Table 5:

Comparison of major surveys carried out at 15 m listed by mission, then by decreasing areal coverage.

Satellite	Survey	Area	Sensitivity	Sources	Volume
		(deg2)	(mJy)	(number)	(Mpc3)
AKARI	NEP-wide1	5.8	0.25*	10686	57.2
AKARI	NEP-deep2	0.6	0.1*	6737	6.17
AKARI	NEP-PV3	0.02	0.07	277	0.21
AKARI	Abell 22184	0.034	0.042	565	0.35
Spitzer	HDF-S5	0.04 (0.003)	0.09 (0.04)	515	0.41 (0.031)
Spitzer	HDF-N6	0.01	0.08	153	0.1
ISO	ELAIS S17	4.17	0.5	736	38.86
ISO	ELAIS N17	2.67	0.5	490	24.88
ISO	ELAIS N27	2.67	0.5	566	24.88
ISO	ELAIS N37	0.88	0.5	131	8.2
ISO	Lockman hole shallow8	0.55	0.25	457	5.41
ISO	Marano deep9	0.25	0.3	180	2.44
ISO	Lockman hole deep10	0.14	0.2	283	1.39
ISO	ELAIS S211	0.12	0.4	43	1.15
ISO	CFRS 1452 field12	0.028	0.4	41	0.27
ISO	Marano UDSR9	0.025	0.3	142	0.244
ISO	Marano UDSF9	0.025	0.3	137	0.244
ISO	A370 cluster13	0.009	0.2	20	0.09
ISO	HDF-S14	0.008	0.25	24	0.079
ISO	HDF-N15	0.007	0.2	19	0.069
ISO	A2218 cluster13	0.006	0.1	46	0.062
ISO	A2390 cluster16	0.0015	0.1	34	0.015

Notes. ^(*) 5 sensitivity above the noise.

References. ¹ Lee et al. (2008); ² Wada et al. (2008); ³ Lee et al. (2008); ⁴ Hopwood (2010); ⁵ Teplitz et al. (2005); ⁶ Teplitz et al. (2005); ⁷ Vaccari et al. (2005); ⁸ Fadda et al. (2004); ⁹ Elbaz et al. (1999); ¹⁰ Rodighiero et al. (2004); ¹¹ Pozzi et al. (2003); ¹² Flores et al. (1999); ¹³ Metcalfe et al. (2003); ¹⁴ Oliver et al. (2002); ¹⁵ Serjeant et al. (1997); ¹⁶ Altieri et al. (1999).