出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：High time resolution (HTRA) observations of phenomena such as occultations, transits and photometric lightcurves can provide direct and indirect information unaccessible to many other techniques. I will outline the scientific drivers for HTRA in these areas, and highlight some representative results in areas of stellar and planetary physics. I will review the observational capabilities available at present, in particular at the European Southern Observatory, and those that could become available in the near future.
