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

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

2011-11-09

arxiv.org/abs/1111.2101v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

3 pages, 2 figures and 1 table. Proceeding submitted for the 20th Stellar Pulsation Conference (Impact of New Instruments and

Scientific paper

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.

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