δ Scuti stars with STARE: a project on planetary transits and stellar variability

Bibcode
2002ESASP.485..245A
Alonso, R.; Brown, T. M.; Belmonte, J. A.; Charbonneau, D.; Fox Machado, L.; Pallé, P. L.
Referencia bibliográfica

In: Proceedings of the First Eddington Workshop on Stellar Structure and Habitable Planet Finding, 11 - 15 June 2001, Córdoba, Spain. Editor: B. Battrick, Scientific editors: F. Favata, I. W. Roxburgh & D. Galadi. ESA SP-485, Noordwijk: ESA Publications Division, ISBN 92-9092-781-X, 2002, p. 245 - 248

Fecha de publicación:
1
2002
Número de autores
6
Número de autores del IAC
0
Número de citas
0
Número de citas referidas
0
Descripción
In this contribution, we show the capability of STARE to obtain frequencies and amplitudes from high temporal resolution δ Scuti spectra. Lightcurves of 13 new field δ Scuti stars are analyzed and a total of 21 oscillation modes are found in a single field. Noise level in the spectra falls bellow 3 mmag for stars fainter than magnitude 9. Subsequent analysis of the other observed fields, a new location for STARE, as well as the sharing of data with similar projects will provide higher-quality results and a valuable δ Scuti database, which would be useful for follow-up observations.
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Tránsitos

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