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Fig. 5.


68% and 95% likelihood contours for the Schechter parameters α and M*, for the different galaxy types in different panels. Black: schechter parameters of field galaxy population. Other colours: schechter parameters of the cluster galaxies, in different radial bins, as indicated. The lines within the contours indicate how cosmic variance (+/−1σ) affects the best-fit Schechter parameters. That effect is strongest for the star-forming galaxies at large clustercentric distances, where the overdensity compared to the background is lowest.

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