Cosmic star-formation history from a non-parametric inversion of infrared galaxy counts | A&A

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Table C.1:

Fraction of the CIRB resolved by confusion-limited Herschel surveys.
	PACS 70 $\mu$ m	PACS 100 $\mu$ m	PACS 160 $\mu$ m	SPIRE 250 $\mu$ m	SPIRE 350 $\mu$ m	SPIRE 500 $\mu$ m
$F_{\rm confusion}$ (mJy)	0.056	0.54	10.0	20.0	25.1	25.1
IGL $^{\rm a}$ @ $F_{\rm confusion}$	9.14	12.3	6.27	1.98	0.55	0.058
CIRB $^{\rm a}$	9.51	14.0	15.3	10.3	5.47	2.29
% CIRB resolved	96.1%	87.8%	41.1%	19.1 %	10.0 %	2.5 %

^a Units: nW m^-2 sr^-1.

Source LaTeX | All tables | In the text