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Table 1.

Median Hα-based SFRs in stellar mass bins in the ALT sample at z = 3.7 − 5.1.

log(M/M) log(SFR/M yr−1) Mass completeness
6 . 8 0.3 + 0.2 Mathematical equation: $ 6.8 ^{+0.2}_{-0.3} $ 0 . 31 0.21 + 0.20 Mathematical equation: $ -0.31^{+0.20}_{-0.21} $ 5%
7 . 3 0.3 + 0.3 Mathematical equation: $ 7.3 ^{+0.3}_{-0.3} $ 0 . 13 0.22 + 0.21 Mathematical equation: $ -0.13^{+0.21}_{-0.22} $ 28%
7 . 9 0.3 + 0.3 Mathematical equation: $ 7.9 ^{+0.3}_{-0.3} $ 0 . 04 0.29 + 0.36 Mathematical equation: $ 0.04^{+0.36}_{-0.29} $ 70%
8 . 5 0.3 + 0.3 Mathematical equation: $ 8.5 ^{+0.3}_{-0.3} $ 0 . 26 0.38 + 0.43 Mathematical equation: $ 0.26^{+0.43}_{-0.38} $ 90%
9 . 0 0.3 + 0.4 Mathematical equation: $ 9.0 ^{+0.4}_{-0.3} $ 0 . 66 0.36 + 0.35 Mathematical equation: $ 0.66^{+0.35}_{-0.36} $ 98%
9 . 6 0.3 + 0.4 Mathematical equation: $ 9.6 ^{+0.4}_{-0.3} $ 1 . 09 0.52 + 0.45 Mathematical equation: $ 1.09^{+0.45}_{-0.52} $ 100%

Notes. We list the median values in each bin, and the errors correspond to the 16th and 84th percentiles, respectively. We also list the median mass completeness of our SFR-selected sample in each mass bin, estimated as described in Appendix A.

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