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Table 4.
Best HOD fit large-scale bias factor and typical DMH mass for the LAE subsamples.
| Subsample | ⟨z⟩ | b | log(Mh/[h−1 M⊙]) |
|---|---|---|---|
| MUSE-Wide high L | 4.1 |
 |
 |
| MUSE-Wide low L | 3.7 |
 |
 |
| MUSE-Deep high L | 4.5 |
 |
 |
| MUSE-Deep low L | 3.7 |
 |
 |
| MXDF high L | 4.5 |
 |
 |
| MXDF low L | 4.0 |
 |
 |
Notes. ⟨z⟩ is the median redshift of the subsample. The uncertainties do not include cosmic sample variance.
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