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[vsnet-chat 5219] Re: GK Per 118 S COMP
- Date: Wed, 6 Mar 2002 01:21:03 -0700 (MST)
- To: tkato@kusastro.kyoto-u.ac.jp
- From: Brian Skiff <Brian.Skiff@lowell.edu>
- Subject: [vsnet-chat 5219] Re: GK Per 118 S COMP
- Cc: vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
It looks as though the GSC magnitudes are running ~0.2 mag. brighter
than V for the stars Kato-san showed. Thus Linnolt's estimate of 11.5
(versus 11.32 in the GSC) looks about right.
I'd forgotten about the skeleton sequence I did for this field.
Too bad I missed '118 S', since I worked only from the larger-scale
(f) chart to keep the sequence as close as possible to the variable.
Too far away for Arne to have observed also.
\Brian
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