Prospector: Stellar population inference from spectra and SEDs
Abstract
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.
- Publication:
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Astrophysics Source Code Library
- Pub Date:
- May 2019
- Bibcode:
- 2019ascl.soft05025J
- Keywords:
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- Software