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Data and best-fitting stellar populations model.
Lu, J. R. et al. Stellar populations in the central 0.5 pc of the Galaxy.
Schaerer, D. On the properties of massive Population III stars and metal-free stellar populations.
Developing an alternative method to measure the history of stellar populations" Optical photometry and in particular color-magnitude diagrams are a standard tool for studies of stellar populations.
Galaxies can be described in terms of their structure, dynamics and stellar populations.
Our final objects have structure and stellar populations consistent with observed dwarf galaxies.
Different stellar populations tell astronomers different things about the history of a galaxy.
In this context, we present a flexible hierarchical model for analyzing stellar populations.
We investigated the efficiency of estimating characteristics of stellar populations (SP) and Active Galactic Nuclei (AGN) emission using ULySS code.
So a star with a given colour could belong to one of several different stellar populations with different luminosities.
The estimation of properties of stellar populations provides an example of statistical modeling with such a 'look-up table' likelihood.
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CEO of Professional Science Editing for Scientists @ prosciediting.com