The evolution of the star formation activity per halo mass up to redshift ∼1.6 as seen by Herschel

Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly. To understand where and when the quenching processes takes place, we study the evolution of the total star formation rate per unit total halo mass (Σ(SFR)/M) in three different mass scales: low mass...

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التفاصيل البيبلوغرافية
المؤلفون الرئيسيون:	Popesso, P, Biviano, A, Rodighiero, G, Baronchelli, I, Salvato, M, Saintonge, A, Finoguenov, A, Magnelli, B, Gruppioni, C, Pozzi, F, Lutz, D, Elbaz, D, Altieri, B, Andreani, P, Aussel, H, Berta, S, Capak, P, Cava, A, Cimatti, A, Coia, D, Daddi, E, Dannerbauer, H, Dickinson, M, Dasyra, K, Fadda, D
التنسيق:	Journal article
اللغة:	English
منشور في:	2012

The evolution of the star formation activity per halo mass up to redshift ∼1.6 as seen by Herschel

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