HerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observations

HerMES: deep galaxy number counts from a P(D) fluctuation analysis of SPIRE Science Demonstration Phase observations

Dusty, star-forming galaxies contribute to a bright, currently unresolved cosmic far-infrared background. Deep Herschel-Spectral and Photometric Imaging Receiver (SPIRE) images designed to detect and characterize the galaxies that comprise this background are highly confused, such that the bulk lies...

詳細記述

書誌詳細
主要な著者: Glenn, J, Conley, A, Bethermin, M, Altieri, B, Amblard, A, Arumugam, V, Aussel, H, Babbedge, T, Blain, A, Bock, J, Boselli, A, Buat, V, Castro-Rodriguez, N, Cava, A, Chanial, P, Clements, D, Conversi, L, Cooray, A, Dowell, C, Dwek, E, Eales, S, Elbaz, D, Ellsworth-Bowers, T, Fox, M, Franceschini, A
フォーマット: Journal article
言語:English
出版事項: 2010

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