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[ascl:2111.017] pySYD: Measuring global asteroseismic parameters

pySYD detects solar-like oscillations and measures global asteroseismic parameters. The code is a python-based implementation of the IDL-based SYD pipeline by Huber et al. (2009), which was extensively used to measure asteroseismic parameters for Kepler stars, and adapts the well-tested methodology from SYD and also improves these existing analyses. It also provides additional capabilities, including an automated best-fit background model selection, parallel processing, the ability to samples for further analyses, and an accessible and command-line friendly interface. PySYD provides best-fit values and uncertainties for the granulation background, frequency of maximum power, large frequency separation, and mean oscillation amplitudes.

Code site:
https://github.com/ashleychontos/pySYD
Used in:
https://ui.adsabs.harvard.edu/abs/2021arXiv210914058M
Described in:
https://ui.adsabs.harvard.edu/abs/2021arXiv210800582C
Bibcode:
2021ascl.soft11017C

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ascl:2111.017
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