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

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

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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...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: 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
Aineistotyyppi: Journal article
Kieli:English
Julkaistu: 2010

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