HerMES: SPIRE galaxy number counts at 250, 350, and 500 μ m

Emission at far-infrared wavelengths makes up a significant fraction of the total light detected from galaxies over the age of Universe. Herschel provides an opportunity for studying galaxies at the peak wavelength of their emission. Our aim is to provide a benchmark for models of galaxy population...

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Xehetasun bibliografikoak
Egile Nagusiak:	Oliver, S, Wang, L, Smith, A, Altieri, B, Amblard, A, Arumugam, V, Auld, R, Aussel, H, Babbedge, T, Blain, A, Bock, J, Boselli, A, Buat, V, Burgarella, D, Castro-Rodríguez, N, Cava, A, Chanial, P, Clements, D, Conley, A, Conversi, L, Cooray, A, Dowell, C, Dwek, E, Eales, S, Elbaz, D
Formatua:	Journal article
Hizkuntza:	English
Argitaratua:	2010

HerMES: SPIRE galaxy number counts at 250, 350, and 500 μ m

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