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ASCL Code Record

[ascl:1905.026] SEDPY: Modules for storing and operating on astronomical source spectral energy distribution

SEDPY performs a variety of tasks for astronomical spectral energy distributions. It can generate synthetic photometry through any filter, provides detailed modeling of extinction curves, and offers basic aperture photometry algorithms. SEDPY can also store and interpolate model SEDs, convolve absolute or apparent fluxes, and calculate rest-frame magnitudes.

Code site:
https://github.com/bd-j/sedpy
Used in:
https://ui.adsabs.harvard.edu/abs/2020MNRAS.492.5167V
Bibcode:
2019ascl.soft05026J
Preferred citation method:

https://doi.org/10.5281/zenodo.4582723


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ascl:1905.026
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