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Related papers: The hosts of $z=2$ QSOs

200 papers

We have conducted a NIR study of the environments of seven radio-loud quasars at redshifts 1<z<1.6. In present paper we describe deep $K$ band images obtained for the fields of ~6X6 arcmin around the quasars with 3$\sigma$ limiting…

Astrophysics · Physics 2009-11-07 S. F. Sanchez , J. I. Gonzalez-Serrano

Some recent work on radio source fields at z~0.7 and z~4 is discussed. At z~0.7 we find that radio-loud quasars are typically found in moderately rich environments independent of radio luminosity, consistent with previous results at z~0.5.…

Astrophysics · Physics 2007-05-23 M. Lacy

We test the hypothesis whether high redshift QSOs would preferentially appear in small groups or pairs, and if they are associated with massive, young clusters. We carried out a photometric search for \Ly emitters on scales $\lesssim 10…

Astrophysics · Physics 2009-11-07 L. Infante , J. Varela , M. Moles , G. Hertling , A. Garcia , F. Menanteau

Based on images from the FIRST survey of the radio sky at 1.4 GHz, the positions of $\sim$5200 hotspots in $\sim$2870 radio galaxies and quasars were compiled, and linear sizes and radio luminosities were derived from the hosts redshifts.…

Astrophysics of Galaxies · Physics 2019-08-28 Pedro A. de la Rosa Valdés , Heinz Andernach

We have undertaken a project to investigate the host galaxies and environments of a sample of quasars at z~4. In this paper, we describe deep near-infrared imaging of 34 targets using the Magellan I and Gemini North telescopes. We discuss…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 K. K. McLeod , Jill Bechtold

We highlight some of the principal results from our recent Hubble Space Telescope studies of quasars and radio galaxies. The hosts of these powerful AGN are normal massive ellipticals which lie on the region of the fundamental plane…

Astrophysics · Physics 2009-11-07 James S. Dunlop , Ross J. Mclure

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…

Astrophysics · Physics 2009-10-31 K. K. McLeod , G. H. Rieke , L. J. Storrie-Lombardi

We investigate the properties of the host galaxies of X-ray selected (high frequency peaked) BL Lac objects using a large and homogeneous data set of high spatial resolution R-band observations of 52 BL Lacs in the EMSS and Slew samples.…

Astrophysics · Physics 2007-05-23 R. Falomo , J. K. Kotilainen

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…

Astrophysics of Galaxies · Physics 2015-06-18 R. Falomo , D. Bettoni , K. Karhunen , J. K. Kotilainen , M. Uslenghi

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…

Astrophysics · Physics 2009-11-10 B. Kuhlbrodt , E. Orndahl , L. Wisotzki , K. Jahnke

We present deep near-infrared $K_{\rm s}$-band imaging for 35 of the 53 sources from the high-redshift ($z > 2$) radio galaxy candidate sample defined in Broderick et al. (2022). These images were obtained using the High-Acuity Widefield…

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…

We present optical spectroscopy of the host galaxies of 4 QSO's: PG1444+407, PKS 2349-147, 3C 323.1, and 4C 31.63 having a redshift range (0.1 < z < 0.3). The spectra were obtained at the Keck Observatory with the LRIS instrument offset 2-4…

Astrophysics · Physics 2009-11-07 J. S. Miller , A. I. Sheinis

We report the discovery of a candidate dual QSO at z=1.889, a redshift that is in the era known as "cosmic noon" where most of the Universe's black hole and stellar mass growth occurred. The source was identified in Hubble Space Telescope…

Recognizing the properties of the host galaxies of quasi-stellar objects (QSOs) is essential to understand the suspected coevolution of central supermassive black holes (BHs) and their host galaxies. We selected a subsample of the…

(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…

Astrophysics · Physics 2009-11-13 C. Villforth , J. Heidt , K. Nilsson

The dichotomy between radio-loud and radio-quiet QSOs is not simply one of host morphology. While spiral galaxies almost exclusively host radio-quiet QSOs, ellipticals can host either radio-louds or radio-quiets. We find that a combination…

Cosmology and Nongalactic Astrophysics · Physics 2011-03-02 Timothy S. Hamilton

We used the Near Infrared Camera on Keck I to obtain Ks-band images of four candidate high-redshift radio galaxies selected using optical and radio data in the NOAO Deep Wide-Field Survey in Bootes. Our targets have 1.4 GHz radio flux…

We investigate multicolour imaging data of a complete sample of low redshift (z<0.2) QSO host galaxies. The sample was imaged in four optical (BVRi) and three near-infrared bands (JHKs), and in addition spectroscopic data is available for a…

Astrophysics · Physics 2007-05-23 K. Jahnke , B. Kuhlbrodt , E. Orndahl , L. Wisotzki

We have studied the distribution of $B_J<20.5$ galaxies from the ROE/NRL COSMOS/UKST catalogue around two samples of $z>0.3$ QSOs with similar redshift distributions. The first sample is formed by 144 radio-loud QSOs from the Parkes…

Astrophysics · Physics 2016-08-30 N. Benitez , E. Martinez-Gonzalez , IFCA
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