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We describe modifications to the joint stepwise maximum likelihood method ofCole (2011) in order to simultaneously fit the GAMA-II galaxy luminosityfunction (LF), corrected for radial density variations, and its evolution withredshift. The whole sample is reasonably well-fit with luminosity (Qe) anddensity (Pe) evolution parameters Qe, Pe = 1.0, 1.0 but with significantdegeneracies characterized by Qe = 1.4 - 0.4Pe. Blue galaxies exhibit largerluminosity density evolution than red galaxies, as expected. We present theevolution-corrected r-band LF for the whole sample and for blue and redsub-samples, using both Petrosian and Sersic magnitudes. Petrosian magnitudesmiss a substantial fraction of the flux of de Vaucouleurs profile galaxies: theSersic LF is substantially higher than the Petrosian LF at the bright end.

Galaxy and Mass Assembly (GAMA): maximum likelihood determination of the luminosity function and its evolution