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Table 2:

Number counts deduced from source extraction. The not normalized counts can be obtained dividing the S2.5.dN/dS column by the $S_{\rm mean}$ column.

Wavelength 		$S_{\rm mean}$ $S_{\rm min}$ $S_{\rm max}$ $N_{\rm sources}$ S2.5. ${\rm d}N/{\rm d}S$ $\sigma_{S^{2.5}.{\rm d}N/{\rm d}S}$ Method
$\mu $m mJy galaxies gal Jy $^{1.5}~{\rm sr}^{-1}$  
250 79 64 97 26 4451 1203 Prior
250 116 97 140 5 4529 2090 Deep
250 168 140 203 3 4040 2377 Deep
250 261 203 336 34 2987 784 Shallow
250 430 336 552 5 1023 479 Shallow
250 708 552 910 1 445 449 Shallow
250 1168 910 1500 2 1939 1401 Shallow
350 67 54 83 17 1913 630 Prior
350 115 83 161 2 955 687 Deep
350 223 161 310 16 854 299 Shallow
350 431 310 600 2 314 228 Shallow
500 61 49 76 7 388 178 Prior
500 99 76 131 1 443 448 Deep
500 185 131 262 4 129 99 Shallow


Source LaTeX | All tables | In the text

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