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[ascl:1905.025] Prospector: Stellar population inference from spectra and SEDs

Prospector conducts principled inference of stellar population properties from photometric and/or spectroscopic data. The code combine photometric and spectroscopic data rigorously using a flexible spectroscopic calibration model and infer high-dimensional stellar population properties using parameteric SFHs (with ensemble MCMC sampling). Prospector also constrains the linear combination of stellar population components that are present in a galaxy (e.g. non-parametric SFHs) using spectra and/or photometry, and fits individual stellar spectra using large interpolated grids.

Code site:
https://github.com/bd-j/prospector/tree/v0.1 https://doi.org/10.5281/zenodo.1116490
Used in:
https://ui.adsabs.harvard.edu/abs/2019arXiv190504310S
Described in:
https://ui.adsabs.harvard.edu/abs/2017ApJ...837..170L
Bibcode:
2019ascl.soft05025J

Views: 336

ascl:1905.025
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