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 halos (field galaxies), groups, and clusters, up to a redshift z ≈ 1.6. Methods. We use deep far-infrared PACS data at 100 and 160 μm to accurately estimate the total star formation rate of the luminous infrared galaxy population of 9 clusters with mass ~1015 M⊙, and 9 groups/poor clusters with mass ~5 × 1013 M⊙. Estimates of the field Σ(SFR)/M are derived from the literature, by dividing the star formation rate density by the mean com...
International audienceWe study the evolution of the total star formation (SF) activity, total stella...
International audienceWe study the evolution of the total star formation (SF) activity, total stella...
Context. The most striking feature of the cosmic star formation history (CSFH) of the Universe is a ...
Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
We study the evolution of the total star formation (SF) activity, total stellar mass (\u3a3M*) and h...
We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM*) and halo ...
We study the evolution of the total star formation (SF) activity, total stellar mass (∑M*) and halo ...
We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM*) and halo ...
International audienceWe study the evolution of the total star formation (SF) activity, total stella...
International audienceWe study the evolution of the total star formation (SF) activity, total stella...
International audienceWe study the evolution of the total star formation (SF) activity, total stella...
Context. The most striking feature of the cosmic star formation history (CSFH) of the Universe is a ...
Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims: Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
Aims. Star formation in massive galaxies is quenched at some point during hierarchical mass assembly...
We study the evolution of the total star formation (SF) activity, total stellar mass (\u3a3M*) and h...
We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM*) and halo ...
We study the evolution of the total star formation (SF) activity, total stellar mass (∑M*) and halo ...
We study the evolution of the total star formation (SF) activity, total stellar mass (ΣM*) and halo ...
International audienceWe study the evolution of the total star formation (SF) activity, total stella...
International audienceWe study the evolution of the total star formation (SF) activity, total stella...
International audienceWe study the evolution of the total star formation (SF) activity, total stella...
Context. The most striking feature of the cosmic star formation history (CSFH) of the Universe is a ...