Open Cluster Survey
The Open Cluster Survey uses the SITe3 CCD (24 arcmin x 15 arcmin) on the Carnegie Henrietta Swope 1m Telescope at Las Campanas Observatory, Chile, to monitor open clusters for the existence of planetary transits with a time sampling of about 1 image per 7minutes.
Click on the links below to obtain details about the program. Since this page is still under construction, some of the links may not yet be active.
Program Description
Photometric Reduction Techniques
Transit Finding Techniques
Data Archive Access
General Information
NGC 2660 -- Feb 2003
Links to