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相关论文: Near-IR Properties of Quasar Host Galaxies

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We have detected the host galaxies of 16 nearby, radio-quiet quasars using images obtained with the Near-Infrared Camera and Multi-Object Spectrometer (NICMOS). We confirm that these luminous quasars tend to live in luminous, early-type…

天体物理学 · 物理学 2009-10-31 K. K. McLeod , G. H. Rieke , L. J. Storrie-Lombardi

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

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 have made a deep NICMOS imaging study of a sample of 5 z ~ 2 - 3 radio-quiet quasars with low absolute nuclear luminosities, and we have detected apparent host galaxies in all of these. Most of the hosts have luminosities approximately…

天体物理学 · 物理学 2009-10-31 S. E. Ridgway , T. M. Heckman , D. Calzetti , M. Lehnert

We will present the results of a NICMOS H-band imaging survey of a small sample of z ~ 2 to 3 radio-quiet quasars. We have resolved extension in at least 4 of 5 objects and find evidence for a wide range in the morphologies and magnitudes…

天体物理学 · 物理学 2009-10-31 S. Ridgway , T. Heckman , D. Calzetti , M. Lehnert

We have obtained Near-Infrared Camera and Multi-Object Spectrometer images of 16 radio quiet quasars observed as part of a project to investigate the ``luminosity/host-mass limit.'' The limit results were presented in McLeod, Rieke, &…

天体物理学 · 物理学 2009-10-31 K. K. McLeod , B. A. McLeod

HST observations of eight intrinsically luminous quasars with redshifts between $0.16$ and~$0.29$ are presented. Seven companion galaxies brighter than $M_V = -16.5$ lie within a projected distance of 25 kpc of the quasars; three of the…

天体物理学 · 物理学 2016-08-30 John N. Bahcall , Sofia Kirhakos , Donald P. Schneider

We present and analyse the deepest, high-quality Ks-band images ever obtained of luminous quasars at z~4, in an attempt to determine the basic properties of their host galaxies less than 1 Gyr after the first recorded appearance of black…

宇宙学与河外天体物理 · 物理学 2015-05-28 Thomas A. Targett , James S. Dunlop , Ross J. McLure

We present H-band observations of gravitationally lensed QSO host galaxies obtained with NICMOS on HST as part of the CfA-Arizona-Gravitational-Lens-Survey (CASTLES). The detections are greatly facilitated by the lensing magnification in…

天体物理学 · 物理学 2007-05-23 H. -W. Rix , E. Falco , C. Impey , C. Kochanek , J. Lehar , B. McLeod , J. Munoz , C. Peng

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

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 stellar velocity dispersion measurements in the host galaxies of 10 luminous quasars (M_V < -23) using the Ca H&K lines in off-nuclear spectra. We combine these data with effective radii and magnitudes from the literature to…

天体物理学 · 物理学 2009-11-13 Marsha J. Wolf , Andrew I. Sheinis

We present the results of a deep K-band imaging study which reveals the host galaxies around a sample of luminous radio-quiet quasars. The K-band images, obtained at UKIRT, are of sufficient quality to allow accurate modelling of the…

天体物理学 · 物理学 2009-10-31 W. J. Percival , L. Miller , R. J. McLure , J. S. Dunlop

We present results of a deep HST/WFPC2 imaging study of 17 quasars at z~0.4, designed to determine the properties of their host galaxies. The sample consists of quasars with absolute magnitudes in the range -24>M_V>-28, allowing us to…

天体物理学 · 物理学 2007-05-23 D. J. E. Floyd , M. J. Kukula , J. S. Dunlop , R. J. McLure , L. Miller , W. J. Percival , S. A. Baum , C. P. O'Dea

We present the results of our recent Hubble Space Telescope imaging study, in which we have successfully deconvolved host and nuclear flux for the some of the most luminous quasars in the Universe. Host morphologies have been recovered for…

天体物理学 · 物理学 2007-05-23 David J. E. Floyd

We present near-infrared imaging obtained with ESO VLT/ISAAC of a sample of 16 low luminosity radio-quiet quasars at the epoch around the peak of the quasar activity (2 < z < 3), aimed at investigating their host galaxies. For 11 quasars,…

宇宙学与河外天体物理 · 物理学 2015-05-13 J. K. Kotilainen , R. Falomo , R. Decarli , A. Treves , M. Uslenghi , R. Scarpa

We present high spatial resolution near-infrared H-band (1.65 microns) images, taken with ISAAC on UT1 of ESO VLT, of three radio-loud quasars at z = 1.5, as a pilot study for imaging of a larger sample of radio-loud and radio-quiet quasars…

天体物理学 · 物理学 2009-10-31 Renato Falomo , Jari Kotilainen , Aldo Treves

A recent study suggests that the quasar HE 0450-2958 is hosted by a galaxy substantially fainter than that inferred from the correlation between black hole mass and bulge luminosity. As this result has significant bearings on galaxy and…

天体物理学 · 物理学 2010-11-05 Minjin Kim , Luis C. Ho , Chien Y. Peng , Myungshin Im

Gravitational lensing assists in the detection of quasar hosts by amplifying and distorting the host light away from the unresolved quasar core images. We present the results of HST observations of 30 quasar hosts at redshifts 1 < z < 4.5.…

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
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