- UHRA Home
- Browsing by Author
Browsing by Author "Hill, G.J."
Now showing items 1-7 of 7
-
Evidence of different star formation histories for high- and low-luminosity radio galaxies
Herbert, P.D.; Jarvis, M.J.; Willott, C.J.; McLure, R.J.; Mitchell, E.; Rawlings, S.; Hill, G.J.; Dunlop, J.S. (2010)We present the results of our investigation into the stellar populations of 24 radio galaxies at z≃ 0.5 drawn from four complete, low-frequency-selected radio surveys. We use the strength of the 4000-Å break as an indicator ... -
The evolution of the fundamental plane of radio galaxies from z∼ 0.5 to the present day
Herbert, Peter; Jarvis, M.J.; Willcott, C.J.; McLure, R.J.; Mitchell, E.; Rawlings, S.; Hill, G.J.; Dunlop, J.S. (2011)We present deep spectroscopic data for a 24-object subsample of our full 41-object z∼ 0.5 radio galaxy sample in order to investigate the evolution of the Fundamental Plane of radio galaxies. We find that the low-luminosity, ... -
A large area search for radion-loud quasars within the epoch of reionization
Jarvis, M.J.; Rawlings, S.; Barrio, F.E.; Hill, G.J.; Bauer, A.; Croft, S. (2004) -
A large area search for radion-loud quasars within the epoch of reionization
Jarvis, M.J.; Rawlings, S.; Barrio, F.E.; Hill, G.J.; Bauer, A.; Croft, S. (World Scientific Publishing, 2004)The Universe became fully reionized, and observable optically, at a time corresponding to redshift z ~ 6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that ... -
A sample of radio galaxies spanning three decades in radio luminosity - I. The host-galaxy properties and black-hole masses
McLure, R.J.; Willott, C.J.; Jarvis, M.J.; Rawlings, S.; Hill, G.J.; Mitchell, E.; Dunlop, J.S.; Wold, M. (2004) -
A Search for Radio-loud Quasars within the Epoch of Reionization
Jarvis, M.J.; Rawlings, S.; Barrio, F.E.; Hill, G.J.; Bauer, A.; Croft, S. (Astronomical Society of the Pacific, 2004)The Universe became fully reionized, and observable optically, at a time corresponding to redshift z~6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that one ... -
A young, dusty, compact radio source within a Lyα halo
Barrio, F.E.; Jarvis, M.J.; Rawlings, S.; Bauer, A.; Croft, S.; Hill, G.J.; Manchado, A.; McLure, R.J.; Smith, Daniel; Targett, T.A. (2008)