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相关论文: Host galaxies of bright high redshift quasars: Lum…

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We present K band adaptive optics observations of three high-redshift (z ~ 2.2) high-luminosity quasars, all of which were studied for the first time. We also bserved several point spread function (PSF) calibrators, non-simultaneously…

天体物理学 · 物理学 2009-11-10 B. Kuhlbrodt , E. Orndahl , L. Wisotzki , K. Jahnke

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 some results from our HST archival image study of 71 QSO host galaxies. The objects are selected to have z < 0.46 and total absolute magnitude M_V < -23 (H_0=50 km/s/Mpc). This initial study investigates host morphology and radio…

天体物理学 · 物理学 2009-10-31 Timothy S. Hamilton , Stefano Casertano , David A. Turnshek

We report on the analysis of B band imaging data of 57 low-redshift QSOs and Seyfert 1 galaxies selected from the Hamburg/ESO-Survey, for which host galaxy dependent selection biases are greatly reduced compared to other optical surveys.…

天体物理学 · 物理学 2009-11-10 K. Jahnke , L. Wisotzki

We present a photometrical and morphological study of the properties of low redshift (z < 0.5) quasars based on a large and homogeneous dataset of objects derived from the Sloan Digital Sky Survey (DR7). This study over number by a factor…

星系天体物理 · 物理学 2015-06-18 R. Falomo , D. Bettoni , K. Karhunen , J. K. Kotilainen , M. Uslenghi

Three high-redshift (z=2) and high luminosity (M_B < -28 mag for Ho = 50, qo=0.5) QSOs, two radio-quiet one radio-loud, were imaged in R, I and K bands. The luminosities, colours and sizes of the hosts overlap with those of actively…

天体物理学 · 物理学 2007-05-23 I. Aretxaga , R. J. Terlevich , B. J. Boyle

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

(abridged) We present near-infrared Ks-band imaging of 13 high redshift (0.6 < z < 1.3) BL Lac objects. We clearly detect the host in eight objects, and marginally in three others. In all cases, the host galaxy is well represented by an…

天体物理学 · 物理学 2009-11-11 J. K. Kotilainen , T. Hyvonen , R. Falomo

We report {\em JWST}/NIRCam measurements of quasar host galaxy emissions and supermassive black hole (SMBH) masses for six quasars at $5.9<z<7.1$ in the \textit{Emission-line galaxies and Intergalactic Gas in the Epoch of Reionization}…

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 searched the HST archives for unpublished WFPC2 images of low redshift (z<0.5) radio loud quasars (RLQ). This led to the identification of 11 objects. We present here the results of the analysis of these images from which we derive the…

天体物理学 · 物理学 2009-11-10 C. Pagani , R. Falomo , A. Treves

We present a photometrical and morphological multicolor study of the properties of low redshift (z<0.3) quasar hosts based on a large and homogeneous dataset of quasars derived from the Sloan Digital Sky Survey (DR7). We used quasars that…

星系天体物理 · 物理学 2015-11-04 D. Bettoni , R. Falomo , J. K. Kotilainen , K. Karhunen , M. Uslenghi

We present the results of a multi-colour (VIZ) survey for low luminosity (M_B<-23.5) quasars with z~5 using the 12K CCD mosaic camera on CFHT. The survey covers 1.8deg^2 to a limiting magnitude of m_z=22.5(Vega), about two magnitudes…

天体物理学 · 物理学 2009-11-10 R. G. Sharp , D. Crampton , I. M. Hook , R. G. McMahon

We present K-band images of 31 radio quasars selected from the B3-VLA quasar sample. A new method has been developed to detect and restore the host galaxies of these quasars. We have detected the host galaxies of 16 of them. Using these…

天体物理学 · 物理学 2009-11-07 S. F. Sanchez , J. I. Gonzalez-Serrano

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

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 present results of the hosts of four high-redshift ($z \approx 2$) and high luminosity ($M_B \lsim -28$ mag) QSOs, three radio-quiet one radio-loud, imaged in R and K bands. The extensions to the nuclear unresolved source are most likely…

天体物理学 · 物理学 2007-05-23 Itziar Aretxaga , Brian J. Boyle , Roberto J. Terlevich

We present the results of a high resolution (0.27 arcsec/px) near-infrared H band (1.65 micron) imaging survey of a complete sample of 20 flat spectrum radio quasars (FSRQ) extracted from the 2Jy catalogue of radio sources. The observed…

天体物理学 · 物理学 2016-08-30 J. K. Kotilainen , R. Falomo , R. Scarpa

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 K-band imaging and photometry of a sample of 52 radio loud quasars (RQs) selected from the B3 survey with flux densities above 0.5 Jy at 408 MHz. The optical completeness of the sample is 90% and the quasars cover the redshift…

天体物理学 · 物理学 2009-10-30 R. Carballo , S. F. Sanchez , J. I. Gonzalez-Serrano , C. R. Benn , M. Vigotti
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