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[vsnet-chat 1039] Re: UV Per Sequences
- Date: Mon, 13 Jul 98 09:12:45 -0700
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: aah@nofs.navy.mil
- Subject: [vsnet-chat 1039] Re: UV Per Sequences
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Patrick Schmeer asked about the AAVSO stars 120 and 126. The sequence
in Henden/Honeycutt does not include these two stars. I don't remember
why, unless it was due to close companions (we tried to use 'clean' stars
wherever possible) or were too bright (I know the 10-11mag comparison
stars in the field were saturated on our frames). I can go back into the
data and calculate the magnitudes of these two stars if it is necessary
(nice thing about CCD photometry!). However, as Brian said, the vsnet
V-band chart is probably adequate in regard to those two stars. I checked a
few of the fainter stars, and they agree with our sequence to +-0.02mag or so.
Arne
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Arne Henden Instruments/software/CCDs
US Naval Observatory Flagstaff Station Cepheids/photometry/IR
P.O. Box 1149 http://ftp.nofs.navy.mil
Flagstaff, AZ 86002-1149 Voice: (520)779-5132
aah@nofs.navy.mil FAX: (520)774-3626
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