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相关论文: Near-infrared adaptive optics imaging of high reds…

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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 the first results from a major Hubble Space Telescope program designed to investigate the cosmological evolution of quasar host galaxies from z~2 to the present day. Here we describe J and H-band NICMOS imaging of two quasar…

天体物理学 · 物理学 2016-01-13 M. J. Kukula , J. S. Dunlop , R. J. McLure , L. Miller , W. J. Percival , S. A. Baum , C. P. O'Dea

We present near-infrared imaging of the host galaxies of 17 quasars in the redshift range 1 < z < 2, carried out at the ESO VLT UT1 8m telescope under excellent seeing conditions (~0.4 arcsec). The sample includes radio-loud (RLQ) and…

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

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

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 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 VLT/ISAAC near-infrared imaging of the host galaxies of 15 low luminosity quasars at 1 < z < 2. This work complements our studies to trace the cosmological evolution of the host galaxies of high luminosity quasars. The radio-loud…

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

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 near-infrared H-band imaging of 15 intermediate redshift (0.5<z<1) radio quiet quasars (RQQ) in order to characterize the properties of their host galaxies. We are able to clearly detect the surrounding nebulosity in 12 objects,…

天体物理学 · 物理学 2015-06-24 T. Hyvonen , J. K. Kotilainen , E. Orndahl , R. Falomo , M. Uslenghi

There is considerable evidence that powerful radio quasars and radio galaxies are orientation-dependent manifestations of the same parent population: massive spheroids containing correspondingly massive black holes. Following the…

天体物理学 · 物理学 2015-06-24 R. A. E. Fosbury

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

I discuss two programs to study radio-loud quasars at high (z>4) redshift. Quasars are the most luminous, non-transient objects known and are observed to the earliest cosmic epochs. At lower redshifts, radio-loud quasars are associated with…

天体物理学 · 物理学 2007-05-23 Daniel Stern

(abriged)In this paper we study different properties of quasars and their host galaxies at high redshifts up to z~3.4. We compare our results to those of other authors and discuss the correlation between galaxy evolution and quasar…

天体物理学 · 物理学 2009-11-13 C. Villforth , J. Heidt , K. Nilsson

We have used far-infrared data from IRAS, ISO, SWIRE, SCUBA and MAMBO to constrain statistically the mean far-infrared luminosities of quasars. Our quasar compilation at redshifts 0<z<6.5 and I-band luminosities -20<I(AB)<-32 is the first…

星系天体物理 · 物理学 2015-05-13 Stephen Serjeant , Evanthia Hatziminaoglou

We present the first results from a major HST WFPC2 imaging study aimed at providing the first statistically meaningful comparison of the morphologies, luminosities, scalelengths and colours of the host galaxies of radio-quiet quasars,…

天体物理学 · 物理学 2008-11-26 R. J. McLure , J. S. Dunlop , M. J. Kukula , S. A. Baum , C. P. O'Dea , D. H. Hughes

The properties of radio loud active galaxies (radiogalaxies, BL Lac objects and radio loud quasar) at low and high redshift are briefly reviewed and compared. The recently derived empirical relations between central black hole mass and host…

天体物理学 · 物理学 2007-05-23 Renato Falomo

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 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

We present the results of near-infrared H-band (1.65 microns) imaging of 19 steep spectrum radio quasars (SSRQ) in the redshift range 0.5 < z < 1.0. This sample of SSRQs is matched with our previously studied complete sample of 20 flat…

天体物理学 · 物理学 2007-05-23 J. K. Kotilainen , R. Falomo

We present near-IR images of five luminous quasars at z~2 and one at z~4 obtained with an experimental adaptive optics instrument at the ESO Very Large Telescope. The observations are part of a program aimed at demonstrating the…

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