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[vsnet-newvar 986] New variable star MisV1125

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1125).

MisV1125
  R.A.  21h42m07s.31
  Decl. +46o46'29".4  (2000.0)
  Mag.  11.9-12.5C
  Type  SR?
= USNO-A2.0 1350.14746161  21h42m07s.276 +46o46'29".76  Mag(R):14.9  Mag(B):18.8
= 2MASS 214207.287 +464629.77 (2000.0)  7.782  6.764  6.264

  http://vsnet.aerith.net/misao/data/MisV/MisV1125.gif

MisV1125 19990724.62975 12.46C Mis KAF-1600 - KenIchi_Kadota
MisV1125 19990724.63019 12.45C Mis KAF-1600 - KenIchi_Kadota
MisV1125 20000804.57592 12.00C Mis KAF-1600 - Nobuo_Ohkura
MisV1125 20000804.57777 11.88C Mis KAF-1600 - Nobuo_Ohkura
MisV1125 20000804.57962 11.85C Mis KAF-1600 - Nobuo_Ohkura
MisV1125 20000917.50147 11.98C Mis KAF-1600 - Nobuo_Ohkura
MisV1125 20000917.50333 11.98C Mis KAF-1600 - Nobuo_Ohkura
MisV1125 20000917.50518 11.95C Mis KAF-1600 - Nobuo_Ohkura
MisV1125 20001009.47597 12.13C Mis KAF-1600 - Nobuo_Ohkura
MisV1125 20001009.47782 12.14C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1125.

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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