دورية أكاديمية

An Extremely Bright QSO at z = 2.89.

التفاصيل البيبلوغرافية
العنوان: An Extremely Bright QSO at z = 2.89.
المؤلفون: Jeram, Sarik, Gonzalez, Anthony, Eikenberry, Stephen, Stern, Daniel, Oliveira, Claudia Lucia Mendes de, Nakazono, Lilianne Mariko Izuti, Ackley, Kendall
المصدر: Astrophysical Journal; 8/10/2020, Vol. 899 Issue 1, p1-6, 6p
مصطلحات موضوعية: BLACK holes, ASTRONOMICAL photometry, UNIVERSE, PHOTOMETRY
مستخلص: We report the discovery and confirmation of a bright quasi-stellar object (QSO), 2MASS J13260399 + 7023462, at. 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 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 and 1.3 ± 0.3, respectively. Follow-up Hubble observations confirm it is not gravitationally lensed. [ABSTRACT FROM AUTHOR]
Copyright of Astrophysical Journal is the property of IOP Publishing and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
قاعدة البيانات: Complementary Index
الوصف
تدمد:0004637X
DOI:10.3847/1538-4357/ab9c95