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> regarding variability of HD 162215 > wasn't based on Arne's previous deeper data (I supposed it could be a > saturated measure) but in a V measure in the GCPD: > V= 9.68, B-V= 1.266. > This is from Connelley M., and Sandage A., Photoelectric observations of RS > Ophiuchi, 1978, PASP 70, 600. Stupid of me that I didn't check against the original source but this kind of errors happen one time in a million..: It turns out that the magnitude is V= 9.28 instead of 9.68. This was a typo from the GCPD compiler so this star can now be safely used as a comparison star! Try to put this in one line and see the scanned page that allow us to see the light... http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?journal=PASP.&year=1958 &volume=..70&letter=.&db_key=AST&page_ind=698&plate_select=NO&data_type=GIF& type=SCREEN_GIF Regards, Sebastian
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