Table C.3.
Star formation surface density (ΣSFR) as a function of distance to the MS of SFGs.
| Δ log(SSFR)MS (dex) | 0.35 < z < 0.65 | 0.65 < z < 0.95 | 0.95 < z < 1.30 | 1.30 < z < 1.75 | 1.75 < z < 2.25 |
|---|---|---|---|---|---|
| [−0.3, 0.3] |  |
 |
 |
 |
 |
| [0.3, 0.9] |  |
 |
 |
 |
 |
| >0.9 (a) |  |
 |
 |
 |
 |
Notes. ΣSFR is given in M⊙ yr−1 kpc−2. The uncertainties correspond to the 16th and 84th percentiles of the ΣSFR distribution per Δ log(SSFR)MS bin. The minimum stellar mass probed throughout the different redshift bins is 
, 10.2, 10.5, 10.5, and 10.7.
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