Comparison of échelle spectra to synthetic models has become a computational statistics challenge, with over 10,000 individual spectral lines affecting a typical cool star échelle spectrum. Telluric artifacts, imperfect line lists, inexact continuum placement, and inflexible models frustrate the scientific promise of these information-rich data sets. Here we debut an interpretable machine-learning framework
- Award ID(s):
- 1707419
- Publication Date:
- NSF-PAR ID:
- 10111444
- Journal Name:
- International Conference on Atomic Processes in Plasmas
- Sponsoring Org:
- National Science Foundation
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