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

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