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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 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 the results of Chandra observations of six radio-loud quasars (RLQs) and one optically bright radio-quiet quasar (RQQ) at z = 4.1-4.4. These observations cover a representative sample of RLQs with moderate radio-loudness (R ~…

Astrophysics · Physics 2009-11-10 L. C. Bassett , W. N. Brandt , D. P. Schneider , C. Vignali , G. Chartas , G. P. Garmire

We present results from Chandra observations of the cluster lens SDSS J1029+2623 at z_l=0.58, which is a gravitationally lensed quasar with the largest known image separation. We clearly detect X-ray emission both from the lensing cluster…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Naomi Ota , Masamune Oguri , Xinyu Dai , Christopher S. Kochanek , Gordon T. Richards , Eran O. Ofek , Roger D. Blandford , Tim Schrabback , Naohisa Inada

We present {\it Chandra} X-ray Observatory observations of Giga-Hertz Peaked Spectrum (GPS) and Compact Steep Spectrum (CSS) radio sources. The {\it Chandra} sample contains 13 quasars and 3 galaxies with measured 2-10 keV X-ray luminosity…

We present the first results of the Chandra and optical follow-up observations of hard X-ray sources detected in the ASCA Medium Sensitivity Survey (AMSS). Optical identifications are made for five objects. Three of them show either weak or…

We present \emph{Chandra} monitoring data for six gravitationally lensed quasars: QJ 0158$-$4325, HE 0435$-$1223, HE 1104$-$1805, SDSS 0924+0219, SDSS 1004+4112, and Q 2237+0305. We detect X-ray microlensing variability in all six lenses…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Bin Chen , Xinyu Dai , Christopher S. Kochanek , George Chartas , Jeffery A. Blackburne , Christopher W. Morgan

We present the first X-ray observation at sub-arcsecond resolution of the high-redshift ($z=6.18$) radio-loud quasar CFHQS J142952+544717 (J1429). The ~100 net-count 0.3-7 keV spectrum obtained from $\sim 30$ ksec Chandra exposure is best…

High Energy Astrophysical Phenomena · Physics 2023-07-12 G. Migliori , A. Siemiginowska , M. Sobolewska , C. C. Cheung , Ł. Stawarz , D. Schwartz , B. Snios , A. Saxena , V. Kashyap

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

We present a comprehensive analysis of Chandra X-ray observations of 15 young radio quasars at redshifts $4.5 < z < 5.0$. All sources are detected in the $0.5-7.0$ keV energy band. Emission spectra are extracted, and the average photon…

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

X-ray observations provide a unique probe of the accretion disk corona of supermassive black holes (SMBHs). In this paper, we present a uniform \emph{Chandra} X-ray data analysis of a sample of 152 $z\geq4.5$ quasars. We firmly detect 46…

High Energy Astrophysical Phenomena · Physics 2021-05-26 Jiang-Tao Li , Feige Wang , Jinyi Yang , Joel N. Bregman , Xiaohui Fan , Yuchen Zhang

Utilizing 21 new Chandra observations as well as archival Chandra, ROSAT, and XMM-Newton data, we study the X-ray properties of a representative sample of 59 of the most optically luminous quasars in the Universe (M_i~~-29.3 to -30.2)…

We report optical spectroscopic identifications of 10 hard (2-10 keV) X-ray selected sources discovered by Chandra. The X-ray flux of the sources ranges between 1.5 and 25 x 10-14 cgs, the lower value being 3 times fainter than in previous…

Astrophysics · Physics 2009-10-31 F. Fiore , F. La Franca , C. Vignali , A. Comastri , G. Matt , G. C. Perola , M. Cappi , M. Elvis , F. Nicastro

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 use a Chandra X-ray observation of the gravitationally lensed system MGB2016+112 at z=3.273 to elucidate presence of at least two X-ray sources. We find that these sources are consistent with the VLBI components measured by…

High Energy Astrophysical Phenomena · Physics 2021-08-25 Daniel Schwartz , Cristiana Spingola , Anna Barnacka

Our 5 ks Chandra ACIS-S observation of the globular cluster NGC 6652 detected 7 X-ray sources, 3 of which are previously unidentified. This cluster hosts a well-known bright low-mass X-ray binary, source A (or XB 1832-330). Source B shows…

High Energy Astrophysical Phenomena · Physics 2015-05-28 G. Coomber , C. O. Heinke , H. N. Cohn , P. M. Lugger , J. E. Grindlay

Chandra X-ray observations of the high redshift (z =1.532) radio-loud quasar 3C270.1 in 2008 February show the nucleus to have a power-law spectrum, Gamma = 1.66 +/- 0.08, typical of a radio-loud quasar, and a marginally-detected Fe Kalpha…

We report the discovery and ground based observations of the new gravitational lens CTQ 414. The source quasar lies at a redshift of z = 1.29 with a B magnitude of 17.6. Ground based optical imaging reveals two point sources separated by…

Astrophysics · Physics 2009-10-31 Nicholas D. Morgan , Alan Dressler , Jose Maza , Paul L. Schechter , Joshua N. Winn

Submillimeter (and in some cases millimeter) wavelength continuum measurements are presented for a sample of 40 active galactic nuclei (probably all quasars) lensed by foreground galaxies. The object of this study is to use the lensing…

Astrophysics · Physics 2009-11-07 Richard Barvainis , Rob Ivison