Spitzer deep and wide legacy mid- and far-infrared number counts and lower limits of cosmic infrared background

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Table 6:

Stacking extragalactic number counts at 160 $\mu$ m.
$\langle S\rangle$	d $N/{\rm d}S.S^{2.5}$	$\sigma_{\rm clus.}$	$\sigma_{\rm clus.+calib.}$	Field
(in mJy)	(in gal Jy^1.5 sr^-1)
$3.11\pm 0.46$	6795.	2163.	2485.	GTO CDFS
$4.71\pm 0.16$	9458.	1236.	2104.	COSMOS
$6.74\pm 0.22$	13203.	1627.	2880.	COSMOS
$9.65\pm 0.26$	18057.	2307.	3986.	COSMOS
$12.95\pm 0.37$	19075.	2388.	4182.	COSMOS
$19.82\pm 0.48$	22366.	2944.	4987.	SWIRE EN1
$25.71\pm 0.81$	20798.	2811.	4682.	SWIRE EN1
$33.74\pm 0.98$	16567.	2671.	4004.	SWIRE EN1
$45.18\pm 2.08$	20089.	4849.	6049.	SWIRE EN1

Notes. $\sigma_{\rm clus.}$ is the uncertainty taking into account clustering (see Sect. 4.5). $\sigma_{\rm clus.+calib.}$ takes into account both clustering and calibration (Stansberry et al. 2007).

Source LaTeX | All tables | In the text

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