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Accurate and Robust Stellar Rotation Periods Catalog for 82771 Kepler Stars Using Deep Learning

  • Authors: Ilay Kamai, Hagai B. Perets

Ilay Kamai and Hagai B. Perets 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 4.

Results of our model (upper left) vs. implementations of ACF (upper right) and GPS (lower) on our test data set. In the left panel, the color represents the model's confidence levels. The sharp drop of samples, seen at 10 days, is a result of the prior distribution of periods (see Table 1). This distribution was also implemented in S. Aigrain et al. (2015) and motivated by the bimodality found by A. McQuillan et al. (2013; 2014).

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