Surface rotation of solar-like oscillating stars

TL;DR

This paper investigates methods to determine the surface rotation rates of solar-like oscillating stars observed by Kepler, aiming to improve understanding of stellar rotation.

Contribution

It introduces and compares different techniques for extracting surface rotation rates from Kepler data of solar-like oscillators.

Findings

Multiple methods successfully extract rotation rates

Results enhance stellar rotation understanding

Method comparison highlights best approaches

Abstract

In this work, we use different methods to extract the surface rotation rate of Kepler targets showing solar-like oscillations.