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Stellar Population Inference with Prospector
[article]
2020
arXiv
pre-print
Inference of the physical properties of stellar populations from observed photometry and spectroscopy is a key goal in the study of galaxy evolution. In recent years the quality and quantity of the available data has increased, and there have been corresponding efforts to increase the realism of the stellar population models used to interpret these observations. Describing the observed galaxy spectral energy distributions in detail now requires physical models with a large number of highly
arXiv:2012.01426v1
fatcat:6kqwmxtqgbb43mx4rsnxonkxme