wdtools: Spectroscopic analysis of white dwarfs
Abstract
wdtools characterizes the atmospheric parameters of white dwarfs using spectroscopic data. The flagship class is the generative fitting pipeline (GFP), which fits ab initio theoretical models to observed spectra in a Bayesian framework using high-speed neural networks to interpolate synthetic spectra.
- Publication:
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Astrophysics Source Code Library
- Pub Date:
- July 2020
- Bibcode:
- 2020ascl.soft07013C
- Keywords:
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- Software