Robust period estimation using mutual information for multi-band light curves in the synoptic survey era
Pablo Huijse, Pablo A. Estevez, Francisco Forster, Scott F., Daniel, Andrew J. Connolly, Pavlos Protopapas, Rodrigo Carrasco and, Jose C. Principe

TL;DR
This paper introduces a robust, model-free method based on quadratic mutual information for estimating periods in multi-band light curves, significantly improving accuracy and noise robustness in sparse, multi-band astronomical data.
Contribution
It presents a novel QMI-based period estimation method that outperforms traditional techniques and effectively combines multi-band data without assuming specific light curve models.
Findings
Aggregating multi-band data increases period recovery by up to 50%.
QMI method recovers true periods 10-30% more often than Lomb-Scargle and ANOVA.
The method is robust to noise and varying light curve lengths.
Abstract
The Large Synoptic Survey Telescope (LSST) will produce an unprecedented amount of light curves using six optical bands. Robust and efficient methods that can aggregate data from multidimensional sparsely-sampled time series are needed. In this paper we present a new method for light curve period estimation based on the quadratic mutual information (QMI). The proposed method does not assume a particular model for the light curve nor its underlying probability density and it is robust to non-Gaussian noise and outliers. By combining the QMI from several bands the true period can be estimated even when no single-band QMI yields the period. Period recovery performance as a function of average magnitude and sample size is measured using 30,000 synthetic multi-band light curves of RR Lyrae and Cepheid variables generated by the LSST Operations and Catalog simulators. The results show that…
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