Table D.1.
Best-fit clustering parameters from 2pcf measurements.
| r0 [h−1 Mpc] | γ | bPL | bHOD | log(MDMH/[h−1 M⊙]) |
|---|---|---|---|---|
 |
 |
 |
 |
 |
Notes. The correlation length and slope, the linear bias factor assuming a PL correlation function, the linear bias factor and typical dark matter halo masses from the HOD model are indicated. The uncertainties in the bias factors and DMH masses reflect the statistical error on r0 only.
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