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[vsnet-newvar 821] New variable star MisV1065
- Date: Wed, 18 Apr 2001 20:50:52 -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 821] New variable star MisV1065
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1065).
MisV1065
R.A. 21h58m40s.60
Decl. +55o18'03".3 (2000.0)
Mag. 12.8-13.4C
Type SR:
= USNO-A2.0 1425.12605262 21h58m40s.960 +55o18'10".32 Mag(R):16.0 Mag(B):17.2
http://vsnet.aerith.net/misao/data/MisV/MisV1065.gif
MisV1065 19990520.77319 12.90C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990520.77362 12.96C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990709.69525 12.99C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990709.69569 13.05C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990817.76182 13.17C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990817.76227 13.12C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990821.73261 13.20C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990821.73306 13.24C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990831.65364 13.33C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990831.65404 13.28C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990912.74142 13.24C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990912.74202 13.07C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990923.51293 13.32C Mis KAF-1600 - KenIchi_Kadota
MisV1065 19990923.51337 13.38C Mis KAF-1600 - KenIchi_Kadota
MisV1065 20000829.51094 12.81C Mis KAF-1600 - Nobuo_Ohkura
MisV1065 20000829.51279 12.79C Mis KAF-1600 - Nobuo_Ohkura
MisV1065 20000829.51466 12.76C Mis KAF-1600 - Nobuo_Ohkura
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1065.
It was picked up by Seiichi Yoshida from the candidates of new
variable stars detected by the PIXY system 2 from images taken by
Nobuo Ohkura comparing with images taken by KenIchi Kadota, and
confirmed by KenIchi Kadota.
The identification is researched by Taichi Kato (Kyoto University),
John Greaves (the United Kingdom), and Seiichi Yoshida.
The magnitude are measured automatically by the PIXY system 2.
About the MISAO Project and the PIXY system 2:
http://vsnet.aerith.net/misao/
--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/
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vsnet-adm@kusastro.kyoto-u.ac.jp
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