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相关论文: Hosts of Type II Quasars: an HST Study

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Type II quasars are luminous Active Galactic Nuclei whose centers are obscured by large amounts of gas and dust. In this paper we present 3-band HST images of nine type II quasars with redshifts 0.2 < z < 0.4 selected from the Sloan Digital…

At low redshifts, dust-obscured quasars often have strong yet narrow permitted lines in the rest-frame optical and ultraviolet, excited by the central active nucleus, earning the designation Type II quasars. We present a sample of 145…

A sample of 16 quasars selected from the Large Bright Quasar Survey in the redshift range 0.4 < z < 0.5 has been imaged in the R band with the Planetary Camera on the WFPC2 instrument of the Hubble Space Telescope. The host galaxy…

天体物理学 · 物理学 2009-10-30 Eric J. Hooper , Chris D. Impey , Craig B. Foltz

We have conducted spectropolarimetry of 12 type II (obscured) quasar candidates selected from the spectroscopic database of the Sloan Digital Sky Survey based on their emission line properties. Polarization was detected in all objects, with…

Some recent observations of nearby quasars with HST have apparently failed to detect host galaxies. We review the HST observations as well as near infrared ground-based observations of the same objects. We find that the quasar hosts can be…

天体物理学 · 物理学 2009-10-28 K. K. McLeod , G. H. Rieke

We present Hubble Space Telescope images, and spectral energy distributions from optical to infrared wavelengths for a sample of six 0.3<z<0.8 type-2 quasars selected in the mid-infrared using data from the Spitzer Space Telescope. All the…

天体物理学 · 物理学 2009-11-13 M. Lacy , A. Sajina , A. O. Petric , N. Seymour , G. Canalizo , S. E. Ridgway , L. Armus , L. J. Storrie-Lombardi

Type 2 quasars are luminous active galactic nuclei (AGN) whose central regions are obscured by large amounts of gas and dust. In this paper, we present a catalog of type 2 quasars from the Sloan Digital Sky Survey (SDSS), selected based on…

We describe progress in a programme to study a sample of sources typical of those which contribute a large fraction of the hard X-ray background. The sources are selected from the fields of approximately 10 ks Chandra cluster observations…

天体物理学 · 物理学 2007-05-23 P. Gandhi , C. S. Crawford , A. C. Fabian , R. J. Wilman , R. M. Johnstone , A. J. Barger , L. L. Cowie

Luminous type-2 quasars in which the glow from the central black hole is obscured by dust are ideal targets for studying their host galaxies and the quasars' effect on galaxy evolution. Such feedback appears ubiquitous in luminous obscured…

星系天体物理 · 物理学 2016-02-03 Dominika Wylezalek , Nadia L. Zakamska , Guilin Liu , Georges Obied

Type II quasars are luminous AGNs whose central engines and broad-line regions are obscured by intervening material; such objects only recently have been discovered in appreciable numbers. We study the multiwavelength properties of 291 type…

A description is given of the method used to extract quasar host-galaxy parameters from the deep Hubble Space Telescope quasar images presented by McLure et al. (1999) and Dunlop et al. (2000). We then give the results of extensive testing…

天体物理学 · 物理学 2009-10-31 R. J. McLure , J. S. Dunlop , M. J. Kukula

Strong upper limits are placed on the visual-band brightnesses of galactic hosts for four luminous, radio-quiet quasars with redshifts between $0.16$ and~$0.24$ that were studied with the HST's Wide Field/Planetary Camera-2. Typical upper…

天体物理学 · 物理学 2009-10-22 John N. Bahcall , Sofia Kirhakos , Donald P. Schneider

Type 2 quasars are luminous Active Galactic Nuclei whose central engines are seen through large amounts of gas and dust. We present Spitzer spectra of twelve type 2 quasars selected on the basis of their optical emission line properties.…

天体物理学 · 物理学 2010-05-27 Nadia L. Zakamska , Laura Gomez , Michael A. Strauss , Julian H. Krolik

Recent X-ray surveys with Chandra and XMM-Newton have found several genuine Type II quasars, the long sought-after population of high-luminosity (high-redshift) Seyfert 2 galaxies, and a sizable number of Type II quasar candidates. However,…

天体物理学 · 物理学 2007-05-23 C. Vignali , D. M. Alexander , A. Comastri

Observations with the Wide-Field Camera of the Hubble Space Telescope are presented for a representative sample of 20 intrinsically luminous quasars with redshifts smaller than 0.30. These observations show that luminous quasars occur in…

天体物理学 · 物理学 2011-07-18 John N. Bahcall , Sofia Kirhakos , David H. Saxe , Donald P. Schneider

We present near-infrared imaging with ESO VLT+ISAAC of the host galaxies of low luminosity quasars in the redshift range 1 < z < 2, aimed at investigating the relationship between the nuclear and host galaxy luminosities at high redshift.…

天体物理学 · 物理学 2011-02-11 J. K. Kotilainen , R. Falomo , M. Labita , A. Treves , M. Uslenghi

We present optical through radio observations of the host galaxies of two dust obscured, luminous quasars selected in the mid-infrared, at z=2.62 and z=2.99, including a search for CO emission. Our limits on the CO luminosities are…

宇宙学与河外天体物理 · 物理学 2015-05-30 Mark Lacy , Andreea O. Petric , Alejo Martinez-Sansigre , Susan E. Ridgway , Anna Sajina , Tanya Urrutia , Duncan Farrah

Type II quasars are the long-sought luminous analogs of type II (narrow emission line) Seyfert galaxies, suggested by unification models of active galactic nuclei (AGN) and postulated to account for an appreciable fraction of the cosmic…

We present NuSTAR hard X-ray (3-79 keV) observations of three Type 2 quasars at z ~ 0.4-0.5, optically selected from the Sloan Digital Sky Survey (SDSS). Although the quasars show evidence for being heavily obscured Compton-thick systems on…

We present multicolour images of the hosts of three z=2 QSOs previously detected in R-band by our group. The luminosities, colours and sizes of the hosts overlap with those of actively star-forming galaxies in the nearby Universe. Radial…

天体物理学 · 物理学 2009-10-30 I. Aretxaga , R. J. Terlevich , B. J. Boyle
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