activity
20102018
most citedGalaxy and Mass Assembly (GAMA): FUV, NUV, ugrizYJHK Petrosian, Kron and Sèrsic photometry

129 citations · 596 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2018★ 45 cited

The Causes of the Red Sequence, the Blue Cloud, the Green Valley and the Green Mountain

Stephen Eales, Maarten Baes, Nathan Bourne +23

The galaxies found in optical surveys fall in two distinct regions of a diagram of optical colour versus absolute magnitude: the red sequence and the blue cloud with the green vall…

astro-ph.GA2016★ 32 cited

VALES: II. The physical conditions of interstellar gas in normal star-forming galaxies up to z=0.2 revealed by ALMA

T. M. Hughes, E. Ibar, V. Villanueva +18

We use new Band-3 CO(1-0) observations taken with the Atacama Large Millimeter/submillimeter Array (ALMA) to study the physical conditions in the interstellar gas of a sample of 27…

astro-ph.CO2014★ 31 cited

Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing

J. González-Nuevo, A. Lapi, M. Negrello +25

We report a highly significant () spatial correlation between galaxies with mJy detected in the equatorial fields of the \textsl{Herschel} Astrophysica…

astro-ph.CO2012★ 63 cited

Herschel-ATLAS/GAMA: a difference between star-formation rates in strong-line and weak-line radio galaxies

M. J. Hardcastle, J. H. Y. Ching, J. S. Virdee +25

We have constructed a sample of radio-loud objects with optical spectroscopy from the Galaxy and Mass Assembly (GAMA) project over the Herschel-ATLAS Phase 1 fields. Classifying th…

astro-ph.CO2010★ 129 cited

Galaxy and Mass Assembly (GAMA): FUV, NUV, ugrizYJHK Petrosian, Kron and Sèrsic photometry

David T. Hill, Lee S. Kelvin, Simon P. Driver +33

In order to generate credible 0.1-2 μm SEDs, the GAMA project requires many Gigabytes of imaging data from a number of instruments to be re-processed into a standard format. In thi…

astro-ph.EP2010★ 16 cited

A search for debris disks in the Herschel ATLAS

M. A. Thompson, D. J. B. Smith, J. A. Stevens +42

Aims: We aim to demonstrate that the Herschel ATLAS (H-ATLAS) is suitable for a blind and unbiased survey for debris disks by identifying candidate debris disks associated with mai…