New Suns in the Cosmos?
D. B. de Freitas, I. C. Le\~ao, C. E. F. Lopes, F. Paz-Chinchon, B. L., Canto Martins, S. Alves, J. R. De Medeiros, M. Catelan

TL;DR
This study identifies three stars with rotation and photometric behaviors similar to the Sun using light curve analysis, introducing a novel fractality-based method to distinguish Sun-like stars.
Contribution
The paper presents a new approach employing the Hurst exponent to better identify Sun-like stars beyond just rotation period similarity.
Findings
CoRoT ID 105693572 closely matches solar rotation properties.
Hurst exponent effectively discriminates Sun-like behavior.
Stars with similar rotation periods can differ in photometric complexity.
Abstract
The present work reports on the discovery of three stars that we have identified to be rotating Sun-like stars, based on rotational modulation signatures inferred from light curves from the CoRoT mission's Public Archives. In our analysis, we performed an initial selection based on rotation period and position in the Period-- diagram. This revealed that the stars CoRoT IDs 100746852, 102709980, and 105693572 provide potentially good matches to the Sun with similar rotation period. To refine our analysis, we applied a novel procedure, taking into account the fluctuations of the features associated to photometric modulation at different time intervals and the fractality traces that are present in the light curves of the Sun and of these "New Sun" candidates alike. In this sense, we computed the so-called Hurst exponent for the referred stars, for a sample of fourteen CoRoT…
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