Title | EXPLORATORY CHANDRA OBSERVATION OF THE ULTRALUMINOUS QUASAR SDSS J010013.02+280225.8 AT REDSHIFT 6.30 |
Authors | Ai, Yanli Dou, Liming Fan, Xiaohui Wang, Feige Wu, Xue-Bing Bian, Fuyan |
Affiliation | Sun Yat Sen Univ, Sch Phys & Astron, Guangzhou 510275, Guangdong, Peoples R China. Univ Sci & Technol China, Dept Astron, Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China. Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA. Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China. Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China. Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia. |
Keywords | quasars: individual (SDSS J010013.02+280225.8) DIGITAL SKY SURVEY ACTIVE GALACTIC NUCLEI EMISSION-LINE QUASARS X-RAY INSIGHTS BLACK-HOLE ACCRETION RATES EDDINGTON RATIO DATA RELEASE FINAL DATA DISCOVERY |
Issue Date | 2016 |
Publisher | ASTROPHYSICAL JOURNAL LETTERS |
Citation | ASTROPHYSICAL JOURNAL LETTERS.2016,823,(2). |
Abstract | We report exploratory Chandra observations of the ultraluminous quasar SDSS J010013.02+280225.8 at redshift 6.30. The quasar is clearly detected by Chandra with a possible component of extended emission. The rest-frame 2-10 keV luminosity is 9.0(+4.5)(+9.1) x 10(45) erg s(-1) with an inferred photon index of G = 3.03(-0.70)(+0.78). This quasar is X-ray bright, with an inferred X-ray-to-optical flux ratio alpha(ox) = -1.22(-0.05)(+0.07), higher than the values found in other quasars of comparable ultraviolet luminosity. The properties inferred from this exploratory observation indicate that this ultraluminous quasar might be growing with super-Eddington accretion and probably viewed with a small inclination angle. Deep X-ray observations will help to probe the plausible extended emission and better constrain the spectral features for this ultraluminous quasar. |
URI | http://hdl.handle.net/20.500.11897/438117 |
ISSN | 2041-8205 |
DOI | 10.3847/2041-8205/823/2/L37 |
Indexed | SCI(E) |
Appears in Collections: | 科维理天文与天体物理研究所 物理学院 |