The LF of TP-AGB stars in the LMC and SMC
  We show that Montecarlo simulations of the TP-AGB stellar population in the LMC and SMC galaxies using the CB* models produce LF and color distributions that are in closer agreement with observations than those obtained with the BC03 and CB07 models. This is a progress report of work that will be published elsewhere. 
Gustavo Bruzual, Stephane Charlot, Rosa Gonzalez Lopezlira, Sundar   Srinivasan, Martha L. Boyer, and David Riebel
astro-ph.CO