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The HerMES SPIRE submillimeter local luminosity function

Abstract:

Local luminosity functions are fundamental benchmarks for high-redshift galaxy formation and evolution studies as well as for models describing these processes. Determining the local luminosity function in the submillimeter range can help to better constrain in particular the bolometric luminosity density in the local Universe, and Herschel offers the first opportunity to do so in an unbiased way by imaging large sky areas at several submillimeter wavelengths. We present the first Herschel me...

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Publisher copy:
10.1051/0004-6361/201014694

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Journal:
Astronomy and Astrophysics
Volume:
518
Issue:
2
Publication date:
2010-07-16
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
URN:
uuid:ba0023b2-0d2b-430f-b48c-9ebdcabfe337
Source identifiers:
202827
Local pid:
pubs:202827

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