Robust Gaussian Process Regression Based on Iterative Trimming
arXiv:2011.11057 · doi:10.1016/j.ascom.2021.100483
Abstract
The Gaussian process (GP) regression can be severely biased when the data are contaminated by outliers. This paper presents a new robust GP regression algorithm that iteratively trims the most extreme data points. While the new algorithm retains the attractive properties of the standard GP as a nonparametric and flexible regression method, it can greatly improve the model accuracy for contaminated data even in the presence of extreme or abundant outliers. It is also easier to implement compared with previous robust GP variants that rely on approximate inference. Applied to a wide range of experiments with different contamination levels, the proposed method significantly outperforms the standard GP and the popular robust GP variant with the Student-t likelihood in most test cases. In addition, as a practical example in the astrophysical study, we show that this method can precisely determine the main-sequence ridge line in the color-magnitude diagram of star clusters.
arXiv commentmajor revision, 11 pages, 8 figures, 2 tables; accepted by Astronomy and Computing; code available at https://github.com/syrte/robustgp/
References in corpus (5)
- PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
- Fast and scalable Gaussian process modeling with applications to astronomical time series
- The Coyote Universe II: Cosmological Models and Precision Emulation of the Nonlinear Matter Power Spectrum
- The Aemulus Project II: Emulating the Halo Mass Function
- Modelling unresolved binaries of open clusters in color-magnitude diagram. I. method and application of NGC3532
Cited by in corpus (8)
- On long-term fatigue damage estimation for a floating offshore wind turbine using a surrogate model
- MiMO: Mixture Model for Open Clusters in Color-Magnitude Diagrams
- An empirical isochrone archive for nearby open clusters
- Photometric Determination of Unresolved Main-sequence Binaries in the Pleiades: Binary Fraction and Mass Ratio Distribution
- Multiple stellar populations at less evolved stages-II: no evidence of significant helium spread among NGC 1846 dwarfs
- Tidal Tails of Nearby Open Clusters. II. A Review of Simulated Properties and the Reliability of Observational Catalogues
- Multiple stellar populations at less evolved stages-III: a possible helium spread in NGC 2210
- Tidal tails in open clusters: Morphology, binary fraction, dynamics, and rotation