Table 3.
Best-fit HOD parameters for the main samples of LAEs.
| ⟨z⟩ | log(Mmin/[h−1 M⊙]) | log(M1/Mmin) | α | fsat | b | log(Mh/[h−1 M⊙]) | |
|---|---|---|---|---|---|---|---|
| MUSE-Wide | 4.0 |
 |
 |
 |
 |
 |
 |
| MUSE-Deep | 4.1 |
 |
 |
 |
 |
 |
 |
| MXDF | 4.2 |
 |
 |
 |
 |
 |
 |
Notes. ⟨z⟩ is the median redshift of the sample. Mmin, M1 are the threshold DMH masses to host a central and a satellite LAE, respectively. α is the high-mass power-law slope of the number of satellite galaxies, fsat is the satellite fraction, b is the large-scale bias factor and Mh is the typical DMH mass of the galaxy sample.
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