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Table 3.
Percentages of galaxies located above (top line) and within (bottom line) the Vulcani et al. (2016) main sequence (MS) for our four samples and for the RPS candidates of MACS0717, all the samples being cut at 109 ≤ M ≤ 1010.5 M⊙.
| Sample 1 | Sample 2 | Sample 3 | Sample 4 | MACS0717 | |
|---|---|---|---|---|---|
| Above MS | 50% | 47% | 13% | 18% | 38% |
| In MS | 5% | 32% | 20% | 20% | 41% |
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