Galaxy And Mass Assembly (GAMA): Trends in galaxy colours, morphology,
  and stellar populations with large scale structure, group, and pair
  environments
  We explore trends in galaxy properties with Mpc-scale structures using
catalogues of environment and large scale structure from the Galaxy And Mass
Assembly (GAMA) survey. Existing GAMA catalogues of large scale structure,
group and pair membership allow us to construct galaxy stellar mass functions
for different environmental types. To avoid simply extracting the known
underlying correlations between galaxy properties and stellar mass, we create a
mass matched sample of galaxies with stellar masses between $9.5 \leq
\log{M_*/h^{-2} M_{\odot}} \leq 11$ for each environmental population. Using
these samples, we show that mass normalised galaxies in different large scale
environments have similar energy outputs, $u-r$ colours, luminosities, and
morphologies. Extending our analysis to group and pair environments, we show
galaxies that are not in groups or pairs exhibit similar characteristics to
each other regardless of broader environment. For our mass controlled sample,
we fail to see a strong dependence of S\'{e}rsic index or galaxy luminosity on
halo mass, but do find that it correlates very strongly with colour. Repeating
our analysis for galaxies that have not been mass controlled introduces and
amplifies trends in the properties of galaxies in pairs, groups, and large
scale structure, indicating that stellar mass is the most important predictor
of the galaxy properties we examine, as opposed to environmental
classifications.
