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Long-Term High-Precision Monitoring of Variable Stars

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Gilbert Burki

Observatoire de Genève, CH-1290 Sauverny, Switzerland

Long-term and high-precision photometric and/or spectroscopic monitoring is required for the study of some variable stars: supergiants, slowly pulsating B-stars, stars with activity cycles and/or amplitude modulation, and so on. These observations require stable and dedicated instrumentation.

Link to article on ADS

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