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Journal article

HerMES: SPIRE galaxy number counts at 250, 350, and 500 μ m

Abstract:

Emission at far-infrared wavelengths makes up a significant fraction of the total light detected from galaxies over the age of Universe. Herschel provides an opportunity for studying galaxies at the peak wavelength of their emission. Our aim is to provide a benchmark for models of galaxy population evolution and to test pre-existing models of galaxies. With the Herschel Multi-tiered Extra-galactic survey, HerMES, we have observed a number of fields of different areas and sensitivity using the...

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Journal:
Astronomy and Astrophysics
Volume:
518
Issue:
7-8
Publication date:
2010-07-16
EISSN:
1432-0746
ISSN:
0004-6361
URN:
uuid:563034f8-0699-4327-bdde-f8b3d9657cec
Source identifiers:
202829
Local pid:
pubs:202829

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