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

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Table 5:

Stacking extragalactic number counts at 70 $\mu$ 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)
$0.38\pm 0.05$	246.	72.	76.	FIDEL CDFS
$0.64\pm 0.07$	517.	109.	122.	FIDEL CDFS
$0.94\pm 0.03$	646.	80.	105.	COSMOS
$1.48\pm 0.04$	1218.	151.	198.	COSMOS
$2.14\pm 0.05$	1456.	183.	239.	COSMOS
$3.27\pm 0.07$	1657.	211.	273.	COSMOS

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 (Gordon et al. 2007).

Source LaTeX | All tables | In the text

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