CCD drift-scan imaging lunar occultations: A feasible approach for sub-meter class telescopes

A CCD drift-scanning technique for lunar occultation (LO) observations is p resented. While this approach has been addressed before by Sturmann (1994) for the case of large telescopes, the technical validity has never been dis cussed for sub-meter class telescopes. In contrast to Sturmann's scheme, th e proposed technique places the CCD in the image plane of the telescope. Th is does not represent a problem in the case of small telescopes, where the practical angular resolution attainable by LO is not limited by aperture sm oothing. Photon-generated charge is read out at millisecond rates on a colu mn by column basis, as the diffraction pattern of the occulted star is bein g tracked. Two LO events (SAO 79031 and SAO 77911) were observed to demonst rate the feasibility of the method. Data analysis was carried out, yielding unresolved angular diameters for both objects. We show, however, that the technique could be useful for close binary detections with small telescopes . A discussion of the limiting resolution and magnitude imposed by our inst rumentation is carried out, showing that the drift-scanning technique could be extended to 1-2 m telescopes for stellar diameter determination purpose s. Finally, we point out that the technical demands required by this techni que can be easily met by most small professional observatories and advanced amateurs.