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Table 4.

Most likely parameters when fitting to Eq. (9).

Sample n z σz M0 σM0 S0 σS0 γ σγ Scatter σScatter χ2
sSFR 4777 0.57 0.03 11.44 0.50 2.02 0.44 1.08 0.27 0.06 0.08 8.67
4770 0.67 0.03 11.48 0.48 2.22 0.49 1.15 0.29 0.05 0.09 10.04
4487 0.78 0.04 11.53 0.53 2.34 0.58 1.24 0.30 0.01 0.10 10.24 (b)
4026 0.96 0.09 11.90 0.48 2.61 0.45 1.07 0.41 0.06 0.10 9.24 (b)

NUVrJ 6043 0.57 0.03 9.85 (a) 1.15 0.57 0.38 1.42 0.44 0.07 0.11 5.73 (a)
6237 0.67 0.03 10.15 (a) 1.33 0.67 0.45 0.75 0.42 0.02 0.13 4.96 (a)
5812 0.78 0.04 11.66 0.79 2.41 0.62 1.37 0.53 0.07 0.17 7.34
4776 0.95 0.08 10.83 (a) 0.91 1.43 0.48 1.26 0.62 0.02 0.14 5.88

NUVrK 6055 0.57 0.03 9.76 (a) 1.08 0.52 0.38 1.76 0.44 0.06 0.11 5.76 (b)
6264 0.67 0.03 10.23 (a) 1.25 0.67 0.37 1.11 0.40 0.07 0.13 5.39 (b)
5803 0.78 0.04 10.84 (a) 1.27 1.30 0.53 1.23 0.51 0.08 0.15 5.80 (b)
4812 0.95 0.08 10.67 (a) 0.88 1.34 0.53 1.57 0.59 0.04 0.15 6.74

u − r 4762 0.57 0.03 11.24 (a) 0.55 1.71 0.44 1.09 0.34 0.01 0.10 5.85
4800 0.67 0.03 11.45 0.44 1.92 0.39 1.05 0.39 0.17 0.14 6.13
4697 0.78 0.04 11.49 (a) 0.50 2.37 0.41 1.36 0.49 0.02 0.14 5.90
4211 0.96 0.09 11.34 0.57 2.19 0.45 1.40 0.52 0.15 0.13 5.34

UVJ 5307 0.57 0.03 10.05 (a) 1.03 0.73 0.45 1.38 0.44 0.14 0.11 5.85
5389 0.67 0.03 10.58 (a) 1.22 0.95 0.44 0.97 0.44 0.05 0.13 4.83 (b)
5194 0.78 0.04 11.34 (a) 0.67 2.26 0.60 1.66 0.55 0.14 0.17 7.40
4481 0.95 0.09 10.78 (a) 0.80 1.61 0.45 1.87 0.64 0.14 0.14 5.72 (b)

BPT 2044 0.57 0.03 10.20 (a) 0.87 0.68 0.42 1.12 0.50 0.13 0.11 6.18 (b)
1058 0.67 0.03 10.66 (a) 0.96 0.88 0.42 0.70 0.51 0.00 0.14 2.77
1371 0.78 0.04 10.57 (a) 1.29 0.99 0.42 1.16 0.52 0.24 0.17 4.68 (b)
87 0.87 0.01 9.57 (a) 1.23 0.77 0.34 1.76 0.66 0.04 0.16 2.83

D4000 5947 0.57 0.03 9.94 (a) 1.31 0.50 0.42 0.91 0.46 0.08 0.11 5.36
6050 0.67 0.03 10.14 (a) 1.40 0.66 0.45 1.12 0.45 0.11 0.13 4.94 (b)
5625 0.78 0.04 10.28 (a) 1.64 0.69 0.48 1.30 0.49 0.15 0.15 4.77
4388 0.95 0.08 10.45 (a) 1.20 1.07 0.52 1.64 0.67 0.15 0.16 5.07 (b)

Notes.

(a)

M0 is inside of accepted range for turn-over, see text for ranges.

(b)

χ2 is lower than when fitted with Eq. (8).

n is the number of galaxies in the redshift bin, S0 is the value of S that the function approaches at high-mass, M0 is the turn-over mass in log(M), γ is the low mass slope, σx is the uncertainty on x, χ2 is the χ2 of the best fit, and TO is if there is evidence of a high-mass turnover (Y) or not (N). Redshifts and their uncertainties are the average redshift of the sample and sample standard deviation.

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