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 2:

Differential number counts at 24 $\mu$ m.
$\langle S\rangle$	$S_{\rm min}$	$S_{\rm max}$	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
0.040	0.035	0.044	17.5	1.0	1.1	1.3	0.2
0.050	0.044	0.056	21.4	1.0	1.1	1.4	0.2
0.064	0.056	0.071	28.2	1.2	1.5	1.8	0.2
0.081	0.071	0.090	36.2	1.5	1.9	2.4	0.2
0.102	0.090	0.114	52.6	1.3	1.9	2.9	0.6
0.130	0.114	0.145	64.1	1.0	1.7	3.1	3.4
0.164	0.145	0.184	78.7	1.1	2.2	3.8	3.4
0.208	0.184	0.233	89.8	1.3	2.8	4.5	3.4
0.264	0.233	0.295	96.5	1.5	3.3	5.1	3.4
0.335	0.295	0.374	112.0	0.8	1.8	4.8	37.2
0.424	0.374	0.474	103.7	0.6	1.7	4.5	46.1
0.538	0.474	0.601	91.9	0.6	1.5	4.0	53.6
0.681	0.601	0.762	81.2	0.6	1.5	3.6	53.6
0.863	0.762	0.965	72.8	0.7	1.6	3.3	53.6
1.094	0.965	1.223	65.3	0.8	1.6	3.1	53.6
1.387	1.223	1.550	60.8	0.9	1.7	3.0	53.6
1.758	1.550	1.965	56.7	1.0	1.8	2.9	53.6
2.228	1.965	2.490	55.4	1.2	2.1	3.0	53.6
2.823	2.490	3.156	54.0	1.5	2.3	3.2	53.6
3.578	3.156	4.000	55.9	1.8	2.7	3.5	53.6
5.807	4.000	7.615	54.8	1.5	2.9	3.6	53.6
11.055	7.615	14.496	46.9	2.3	3.6	4.1	53.6
21.045	14.496	27.595	36.4	3.3	4.4	4.6	53.6
40.063	27.595	52.531	43.4	5.9	7.7	7.9	53.6
76.265	52.531	100.000	47.7	9.9	12.0	12.2	53.6

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

Source LaTeX | All tables | In the text

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