activity
20122018
most citedHerschel-ATLAS/GAMA: a difference between star-formation rates in strong-line and weak-line radio galaxies

63 citations · 200 across the 5 of their papers we have counts for

collaborators

5 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.GA2017★ 45 cited

An imperfectly passive nature: Bright sub-millimeter emission from dust-obscured star formation in the z=3.717 "passive" system, ZF20115

J. M. Simpson, Ian Smail, Wei-Hao Wang +28

The identification of high-redshift massive galaxies with old stellar populations may pose challenges to some models of galaxy formation. However, to securely classify a galaxy as…

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.CO2013★ 16 cited

{\em Herschel}-ATLAS/GAMA: The Environmental Density of Far-Infrared Bright Galaxies at

C. S. Burton, Matt J. Jarvis, D. J. B. Smith +21

We compare the environmental and star formation properties of far-infrared detected and non--far-infrared detected galaxies out to . Using optical spectroscopy and photo…

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…