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[vsnet-chat 5409] Re: CGCS 2792
- Date: Sat, 20 Jul 2002 07:25:40 EDT
- To: vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
- From: DWest61506@aol.com
- Subject: [vsnet-chat 5409] Re: CGCS 2792
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
In a message dated 7/20/2002 2:00:41 AM Central Standard Time, Brian.Skiff@lowell.edu writes:
< Also, given that the V system is not defined redder than B-V > 2.0 or so,
remember that it will be impossible to do other than differential
photometry on the star, and only with a single, fixed instrument. The
systematic errors from device to device will have to be adjusted out
after the fact.>
Brian:
Please explain your comments more fully - I am confused. I know the original Johnson paper doesn't cover B-V >2, but Landolt has a few stars with B-V >2. Why could you only measure the star with a single fixed instrument?
Thanks,
Doug West
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