activity
20102022
most citedThe Primordial Inflation Explorer (PIXIE): A Nulling Polarimeter for Cosmic Microwave Background Observations

664 citations · 1.3k across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2022★ 9 cited

Mid-infrared imaging of Supernova 1987A

Mikako Matsuura, Roger Wesson, Richard G. Arendt +9

At a distance of 50 kpc, Supernova 1987A is an ideal target to study how a young supernova (SN) evolves in time. Its equatorial ring, filled with material expelled from the progeni…

astro-ph.CO2011★ 664 cited

The Primordial Inflation Explorer (PIXIE): A Nulling Polarimeter for Cosmic Microwave Background Observations

A. Kogut, D. J. Fixsen, D. T. Chuss +9

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission to measure the gravity-wave signature of primordial inflation through its distinctive imprint on the linear p…

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…