Spectroscopic follow-up of a cluster candidate at z = 1.45

(2007)

Authors:

Caroline van Breukelen, Garret Cotter, Steve Rawlings, Tony Readhead, David Bonfield, Lee Clewley, Rob Ivison, Matt Jarvis, Chris Simpson, Mike Watson

The LOFAR Transients Key Project

Sissa Medialab Srl (2007) 104

Authors:

Rob Fender, Ralph AMJ Wijers, Ben Stappers, Robert Braun, Michael W Wise, Thijs Coenen, Heino Falcke, Jean-Mathias Griessmeier, Michiel Van Haarlem, Peter G Jonker, Casey Law, Sera Markoff, Joseph Masters, James CA Miller-Jones, Rachel Osten, Bart Scheers, Hanno Spreeuw, John D Swinbank, Corina Vogt, Rudy Wijnands, Philippe Zarka

Linking Jet Emission, X-ray States and Hard X-ray Tails in the Neutron Star X-ray Binary GX 17+2

(2007)

Authors:

S Migliari, JCA Miller-Jones, RP Fender, J Homan, T Di Salvo, RE Rothschild, MP Rupen, JA Tomsick, R Wijnands, M van der Klis

Evidence for a jet contribution to the optical/infrared light of neutron star X-ray binaries

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 379:3 (2007) 1108-1116

Authors:

DM Russell, RP Fender, PG Jonker

The prevalence of FRI radio quasars

ArXiv 0708.1145 (2007)

Authors:

Ian Heywood, Katherine M Blundell, Steve Rawlings

Abstract:

We present deep, multi-VLA-configuration radio images for a set of 18 quasars, having redshifts between 0.36 and 2.5, from the 7C quasar survey. Approximately one quarter of these quasars have FRI-type twin-jet structures and the remainder are a broad range of wide angle tail, fat double, classical double, core-jet and hybrid sources. These images demonstrate that FRI quasars are prevalent in the universe, rather than non-existent as had been suggested in the literature prior to the serendipitous discovery of the first FRI quasar a few years ago, the optically powerful "radio quiet" quasar E1821+643. Some of the FRI quasars have radio luminosities exceeding the traditional FRI / FRII break luminosity, however we find no evidence for FRII quasars with luminosities significantly below the break. We consider whether the existence of such high luminosity FRI structures is due to the increasingly inhomogeneous environments in the higher redshift universe.