Testing the recovery of stellar rotation signals from Kepler light curves using a blind hare-and-hounds exercise
Testing the recovery of stellar rotation signals from Kepler light curves using a blind hare-and-hounds exercise
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DOI:
10.1093/mnras/stv853
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发表时间:
2015-04
影响因子:
4.8
通讯作者:
S. Aigrain;J. Llama;Tugdual Ceillier;M. L. D. Chagas;J. Davenport;R. García;K. Hay;Antonino Francesco Lanza;A. McQuillan;T. Mazeh;J. D. Medeiros;M. B. Nielsen;T. Reinhold
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文献类型:
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作者:
S. Aigrain;J. Llama;Tugdual Ceillier;M. L. D. Chagas;J. Davenport;R. García;K. Hay;Antonino Francesco Lanza;A. McQuillan;T. Mazeh;J. D. Medeiros;M. B. Nielsen;T. Reinhold
SA’s contribution to this work was supported by the UK Science and Technology Facilities Council through Consolidated Grant ST/K00106X/1. JL acknowledges support through NASA/GALEX grant program under Cooperative Agreement No. NNX12AC19G issued through the Office of Space Science. MLdC acknowledges a CAPES/PNPD fellowship. JRdM and MLdC acknowledge financial support of the INCT INEspac¸o. TC and RAG want to acknowledge the funding of the CNES grant at the CEA, as well as the ANR (Agence Nationale de la Recherche, France) program IDEE (n ANR-12-BS05-0008) ‘Interaction Des Etoiles et des Exoplanetes’.