The HerMES SPIRE submillimeter local luminosity function

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Table 2:

Monochromatic and IR bolometric LLFs ( 0 < z < 0.2). L indicates $\nu~L_\nu$ for the monochromatic LLF and $L_{\rm IR}$ for the IR bolometric LLF.
$\log L$	$\log~(\phi,\sigma)_{250}$	$\log~(\phi,\sigma)_{350}$	$\log~(\phi,\sigma)_{500}$	$\log~(\phi,\sigma)_{\rm IR}$
7.5	-	-	-1.80, -2.69	-
8.0	-1.97, -2.27	-	-2.12, -2.16	-
8.5	-2.23, -2.63	-2.22, -2.92	-2.84, -2.92	-
9.0	-2.19, -3.00	-2.54, -3.05	-3.36, -3.56	-2.15, -3.00
9.5	-2.38, -4.50	-3.14, -3.57	-4.88, -6.14	-2.19, -2.61
10.0	-3.14, -4.28	-4.66, -4.80	-	-2.30, -2.72
10.5	-4.62, -5.23	-	-	-2.49, -3.16
11.0	-	-	-	-3.21, -3.95
11.5	-	-	-	-4.24, -4.65

Notes. L at the bin centers are expressed in $L_\odot$ while LLF estimates and their errors are in ${\rm [Mpc^{-3}~dex^{-1}]}$ .

Source LaTeX | All tables | In the text

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