An Extremely Bright QSO at z = 2.89
Abstract
We report the discovery and confirmation of a bright quasi-stellar object (QSO), 2MASS J13260399 + 7023462, at $z=2.889$ . This QSO is the first spectroscopically confirmed candidate from an ongoing search using the combination of Gaia and Wide-field Infrared Survey Explorer photometry to identify bright QSOs at z > 2, the redshift regime for which the Lyα forest is accessible with ground-based facilities. With a Gaia apparent magnitude G = 16.07, 2MASS J13260399 + 7023462 is one of the brightest QSOs known at z > 2, with only 15 currently known brighter QSOs. Given its inferred ${M}_{1450,\mathrm{AB}}$ magnitude and redshift, it is among the most luminous objects in the universe; the inferred black hole mass and corresponding Eddington ratio are (2.7 ± 0.4) × 1010 ${M}_{\odot }$ and 1.3 ± 0.3, respectively. Follow-up Hubble observations confirm it is not gravitationally lensed.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- August 2020
- DOI:
- 10.3847/1538-4357/ab9c95
- arXiv:
- arXiv:2006.11915
- Bibcode:
- 2020ApJ...899...76J
- Keywords:
-
- Quasars;
- Radio quiet quasars;
- Supermassive black holes;
- High-luminosity active galactic nuclei;
- 1319;
- 1354;
- 1663;
- 2034;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 8 pages, 8 figures, 1 table, Accepted for publication in ApJ