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Herschel PEP/HerMES: the redshift evolution (0 ≤ z ≤ 4) of dust attenuation and of the total (UV+IR) star formation rate density

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Academic year: 2021

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Figure

Table 1 and Fig. 1 show the redshift variation of the LFs in FIR. The known di ff erence in the FIR and FUV LFs (e.g
Fig. 3. Dust attenuation vs. redshift. The boxes are color-coded accord- accord-ing to redshift
Fig. 4. SFRD densities in the FUV (blue), in the FIR (red), and in to- to-tal (i.e., FUV + FIR) in green (other colors are due to overlaps of the previous colors)
Fig. 6. Cosmic sSFR vs. z extrapolated beyond the observed limit at z = 3.6 with different options (see text)

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