English

An Extremely Bright QSO at $z=2.89$

Astrophysics of Galaxies 2020-08-19 v1

Abstract

We report the discovery and confirmation of a bright quasi-stellar object (QSO), 2MASS J13260399+7023462, at z=2.889z=2.889. This QSO is the first spectroscopically confirmed candidate from an ongoing search using the combination of Gaia and WISE photometry to identify bright QSOs at z>2z>2, the redshift regime for which the Lyman-α\alpha forest is accessible with ground-based facilities. With a Gaia apparent magnitude G=16.07G=16.07, 2MASS J13260399+7023462 is one of the brightest QSOs known at z>2z>2, with only 15 currently known brighter QSOs. Given its inferred M1450,ABM_{1450,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±0.42.7 \pm 0.4) ×\times 1010^{10} M_{\odot} and 1.3±0.31.3 \pm 0.3, respectively. Follow-up Hubble observations confirm it is not gravitationally lensed.

Cite

@article{arxiv.2006.11915,
  title  = {An Extremely Bright QSO at $z=2.89$},
  author = {Sarik Jeram and Anthony Gonzalez and Stephen Eikenberry and Daniel Stern and Claudia Lucia Mendes de Oliveira and Lilianne Mariko Izuti Nakazono and Kendall Ackley},
  journal= {arXiv preprint arXiv:2006.11915},
  year   = {2020}
}

Comments

8 pages, 8 figures, 1 table, Accepted for publication in ApJ

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