Open Access
Table 4.
Fraction of galaxies with at least one substructure detected at a rest-frame wavelength of 1 μm as a function of redshift.
| Redshift interval | [1.0, 1.2) | [1.2, 1.4) | [1.4, 1.6) | [1.6, 1.8) | [1.8, 2.0) | [2.0, 2.2) | [2.2, 2.4) | [2.4, 2.6) | [2.6, 2.8) | [2.8, 3.0) | [3.0, 3.2) | [3.2, 3.4) | [3.4, 3.6) | [3.6, 3.8) | [3.8, 4.0] |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Intrinsic – All | 13% | 16% | 18% | 27% | 16% | 25% | 26% | 35% | 25% | 30% | 34% | 33% | 35% | 39% | 31% |
| Optimal – All | 83% | 82% | 77% | 77% | 67% | 63% | 57% | 61% | 49% | 49% | 52% | 46% | 44% | 46% | 36% |
| Intrinsic – clumps | 13% | 16% | 18% | 27% | 16% | 25% | 26% | 35% | 25% | 30% | 34% | 33% | 35% | 39% | 31% |
| Optimal – clumps | 58% | 60% | 56% | 55% | 51% | 45% | 41% | 43% | 35% | 35% | 36% | 31% | 30% | 28% | 22% |
Notes. We separate between all kinds of detections and clumps only (see Sect. 4.2).
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