The role of stellar mass in the cosmic history of star formation as seen by Herschel and ALMA

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Table B.1.

Best-fit parameters of M_gas evolution of the main sequence.

A	B	F	D	β^*

$0 . 136_{- 0.103}^{+ 0.235}$ $0.136^{+0.235}_{-0.103}$	$- 1 . 68_{- 0.63}^{+ 0.56}$ $-1.68^{+0.56}_{-0.63}$	$0 . 897_{- 0.282}^{+ 0.151}$ $0.897^{+0.151}_{-0.282}$	$- 0 . 321_{- 0.088}^{+ 0.090}$ $-0.321^{+0.090}_{-0.088}$	2

Notes. Best-fit parameters of M_gas evolution of the main sequence using Eq. 20 when using the method from Scoville et al. (2016) only. ^* indicates that this parameter was fixed during the fit.

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