Image Details
Caption: Figure 4.
Mean logarithmic halo mass for three different values of
W
r
.
log
M
evolves strongly with redshift for weak absorbers but is nearly flat for strong absorbers. At
z < 1, this produces the
b
W
–
W
r
anti-correlation. At
z ~ 1.3,
W
r
is roughly independent of redshift. At higher
z,
W
r
, and
b
W
are positively correlated.
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