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Table 1

Summary of data used in Fig. 1.

Reference N λobs Slim Method
μm mJy

Berta et al. (2011) 5360 100 9 a, b
Béthermin et al. (2012b) 2517 250 20 a, b
Geach et al. (2013) 60 450 5 b
Casey et al. (2013) 78 450 13 b
Wardlow et al. (2011) 72 850 4 b
Simpson et al. (2014) 77 850 4 b, e
Chapman et al. (2005) 73 850 3 c
Smolcic et al. (2012) 28 1100 1.4 b, e
Michałowski et al. (2012) 95 1100 1 b
Yun et al. (2012) 27 1100 2 b
Weiß et al. (2013) 23 1400 20 d, f
Staguhn et al. (2014) 5 2000 0.24 b, c

Notes. a) extraction of the sources based on PSF-fitting codes using short-wavelength priors; b) photometric redshifts; c) optical/near-infrared spectroscopic redshift after radio identification; d) millimeter spectroscopic redshift; e) identification of the optical/near-infrared counterparts using high-resolution (sub-)millimeter data.

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