中文
相关论文

相关论文: Peering through the dust II: $XMM-Newton$ observat…

200 篇论文

Some reddened quasars appear to be transitional objects in the merger-induced black hole growth/galaxy evolution paradigm, where a heavily obscured nucleus starts to be unveiled by powerful quasar winds evacuating the surrounding cocoon of…

We present an analysis of the X-ray properties 10 luminous, dust-reddened quasars from the FIRST-2MASS (F2M) survey based on new and archival Chandra observations. These systems are interpreted to be young, transitional objects predicted by…

星系天体物理 · 物理学 2024-01-08 Eilat Glikman , Stephanie LaMassa , Enrico Piconcelli , Luca Zappacosta , Mark Lacy

We present a sample of 120 dust-reddened quasars identified by matching radio sources detected at 1.4 GHz in the FIRST survey with the near-infrared 2MASS catalog and color-selecting red sources. Optical and/or near-infrared spectroscopy…

We present results of a study of 12 dust-reddened quasars with 0.4 < z < 2.65 and reddenings in the range 0.15 < E(B-V) < 1.7. We obtained ACIS-S X-ray spectra of these quasars, estimated the column densities towards them, and hence…

天体物理学 · 物理学 2009-11-10 Tanya Urrutia , Mark Lacy , Michael D. Gregg , Robert H. Becker

We report results from a 50 ks XMM-Newton observation of the dust-reddened broad-line quasar FTM 0830+3759 (z=0.413) selected from the FIRST/2MASS Red Quasar survey. For this AGN, a very short 9 ks Chandra exposure had suggested a…

宇宙学与河外天体物理 · 物理学 2015-05-18 E. Piconcelli , C. Vignali , S. Bianchi , F. Nicastro , G. Miniutti , F. Fiore

We present new X-ray observations of luminous heavily dust-reddened quasars (HRQs) selected from infrared sky surveys. HRQs appear to be a dominant population at high redshifts and the highest luminosities, and may be associated with a…

高能天体物理现象 · 物理学 2020-05-13 G. B. Lansbury , M. Banerji , A. C. Fabian , M. J. Temple

First indications of the warm/hot intergalactic medium, tracing out the large scale structure of the universe, have been obtained in sensitive Chandra and XMM-Newton high resolution absorption line spectroscopy of bright blazars. High…

天体物理学 · 物理学 2007-05-23 Guenther Hasinger

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…

We present Hubble ACS images of thirteen dust reddened Type-1 quasars selected from the FIRST/2MASS Red Quasar Survey. These quasars have high intrinsic luminosities after correction for dust obscuration (-23.5 > M_B > -26.2 from…

天体物理学 · 物理学 2009-11-13 Tanya Urrutia , Mark Lacy , Robert H. Becker

We present the results of XMM-Newton observations of four high-z quasars, two radio-loud and two radio-quiet. One of the radio-loud objects, PKS 2126-158, clearly shows absorption in excess of the galactic value as claimed before from ASCA…

天体物理学 · 物理学 2011-05-23 E. Ferrero , W. Brinkmann

We present the results of NuSTAR and XMM-Newton observations of the two ultraluminous X-ray sources (ULX) NGC 1313 X-1 and X-2. The combined spectral bandpass of the two satellites enables us to produce the first spectrum of X-1 between 0.3…

We used the Hubble Space Telescope WFC3 near-infrared camera to image the host galaxies of a sample of eleven luminous, dust-reddened quasars at z ~ 2 -- the peak epoch of black hole growth and star formation in the Universe -- to test the…

星系天体物理 · 物理学 2015-04-10 Eilat Glikman , Brooke Simmons , Madeline Mailly , Kevin Schawinski , C. M. Urry , M. Lacy

We present short \chandra observations of twelve bright (i<18) z_em~1.5 quasars from the Sloan Digital Sky Survey chosen to have significantly redder optical colors than most quasars at the same redshift. Of the five quasars with optical…

We explore the connection between absorption by neutral gas and extinction by dust in mid-infrared (IR) selected luminous quasars. We use a sample of 33 quasars at redshifts 0.7 < z < 3 in the 9 deg^2 Bo\"otes multiwavelength survey field…

星系天体物理 · 物理学 2014-06-25 Shawn M. Usman , Stephen S. Murray , Ryan C. Hickox , Mark Brodwin

We present X-ray imaging and spectroscopy of the redshift z=7.084 radio-quiet quasar ULAS J112001.48+064124.3 obtained with Chandra and XMM-Newton. The quasar is detected as a point source with both observatories. The Chandra observation…

宇宙学与河外天体物理 · 物理学 2015-06-17 M. J. Page , C. Simpson , D. J. Mortlock , S. J. Warren , P. C. Hewett , B. P. Venemans , R. G. McMahon

We present mid-infrared spectra and photometry of thirteen redshift 0.4<z<1 dust-reddened quasars obtained with Spitzer IRS and MIPS. We compare properties derived from their infrared spectral energy distributions (intrinsic AGN luminosity…

宇宙学与河外天体物理 · 物理学 2012-09-27 Tanya Urrutia , Mark Lacy , Henrik Spoon , Eilat Glikman , Andreea Petric , Bernhard Schulz

Dust-obscured galaxies (DOGs) containing central supermassive black holes (SMBHs) that are rapidly accreting (i.e., having high Eddington ratios, $\lambda_\mathrm{Edd}$) may represent a key phase closest to the peak of both the black-hole…

星系天体物理 · 物理学 2024-10-29 Nathan Cristello , Fan Zou , William N. Brandt , Zhibo Yu , Fabio Vito , Shifu Zhu

We report on a NuSTAR and XMM-Newton program that has observed a sample of three extremely luminous, heavily obscured WISE-selected AGN at z~2 in a broad X-ray band (0.1 - 79 keV). The parent sample, selected to be faint or undetected in…

We present XMM-Newton X-ray spectra and optical photometry of four high redshift (z=2.96-3.77) quasars, [HB89] 0438-436, [HB89] 2000-330, [SP89] 1107+487 and RX J122135.6+280613; of these four objects the former two are radio-loud, the…

天体物理学 · 物理学 2008-11-26 C. Brocksopp , E. M. Puchnarewicz , K. O. Mason , F. A. Cordova , W. C. Priedhorsky

XMM-Newton spectra of five red, 2MASS AGN, selected from a sample observed by Chandra to be relatively X-ray bright and to cover a range of hardness ratios, confirm the presence of substantial absorbing material in three sources with…

天体物理学 · 物理学 2016-08-30 B. J. Wilkes , K. A. Pounds , G. D. Schmidt , P. S. Smith , R. M. Cutri , H. Ghosh , B. Nelson , D. C. Hines
‹ 上一页 1 2 3 10 下一页 ›