Photoelectric Photometry At Szeged Observatory (Abstract)

Volume 35 number 1 (2007)

L. L. Kiss

Kasz†s Kasz†s

Abstract

(Abstract only) Extensive photoelectric photometry was carried out at Szeged Observatory using the 0.4-m Cassegrain-type telescope with an SSP-5A photometer during 1994–1997. 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.