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Table 3

Summary of different galaxy populations discussed in Sect. 4.9.

Population N sample a z M ⋆ b b,c red [kpc] Reference
z ≤ 3 SMGs 88 0.86−2.93 (2.03) 9.58−11.84 (11.20) 10.29−11.86 (11.26) ... This work
z ≤ 3 SMGs 52 1.33−2.97 (2.10) 8.38−11.89 (10.58) ... ... da Cunha et al. (2015)
z> 3 SMGs 36 3.06−6.40 (3.91) 10.30−12.25 (10.95) 10.51−12.25 (11.09) ... This work
z> 3 SMGs 47 3.03−6.12 (3.67) 10.21−11.87 (10.92) ... ... da Cunha et al. (2015)
cSFGs 59 2.03−2.98 (2.35) 10.01−11.73 (10.89) ... 0.04−7.04 (1.34) Fang et al. (2015)
cSFGs 45 1.97−2.79 (2.43) 10.20−11.28 (10.82) ... 0.29−2.97 (1.0) Barro et al. (2014)
cQGs 85 0.213−0.746 (0.438) 11.05−11.85 (11.41) ... 1.18−9.04 (3.99) Zahid et al. (2015)
cQGs 56 0.901−1.598 (1.242) 10.27−11.34 (10.84) ... 0.73−7.18 (1.96) Belli et al. (2014)
cQGs 7 1.39−2.47 (1.76) 10.44−11.60 (10.74−11.0)e ... 0.6−5.6 (0.8)e Daddi et al. (2005)
cQGs 34 1.84−2.28 (2.08) 10.62−11.68 (10.96) ... 0.46−10.0 (2.67) Krogager et al. (2014)
cQGs 9 2.02−2.56 (2.34) 10.75−11.47 (11.21) ... 0.47−2.38 (0.92) van Dokkum et al. (2008)
cQGs 16 3.46−4.05 (3.61) 10.60−11.25 (10.88) ... 0.27−3.22 (0.58) Straatman et al. (2015)
ETGs 12 1.242−1.910 (1.396) 11.03−11.59 (11.19) ... 1.5−4.34 (2.5) Gargiulo et al. (2016)

Notes. For each parameter, we give the range of values, and the median value is given in parenthesis.

(a)

Number of sources in the sample.

(b)

The stellar masses are normalised to a Chabrier (2003) IMF, and given in units of log (M⋆/M⊙).

(c)

The estimated final stellar masses of our SMGs were calculated by assuming a SFE of 10% (see text for details).

(d)

Circularised effective radius.

(e)

The stellar mass ranges were calculated from the range of values reported in Table 3 of Daddi et al. (2005), while the effective radii were read from their Fig. 12.

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