activity
19982013
most citedThe Herschel-SPIRE instrument and its in-flight performance

2.2k citations · 3k across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2013★ 94 cited

HerMES: Clusters of Dusty Galaxies Uncovered by Herschel and Planck

D. L. Clements, F. G. Braglia, A. Hyde +21

The potential for Planck to detect clusters of dusty, star-forming galaxies at z greater than 1 is tested by examining the Herschel-SPIRE images of Planck Early Release Compact Sou…

astro-ph.CO2013★ 62 cited

A Herschel Survey of the [N II] 205 micron Line in Local Luminous Infrared Galaxies --- The [N II] 205 micron Emission as a Star Formation Rate Indicator

Yinghe Zhao, Nanyao Lu, C. Kevin Xu +16

We present, for the first time, a statistical study of [N II] 205 mciron line emission for a large sample of local luminous infrared galaxies using Herschel Spectral and Photometri…

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.IM2010★ 2.2k cited

The Herschel-SPIRE instrument and its in-flight performance

M. J. Griffin, A. Abergel, A. Abreu +176

The Spectral and Photometric Imaging Receiver (SPIRE), is the Herschel Space Observatory`s submillimetre camera and spectrometer. It contains a three-band imaging photometer operat…

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…