Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-11T05:51:15.687Z Has data issue: false hasContentIssue false

Building a Large Solar Analog Sample Using K2

Published online by Cambridge University Press:  27 November 2018

Derek L. Buzasi*
Affiliation:
Dept. of Chemistry & Physics, Florida Gulf Coast University, 10501 FGCU Blvd. S., Fort Myers, FL 33965USA email: dbuzasi@fgcu.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have begun a project aimed at providing a large consistent set of well- vetted solar analogs in order to address questions of stellar rotation, activity, dynamos, and gyrochronology. We make use of the K2 mission fields to obtain precise photometric time series, supplemented by ground-based photometric and spectroscopic data for promising candidates. From this data we will derive rotation periods, spot coverages, and flare rates for a well- defined and well-calibrated sample of solar analogs.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Aigrain, S., Parviainen, H., & Pope, B. 2016, MNRAS, 459, 2408. (K2SC, K2SCP)Google Scholar
Buzasi, D., Lezcano, A., & Preston, H. 2016, JSWSC, 6, 38.Google Scholar
Buzasi, D., Carboneau, L., Hessler, C., Lezcano, A., & Preston, H. 2016, Proc. IAU, 29, 673. (K2SP)Google Scholar
Luger, R. et al 2016, AJ, 152, 100. (K2EV)Google Scholar
Mathur, S. et al. 2011, ApJ, 741, 119.Google Scholar
Vanderburg, A. & Johnson, J. 2014, PASP, 126, 948. (K2SFF)Google Scholar
Van Cleve, et al. 2016, PASP, 128, 5002. (K2)Google Scholar