Evidence for anisotropic quenching in massive galaxy clusters at
  $z\approx0.5$
  A recent observational result finds that the quenching of satellites in
groups at $z=0.08$ has an angular dependence relative to the semi-major axis of
the central galaxy. This observation is described as `anisotropic quenching' or
`angular conformity'. In this paper I study the variation in the colour of a
mass limited sample of satellite galaxies relative to their angle from the
major axis of the Brightest Cluster Galaxy in the CLASH clusters up to
$z\sim0.5$, 4 Gyr further in lookback time. The same result is found: galaxies
close to the major axis are more quenched than those along the minor axis. I
also find that the star-forming galaxies tend to avoid a region +/-45 degrees
from the major axis. This quenching signal is thought to be driven by AGN
outflows along the minor axis, reducing the density of the intergalactic medium
and thus the strength of ram pressure. Here I will discuss potential
alternative mechanisms. Finally, I note that the advent of the Legacy Survey of
Space and Time (LSST) and Euclid surveys will allow for a more detailed study
of this phenomenon and its evolution.
