Galactic conformity measured in semi-analytic models
  We study the correlation between the specific star formation rate of central
galaxies and neighbour galaxies, also known as 'galactic conformity', out to 20
Mpc/h using three semi-analytic models (SAMs, one from L-GALAXIES and other two
from GALFORM). The aim is to establish whether SAMs are able to show galactic
conformity using different models and selection criteria. In all the models,
when the selection of primary galaxies is based on an isolation criterion in
real space, the mean fraction of quenched galaxies around quenched primary
galaxies is higher than that around star-forming primary galaxies of the same
stellar mass. The overall signal of conformity decreases when we remove
satellites selected as primary galaxies, but the effect is much stronger in
GALFORM models compared with the L-GALAXIES model. We find this difference is
partially explained by the fact that in GALFORM once a galaxy becomes a
satellite remains as such, whereas satellites can become centrals at a later
time in L-GALAXIES. The signal of conformity decreases down to 60% in the
L-GALAXIES model after removing central galaxies that were ejected from their
host halo in the past. Galactic conformity is also influenced by primary
galaxies at fixed stellar mass that reside in dark matter haloes of different
masses. Finally, we explore a proxy of conformity between distinct haloes. In
this case the conformity is weak beyond ~ 3 Mpc/h (<3% in L-GALAXIES, <1-2% in
GALFORM models). Therefore, it seems difficult that conformity is directly
related with a long-range effect.
