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The VIMOS Public Extragalactic Redshift Survey (VIPERS) : The decline of cosmic star formation: quenching, mass, and environment connections

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Figure

Fig. 2. Density distribution of the VIPERS galaxies in three redshiftbins (three columns) for the entire sample (black histogram), for galax-
Fig. 4. Stellar mass cumulative distributions in three redshift bins(0.51 < z ≤ 0.65, 0.65 < z ≤ 0.8, and 0.8 < z ≤ 0.9 from top tobottom), for galaxies above the mass limits log(Mlim/M⊙) = 10.38,10.66, and 10.89, respectively, in the three redshift bins
Table 1. Number of active and passive galaxies in each redshift andgalaxies are defined according to their position in the NUVstellar mass bin for the LD and HD environments
Fig. 5. Ratio of the number of active over passive galaxies (noise in the counts of active and passive galaxies (if we use the error formula for small samples suggested in Gehrels 1986, the error bars do notsSFRchange significantly)
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