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Table 1

Slope and intercept (log 10SFR = a + b·log 10(M9)) of the main sequence in different redshift bins and for different SFRIR derivation methods.

Method 0.5 ≤ z< 1 1 ≤ z< 2 2 ≤ z< 3

a b a b a b

SFR UV 0.18±0.03 0.93±0.03 0.32±0.06 0.86±0.05 0.40±0.05 0.83±0.05
SFR UV + SFR 0.15±0.04 0.88±0.04 0.32±0.06 0.85±0.06 0.39±0.06 0.83±0.06
SFR UV + SFR 0.14±0.04 0.87±0.04 0.32±0.05 0.87±0.05 0.39±0.04 0.88±0.04
SFR UV + SFR 0.16±0.04 0.90±0.04 0.32±0.06 0.84±0.05 0.38±0.03 0.93±0.04
SFR UV + SFR 0.15±0.03 0.89±0.03 0.32±0.06 0.85±0.05 0.39±0.05 0.85±0.05
SFR UV + SFR 0.18±0.03 0.93±0.03 0.32±0.05 0.88±0.05 0.40±0.07 0.82±0.07

Notes. The MS is derived by using an ODR fitting to the mean position of the MS Gaussian component in the SFR distribution inside each 0.25 dex stellar mass bin.

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