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Related papers: X-rays from the redshift 7.1 quasar ULAS J1120+064…

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A brief Chandra observation of the ultraluminous quasar, SDSS J010013.02+280225.8 at redshift 6.326, showed it to be a relatively bright, soft X-ray source with a count rate of about 1 ct/ks. In this paper we present results for the quasar…

Astrophysics of Galaxies · Physics 2017-07-19 Yanli Ai , A. C. Fabian , Xiaohui Fan , S. A. Walker , G. Ghisellini , T. Sbarrato , Liming Dou , Feige Wang , Xue-Bing Wu , Longlong Feng

We aim at probing the emission mechanism of the accreting super massive black holes in the high redshift Universe. We study the X-ray spectrum of ULAS1120+0641, the highest redshift quasar detected so far at z=7.085, which has been deeply…

Astrophysics of Galaxies · Physics 2015-06-18 A. Moretti , L. Ballo , V. Braito , A. Caccianiga , R. Della Ceca , R. Gilli , R. Salvaterra , P. Severgnini , C. Vignali

We report on Chandra and XMM-Newton observations of a sample of 13 quasars at z~4.7-5.4 mostly taken from the Sloan Digital Sky Survey (SDSS). The present sample complements previous X-ray studies of z>4 quasars, in which the majority of…

We present radio and X-ray observations of the recently discovered $z=6.13$ radio-powerful quasar RACS J032021.44$-$352104.1 using uGMRT, ATCA, LBA, and Chandra. The observed radio properties are in line with what is typically observed in…

We report on our XMM observations of the high redshift quasars BR 2237--0607 (z=4.558) and BR 0351--1034 (z=4.351), together with 14 other z>4 objects found in the XMM public archive. Contrary to former reports, we do not find high redshift…

Astrophysics · Physics 2010-11-11 D. Grupe , S. Mathur , B. Wilkes , P. Osmer

We report exploratory \chandra\ observation 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…

Astrophysics of Galaxies · Physics 2016-06-08 Yanli Ai , Liming Dou , Xiaohui Fan , Feige Wang , Xue-Bing Wu , Fuyan Bian

We present a 45 ks Chandra observation of the quasar ULAS J1342+0928 at z=7.54. We detect 14.0^{+4.8}_{-3.7} counts from the quasar in the observed-frame energy range 0.5-7.0 keV (6-sigma detection), representing the most distant…

Astrophysics of Galaxies · Physics 2018-07-10 E. Bañados , T. Connor , D. Stern , J. Mulchaey , X. Fan , R. Decarli , E. P. Farina , C. Mazzucchelli , B. P. Venemans , F. Walter , F. Wang , J. Yang

We present results from a new XMM-Newton observation of the high-redshift quasar RXJ1028.6-0844 at a redshift of 4.276. The soft X-ray spectral flattening, as reported by a study with ASCA previously (Yuan et al. 2000, ApJ 545, 625), is…

Astrophysics · Physics 2009-09-17 W. Yuan , A. C. Fabian , A. Celotti , R. G. McMahon , M. Matsuoka

We present a systematic analysis of X-ray archival data of all the 29 quasars (QSOs) at $z$ > 5.5 observed so far with Chandra, XMM-Newton and Swift-XRT, including the most-distant quasar ever discovered, ULAS J1120+0641 ($z$ = 7.08). This…

Astrophysics of Galaxies · Physics 2017-07-26 R. Nanni , C. Vignali , R. Gilli , A. Moretti , W. N. Brandt

The intergalactic medium was not completely reionized until approximately a billion years after the Big Bang, as revealed by observations of quasars with redshifts of less than 6.5. It has been difficult to probe to higher redshifts,…

Optical and near-infrared (NIR) spectra are presented for ULAS J131911.29+095951.4 (hereafter ULAS J1319+0950), a new redshift z = 6.127 +/- 0.004 quasar discovered in the Third Data Release (DR3) of the UKIRT Infrared Deep Sky Survey…

We report Chandra detection of three UV bright radio quiet quasars at $z\gtrsim5$. We have collected a sufficient number of photons to extract an X-ray spectrum of each quasar to measure their basic X-ray properties, such as the X-ray flux,…

High Energy Astrophysical Phenomena · Physics 2021-01-27 Jiang-Tao Li , Feige Wang , Jinyi Yang , Yuchen Zhang , Yuming Fu , Fuyan Bian , Joel N. Bregman , Xiaohui Fan , Qiong Li , Xue-Bing Wu , Xiaodi Yu

We report on Chandra observations of three quasars SDSSP J083643+005453, SDSSP J103027+052455, and SDSSP J130608+035626 at redshifts 5.82, 6.28 and 5.99 respectively. All the three sources are clearly detected in the X-ray band, up to rest…

Astrophysics · Physics 2009-11-07 Smita Mathur , Belinda Wilkes , Himel Ghosh

We are carrying out sensitive X-ray observations with Chandra and XMM of type II quasars selected from the Sloan Digital Sky Survey based on their optical emission line properties. We present observations of four objects at redshifts 0.4 <…

Astrophysics · Physics 2009-11-13 A. Ptak , N. Zakamska , M. Strauss , J. Krolik , T. Heckman , D. Schneider , J. Brinkmann

We observed 17 optically-selected, radio-quiet high-redshift quasars with the Chandra Observatory ACIS, and detected 16 of them. The quasars have redshift between 3.70 and 6.28 and include the highest redshift quasars known. When compared…

We present results from X-ray observations of the quadruply lensed quasar RX J0911.4+0551 using data obtained with the Advanced CCD Imaging Spectrometer (ACIS) on board the Chandra X-ray Observatory. The 29 ks observation detects a total of…

Chandra snapshot observations of the three most distant quasars then known, at redshifts 5.82, 5.99, and 6.28, gave signficant detections even in the short, 6 -- 8 ks, observations. The X-ray to optical luminosity ratios indicate that…

Astrophysics · Physics 2007-05-23 D. A. Schwartz , C. C. Cheung , J. F. C. Wardle

We present deep Chandra observations of PSO J231.6576$-$20.8335, a quasar at redshift z=6.59 with a nearby (${\sim}8$ proper kpc) companion galaxy. ALMA observed both the quasar and companion to be bright in [C II], and the system has…

We report on deep XMM-Newton and NuSTAR observations of the high redshift, z=2.94, extremely red quasar (ERQ), SDSS J165202.60+172852.4, with known galactic ionized outflows detected via spatially-resolved [OIII] emission lines. X-ray…

We report new Chandra observations of seven optically faint, z \sim 4 radio-quiet quasars. We have combined these new observations with previous Chandra observations of radio-quiet quasars to create a sample of 174 sources. These sources…

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