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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