English

Overfitting and correlations in model fitting with separation ratios

Solar and Stellar Astrophysics 2018-08-24 v1

Abstract

The r01r_{01} and r10r_{10} separation ratios are not independent so combing them into a single series r010r_{010} 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 r02r_{02} ratios are strongly correlated with r10r_{10} and r01r_{01} ratios, they should be combined into a single series r102r_{102} (or r012r_{012}), which are not overfitted, and models and observation compared using the covariance matrix cov102cov_{102} (or cov012cov_{012}) 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

R2 v1 2026-06-23T03:41:23.650Z