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Statistics of Stellar Variability in Kepler Data with ARC Systematics Removal

Published online by Cambridge University Press:  20 April 2012

Amy McQuillan
Affiliation:
Department of Physics, University of Oxford, Oxford, OX1 3RH, UK email: [email protected], [email protected]
Suzanne Aigrain
Affiliation:
Department of Physics, University of Oxford, Oxford, OX1 3RH, UK email: [email protected], [email protected]
Stephen Roberts
Affiliation:
Department of Engineering Science, University of Oxford, Oxford, OX1 3PJ, UK email: [email protected]
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Abstract

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We investigate the variability properties of main-sequence stars in the first month of Kepler data, using a new astrophysically robust systematics correction. We find that 36% appear more variable than the Sun, and confirm the trend of increasing variability with decreasing effective temperature. We define low- and high-variability samples, with a cut at twice the level of the active Sun, and compare properties of the stars belonging to each sample. We find tentative evidence that the more active stars have lower proper motions. The frequency content of the variability shows clear evidence for periodic or quasi-periodic behaviour in 16% of stars, and highlights significant differences in the nature of variability between spectral types. Most A and F stars have short periods (< 2 days) and highly sinusoidal variability, suggestive of pulsations, whilst G, K and M stars tend to have longer periods (> 5 days, with a trend towards longer periods at later spectral types) and show a mixture of periodic and stochastic variability, indicative of activity. Finally, we use autoregressive models to characterise the stochastic component of the variability, and show that its typical amplitude and time-scale increase towards later spectral types, which we interpret as an increase in the characteristic size and life-time of active regions. Full details will be published shortly.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

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McQuillan, A., Aigrain, S., & Roberts, S. 2011, submitted to A&AGoogle Scholar