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[vsnet-chat 2508] B-V to V-R
- Date: Thu, 6 Jan 2000 12:11:56 -0700 (MST)
- To: aavso-discussion@physics.mcmaster.ca, vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Brian Skiff <bas@lowell.edu>
- Subject: [vsnet-chat 2508] B-V to V-R
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
A simple regression against colors of Landolt stars yields:
(V-R) = 0.508(B-V) + 0.040
or: R = V - 0.508(B-V) - 0.040
Note that the sign difference on the zero-point is opposite what Arne posted,
which was my arithmetic error, not his. This relation works quite well
for stars bluer than B-V = 1.2. More complex functional forms were derived
by John Caldwell and published in the South African Astronomical OBservatory
Circulars a few years ago. These cover all the UBVRIJHK, uvby, and DDO
colors with extended range in color space.
\Brian
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