Wofford, A., S. Charlot, G. Bruzual, J. J. Eldridge, D. Calzetti, A. Adamo, M. Cignoni, S. E. de Mink, D. A. Gouliermis, K. Grasha, E. K. Grebel, J. C. Lee, G. Östlin, L. J. Smith, L. Ubeda and E. Zackrisson: A comprehensive comparative test of seven widely used spectral synthesis models against multi-band photometry of young massive-star clusters. In: Monthly Notices of the Royal Astronomical Society 457, 4, 4296-4322 (2016).
url: http://adsabs.harvard.edu/abs/2016MNRAS.457.4296W
Walcher, C. J., R. M. Yates, I. Minchev, C. Chiappini, M. Bergemann, G. Bruzual, S. Charlot, P. R. T. Coelho, A. Gallazzi and M. Martig: Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia. In: Astronomy and Astrophysics 594, (2016).
url: http://cdsads.u-strasbg.fr/abs/2016A%26A...594A..61W
Eminian, C., G. Kauffmann, S. Charlot, V. Wild, G. Bruzual, A. Rettura and J. Loveday: Physical interpretation of the near-infrared colours of low-redshift galaxies. In: Monthly Notices of the Royal Astronomical Society 384, 3, 930-942 (2008).
doi: 10.1111/j.1365-2966.2007.12742.x
Coelho, P., G. Bruzual, S. Charlot, A. Weiss, B. Barbuy and J. W. Ferguson: Spectral models for solar-scaled and α-enhanced stellar populations. In: Monthly Notices of the Royal Astronomical Society 382, 2, 498-514 (2007).
doi: 10.1111/j.1365-2966.2007.12364.x
Coelho, P., G. Bruzual, S. Charlot, A. Weiss and B. Barbuy: High resolution spectral models for solar scaled and α-enhanced compositions. In: Stellar Populations as Building Blocks of Galaxies, (Eds.) A. Vazdekis, R. Peletier. IAU Symposium and Colloquium Proceedings Series IAU Symposium 241. Cambridge University Press, Cambridge, UK (2007) 138-142.
localid: Reihe: IAU...., 241 p.138-142
doi: 10.1017/S1743921307007648
Bruzual, G. and S. Charlot: Stellar population synthesis at the resolution of 2003. In: Monthly Notices of the Royal Astronomical Society 344, 1, 1000-1028 (2003).
Cardiel, N., J. Gorgas, P. Sánchez-Blázquez, A. J. Cenarro, S. Pedraz, G. Bruzual and J. Klement: Using spectroscopic data to disentangle stellar population properties. In: Astronomy and Astrophysics 409, 511-522 (2003).
http://edoc.mpg.de
The Max Planck Society does not take any responsibility for the content of this export.