The clustering of H β + [O iii] and [O ii] emitters since z ∼ 5: dependencies with line luminosity and stellar mass

Author:

Khostovan A A1,Sobral D23ORCID,Mobasher B1,Best P N4,Smail I56,Matthee J3,Darvish B7,Nayyeri H8,Hemmati S9,Stott J P210ORCID

Affiliation:

1. Department of Physics & Astronomy, University of California, Riverside, USA

2. Department of Physics, Lancaster University, Lancaster, LA1 4YB, UK

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

4. SUPA, Institute for Astronomy, Royal Observatory of Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK

5. Centre for Extragalactic Astrophysics, Department of Physics, Durham University, Durham DH1 3LE, UK

6. Institute for Computational Cosmology, Durham University, Durham DH1 3LE, UK

7. Cahill Center for Astronomy and Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA

8. Department of Physics & Astronomy, University of California, Irvine, CA 92697, USA

9. Infrared Processing and Analysis Center, California Institute of Technology, Pasadena, CA 91125, USA

10. Sub-department of Astrophysics, Department of Physics, University of Oxford, Oxford OX1 3RH, UK

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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