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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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