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[vsnet-chat 1039] Re: UV Per Sequences



  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
--------------------------------------------------------------------
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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