[Aavso-photometry] Photometry with an Optec SSP-3
arne
arne at aavso.org
Tue Sep 4 16:36:55 EDT 2007
Larry Gorski wrote:
> Hello:
>
> While I've observed variable stars for several years most of observational work has been visual and many years ago. Years ago I purchased an Optec SSP-3 (Generation 1) photometer but I haven't used it for years until I recently tbrushed off the cobwebs. One star that I used to monitor photometrically was R Sct so my inclination was to start with R Sct again. My setup at home is simple. Optec SSP-3 (Generation 1) at the back end of C-8 (circa 1980). In order to improve the quality of my efforts, I searched the AAVSO PEP Charts for a R Sct "P" chart . There wasn't any. My question is "Which star, if any, is the star that is typically used as a comparison star and a check star?"
>
> Thanks for your input.
>
R Sct is not on the PEP "program", which is why there is no PEP chart.
This RV Tau variable ranges from V=4.5 at maximum (pretty consistent)
to V=8.5 at minimum (but with minima from 6th to 8.5, not very
consistent). Matt Templeton has looked at its variation; Janet was
a coauthor on an R Sct paper; Al Gilmore and Pam Kilmartin, southern
members/observers at Mt. John worked on R Sct with Karen Pollard for years.
The normal comparison stars for R Sct are
ID SAO# RA (1950) DEC V (B-V) (V-Rc) (V-Ic)
comp 142661 18:47:00 -05:58 5.99 1.60 0.83 1.55
check 142598 18:43:21 -06:18 7.92 1.26 0.65 1.30
(from Pollard et al., 1996, MNRAS 279, 949)
Note that these are 1950 coordinates.
Arne
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