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Related papers: X-ray Emission from the Host Clusters of Powerful …

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We present a Chandra observation of the only low redshift, z=0.299, galaxy cluster to contain a highly luminous radio-quiet quasar, H1821+643. By simulating the quasar PSF, we subtract the quasar contribution from the cluster core and…

High Energy Astrophysical Phenomena · Physics 2010-08-23 H. R. Russell , A. C. Fabian , J. S. Sanders , R. M. Johnstone , K. M. Blundell , W. N. Brandt , C. S. Crawford

We report the results of a search for X-ray emission from quasar host clusters at moderate redshift using the {\sl ROSAT} HRI. We detect no emission from the host clusters of 3C~263 (z=0.646) and PKS~2352-34 (z=0.706) to 3$\sigma$\ limits…

Astrophysics · Physics 2009-10-28 Patrick B. Hall , Erica Ellingson , Richard F. Green , Howard Yee

We report the first significant detection of an X-ray cluster associated with a powerful (L(bol) ~1e47 erg/sec) radio-loud quasar at high redshift (z=1.06). Diffuse X-ray emission is detected out to ~120 kpc from the CSS quasar 3C 186. A…

As a pilot study to investigate the distribution of matter in the fields of powerful AGN, we present weak lensing observations of deep fields centered on the radio-quiet quasar E1821 + 643, the radio galaxy 3C295, and the two radio-loud…

Astrophysics · Physics 2009-11-07 M. Wold , M. Lacy , H. Dahle , P. B. Lilje , S. E. Ridgway

We report the Chandra discovery of an X-ray cluster at redshift z = 1.063 associated with the Compact Steep Spectrum radio loud quasar 3C 186 (Q0740+380). Diffuse X-ray emission is detected out to ~120 kpc from the quasar and contains…

We investigate the properties of the environment around 20 powerful radio galaxies and quasars at redshifts between 0.45 and 1. Using XMM-Newton and Chandra observations we probe the spatial distribution and the temperature of the cluster…

Astrophysics · Physics 2009-11-13 Elena Belsole , Diana M. Worrall , Martin J. Hardcastle , Judith H. Croston

We report results of an 18 ks exposure with the ACIS instrument on Chandra of the powerful z = 0.62 radio galaxy 3C 220.1. The X-ray emission separates into cluster gas of emission-weighted kT ~ 5 keV and 0.7-12 keV luminosity (to a radius…

Astrophysics · Physics 2009-11-06 D. M. Worrall , M. Birkinshaw , M. J. Hardcastle , C. R. Lawrence

We present the first results from a new, deep (200ks) Chandra observation of the X-ray luminous galaxy cluster surrounding the powerful (L ~10^47 erg/s), high-redshift (z=1.067), compact-steep-spectrum radio-loud quasar 3C186. The diffuse…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Aneta Siemiginowska , D. J. Burke , Thomas L. Aldcroft , D. M. Worrall , S. Allen , Jill Bechtold , Tracy Clarke , C. C. Cheung

We present a deep Suzaku observation of H1821+643, an extremely rare example of a powerful quasar hosted by the central massive galaxy of a rich cooling-core cluster of galaxies. Informed by previous Chandra studies of the cluster, we…

We report the detection of extended X-ray emission around several powerful 3CR quasars with redshifts out to 0.73. The ROSAT HRI images of the quasars have been corrected for spacecraft wobble and compared with an empirical point-spread…

Astrophysics · Physics 2009-10-31 C. S. Crawford , I. Lehmann , A. C. Fabian , M. N. Bremer , G. Hasinger

H1821+643 is the nearest quasar hosted by a galaxy cluster. The energy output by the quasar, in the form of intense radiation and radio jets, is captured by the surrounding hot atmosphere. Here we present a new deep Chandra observation of…

High Energy Astrophysical Phenomena · Physics 2024-01-09 H. R. Russell , P. E. J. Nulsen , A. C. Fabian , T. E. Braben , W. N. Brandt , L. Clews , M. McDonald , C. S. Reynolds , J. S. Sanders , S. Veilleux

Recent X-ray observations of the rich galaxy cluster CL 0939+4713 at z = 0.41 with the ROSAT/HRI as well as with the ASCA/GIS and ASCA/SIS are presented and analysed. With the high resolution imaging data we confirm and extend the earlier…

Astrophysics · Physics 2007-05-23 S. Schindler , P. Belloni , Y. Ikebe , M. Hattori , J. Wambsganss , Y. Tanaka

H1821+643 is the most X-ray luminous non-beamed AGN of $L_\mathrm{14-150 keV}= 5.2\times 10^{45}$ erg s$^{-1}$ in the Swift/BAT ultra-hard X-ray survey and it is also a hyper-luminous infrared (IR) galaxy $L_\mathrm{IR} = 10^{13.2} L_\odot$…

In our ongoing multi-wavelength study of cluster AGN, we find ~75% of the spectroscopically identified cluster X-ray point sources (XPS) with L(0.3-8.0keV)>10^{42} erg s^{-1} and cluster radio galaxies with P(1.4 GHz) > 3x10^{23} W Hz^{-1}…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Quyen N. Hart , John T. Stocke , Eric J. Hallman

(abridged) MR2251-178 was the first quasar initially discovered in X-rays, and the first one found to host a warm absorber. The quasar turned out to be an outstanding object in many respects. It has a high ratio of X-ray/optical luminosity,…

Astrophysics · Physics 2009-11-06 Stefanie Komossa

We present the high-resolution X-ray spectrum of the low-redshift quasar H 1821+643 and its surrounding hot cluster observed with the Chandra High Energy Transmission Grating Spectrometer (HETGS). An iron emission line attributed to the…

Astrophysics · Physics 2015-06-24 T. Fang , D. S. Davis , J. C. Lee , H. L. Marshall , G. L. Bryan , C. R. Canizares

We present a multifrequency analysis of the radio galaxy 3CR 196.1 ($z = 0.198$), associated with the brightest galaxy of the cool core cluster CIZAJ0815.4-0303. This nearby radio galaxy shows a hybrid radio morphology and an X-ray cavity,…

We are looking for radio `relics' and `halos' in an X-ray selected sample of clusters of galaxies. These radio features are not a product of the Active Galactic Nuclei (AGN)-mechanism, but more likely are associated with past cluster merger…

Cosmology and Nongalactic Astrophysics · Physics 2012-09-05 Nectaria A. B. Gizani

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…

Hyper-luminous infrared galaxies (HyLIRGs) lie at the extreme luminosity end of the IR galaxy population with $L_{\rm IR}>10^{13}$L$_\odot$. They are thought to be closer counterparts of the more distant sub-mm galaxies, and should…

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