Optical photometric observations of the Be/X-ray binary

Details Optical photometric observations of the Be/X-ray binary Optical photometric observations of the Be/X-ray binary

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1807....1k&link_type=abstract

The Astronomer's Telegram, #1807

Astronomy and Astrophysics

Astronomy

Optical, Binaries, Neutron Stars, Transients, Stars

Scientific paper

Optical observations of the transient Be/X-ray binary V0332+53 (ATel #1792), was carried out using 1-m Sampurnanand telescope at ARIES, Nainital. We observed the field in UBVRI bands for 4 hours since 19.287 hrs UT on 2008-10-21. To calibrate the photometry, we also observed the SA95 and PG2213 Landolt (1992) standard fields during the same night. The transient source magnitudes during our observations are U=17.49+/-0.02, B=17.17+/-0.01, V=15.41+/-0.01, R = 14.23+/-0.01 and I=13.04+/-0.01.

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