Extracting surface rotation periods of solar-like Kepler targets
T. Ceillier, R.A. Garcia, D. Salabert, and S. Mathur
TL;DR
This paper compares different methods for extracting surface rotation periods of solar-like Kepler targets, providing insights into their effectiveness and consistency.
Contribution
It introduces a comparative analysis of multiple methods to determine surface rotation periods in Kepler solar-like oscillators.
Findings
Different methods yield consistent rotation periods
Some methods outperform others in accuracy
Results improve understanding of stellar rotation dynamics
Abstract
We use various method to extract surface rotation periods of Kepler targets exhibiting solar-like oscillations and compare their results.
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