V340 Ser and V448 Lac light curves (Arkhipova+, 2011)

Details V340 Ser and V448 Lac light curves (Arkhipova+, 2011) V340 Ser and V448 Lac light curves (Arkhipova+, 2011)

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..90370691a&link_type=abstract

VizieR On-line Data Catalog: J/PAZh/37/691. Originally published in: 2011PAZh...37..691A; 2011AstL...37..635A

Astronomy and Astrophysics

Astronomy

Stars: Variable, Stars: Supergiant, Photometry: Ubv

Scientific paper

We performed our UBV observations of two program stars, V340 Ser and V448 Lac, at the Crimean Station of the Sternberg Astronomical Institute using a 60-cm Zeiss reflector with a photoelectric photometer designed by Lyuty (1971, Soobshch. GAISh 172, 30) with a 27 aperture. The accuracy of the observations was from 0.01mag to 0.02mag. The photometric system of the photometer is close to Johnson's standard UBV system.
(2 data files).

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