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We used the Hubble Space Telescope WFC3 near-infrared camera to image the host galaxies of a sample of eleven luminous, dust-reddened quasars at z ~ 2 -- the peak epoch of black hole growth and star formation in the Universe -- to test the…

Astrophysics of Galaxies · Physics 2015-04-10 Eilat Glikman , Brooke Simmons , Madeline Mailly , Kevin Schawinski , C. M. Urry , M. Lacy

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…

Astrophysics · Physics 2009-11-13 J. K. Kotilainen , R. Falomo , A. Treves , M. Uslenghi

Luminous type-2 quasars in which the glow from the central black hole is obscured by dust are ideal targets for studying their host galaxies and the quasars' effect on galaxy evolution. Such feedback appears ubiquitous in luminous obscured…

Astrophysics of Galaxies · Physics 2016-02-03 Dominika Wylezalek , Nadia L. Zakamska , Guilin Liu , Georges Obied

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…

Astrophysics · Physics 2009-11-10 R. Falomo , J. K. Kotilainen , C. Pagani , R. Scarpa , A. Treves

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,…

Astrophysics · Physics 2015-06-24 T. Hyvonen , J. K. Kotilainen , E. Orndahl , R. Falomo , 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.…

Astrophysics · Physics 2011-02-11 J. K. Kotilainen , R. Falomo , M. Labita , A. Treves , M. Uslenghi

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…

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

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…

Astrophysics · Physics 2011-07-18 John N. Bahcall , Sofia Kirhakos , David H. Saxe , Donald P. Schneider

We present deep HST/WFPC2, rest-frame U images of 17 ~L* quasars at z=1 and z=2 (V and I bands respectively), designed to explore the host galaxies. We fit the images with simple axisymmetric galaxy models, including a point-source, in…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 David J. E. Floyd , James S. Dunlop , Marek J. Kukula , Michael J. I. Brown , Ross J. McLure , Stefi A. Baum , Christopher P. O'Dea

We present Hubble ACS images of thirteen dust reddened Type-1 quasars selected from the FIRST/2MASS Red Quasar Survey. These quasars have high intrinsic luminosities after correction for dust obscuration (-23.5 > M_B > -26.2 from…

Astrophysics · Physics 2009-11-13 Tanya Urrutia , Mark Lacy , Robert H. Becker

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,…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 J. K. Kotilainen , R. Falomo , R. Decarli , A. Treves , M. Uslenghi , R. Scarpa

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…

Astrophysics · Physics 2016-08-30 J. K. Kotilainen , R. Falomo , R. Scarpa

Uncovering bright quasars' host galaxies at cosmic noon is challenging because of the high contrast between the quasar and its host and redshifted light, making them primarily visible in the infrared. We present JWST NIRSpec integral field…

Quasars may have played a key role in limiting the stellar mass of massive galaxies. Identifying those quasars in the process of removing star formation fuel from their hosts is an exciting ongoing challenge in extragalactic astronomy. In…

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…

The properties of high redshift quasar host galaxies are studied, in order to investigate the connection between galaxy evolution, nuclear activity, and the formation of supermassive black holes. We combine new near-infrared observations of…

Astrophysics · Physics 2009-11-13 R. Falomo , A. Treves , J. K. Kotilainen , R. Scarpa , M. Uslenghi

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…

Astrophysics · Physics 2009-11-10 C. Pagani , R. Falomo , A. 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…

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

Type II quasars are luminous Active Galactic Nuclei whose centers are obscured by large amounts of gas and dust. In this contribution we present 3-band HST images of nine type II quasars with redshifts 0.25<z<0.4 selected from the Sloan…

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…

Astrophysics · Physics 2009-10-31 Renato Falomo , Jari Kotilainen , Aldo Treves
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