Table 3.
Open in new tab

Estimates of the biweight location and scale of rest-frame g − r colour and stellar mass for the low halo mass clusters subsample.

Redshiftg − rδ(g − r)log (M*/M⊙)δlog (M*/M⊙)
0.05–0.150.720.0611.40.3
0.15–0.250.730.0511.40.3
0.25–0.350.740.0611.40.2
0.05–0.350.730.06
Redshiftg − rδ(g − r)log (M*/M⊙)δlog (M*/M⊙)
0.05–0.150.720.0611.40.3
0.15–0.250.730.0511.40.3
0.25–0.350.740.0611.40.2
0.05–0.350.730.06
Table 3.
Open in new tab

Estimates of the biweight location and scale of rest-frame g − r colour and stellar mass for the low halo mass clusters subsample.

Redshiftg − rδ(g − r)log (M*/M⊙)δlog (M*/M⊙)
0.05–0.150.720.0611.40.3
0.15–0.250.730.0511.40.3
0.25–0.350.740.0611.40.2
0.05–0.350.730.06
Redshiftg − rδ(g − r)log (M*/M⊙)δlog (M*/M⊙)
0.05–0.150.720.0611.40.3
0.15–0.250.730.0511.40.3
0.25–0.350.740.0611.40.2
0.05–0.350.730.06
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