activity
20102023
most citedThe Herschel Multi-tiered Extragalactic Survey: HerMES

800 citations · 2.1k across the 22 of their papers we have counts for

collaborators
Showing 2010Show all

6 papers · 1 filter

astro-ph.CO2010★ 16 cited

HerMES : SPIRE detection of high redshift massive compact galaxies in GOODS-N field

A. Cava, G. Rodighiero, I. Perez-Fournon +47

We have analysed the rest-frame far infrared (FIR) properties of a sample of massive (Mstar > 10^11Msun) galaxies at 2<z<3 in the GOODS (Great Observatories Origins Deep Survey) No…

astro-ph.CO2010★ 47 cited

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…

astro-ph.CO2010★ 65 cited

The HerMES SPIRE submillimeter local luminosity function

M. Vaccari, L. Marchetti, A. Franceschini +77

Local luminosity functions are fundamental benchmarks for high-redshift galaxy formation and evolution studies as well as for models describing these processes. Determining the loc…

astro-ph.CO2010★ 158 cited

HerMES: Far-infrared properties of known AGN in the HerMES fields

E. Hatziminaoglou, A. Omont, J. A. Stevens +72

Nuclear and starburst activity are known to often occur concomitantly. Herschel-SPIRE provides sampling of the FIR SEDs of type 1 and type 2 AGN, allowing for the separation betwee…

astro-ph.CO2010★ 58 cited

First results from HerMES on the evolution of the submillimetre luminosity function

S. Eales, G. Raymond, I. G. Roseboom +81

We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 microns, close to the peak of the far-infrared background. We have used the re…

astro-ph.CO2010★ 249 cited

The far-infrared/radio correlation as probed by Herschel

R. J. Ivison, B. Magnelli, E. Ibar +100

We set out to determine the ratio, q(IR), of rest-frame 8-1000um flux, S(IR), to monochromatic radio flux, S(1.4GHz), for galaxies selected at far-IR and radio wavelengths, to sear…