activity
20102013
collaborators

6 papers

astro-ph.CO2013

The Herschel census of infrared SEDs through cosmic time

Myrto Symeonidis, M. Vaccari, S. Berta +57

Using Herschel data from the deepest SPIRE and PACS surveys (HerMES and PEP) in COSMOS and GOODS (N+S), we examine the dust properties of IR-luminous (L_IR>10^10 L_sun) galaxies at…

astro-ph.CO2012

Evolution of the far-infrared luminosity functions in the Spitzer Wide-area Infrared Extragalactic Legacy Survey

H. Patel, D. L. Clements, M. Vaccari +3

We present new observational determination of the evolution of the rest-frame 70 and 160 micron and total infrared (TIR) galaxy luminosity functions (LFs) using 70 micron data from…

astro-ph.CO2012

The Herschel Multi-tiered Extragalactic Survey: HerMES

HerMES Collaboration, S. J. Oliver, J. Bock +102

The Herschel Multi-tiered Extragalactic Survey, HerMES, is a legacy program designed to map a set of nested fields totalling ~380 deg^2. Fields range in size from 0.01 to ~20 deg^2…

astro-ph.CO2010

Spectroscopic follow-up of 70μm sources in Spitzer Wide-area Infrared Extragalactic Legacy Survey

H. Patel, D. L. Clements, M. Rowan-Robinson +1

We present spectroscopic follow-up observations of 70μm selected galaxies from the SWIRE XMMLSS and Lockman Hole fields. We have measured spectroscopic redshifts for 293 new source…

astro-ph.CO2010

The Herschel Multi-Tiered Extragalactic Survey: Source Extraction and Cross-Identifications in Confusion-Dominated SPIRE Images

I. G. Roseboom, S. J. Oliver, M. Kunz +83

We present the cross-identification and source photometry techniques used to process Herschel SPIRE imaging taken as part of the Herschel Multi-Tiered Extragalactic Survey (HerMES)…

astro-ph.CO2010

Cold dust and young starbursts: spectral energy distributions of Herschel SPIRE sources from the HerMES survey

Michael Rowan-Robinson, Herschel-SPIRE HerMES consortium

We present spectral energy distributions (SEDs) for 68 Herschel sources detected at 5-sigma at 250, 350 and 500 mu in the HerMES SWIRE-Lockman field. We explore whether existing mo…