Quasi-periodic Gaussian Processes for stellar activity: from physical to kernel parameters (2022)
Attributed to:
Astrophysics at Oxford 2019-2022
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2207.12164
Publication URI: https://arxiv.org/abs/2207.12164
Type: Other