Over half of the far-infrared background light comes from galaxies at z ≥ 1.2-Reference-Cited by-同舟云学术

Over half of the far-infrared background light comes from galaxies at z ≥ 1.2

Published:2009-04 Issue:7239 Volume:458 Page:737-739
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Devlin Mark J.,Ade Peter A. R.,Aretxaga Itziar,Bock James J.,Chapin Edward L.,Griffin Matthew,Gundersen Joshua O.,Halpern Mark,Hargrave Peter C.,Hughes David H.,Klein Jeff,Marsden Gaelen,Martin Peter G.,Mauskopf Philip,Moncelsi Lorenzo,Netterfield Calvin B.,Ngo Henry,Olmi Luca,Pascale Enzo,Patanchon Guillaume,Rex Marie,Scott Douglas,Semisch Christopher,Thomas Nicholas,Truch Matthew D. P.,Tucker Carole,Tucker Gregory S.,Viero Marco P.,Wiebe Donald V.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature07918.pdf

Reference28 articles.

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3. Barger, A. J. et al. Submillimetre-wavelength detection of dusty star-forming galaxies at high redshift. Nature 394, 248–251 (1998)

4. Greve, T. R. et al. A 1200-µm MAMBO survey of ELAISN2 and the Lockman Hole - I. Maps, sources and number counts. Mon. Not. R. Astron. Soc. 354, 779–797 (2004)

5. Coppin, K. et al. The SCUBA Half-Degree Extragalactic Survey - II. Submillimetre maps, catalogue and number counts. Mon. Not. R. Astron. Soc. 372, 1621–1652 (2006)

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