Photoelectric Photometry At Szeged Observatory

Details Photoelectric Photometry At Szeged Observatory Photoelectric Photometry At Szeged Observatory

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006javso..35..226k&link_type=abstract

The Journal of the American Association of Variable Star Observers, Vol. 35, No. 1, p. 226

Physics

1

Scientific paper

Extensive photoelectric photometry was carried out at Szeged Observatory using the 0.4-m Cassegrain-type telescope with an SSP-5A photometer between 1994-1997. We have observed mainly pulsating stars (Cepheids, ? 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.

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