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Table A.1

continued.

M (log M)

M10a H11b H11c C10d C10e C10f C10g C10h C10i
Padova BC03 M05 BC03 BC03 BC03 M05 M05 M05
SMG z double single single 1burst tau 2burst 1burst tau 2burst

SMMJ163627.94+405811.2 3.180 10.985 10.580 10.249 10.420 10.760 11.090 10.590 10.730 11.120
SMMJ163631.47+405546.9 2.283 11.435 10.830 10.699 10.860 10.420 10.860 11.180 8.610 11.660
SMMJ163639.01+405635.9 1.495 10.975 10.700 10.539 11.210 10.330 11.210 11.220 8.510 11.520
SMMJ163650.43+405734.5 2.378 11.315 11.160 10.939 11.580 11.590 11.580 11.720 11.720 12.180
SMMJ163658.19+410523.8 2.454 11.515 11.110 10.959 11.050 11.750 11.910 11.350 11.700 11.760
SMMJ163658.78+405728.1 1.190 11.235 10.990 10.839 10.800 10.380 10.800 11.110 8.960 11.480
SMMJ163704.34+410530.3 0.840 10.595 9.940 9.759 9.980 9.950 10.540 10.210 9.410 10.620
SMMJ163706.51+405313.8 2.374 11.655 11.210 11.079 11.460 11.230 12.010 11.670 10.530 12.090
SMMJ221724.69+001242.1 0.510 11.055 –99.000 –99.000 10.580 10.150 11.680 10.890 8.340 11.900
SMMJ221725.97+001238.9 3.094 11.705 –99.000 –99.000 10.860 11.480 11.470 11.170 11.380 11.510
SMMJ221733.02+000906.0 0.926 11.385 –99.000 –99.000 12.000 12.000 12.000 12.100 12.090 11.760
SMMJ221733.12+001120.2 0.652 11.075 10.700 10.579 10.420 10.550 10.420 10.740 10.140 11.680
SMMJ221733.91+001352.1 2.555 11.715 11.160 10.959 11.200 11.520 11.860 11.490 11.090 11.890
SMMJ221735.15+001537.2 3.098 11.115 10.710 10.459 10.620 11.050 11.280 10.900 10.970 11.280
SMMJ221735.84+001558.9 3.089 11.155 10.860 10.689 10.930 11.350 11.720 11.220 11.070 11.600
SMMJ221737.39+001025.1 2.614 11.315 –99.000 –99.000 10.960 11.470 11.370 11.010 11.410 11.490
SMMJ221804.42+002154.4 2.517 11.035 10.920 10.739 10.800 10.450 11.470 11.080 10.230 11.500
SMMJ221806.77+001245.7 3.623 11.315 11.010 10.839 11.330 11.730 11.990 11.600 11.570 12.140

Notes. The Chabrier (2003) IMF is assumed. –99 indicates the lack of an estimate for a given SMG. References: M10 (Michałowski et al. 2010a); H11 (Hainline et al. 2011); C10 (Cirasuolo et al. 2010); BC03 (Bruzual & Charlot 2003); M05 (Maraston 2005).

(a)

Stellar mass derived by M10.

(b)

Stellar mass derived by H11 with BC03 models.

(c)

Stellar mass derived by H11 with M05 models.

(d)

Stellar mass derived as in C10 with BC03 models and single-burst SFH.

(e)

Stellar mass derived as in C10 with BC03 models and tau SFH.

(f)

Stellar mass derived as in C10 with BC03 models and double-burst SFH.

(g)

Stellar mass derived as in C10 with M05 models and single-burst SFH.

(h)

Stellar mass derived as in C10 with M05 models and tau SFH.

(i)

Stellar mass derived as in C10 with M05 models and double-burst SFH.

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