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Ground-Based BVRI Follow-Up Observations of the Cepheid V1154 Cyg in Kepler's Field

The almost un-interrupted observations from Kepler Space Telescope can be used to search for Earth-size and larger planets around other stars, as well as for stellar variability and asteroseismological study. However, the Kepler's observations are carried out with a single broad-band filter, and ground-based follow-up observations are needed to complement Kepler's light curves to fully characterize the properties of the target stars. Here we present ground-based optical (BVRI) followup observations of V1154 Cyg, the only Cepheid in the Kepler field of view, and deriving basic properties of this star.

preprint2011arXivOpen access
C. -C. NgeowR. SzaboL. SzabadosA. HendenM. A. T. Groenewegenthe Kepler Cepheid Working Group
astro-ph.SR
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C. -C. NgeowR. SzaboL. SzabadosA. HendenM. A. T. Groenewegenthe Kepler Cepheid Working Group

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