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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 report on exploratory Chandra observations of five galactic nuclei that were found to be X-ray bright during the ROSAT all-sky survey (with L_X > 10^43 erg s^-1) but subsequently exhibited a dramatic decline in X-ray luminosity. Very…

Astrophysics · Physics 2009-11-10 S. Vaughan , R. Edelson , R. S. Warwick

Recent work has demonstrated the potential of gravitationally lensed quasars to extend measurements of black hole spin out to high-redshift with the current generation of X-ray observatories. Here we present an analysis of a large sample of…

High Energy Astrophysical Phenomena · Physics 2015-06-03 D. J. Walton , M. T. Reynolds , J. M. Miller , R. C. Reis , D. Stern , F. A. Harrison

The Extended Chandra Deep Field-South (ECDFS) survey consists of 4 Chandra ACIS-I pointings and covers $\approx$ 1100 square arcminutes ($\approx$ 0.3 deg$^2$) centered on the original CDF-S field to a depth of approximately 228 ks. This is…

Astrophysics · Physics 2008-11-26 Shanil Virani , Ezequiel Treister , C. Megan Urry , Eric Gawiser

We measure the near-infrared properties of 42 X-ray detected sources from the Chandra Deep Fields North and South, the majority of which lie within the NICMOS Hubble Deep Field North and Ultra Deep Field. We detect all 42 Chandra sources…

Astrophysics · Physics 2009-11-10 James W. Colbert , Harry Teplitz , Lin Yan , Matthew Malkan , Patrick McCarthy

The relatively nearby (distance=24.1 Mpc) elliptical galaxy NGC821, hosting a central massive black hole but inactive at all wavelengths, was observed with Chandra for a total exposure of 230 ksec, to search for nuclear emission and gas…

Astrophysics · Physics 2009-11-13 S. Pellegrini , A. Baldi , D. W. Kim , G. Fabbiano , R. Soria , A. Siemiginowska , M. Elvis

We present Gemini spectroscopy for 21 candidate optical counterparts to X-ray sources discovered in the Galactic Bulge Survey (GBS). For the majority of the 21 sources, the optical spectroscopy establishes that they are indeed the likely…

High Energy Astrophysical Phenomena · Physics 2015-03-30 Jianfeng Wu , P. G. Jonker , M. A. P. Torres , C. T. Britt , C. B. Johnson , R. I. Hynes , S. Greiss , D. T. H. Steeghs , T. J. Maccarone , C. O. Heinke , T. Wevers

In this work, we calculated the sizes of unresolved X-ray emission regions in three gravitationally lensed radio-loud quasars, B\,1422+231, MG\,J0414+0534 and Q\,0957+561, using a combination of imaging and spectral analysis on the X-ray…

Cosmology and Nongalactic Astrophysics · Physics 2021-04-12 Mustafa Burak Dogruel , Xinyu Dai , Eduardo Guerras , Matthew Cornachione , Christopher W. Morgan

We carried out new observations of two fields in the northern ring of M31 with XMM-Newton with two exposures of 100 ks each and obtained a complete list of X-ray sources down to a sensitivity limit of ~7 x 10^34 erg s^-1 (0.5 - 2.0 keV).…

We report on a deep XMM-Newton EPIC observation of the globular cluster Omega Cen performed on August 13th, 2001. We have detected 11 and 27 faint X-ray sources in the core and half mass radii, searching down to a luminosity of 1.3 x…

Astrophysics · Physics 2009-11-07 Bruce Gendre , Didier Barret , Natalie A. Webb

K-band spectra of young stellar candidates in four southern hemisphere clusters have been obtained with the near-infrared spectrograph GNIRS in Gemini South. The clusters are associated with IRAS sources that have colours characteristic of…

Astrophysics · Physics 2009-11-13 A. Roman-Lopes , Z. Abraham , R. Ortiz , A. Rodrigues-Ardila

We present the properties of the discrete X-ray sources detected in our monitoring program of the `typical' elliptical galaxy, NGC 3379, observed with Chandra ACIS-S in five separate pointings, resulting in a co-added exposure of 324-ks.…

We investigate the relationship between the hard X-ray photon index $\Gamma$ and the Eddington ratio ($\xi=L_{X}(0.5-25 \rm keV)/L_{Edd}$) in six X-ray binaries (XRBs) with well constrained black hole masses and distances. We find that…

Astrophysics · Physics 2009-11-13 Qingwen Wu , Minfeng Gu

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 a search for nuclear X-ray emission in the brightest cluster galaxies (BCGs) of a sample of groups and clusters of galaxies extracted from the Chandra archive. The exquisite angular resolution of Chandra allows us to obtain…

Astrophysics of Galaxies · Physics 2018-06-21 Lilan Yang , Paolo Tozzi , Heng Yu , Elisabeta Lusso , Massimo Gaspari , Roberto Gilli , Emanuele Nardini , Guido Risaliti

We provide X-ray constraints and perform the first X-ray spectral analyses for bright (f_850>=5mJy; S/N>=4) SCUBA sources in an 8.4'x8.4' area of the 2 Ms Chandra Deep Field-North survey containing the Hubble Deep Field-North. X-ray…

This study represents the most sensitive Chandra X-ray point source catalogue of M31. Using 133 publicly available Chandra ACIS-I/S observations totalling ~1 Ms, we detected 795 X-ray sources in the bulge, northeast, and southwest fields of…

Astrophysics of Galaxies · Physics 2016-07-07 N. Vulic , S. C. Gallagher , P. Barmby

We observed B1600+434 and B1608+656 with CXO/ACIS, detecting both quasar images in B1600+434 and three of four images in B1608+656. We did not detect significant X-ray emission from nearby galaxy groups or clusters associated with each lens…

Astrophysics · Physics 2009-11-10 Xinyu Dai , Christopher S. Kochanek

We report on the results of observations of hard X-ray sources in the Galactic plane with the Chandra X-ray Observatory. The hard X-ray IGR sources were discovered by the INTEGRAL satellite, and the goals of the Chandra observations are to…

Astrophysics · Physics 2009-11-13 John A. Tomsick , Sylvain Chaty , Jerome Rodriguez , Roland Walter , Philip Kaaret

We present the rest-frame ultraviolet-optical spectral properties of 65 broad absorption line (BAL) quasars from the Gemini Near Infrared Spectrograph-Distant Quasar Survey (GNIRS-DQS). These properties are compared with those of 195…