Overfitting and correlations in model fitting with separation ratios
Solar and Stellar Astrophysics
2018-08-24 v1
Abstract
The and separation ratios are not independent so combing them into a single series is overfitting the data, this can lead to almost singular covariance matrices with very large condition numbers, and hence to spurious results when comparing models and observations. Since the ratios are strongly correlated with and ratios, they should be combined into a single series (or ), which are not overfitted, and models and observation compared using the covariance matrix (or ) of the combined set. I illustrate these points by comparing the revised Legacy Project data with my results on the 10 Kepler stars in common.
Cite
@article{arxiv.1808.07556,
title = {Overfitting and correlations in model fitting with separation ratios},
author = {Ian W Roxburgh},
journal= {arXiv preprint arXiv:1808.07556},
year = {2018}
}
Comments
3 pages, 3 figures