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20012013
most citedThe Herschel-SPIRE instrument and its in-flight performance

2.2k citations · 3.1k across the 11 of their papers we have counts for

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8 papers · 1 filter

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…

astro-ph.CO2010★ 30 cited

HerMES: SPIRE/Sub-millimetre Emission from Radio Selected AGN

N. Seymour, M. Symeonidis, M. Page +1

We examine the rest-frame far-infrared emission from powerful radio sources with 1.4GHz luminosity densities of 25<=log(L_1.4/WHz^-1)<=26.5 in the extragalactic Spitzer First Look…

astro-ph.CO2010★ 33 cited

Herschel-SPIRE observations of the disturbed galaxy NGC4438

L. Cortese, G. J. Bendo, A. Boselli +56

We present Herschel-SPIRE observations of the perturbed galaxy NGC4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the gala…

astro-ph.CO2010★ 296 cited

HerMES: The SPIRE confusion limit

H. T. Nguyen, B. Schulz, L. Levenson +69

We report on the sensitivity of SPIRE photometers on the Herschel Space Observatory. Specifically, we measure the confusion noise from observations taken during the Science Demonst…

astro-ph.CO2010★ 37 cited

Mapping the interstellar medium in galaxies with Herschel/SPIRE

S. A. Eales, M. W. L. Smith, C. D. Wilson +57

The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with…