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The host galaxies of radio-loud active galactic nuclei: mass dependences, gas cooling and active galactic nuclei feedback
- P. Best, G. Kauffmann, +4 authors S. White
- Physics
- 1 September 2005
The properties of the host galaxies of a well-defined sample of 2215 radio-loud active galactic nuclei (AGN) with redshifts 0.03 10 23 W Hz -1 is a strong function of stellar mass, rising from nearly… Expand
On the fundamental dichotomy in the local radio-AGN population
- P. Best, T. Heckman
- Physics
- 11 January 2012
A sample of 18 286 radio-loud active galactic nuclei (AGN) is presented, constructed by combining the seventh data release of the Sloan Digital Sky Survey with the NRAO (National Radio Astronomy… Expand
Predicting dust extinction from the stellar mass of a galaxy
We investigate how the typical dust extinction of Hα luminosity from a star-forming galaxy depends upon star formation rate (SFR), metallicity and stellar mass independently, using a sample of ~90… Expand
The Coevolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe
- T. Heckman, P. Best
- Physics
- 18 March 2014
We summarize what large surveys of the contemporary Universe have taught us about the physics and phenomenology of the processes that link the formation and evolution of galaxies with their central… Expand
A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS
This paper presents new deep and wide narrow-band surveys undertaken with United Kingdom Infrared Telescope (UKIRT), Subaru and the Very Large Telescope (VLT), a unique combined effort to select… Expand
A sample of radio-loud active galactic nuclei in the Sloan Digital Sky Survey
- P. Best, G. Kauffmann, T. Heckman, Ž. Ivezić
- Physics
- 13 June 2005
A sample of 2712 radio-luminous galaxies is defined from the second data release of the Sloan Digital Sky Survey (SDSS) by cross-comparing the main spectroscopic galaxy sample with two radio surveys:… Expand
How special are Brightest Group and Cluster Galaxies
- A. D. Linden, P. Best, G. Kauffmann, S. White
- Physics
- 7 November 2006
We use the Sloan Digital Sky Survey (SDSS) to construct a sample of 625 brightest group and cluster galaxies (BCGs) together with control samples of non-BCGs matched in stellar mass, redshift and… Expand
Star formation at z=1.47 from HiZELS: an Hα+[O ii] double-blind study*
This paper presents the results from the first wide and deep dual narrow-band survey to select Hα and [Oii] line emitters at z= 1.47 ± 0.02, exploiting synergies between the United Kingdom Infrared… Expand
Deep multi-frequency radio imaging in the Lockman Hole using the GMRT and VLA - I. The nature of the sub-mJy radio population
In the run up to routine observations with the upcoming generation of radio facilities, the nature of sub-mJy radio population has been hotly debated. Here, we describe multi-frequency data designed… Expand
LOFAR - low frequency array
- M. V. Haarlem, M. Wise, +197 authors J. V. Zwieten
- Physics, Computer Science
- 1 February 2010
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