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20112016
most citedRotation Periods of 34,030 Kepler Main-Sequence Stars: The Full Autocorrelation Sample

725 citations · 2.7k across the 15 of their papers we have counts for

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Showing 2015Show all

4 papers · 1 filter

astro-ph.SR2015★ 40 cited

Time variation of Kepler transits induced by stellar spots - a way to distinguish between prograde and retrograde motion. II. Application to KOIs

Tomer Holczer, Avi Shporer, Tsevi Mazeh +8

Mazeh, Holczer, and Shporer (2015) have presented an approach that can, in principle, use the derived transit timing variation (TTV) of some transiting planets observed by the $Kep…

astro-ph.SR2015★ 178 cited

Testing the recovery of stellar rotation signals from Kepler light curves using a blind hare-and-hounds exercise

S. Aigrain, J. Llama, T. Ceillier +10

We present the results of a blind exercise to test the recoverability of stellar rotation and differential rotation in Kepler light curves. The simulated light curves lasted 1000 d…

astro-ph.EP2015★ 204 cited

Calibrating Gyrochronology using Kepler Asteroseismic targets

Ruth Angus, Suzanne Aigrain, Daniel Foreman-Mackey +1

Among the available methods for dating stars, gyrochronology is a powerful one because it requires knowledge of only the star's mass and rotation period. Gyrochronology relations h…

astro-ph.EP2015★ 148 cited

Photometric Amplitude Distribution of Stellar Rotation of Kepler KOIs-Indication for Spin-Orbit Alignment of Cool Stars and High Obliquity for Hot Stars

Tsevi Mazeh, Hagai B. Perets, Amy McQuillan +1

The observed amplitude of the rotational photometric modulation of a star with spots should depend on the inclination of its rotational axis relative to our line of sight. Therefor…