A Monte Carlo approach to evolution of the far-infrared luminosity function with BLAST-Reference-Cited by-同舟云学术

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A Monte Carlo approach to evolution of the far-infrared luminosity function with BLAST

Published:2011-08-08 Issue:2 Volume:417 Page:1192-1209
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Marsden Gaelen,Chapin Edward L.,Halpern Mark,Patanchon Guillaume,Scott Douglas,Truch Matthew D. P.,Valiante Elisabetta,Viero Marco P.,Wiebe Donald V.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/417/2/1192/3067963/mnras0417-1192.pdf

Reference90 articles.

1. Breaking the ‘redshift deadlock’- II. The redshift distribution for the submillimetre population of galaxies

2. AzTEC half square degree survey of the SHADES fields â I. Maps, catalogues and source counts

3. Can the faint submillimetre galaxies be explained in the Λ cold dark matter model?

4. Spitzerdeep and wide legacy mid- and far-infrared number counts and lower limits of cosmic infrared background

5. Modeling the evolution of infrared galaxies: a parametric backward evolution model

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