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[vsnet-newvar 609] New variable star MisV1018
- Date: Thu, 12 Oct 2000 20:49:07 -0500
- To: dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.ru, vsnet-newvar@kusastro.kyoto-u.ac.jp
- From: Seiichi Yoshida <comet@aerith.net>
- Subject: [vsnet-newvar 609] New variable star MisV1018
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1018).
MisV1018
R.A. 20h30m29s.92
Decl. +29o53'17".4 (2000.0)
Mag. 12.8C-14.6C
Type SR?
= USNO-A2.0_1125.16190106 20 30 29.921 +29 53 17.40 16.0R 18.9B
= 2MASS 203029.909 +295317.02 (2000.0) 8.753 7.659 7.077
http://vsnet.aerith.net/misao/data/MisV/MisV1018.gif
MisV1018 19990605.74506 144C Mis image="KenIchi Kadota"
MisV1018 19990605.74549 146C Mis image="KenIchi Kadota"
MisV1018 20000706.61556 128C Mis image="Nobuo Ohkura"
MisV1018 20000706.61742 128C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1018.
It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.
The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".
The identification with the 2MASS data is by Taichi Kato and John
Greaves.
Please see the URL below for the MISAO Project and the PIXY system.
http://vsnet.aerith.net/misao/
--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp