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 WISE photometry to identify bright QSOs at z>2, the redshift regime for which the Lyman-α 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 M1450,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⊙ and 1.3±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