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[vsnet-chat 6112] (fwd) Re: [vsnet-gcvs 314] (fwd) NMO Campaign

Date: Thu, 6 Mar 2003 14:33:06 +0900 (JST)
To: vsnet-campaign-mira@ooruri.kusastro.kyoto-u.ac.jp,vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp,vsnet-gcvs@ooruri.kusastro.kyoto-u.ac.jp,vsnet-lpv@ooruri.kusastro.kyoto-u.ac.jp
From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
Subject: [vsnet-chat 6112] (fwd) Re: [vsnet-gcvs 314] (fwd) NMO Campaign
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(fwd) Re: [vsnet-gcvs 314] (fwd) [vsnet-chat 6107] Re: NMO Campaign

Date: Wed, 5 Mar 2003 16:18:40 +0300 (MSK)
From: "Nikolai N. Samus" <samus@lnfm1.sai.msu.ru>

The GCVS now has reliable positions for more than 90 (probably more than
95) percent variable stars in the constellations of Volumes I and II of
the printed version. Within a year, at maximum two years, this will be the
case for the whole catalog. As for "proper" magnitudes, I would easily
call unfiltered CCD magnitudes unproper. We try to use well-defined
systems wherever possible; to get the whole catalog uniform in the sense
of the magnitude system, a lot of NEW RESEARCH will be needed. Without it,
the "photometrically uniform" GCVS would become a catalog of BRIGHT
variable stars in a certain sense.

Regards
N. Samus

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