OVERVIEW

Long-term study of variable stars and asteroids lightcurves using a 25cm Meade Schmidt-Cassegrain optical re ecting telescope driven by an altazimuth Mount and along with a SBIG ST-7E CCD camera. B,V and R standard filters attached to a CFW-9 Filter wheel are used. The telescope is also used for observing very close bright extended objects such as planets, comets, nebulae and galaxies.

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