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[vsnet-chat 6898] Re: ccd
- Date: Wed, 24 Sep 2003 01:23:35 -0700 (MST)
- To: hans-goran.lindberg@telia.com
- From: Brian Skiff <Brian.Skiff@lowell.edu>
- Subject: [vsnet-chat 6898] Re: ccd
- Cc: vsnet-chat@kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-chat-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-chat@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
For the relatively blue stars that comprise the typical eclipsers
(B,A,F,G stars), I would try to adjust the magnitude zero-point to
Cousins R using observations of either local comparison stars with
standard magnitudes, or by observing a few standard fields (Landolt, M67
etc.) where R magnitudes are well-established.
\Brian
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