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[vsnet-newvar 985] New variable star MisV1124

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1124).

MisV1124
  R.A.  21h41m43s.62
  Decl. +47o01'47".2  (2000.0)
  Mag.  13.0-13.7C
  Type  SR?
= USNO-A2.0 1350.14730561  21h41m43s.649 +47o01'48".26  Mag(R):14.3  Mag(B):17.5
= 2MASS 214143.592 +470147.36 (2000.0)  9.485  8.264  7.818

  http://vsnet.aerith.net/misao/data/MisV/MisV1124.gif

MisV1124 19990724.62975 13.29C Mis KAF-1600 - KenIchi_Kadota
MisV1124 19990724.63019 13.21C Mis KAF-1600 - KenIchi_Kadota
MisV1124 20000804.57592 13.13C Mis KAF-1600 - Nobuo_Ohkura
MisV1124 20000804.57777 13.05C Mis KAF-1600 - Nobuo_Ohkura
MisV1124 20000804.57962 13.00C Mis KAF-1600 - Nobuo_Ohkura
MisV1124 20000917.50147 13.49C Mis KAF-1600 - Nobuo_Ohkura
MisV1124 20000917.50333 13.55C Mis KAF-1600 - Nobuo_Ohkura
MisV1124 20000917.50518 13.51C Mis KAF-1600 - Nobuo_Ohkura
MisV1124 20001009.47597 13.66C Mis KAF-1600 - Nobuo_Ohkura
MisV1124 20001009.47782 13.65C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1124.

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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