Constraining the star formation rate with the extragalactic background light
Author:
Affiliation:
1. Institute for Nuclear Research of the Russian Academy of Sciences, 60th October Anniversary st. 7a, 117312, Moscow, Russia
2. Faculty of Physics, M V Lomonosov Moscow State University, Vorobyovy Gory, 1-2, 119991, Moscow, Russia
Funder
Russian Science Foundation
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/481/1/557/25687243/sty2144.pdf
Reference54 articles.
1. Modelling the cosmic spectral energy distribution and extragalactic background light over all time
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5. HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background
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