Laszlo L. Kiss Department of Experimental Physics, JATE University, Szeged, Dómtér 9, H-6720
Hungary; current affiliation University of Sydney, School of Physics, A28, NSW
2006
G. Kaszás
Department of Optics, JATE University, Szeged, Hungary
Abstract
Extensive photoelectric photometry was carried out at Szeged
Observatory using the 0.4-m Cassegrain-type telescope with an SSP-5A photometer
during 1994Ð1997. We have observed mainly pulsating stars (Cepheids, δ Scuti-
type variables), although eclipsing binaries have been observed as well. As the
observatory lies in a moderately light-polluted environment, we outline a possible
way that small observatories can pursue scientific projects using UBV and uvby
photometry.