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The Kepler Guest Observer Programme

Published online by Cambridge University Press:  20 April 2012

Thomas Barclay
Thomas Barclay*
Affiliation:
NASA Ames Research Center, MS 244-30, Mountain View, CA 94035, USA Bay Area Environmental Research Institute, Sonoma, CA 95476, USA email: [email protected]
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Abstract

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The Kepler Guest Observer Office is dedicated to the service of the broad science community, with a charter to promote the exploitation of Kepler data and broaden the scientific impact of the Kepler mission. There are four routes by which to gain access to Kepler data: the Guest Observer programme annual call for proposals, the quarterly call for Director's Discretionary Targets, the Kepler Asteroseismic Science Consortium, and by accessing the Kepler public data archive. The Guest Observer Office supports all users of Kepler data no matter which route they took to access data, and to that end have developed software tools which can be used by the community in their data analyses.

Keywords

stars: variables: generaltechniques: photometricmethods: data analysis
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S285: New Horizons in Time-Domain Astronomy , September 2011 , pp. 283 - 285
Copyright
Copyright © International Astronomical Union 2012

References

Antoci, V., et al. , 2011, Nature, 477, 570CrossRefGoogle Scholar
Basri, G., et al. , 2011, AJ, 141, 20CrossRefGoogle Scholar
Beck, P. G., et al. , 2011, Science, 332, 205CrossRefGoogle Scholar
Bedding, T. R., et al. , 2011, Nature, 471, 608CrossRefGoogle Scholar
Borucki, W., et al. , 2009, in: Pont, F., Sasselov, D. & Holman, M. (eds.), Transiting Planets, (IAU S 253) (Cambridge: Cambridge University Press), p. 289Google Scholar
Borucki, W. J., et al. , 2010, Science, 327, 977CrossRefGoogle Scholar
Caldwell, D. A., et al. , 2010, ApJ (Letters), 713, L92CrossRefGoogle Scholar
Carter, J. A., et al. , 2011, Science, 331, 562CrossRefGoogle Scholar
Chaplin, W. J., et al. , 2011, Science, 332, 213CrossRefGoogle Scholar
Derekas, A., et al. , 2011, Science, 332, 216CrossRefGoogle Scholar
Koch, D. G., et al. , 2010, ApJ (Letters), 713, L79CrossRefGoogle Scholar
Meibom, S., et al. , 2011, ApJ (Letters), 733, L9CrossRefGoogle Scholar
Mushotzky, R. F., Edelson, R., Baumgartner, W. H., & Gandhi, P. 2011, arXiv:1111.0672Google Scholar
Slawson, R. W., et al. , 2011, AJ, 142, 160CrossRefGoogle Scholar
Walkowicz, L. M., et al. , 2011, AJ, 141, 50CrossRefGoogle Scholar
Witteborn, F. C., Van Cleve, J. E., Borucki, W., Argabright, V., & Hascall, P. 2011, Proc. SPIE, 8151, 815117Google Scholar