The 0.4 z 1.3 star formation history of the Universe as viewed in the far-infrared

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Volume 496 / No 1 (March II 2009)

A&A, 496 1 (2009) 57-75

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Table 1:

Catalog properties.
Field	Area	Exposure	Flux limit^a	Completeness^b	Contamination^b	# sources
	( $\rm {arcmin^{2}}$ )	( $\rm {s/pixel}$ )	( $\rm {\mu Jy}$ )	( $\%\ {\rm at}\ S=S_{\rm limit}$ )	( $\%\ {\rm at}\ S=S_{\rm limit}$ )	( ${\rm with}\ S \ge S_{\rm limit}$ )
EGS 24	548	14 000	50 (5 $\sigma$ )	75	11	4096
GOODS-S 24	91	35 000	30 (5 $\sigma$ )	81	13	870
GOODS-N 24	194	35 000	30 (5 $\sigma$ )	81	13	2151
ECDFS-O 24	517	8000	70 (5 $\sigma$ )	100	0	2474
EGS 70	548	7200	3000 (6 $\sigma$ )	77	10	322
GOODS-S 70	91	10 800	2500 (6 $\sigma$ )	73	12	44
GOODS-N 70	194	10 800	2500 (6 $\sigma$ )	73	12	119
ECDFS-O 70	517	5750	3500 (6 $\sigma$ )	85	7	195

^a The level of the noise was calculated on the residual images and hence it combines the confusion, instrumental and photon noises.
^b See text for the definition of the completeness and contamination.

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