Ultra-luminous quasars at redshift z > 4.5 from SkyMapper

Author:

Wolf Christian12ORCID,Hon Wei Jeat3,Bian Fuyan4,Onken Christopher A12,Alonzi Noura35,Bessell Michael A1,Li Zefeng12,Schmidt Brian P12,Tisserand Patrick6

Affiliation:

1. Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia

2. ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)

3. School of Physics, University of Melbourne, Parkville, Victoria 3010, Australia

4. European Southern Observatory, Alonso de Córdova 3107, Vitacura, Santiago 19, Chile

5. Department of Physics and Astronomy, King Saud University, Riyadh 11451, Saudi Arabia

6. Institut d’Astrophysique de Paris, Sorbonne Universités, UPMC Univ Paris 6 et CNRS, 98 bis bd Arago, F-75014 Paris, France

Abstract

ABSTRACT The most luminous quasars at high-redshift harbour the fastest growing and most massive black holes in the early Universe. They are exceedingly rare and hard to find. Here, we present our search for the most luminous quasars in the redshift range from z = 4.5 to 5 using data from SkyMapper, Gaia, and WISE. We use colours to select likely high-redshift quasars and reduce the stellar contamination of the candidate set with parallax and proper motion data. In ∼12 500 deg2 of Southern sky, we find 92 candidates brighter than Rp = 18.2. Spectroscopic follow-up has revealed 21 quasars at z ≥ 4 (16 of which are within z = [4.5, 5]), as well as several red quasars, Broad-Absorption-Line (BAL) quasars and objects with unusual spectra, which we tentatively label OFeLoBALQSOs at redshifts of z ≈ 1 to 2. This work lifts the number of known bright z ≥ 4.5 quasars in the Southern hemisphere from 10 to 26 and brings the total number of quasars known at Rp < 18.2 and z ≥ 4.5 to 42.

Funder

ARC

NASA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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