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

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Volume 512 (March-April 2010)

A&A, 512 (2010) A78

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Table 4:

Differential number counts at 160 $\mu$ m. $\sigma _{clustering}$ is the uncertainty taking into account clustering (see Sect. 4.5).
$\langle S\rangle$	$S_{\rm min}$	$S_{\rm max}$	d $N/{\rm d}S.S^{2.5}$	$\sigma_{\rm poisson}$	$\sigma_{\rm clustering}$	$\sigma_{\rm clus.+calib.}$	$\Omega_{\rm used}$
(in mJy)			(in gal Jy^1.5 sr^-1)				deg²
45.747	40.000	51.493	16855.	1312.	2879.	3519.	3.0
58.891	51.493	66.289	14926.	1243.	2704.	3243.	3.0
75.813	66.289	85.336	13498.	1319.	2648.	3104.	3.0
97.596	85.336	109.860	12000.	1407.	2442.	2835.	3.0
125.640	109.860	141.420	10687.	457.	991.	1621.	36.2
161.740	141.420	182.060	7769.	425.	773.	1211.	42.9
208.210	182.060	234.370	7197.	472.	810.	1184.	42.9
268.040	234.370	301.710	5406.	487.	734.	979.	42.9
345.050	301.710	388.400	5397.	585.	843.	1063.	42.9
444.200	388.400	500.000	4759.	662.	891.	1059.	42.9
750.000	500.000	1000.000	6258.	685.	1158.	1380.	42.9
1500.000	1000.000	2000.000	4632.	989.	1379.	1487.	42.9

Notes. $\sigma_{clus.+calib.}$ takes into account both clustering and calibration (Stansberry et al. 2007).

Source LaTeX | All tables | In the text

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