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Related papers: Hosts and Alignment Effect in 0.5 < z < 1 radio so…

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We present an optically-based study of the alignment between the radio axes and the optical major axes of eight z~0.7 radio galaxies in a 7C sample. The radio galaxies in this sample are ~20-times less radio luminous than 3C galaxies at the…

Astrophysics · Physics 2009-10-31 Mark Lacy , Susan E. Ridgway , Margrethe Wold , Per B. Lilje , Steve Rawlings

(abridged) Powerful radio galaxies often display enhanced optical/UV emission regions, elongated and aligned with the radio jet axis. The aim of this series of papers is to separately investigate the effects of radio power and redshift on…

Astrophysics · Physics 2009-11-10 K. J. Inskip , P. N. Best , M. S. Longair , H. J. A. Rottgering

We have obtained redshifts and infrared images for a sample of faint B2/6C radio sources whose fluxes are about six times fainter than those of sources in the bright 3C sample. We now have unambiguous redshifts for 90% of the sources,…

Astrophysics · Physics 2015-06-24 Stephen Eales , Steve Rawlings , Duncan Law-Green , Garret Cotter , Mark Lacy

Hubble Space Telescope images are presented of a sample of 28 3CR radio galaxies with redshifts in the range 0.6 < z < 1.8, together with maps at comparable angular resolution of their radio structure, taken using the Very Large Array.…

Astrophysics · Physics 2015-06-24 P. N. Best , M. S. Longair , H. J. A. R"ottgering

We present K-band imaging of all 49 radio galaxies in the 7C-I and 7C-II regions of the 7C Redshift Survey (7CRS). The low-frequency (151 MHz) selected 7CRS sample contains all sources with flux-densities S_151 > 0.5 Jy in three regions of…

Astrophysics · Physics 2009-11-07 Chris J. Willott , Steve Rawlings , Matt J. Jarvis , Katherine M. Blundell

The large number of differences between high- and low-redshift radio galaxies have almost all been discovered by looking at the bright 3C sample of radio sources. This has the disadvantage that the strong correlation between radio…

Astrophysics · Physics 2007-05-23 Stephen Eales

We present new near-infrared images of z>0.8 radio galaxies from the flux-limited 7C-III sample of radio sources for which we have recently obtained almost complete spectroscopic redshifts. The 7C objects have radio luminosities about 20…

Astrophysics · Physics 2009-10-31 Mark Lacy , Andrew J. Bunker , Susan E. Ridgway

Hubble Space Telescope images of 3CR radio galaxies at redshifts 0.6 < z < 1.8 have shown a remarkable variety of structures, generally aligned along the radio axis, indicating that the radio source strongly influences the optical…

Astrophysics · Physics 2009-10-30 P. N. Best , M. S. Longair , H. J. A. R"ottgering

The results of Hubble Space Telescope and UKIRT imaging observations are presented for a sample of 11 6C radio galaxies with redshifts 0.85 < z < 1.5. The observations of the 6C sources reveal a variety of different features, similar to…

Astrophysics · Physics 2009-11-10 K. J. Inskip , P. N. Best , M. S. Longair , S. Rawlings , H. J. A. Rottgering , S. Eales

We present the results of an HST and ground-based imaging study of a complete 3C sample of z ~ 1 sources, including 5 quasars and 5 radio galaxies. We have resolved continuum structure around all of our quasars in the WFPC2 images and in…

Astrophysics · Physics 2009-10-30 Susan E. Ridgway , Alan Stockton

Using the Spitzer Space Telescope, we have obtained 3.6--24 micron photometry of 38 radio galaxies and 24 quasars from the 3CR catalog at redshift 1<z<2.5. This 178 MHz-selected sample is unbiased with respect to orientation and therefore…

In this paper, the third and final of a series, we present complete K-band imaging and some complementary I-band imaging of the filtered 6C* sample. We find no systematic differences between the K-z relation of 6C* radio galaxies and those…

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 present the second part of an H-band (1.6 microns) atlas of z<0.3 3CR radio galaxies, using the Hubble Space Telescope Near Infrared Camera and Multi-Object Spectrometer (HST NICMOS2). We present new imaging for 21 recently acquired…

We present preliminary results from HST imaging of radio-loud quasar hosts, covering a ~x100 range in radio luminosity but in a narrow redshift range (0.5 to 0.65). The sample was selected from our new, spectroscopically complete 7C survey…

Astrophysics · Physics 2007-05-23 Stephen Serjeant , Steve Rawlings , Mark Lacy

Images from recent radio surveys were used to determine the radio position angles for over 2000 extended radio galaxies with host galaxies brighter than m$_{r}\sim$18 mag. For 1509 of these their optical axis ratios were obtained, and for a…

Astrophysics of Galaxies · Physics 2019-08-28 Lizbeth A. Vazquez Najar , Heinz Andernach

Using a new radio sample, 6C* designed to find radio galaxies at z > 4 along with the complete 3CRR and 6CE sample we extend the radio galaxy K-z relation to z~4.5. The 6C* K-z data significantly improve delineation of the K-z relation for…

We present optical spectropolarimetric and imaging polarimetric observations of four high-redshift radio galaxies (HzRGs) obtained with the 10-m Keck I telescope. A broad Mg II emission line is detected in the total and polarized flux…

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…

Astrophysics · Physics 2009-10-30 Eric J. Hooper , Chris D. Impey , Craig B. Foltz

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…

Astrophysics · Physics 2009-11-07 J. B. Hutchings
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