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[vsnet-campaign-dn 495] UV Gem astrometry and photometry
- Date: Fri, 16 Feb 2001 00:13:49 -0000
- To: <vsnet-campaign-dn@kusastro.kyoto-u.ac.jp>, <vsnet-superoutburst@kusastro.kyoto-u.ac.jp>
- From: "Tonny Vanmunster" <Tonny.Vanmunster@advalvas.be>
- Subject: [vsnet-campaign-dn 495] UV Gem astrometry and photometry
- Cc: "cba-news" <news@cba.phys.columbia.edu>
- Importance: Normal
- In-Reply-To: <200102151340.WAA06216@ceres.kusastro.kyoto-u.ac.jp>
- Reply-To: <Tonny.Vanmunster@advalvas.be>
- Sender: owner-vsnet-campaign-dn@kusastro.kyoto-u.ac.jp
UV Gem astrometry (2001, Feb 15/16) :
RA = 06 38 44.11, Dec = +18 16 11.59 (pretty well in agreement with DWS
1997)
RA Residual = 0.69 arcsec r.m.s., Dec Residual = 0.47 arcsec r.m.s.
Magnitude = 15.96 (unfiltered CCD image)
Using 6 reference stars from USNO-SA2.0 catalog
We also performed a photometry session for several hours, under excellent
conditions. A rough inspection of the resulting light curve doesn't reveal
any obvious periodic modulation to be attributed to superhumps.
Kind regards,
Tonny Vanmunster
CBA Belgium Observatory
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