837 citations · 19.8k across the 253 of their papers we have counts for
6 papers · 2 filters
Modeling the evolution of infrared galaxies: A Parametric backwards evolution model
Matthieu Béthermin, Hervé Dole, Guilaine Lagache +2
We aim at modeling the infrared galaxy evolution in an as simple as possible way and reproduce statistical properties among which the number counts between 15 microns and 1.1 mm, t…
HerMES: Deep Galaxy Number Counts from a P(D) Fluctuation Analysis of SPIRE Science Demonstration Phase Observations
J. Glenn, A. Conley, M. Bethermin +71
Dusty, star forming galaxies contribute to a bright, currently unresolved cosmic far-infrared background. Deep Herschel-SPIRE images designed to detect and characterize the galaxie…
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)…
The Cosmic Far-Infrared Background Buildup Since Redshift 2 at 70 and 160 microns in the COSMOS and GOODS fields
M. Jauzac, H. Dole, E. Le Floc'h +10
The Cosmic Far-Infrared Background (CIB) at wavelengths around 160 μm corresponds to the peak intensity of the whole Extragalactic Background Light, which is being measured with in…
Submillimeter Number Counts at 250, 350 and 500 microns in BLAST data
M. Béthermin, H. Dole, M. Cousin +1
BLAST (Balloon-borne Large-Aperture Submillimeter Telescope) performed the first deep and wide extragalactic survey at 250, 350 and 500 um. The extragalactic number counts at these…
Spitzer Deep and Wide Legacy Mid- and Far-Infrared Number Counts and Lower Limits of Cosmic Infrared Background
Matthieu Béthermin, Hervé Dole, Alexandre Beelen +1
Aims: We want to place stronger lower limits on the Cosmic Infrared Background (CIB) brightness at 24, 70 and 160 um and measure the extragalactic number counts at these wavelength…