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We explore trends in galaxy properties with Mpc-scale structures usingcatalogues of environment and large scale structure from the Galaxy And MassAssembly (GAMA) survey. Existing GAMA catalogues of large scale structure,group and pair membership allow us to construct galaxy stellar mass functionsfor different environmental types. To avoid simply extracting the knownunderlying correlations between galaxy properties and stellar mass, we create amass matched sample of galaxies with stellar masses between $9.5 \leq\log{M_*/h^{-2} M_{\odot}} \leq 11$ for each environmental population. Usingthese samples, we show that mass normalised galaxies in different large scaleenvironments have similar energy outputs, $u-r$ colours, luminosities, andmorphologies. Extending our analysis to group and pair environments, we showgalaxies that are not in groups or pairs exhibit similar characteristics toeach 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 onhalo mass, but do find that it correlates very strongly with colour. Repeatingour analysis for galaxies that have not been mass controlled introduces andamplifies trends in the properties of galaxies in pairs, groups, and largescale structure, indicating that stellar mass is the most important predictorof the galaxy properties we examine, as opposed to environmentalclassifications.

Galaxy And Mass Assembly (GAMA): Trends in galaxy colours, morphology,  and stellar populations with large scale structure, group, and pair  environments