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[vsnet-campaign-dn 2908] V73 Dra
Dear Colleagues,
last night I observed this star with the 0.8-m, f/8 reflector of Campo
Catino Astronomical Observatory, with a R Bessel filter. I observed with
Franco Mallia. Unfortunately, the clouds forced us to end observations after
only one hour.
A quick look to the resulting photometry show a probable, broad
late-superhump. I will be sending our data to Kyoto, once it will be
properly reduced.
We provide astrometry for this target:
R.A.:20 23 38.20; Decl.: +64 36 26.8 (J2000.0)
100 reference stars from USNO A2.0; mean residuals = 0.2"
On Oct. 18.770, 2002, the star was at mag. 16.5Rc (we used the R magnitudes
from USNO A2.0 for the reference stars).
Regards,
Gianluca Masi
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