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Tracers of stellar mass loss - I. Optical and near-IR colours and surface brightness fluctuations
Rosa A. González-Lópezlira, Gustavo Bruzual-A., Stéphane Charlot, Javier Ballesteros-Paredes and Laurent Loinard Monthly Notices of the Royal Astronomical Society 403(3) 1213 (2010) https://doi.org/10.1111/j.1365-2966.2009.16205.x
TP-AGB stars in population synthesis models
Paola Marigo, Léo Girardi, Alessandro Bressan, et al. Proceedings of the International Astronomical Union 5(S262) 36 (2009) https://doi.org/10.1017/S1743921310002498
Simulating the mass-metallicity relation from z $\mathsf{\sim}$ 1
The stellar halo metallicity—luminosity relationship for spiral galaxies
Agostino Renda, Brad K. Gibson, Mustapha Mouhcine, Rodrigo A. Ibata, Daisuke Kawata, Chris Flynn and Chris B. Brook Monthly Notices of the Royal Astronomical Society: Letters 363(1) L16 (2005) https://doi.org/10.1111/j.1745-3933.2005.00075.x
New near-infrared surface brightness fluctuation models
Is the initial mass function of low surface brightness galaxies dominated by low-mass stars?
Hyun-chul Lee, Brad K. Gibson, Chris Flynn, Daisuke Kawata and Michael A. Beasley Monthly Notices of the Royal Astronomical Society 353(1) 113 (2004) https://doi.org/10.1111/j.1365-2966.2004.08049.x
Very luminous carbon stars in the outer disk of the Triangulum spiral galaxy
D. L. Block, K. C. Freeman, I. Puerari, et al. Astrophysics and Space Science Library, Penetrating Bars through Masks of Cosmic Dust 319 15 (2004) https://doi.org/10.1007/978-1-4020-2862-5_2
to Z/Z 