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We present X-ray and multiwavelength studies of a sample of eight high-luminosity active galactic nuclei (AGNs) with disc-like H\beta emission-line profiles selected from the Sloan Digital Sky Survey Data Release 7. These sources have…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 B. Luo , W. N. Brandt , M. Eracleous , Jian Wu , P. B. Hall , A. Rafiee , D. P. Schneider , Jianfeng Wu

While many observed ultra-luminous X-ray sources (ULXs, Lx > 10^39 erg s^-1) could be extragalactic X-ray binaries (XRBs) emitting close to the Eddington limit, the highest-luminosity ULXs (Lx > 3x10^39 erg s^-1) exceed the isotropic…

Astrophysics · Physics 2009-11-13 L. Blecha , N. Ivanova , V. Kalogera , K. Belczynski , J. Fregeau , F. Rasio

We present catalogs for the ~2 Ms Chandra Deep Field-North, currently the deepest X-ray observation of the Universe in the 0.5-8.0 keV band. Five hundred and three (503) X-ray sources are detected over an ~448 sq.arcmin area in up to seven…

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

We present X-ray observations of the nuclear region of 25 Fanaroff-Riley I radio galaxies from the 3CRR and B2 catalogs, using data from the Chandra and XMM archives. We find the presence of a X-ray Central Compact Core (CCCX) in 13/25…

Astrophysics · Physics 2009-11-10 D. Donato , R. M. Sambruna , M. Gliozzi

We present a detailed analysis of high-resolution Chandra observations of the merger system NGC3256, the most IR luminous galaxy in the nearby universe. The X-ray data show that several discrete sources embedded in complex diffuse emission…

Astrophysics · Physics 2009-11-07 P. Lira , M. Ward , A. Zezas , A. Alonso-Herrero , S. Ueno

Estimation of the black hole mass in bright X-ray sources of nearby galaxies is crucial to the understanding of these systems and their formation. However, the present allowed black hole mass range spans five order of magnitude (10Msun < M…

High Energy Astrophysical Phenomena · Physics 2013-08-08 V. Jithesh , K. Jeena , R. Misra , S. Ravindranath , G. C. Dewangan , C. D. Ravikumar , B. R. S. Babu

Hyper-Luminous Infrared Galaxies (HLIRGs) are the most luminous persistent objects in the Universe. They exhibit extremely high star formation rates, and most of them seem to harbour an AGN. They are unique laboratories to investigate…

Astrophysics · Physics 2007-08-29 A. Ruiz , F. J. Carrera , F. Panessa

Gamma Ray Burst (GRB) afterglows close to their peak intensity are among the brightest X-ray sources in the sky. Despite their fast power-law like decay, when fluxes are integrated from minutes up to hours after the GRB event, the…

Astrophysics · Physics 2009-10-31 F. Fiore , F. Nicastro , S. Savaglio , L. Stella , M. Vietri

We investigated the X-ray spectral properties of a collection of low-mass X-ray binaries (LMXBs) within a sample of 15 nearby early-type galaxies observed with Chandra. We find that the spectrum of the sum of the sources in a given galaxy…

Astrophysics · Physics 2009-11-07 Jimmy A. Irwin , Alex E. Athey , Joel N. Bregman

Using the Chandra ACIS-I instruments, we have carried out the deepest X-ray observation on a typical Galactic plane region at l 28.5 deg, where no discrete X-ray sources have been known previously. We have detected, as well as strong…

Astrophysics · Physics 2016-11-03 K. Ebisawa , A. Bamba , H. Kaneda , Y. Maeda , A. Paizis , G. Sato , S. Yamauchi

We present photometric and spectroscopic observations of the X-ray sources detected in the wide-area, moderately deep Chandra Large Area Synoptic X-ray Survey of the Lockman Hole-Northwest field. We have B, V, R, I, and z' photometry for…

Astrophysics · Physics 2009-11-10 A. T. Steffen , A. J. Barger , P. Capak , L. L. Cowie , R. F. Mushotzky , Y. Yang

We report on our search for distant clusters of galaxies based on optical and X-ray follow up observations of X-ray candidates from the SHARC survey. Based on the assumption that the absence of bright optical or radio counterparts to…

Astrophysics · Physics 2009-11-13 C. Adami , M. P. Ulmer , F. Durret , G. Covone , E. Cypriano

We present the spectral analysis of an 87~ks \emph{XMM-Newton} observation of Draco, a nearby dwarf spheroidal galaxy. Of the approximately 35 robust X-ray source detections, we focus our attention on the brightest of these sources, for…

Astrophysics of Galaxies · Physics 2016-04-27 E. Sonbas , B. Rangelov , O. Kargaltsev , K. S. Dhuga , J. Hare , I. Volkov

We present a catalog of 5184 candidate infrared counterparts to X-ray sources detected towards the Galactic center. The X-ray sample contains 9017 point sources detected in this region by the Chandra X-ray Observatory, including data from a…

Astrophysics of Galaxies · Physics 2009-09-28 Jon C. Mauerhan , Michael P. Muno , Mark R. Morris , Franz E. Bauer , Shogo Nishiyama , Tetsuya Nagata

We present new optical and {\it Chandra} observations of the field containing the ultraluminous X-ray source NGC 1313 X-2. On an ESO 3.6 m image, the {\it Chandra} error box embraces a $R=21.6$ point-like object and excludes a previously…

We report the detection of hard X-ray emission (>2 keV) from a number of point sources associated with the very young massive star-forming region IRAS 19410+2336. The X-ray emission is detected from several sources located around the…

Astrophysics · Physics 2009-11-07 H. Beuther , J. Kerp , T. Preibisch , T. Stanke , P. Schilke

Late type non-starburst galaxies have been shown to contain X-ray emitting objects, some being ultraluminous X-ray sources. We report on XMM-Newton observations of 11 nearby, late-type galaxies previously observed with the Hubble Space…

High Energy Astrophysical Phenomena · Physics 2016-01-27 K. Chatterjee , P. Kaaret , M. Brorby , J. J. E. Kajava , F. Grise , S. Farrell , J. Poutanen

We search for unresolved X-ray emission from lensed sources in the FOV of 11 CLASH clusters with Chandra data. We consider the solid angle in the lens plane corresponding to a magnification $\mu>1.5$, that amounts to a total of ~100…

Inspired by the discovery of the Phoenix cluster by the South Pole Telescope team, we initiated a search for other massive clusters of galaxies missing from the standard X-ray catalogs. We began by identifying 25 cluster candidates not…

Astrophysics of Galaxies · Physics 2020-02-24 Megan Donahue , Kelsey Funkhouser , Dana Koeppe , Rachel L. S. Frisbie , G. Mark Voit
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