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[ascl:2205.005] maelstrom: Forward modeling of pulsating stars in binaries

maelstrom models binary orbits through the phase modulation technique. This set of custom PyMC3 models and solvers fit each individual datapoint in the time series by forward modeling the time delay onto the light curve. This approach fully captures variations in a light curve caused by an orbital companion.

Code site:
https://github.com/danhey/maelstrom https://doi.org/10.5281/zenodo.3669395
Used in:
https://ui.adsabs.harvard.edu/abs/2021MNRAS.501.4669E
Described in:
https://ui.adsabs.harvard.edu/abs/2020JOSS....5.2125H
Bibcode:
2022ascl.soft05005H

Views: 1400

ascl:2205.005
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