Research Center , MS 245-6, Moffett Field, CA 94035, USA

16. Leiden Observatory, Leiden University , PO Box 9513, NL-2300 RA Leiden, the Netherlands

17. Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Observatory , SE-439 94 Onsala, Sweden

18. Department of Physics, Centre for Extragalactic Astronomy, Durham University , South Road, Durham DH1 3LE, UK

19. European Southern Observatory , Karl Schwarzschild Strasse 2, D-85748 Garching, Germany

20. Department of Physics and Astronomy, Rutgers, the State University of New Jersey , 136 Frelinghuysen Road, Piscataway, NJ 08854-8019, USA

21. Department of Physics and Astronomy, University of the Western Cape , Robert Sobukwe Road, Bellville 7535, South Africa

22. Aix-Mar seille Univer sitè, CNRS and CNES, Laboratoire d’Astrophysique de Marseille , 38, rue Frèdèric Joliot-Curie, F-13388 Marseille, France

23. Dipartimento di Fisica e Astronomia ‘G. Galilei’, Universit’di Padova , Vicolo dell’Osservatorio 3, I-35122 Padova, Italy

24. Instituto Astrofísica de Canarias (IAC) , E-38205 La Laguna, Tenerife, Spain

25. Departomento de Astrofísica, Universidad de La Laguna , E-38206 La Laguna, Tenerife, Spain

26. School of Physics & Astronomy, University of Nottingham, University Park , Nottingham NG7 2RD, UK

27. Department of Physics and Astronomy ‘Augusto Righi’ (DIFA), University of Bologna , Via Gobetti 93/2, I-40129 Bologna, Italy

28. INAF–Osservatorio di Astrofisica e Scienza dello Spazio , Via Gobetti 93/3, I-40129 Bologna, Italy

29. CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China , Hefei 230026, People’s Republic of China

30. School of Astronomy and Space Sciences, University of Science and Technology of China , Hefei, Anhui 230026, People’s Republic of China

31. Institute of Deep Space Sciences, Deep Space Exploration Laboratory , Hefei 230026, People’s Republic of China

32. Institute of Astronomy, University of Cambridge , Madingley Road, Cambridge CB30HA, UK

33. Departamento de Fisica, Universidad de Oviedo , C. Federico Garcia Lorca 18, E-33007 Oviedo, Spain

34. Instituto Universitario de Ciencias y Tecnologas Espaciales de Asturias (ICTEA) , C. Independencia 13, E-33004 Oviedo, Spain

35. Department of Astronomy, University of Maryland , College Park, MD 20742, USA

36. Instituto Nacional de Astrofísica, Óptica y Electrónica , Tonantzintla, 72000 Puebla, México

37. Institute of Astronomy, Graduate School of Science, The University of Tokyo , 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan

38. Research Center for the Early Universe, Graduate School of Science, The University of Tokyo , 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

39. Department of Astronomy, University of Cape Town , Private Bag X3, Rondebosch 7701, Cape Town, South Africa

40. INAF, Instituto di Radioastronomia-Italian ARC , Via Piero Gobetti 101, I-40129 Bologna, Italy

41. SISSA , Via Bonomea 265, I-34136 Trieste, Italy

42. Joint ALMA Observatory , Alonso de Córdova 3107, Vitacura 763-0355, Santiago de Chile, Chile

43. Sub-department of Astrophysics, University of Oxford, Denys Wilkinson Building , Keble Road, Oxford OX1 3RH, UK

44. National Radio Astronomy Observatory , 520 Edgemont Road, Charlottesville, VA 22903, USA

45. Max-Planck-Institut für Radioastronomie , Auf dem Hügel 69, D-53121 Bonn, Germany

Abstract

ABSTRACTWe analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies between redshifts 1.4 and 4.6 detected by the Atacama Large Millimeter/submillimeter Array. These lines include a total of 156 CO, [C i], and H2O emission lines. For 46 galaxies, we detect two transitions of CO lines, and for these galaxies we find gas properties similar to those of other dusty star-forming galaxy (DSFG) samples. A comparison to photodissociation models suggests that most of Herschel-selected galaxies have similar interstellar medium conditions as local infrared-luminous galaxies and high-redshift DSFGs, although with denser gas and more intense far-ultraviolet radiation fields than normal star-forming galaxies. The line luminosities agree with the luminosity scaling relations across five orders of magnitude, although the star formation and gas surface density distributions (i.e. Schmidt–Kennicutt relation) suggest a different star formation phase in our galaxies (and other DSFGs) compared to local and low-redshift gas-rich, normal star-forming systems. The gas-to-dust ratios of these galaxies are similar to Milky Way values, with no apparent redshift evolution. Four of 46 sources appear to have CO line ratios in excess of the expected maximum (thermalized) profile, suggesting a rare phase in the evolution of DSFGs. Finally, we create a deep stacked spectrum over a wide rest-frame frequency (220–890 GHz) that reveals faint transitions from HCN and CH, in line with previous stacking experiments.

Funder

National Astronomical Observatory of Japan

Japan Society for the Promotion of Science

European Union

Science and Technology Facilities Council

European Research Council

AEI

ERDF

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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