The ESO Distant Cluster Sample: galaxy evolution and environment out to z=1 (2009)
Poggianti, Bianca M., Aragon-Salamanca, Alfonso, Bamford, Steven, Barazza, Fabio, Best, Philip, Clowe, Douglas, ...
The ESO Distant Cluster Survey (EDisCS, P.I. Simon D.M. White, LP 166.A-0162) is an ESO large programme aimed at studying clusters and cluster galaxies at z=0.4-1. How different is the evolution of...
The Environments of Starburst and Post-Starburst Galaxies at z = 0.4-0.8 (2009)
Poggianti, Bianca M., Aragόn-Salamanca, Alfonso, Zaritsky, Dennis, Milvang-Jensen, Bo, Desai, Vandana, ...
Post-starburst (E+A or k+a) spectra, characterized by their exceptionally strong Balmer lines in absorption and the lack of emission lines, belong to galaxies in which the star formation (SF)...
The environments of starburst and post-starburst galaxies at z = 0.4-0.8 (2009)
Poggianti, Bianca M., Aragón-Salamanca, Alfonso, Zaritsky, Dennis, De Lucia, Gabriella, Milvang-Jensen, Bo, Desai, Vandana, ...
The environments of starburst and post-starburst galaxies at z=0.4-0.8 (2008)
Poggianti, Bianca M., Aragon-Salamanca, Alfonso, Zaritsky, Dennis, De Lucia, Gabriella, Milvang-Jensen, Bo, Desai, Vandana, ...
Post-starburst (E+A or k+a) spectra, characterized by their exceptionally strong Balmer lines in absorption and the lack of emission lines, belong to galaxies in which the star formation activity...
Poggianti, Bianca M., Desai, Vandana, Finn, Rose, Bamford, Steven, De Lucia, Gabriella, Varela, Jesus, ...
We investigate how the [O II] properties and the morphologies of galaxies in clusters and groups at z = 0.4–0.8 depend on projected local galaxy density, and compare with the field at similar...
Poggianti, Bianca M., Desai, Vandana, Finn, Rose, Bamford, Steven, De Lucia, Gabriella, Varela, Jesus, ...
We investigate how the [OII] properties and the morphologies of galaxies in clusters and groups at z=0.4-0.8 depend on projected local galaxy density, and compare with the field at similar redshifts...
Exploring the infrared/radio correlation at high redshift (2008)
Ibar, Edo, Cirasuolo, Michele, Ivison, Rob, Best, Philip, Smail, Ian, Biggs, Andy, ...
We have analysed the 24um properties of a radio-selected sample in the Subaru-XMM/Newton Deep Field in order to explore the behaviour of the FIR/radio relation at high redshifts. Statistically, the...
Poggianti, Bianca M., Desai, Vandana, Finn, Rose, Bamford, Steven, De Lucia, Gabriella, Varela, Jesus, ...
High redshift CSS radio galaxies (2007)
Huub Rottgering, Philip Best, Chris Carilli, Malcolm Longair
We discuss CSS radio galaxies from 2 samples of radio sources. The first sample is a complete sample of 28 3CR galaxies with redshifts in the range 0:6 ! z ! 1:8 for which we have HST, UKIRT and VLA...
The cosmological evolution of radio sources with CENSORS (2007)
Brookes, Mairi, Best, Philip, Peacock, John, Dunlop, James, Röttgering, Huub
NASA/JPL
Philip Best, Contributors Paul Alex, David Bacon (edinburgh/portsmouth, David Bersier, Liverpool Jmu, Philip Best (edinburgh, ...
2.1 International extensions of LOFAR............................ 4
The evolution of the star formation activity in galaxies and its dependence on environment (2006)
Poggianti, Bianca M., Von Der Linden, Anja, De Lucia, Gabriella, Desai, Vandana, Simard, Luc, Halliday, Claire, ...
The evolution of the star formation activity in galaxies and its dependence on environment (2006)
Poggianti, Bianca M., Von Der Linden, Anja, De Lucia, Gabriella, Desai, Vandana, Simard, Luc, Halliday, Claire, ...
Galaxy Evolution in Three dimensions : Time, Space and Mass (2003)
Kodama, Tadayuki, Bower, Richard, Best, Philip, Hall, Patrick, Yamada, Toru, Tanaka, Masayuki
There are three major axes to describe the evolution of galaxies, namely, time (redshift), space (environment) and mass (stellar mass). In this article, one topic each will be presented along these...
A single population scheme for FR I and FR II radio galaxies (2002)
The presence of two distant FR I radio galaxies in the Hubble Deep Field plus Flanking Fields indicates that the number density of these objects is about 10-50 times higher at z>1 than in the local...
Hunt,David, Paxton,George, Alexander,James, Best,Philip
The report considers the feasibility of a structural design which will be efficient for shelters of varying lengths utilizing common components. This effort is intended to lead towards a multi-modal...
The evolution of the cluster environments of radio sources at z < 1.8 (2002)
Best, Philip, Lehnert, Matt, Röttgering, Huub, Miley, George
Deep and high resolution radio observations of the Hubble Deep Field and flanking fields have shown the presence of two distant edge-darkened FR I radio galaxies, allowing for the first time an...
A Statistical Study of Emission Lines from High Redshift Radio Galaxies (2000)
De Breuck, Carlos, Rottgering, Huub, Miley, George, Van Breugel, Wil, Best, Philip
We have compiled a sample of 165 radio galaxies from the literature to study the properties of the extended emission line regions and their interaction with the radio source over a large range of...
Apocalypticisim in the fiction of William S. Burroughs, J.G. Ballard, and Thomas Pynchon. (1998)
Thesis (Ph. D.)--University of Durham, 1998.