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Prospector: Stellar population inference from spectra and SEDs

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Ada Coda
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Prospector: Stellar population inference from spectra and SEDs

Postby Ada Coda » Fri May 31, 2019 10:17 pm

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.

Credit: Johnson, Benjamin D.; Leja, Joel L.; Conroy, Charlie; Speagle, Joshua S.

Site: https://doi.org/10.5281/zenodo.1116490
https://ui.adsabs.harvard.edu/abs/2019arXiv190504310S

Bibcode: 2019ascl.soft05025J

Preferred citation method: https://doi.org/10.5281/zenodo.1116490 and http://adsabs.harvard.edu/abs/2017ApJ...837..170L; please see additional citation information here: https://github.com/bd-j/prospector#citation

ID: ascl:1905.025
Last edited by Ada Coda on Thu Jun 13, 2019 5:39 pm, edited 1 time in total.
Reason: Updated code entry.

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