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Table 1

Best-fit parameters assuming a double exponential profile fitted over the 1/Vmax non-parametric sSFR functions.

Median Average
N COSMOS log (sSFR) Φ log (sSFR) log (sSFR) χ 2
M bin z-bin + GOODS σ (Gyr-1) (10-3 Mpc-3) (Gyr-1) (Gyr-1)

9.5–10 combined 0.217 –1.028 2.912 –1.069 –0.940 154.021
0.2–0.4 1080+0 0.22 –0.704 9.377 –0.733 –0.602 29.228
0.4–0.6 643 +45 0.22 –0.562 5.520 –0.591 –0.460 9.621
0.6–0.8 1009+92 0.22 –0.347 6.624 –0.375 –0.245 14.771
0.8–1.0 1111+61 0.22 –0.258 6.815 –0.285 –0.156 21.068
1.0–1.2 546 +60 0.22 –0.072 4.660 –0.099 0.030 31.262
1.2–1.4 180 +29 0.22 –0.028 4.602 –0.057 0.073 9.320

10–10.5 combined 0.184 –1.018 4.183 –1.177 –1.060 324.531
0.2–0.4 991 +0 0.100 –0.230 28.446 –0.765 –0.671 18.421
0.4–0.6 1193+31 0.126 –0.229 12.144 –0.631 –0.532 41.747
0.6–0.8 1698+44 0.183 –0.270 5.883 –0.431 –0.314 15.312
0.8–1.0 2239+40 0.213 –0.180 4.277 –0.233 –0.105 41.264
1.0–1.2 1570+71 0.217 –0.044 2.807 –0.081 0.048 40.360
1.2–1.4 828 +34 0.170 0.245 4.428 0.033 0.146 8.663

10.5–11 combined 0.274 –1.605 1.566 –1.453 –1.300 157.307
0.2–0.4 539 +0 0.269 –1.156 1.474 –1.019 –0.869 4.849
0.4–0.6 697 +11 0.265 –0.981 1.165 –0.855 –0.708 11.454
0.6–0.8 1019+28 0.230 –0.631 1.601 –0.623 –0.490 25.423
0.8–1.0 1466+23 0.223 –0.436 2.008 –0.455 –0.324 38.968
1.0–1.2 947 +31 0.280 –0.496 0.699 –0.323 –0.167 23.345
1.2–1.4 885 +17 0.281 –0.345 0.639 –0.169 –0.013 19.457

11–11.5 combined 0.420 –2.565 0.419 –1.933 –1.691 51.328
0.2–0.4 100+0 0.481 –2.297 0.026 –1.455 –1.161 16.792
0.4–0.6 132+0 0.425 –1.894 0.040 –1.245 –1.000 6.035
0.6–0.8 200+0 0.359 –1.508 0.077 –1.077 –0.878 2.084
0.8–1.0 315+0 0.385 –1.370 0.073 –0.857 –0.641 2.618
1.0–1.2 199+0 0.438 –1.420 0.028 –0.727 –0.471 7.740
1.2–1.4 194+0 0.413 –1.116 0.026 –0.509 –0.272 10.272

Notes.In the lowest stellar mass bin 9.5 < log (M⋆) < 10, we set the value of σ which is not constrained. Systematic uncertainties are not included. We consider that a systematic uncertainty of + 0.1 dex could affect SFR measurement (see Sect. 2). Assuming a systematic uncertainty of ±0.1 dex in the stellar mass, we obtain a systematic uncertainty of in the log (sSFR), the median and the averaged sSFR estimates.

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