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[ascl:1904.011] FortesFit: Flexible spectral energy distribution modelling with a Bayesian backbone

FortesFit efficiently explores and discriminates between various spectral energy distributions (SED) models of astronomical sources. The Python package adds Bayesian inference to a framework that is designed for the easy incorporation and relative assessment of SED models, various fitting engines, and a powerful treatment of priors, especially those that may arise from non-traditional wave-bands such as the X-ray or radio emission, or from spectroscopic measurements. It has been designed with particular emphasis for its scalability to large datasets and surveys.

Code site:
https://pypi.org/project/fortesfit/ https://github.com/vikalibrate/FortesFit
Used in:
http://ui.adsabs.harvard.edu/abs/2018MNRAS.473.5658R
Bibcode:
2019ascl.soft04011R

Views: 351

ascl:1904.011
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