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相关论文: Extensions around z=2 QSOs

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Based on an $R$-band imaging survey of high-redshift ($z \approx 2$) QSOs with the 4.2m WHT, we report the detection of extensions to the nuclear PSFs of two radio-quiet and one radio-loud QSO. The extensions are most likely host galaxies,…

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

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 have been conducting an imaging survey to detect host galaxies of radio-quiet QSOs at high redshift (z = 2), in order to compare them with those of radio-loud objects. Six QSOs were observed in the R passband with the auxiliary port of…

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

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 report the first unambiguous detection of the host galaxy of a normal radio-quiet QSO at high-redshift in K-band. The luminosity of the host comprises about 35% of the total K-band luminosity. Assuming the average colour of QSOs at z=2,…

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

Images are discussed of six QSOs at z=2.3, one QSO-like IRAS source at z=2.3, and one QSO at z=1.1, taken with resolution 0.6 to 0.9 arcsec. Five of the QSOs are radio-quiet. All QSOs except one are just resolved, while the IRAS source has…

天体物理学 · 物理学 2009-10-28 J. B. Hutchings

2 micron broad- and narrow-band imaging with the Gemini-N telescope of five z~4.7 QSOs, has resolved both the host galaxies and [O II] emission-line gas. The resolved fluxes of the host galaxies fall within the extrapolated spread of the…

天体物理学 · 物理学 2009-11-07 J. B. Hutchings

We report on ESO--VLT adaptive optics imaging of one radio-loud quasar at z $\sim$ 3. In spite of the large distance of the object we are able to detect its surrounding extended nebulosity the properties of which are consistent with an…

天体物理学 · 物理学 2009-11-13 R. Falomo , J. K. Kotilainen , R. Scarpa , A. Treves , M. Uslenghi

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

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

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 have obtained the first constraints on extended Ly-alpha emission at z ~ 1 in a sample of five radio galaxies. We detect Ly-alpha emission from four of the five galaxies. The Ly-alpha luminosities range from 0.1 - 4 times 10^43 erg/s and…

宇宙学与河外天体物理 · 物理学 2011-02-11 Andrew W. Zirm , Arjun Dey , Mark Dickinson , Colin J. Norman

We discuss 6 GHz JVLA observations covering a volume-limited sample of 178 low redshift ($0.2 < z < 0.3$) optically selected QSOs. Our 176 radio detections fall into two clear categories: (1) About $20$\% are radio-loud QSOs (RLQs) having…

星系天体物理 · 物理学 2016-11-15 K. I. Kellermann , J. J. Condon , A. E. Kimball , R. A. Perley , Zeljko Ivezic

Deep $B$ and $R$ band images (R<24 and B<25) have been obtained of a field of $\sim 6 \times 6$ arcmin around seven radio-loud quasars with $1<z<1.6$. A statistically significant excess of faint ($22.5<B\le 23.5$ and $22<R\le 23.0$)…

天体物理学 · 物理学 2007-05-23 S. F. Sanchez , J. I. Gonzalez-Serrano

We report the first detection of emission line gas within the host galaxies of high redshift QSOs. This was done using narrow-band imaging at the redshifted wavelengths of [O III] and H alpha, using the PUEO adaptive optics camera of the…

天体物理学 · 物理学 2009-10-31 J. B. Hutchings , S. L. Morris , D. Crampton

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 present rest-frame UV and Ly-alpha images of spatially-resolved structures around five high-redshift radio-loud quasars obtained with the WFPC2 camera on the Hubble Space Telescope. We find that all five quasars are extended and this…

天体物理学 · 物理学 2009-10-31 Matthew D. Lehnert , Wil J. M. van Breugel , Timothy M. Heckman , George K. Miley

We have conducted an optical study of the environments of seven radio-loud quasars at redshifts 1<z<1.6. In this paper we describe deep B and R band images obtained for fields of $\sim6\times$6 arcmin around these quasars with 3$\sigma$…

天体物理学 · 物理学 2007-05-23 S. F. Sanchez , J. I. Gonzalez-Serrano

We report an optical detection of an extended structure around a QSO at z=6.43 (CFHQSJ2329-0301, the highest redshift QSO currently known) in deep z' and z_r-band images of the Subaru/Suprime-Cam. After a careful PSF (QSO) subtraction, a…

宇宙学与河外天体物理 · 物理学 2015-05-14 Tomotsugu Goto , Yousuke Utsumi , Hisanori Furusawa , Satoshi Miyazaki , Yutaka Komiyama

We present an analysis of X-ray variability in a sample of 156 radio quiet quasars taken from the ROSAT archive, covering a redshift range 0.1 < z < 4.1. A maximum likelihood method is used to constrain the amplitude of variability in these…

天体物理学 · 物理学 2009-11-07 J. Manners , O. Almaini , A. Lawrence
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