Fig. 23

Ratio of the extrapolated () over
Herschel total IR luminosity as a function of redshift, for all
clean GOODS–Herschel galaxies.
is
computed by normalizing the main sequence SED to the broadband photometric
measurement at λ. The 5 passbands used for the extrapolation are,
from the top to bottom, Spitzer
MIPS–24 μm, Herschel
PACS–100 μm & 160 μm,
Herschel SPIRE–250 μm &
350 μm.
is
measured using the full set of Herschel measurements at rest-frame
wavelengths λ > 30 μm to normalize the main
sequence SED and by integrating over 8–1000 μm. Black triangles:
AGN. The solid lines with error bars are the sliding median and the 16th and 84th
percentiles around it. Upper panel: SED of M82 and MIPS
24 μm filter at z = 0.25, 0.9, 1.4, 2.
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