SDSS J013127.34032100.1: A newly discovered radio-loud quasar at with extremely high luminosity
arXiv:1410.2689 · doi:10.1088/2041-8205/795/2/L29
Abstract
Only very few z>5 quasars discovered to date are radio-loud, with a radio-to-optical flux ratio (radio-loudness parameter) higher than 10. Here we report the discovery of an optically luminous radio-loud quasar, SDSS J013127.34-032100.1 (J0131-0321 in short), at z=5.18+-0.01 using the Lijiang 2.4m and Magellan telescopes. J0131-0321 has a spectral energy distribution consistent with that of radio-loud quasars. With an i-band magnitude of 18.47 and radio flux density of 33 mJy, its radio-loudness parameter is ~100. The optical and near-infrared spectra taken by Magellan enable us to estimate its bolometric luminosity to be L_bol ~ 1.1E48 erg/s, approximately 4.5 times greater than that of the most distant quasar known to date. The black hole mass of J0131-0321 is estimated to be 2.7E9 solar masses, with an uncertainty up to 0.4 dex. Detailed physical properties of this high-redshift, radio-loud, potentially super-Eddington quasar can be probed in the future with more dedicated and intensive follow-up observations using multi-wavelength facilities.
5 pages, 3 figures, accepted to ApJL
References in corpus (7)
- A Catalog of Quasar Properties from SDSS DR7
- A luminous quasar at a redshift of z = 7.085
- Biases in Virial Black Hole Masses: An SDSS Perspective
- Gemini Near-infrared Spectroscopy of Luminous z~6 Quasars: Chemical Abundances, Black Hole Masses, and MgII Absorption
- The Radio-Loud Fraction of Quasars is a Strong Function of Redshift and Optical Luminosity
- Chandra Observations of the Highest Redshift Quasars from the Sloan Digital Sky Survey
- High-resolution images of five radio quasars at early cosmological epochs
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