Measuring stellar rotation and activity with PLATO

Sylvain N. Breton; Antonino F. Lanza; Sergio Messina; Rafael A. García; Savita Mathur; Angela R. G. Santos; Lisa Bugnet; Enrico Corsaro; Isabella Pagano

arXiv · 2310.01465

Measuring stellar rotation and activity with PLATO

Sylvain N. Breton·Antonino F. Lanza·Sergio Messina·Rafael A. García·Savita Mathur·Angela R. G. Santos·Lisa Bugnet·Enrico Corsaro·Isabella Pagano

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Abstract

Due to be launched late 2026, the PLATO mission will bring the study of main-sequence solar-type and low-mass stars into a new era. In particular, PLATO will provide the community with a stellar sample with solar-type oscillations and activity-induced brightness modulation of unequalled size. We present here the main features of the analysis module that will be dedicated to measure stellar surface rotation and activity in the PLATO Stellar Analysis System.

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BibTeX RIS

Sylvain N. Breton, Antonino F. Lanza, Sergio Messina, Rafael A. García, Savita Mathur, Angela R. G. Santos, Lisa Bugnet, Enrico Corsaro, Isabella Pagano. 2023-10-02. Measuring stellar rotation and activity with PLATO. https://arxiv.org/abs/2310.01465

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