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[vsnet-newvar 1073] New variable star MisV1144

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1144).

MisV1144
  R.A.  21h31m13s.99
  Decl. +47o27'19".7  (2000.0)
  Mag.  12.2-12.8C
  Type  SR?
= USNO-A2.0 1350.14273105  21h31m13s.988 +47o27'20".04  Mag(R):14.1  Mag(B):17.5
= 2MASS 213113.952 +472720.00 (2000.0)  8.807  7.715  7.288

  http://vsnet.aerith.net/misao/data/MisV/MisV1144.gif

MisV1144 19990709.67394 12.70C Mis KAF-1600 - KenIchi_Kadota
MisV1144 19990709.67438 12.79C Mis KAF-1600 - KenIchi_Kadota
MisV1144 20000804.57035 12.22C Mis KAF-1600 - Nobuo_Ohkura
MisV1144 20000804.57220 12.21C Mis KAF-1600 - Nobuo_Ohkura
MisV1144 20000917.49592 12.28C Mis KAF-1600 - Nobuo_Ohkura
MisV1144 20000917.49776 12.36C Mis KAF-1600 - Nobuo_Ohkura
MisV1144 20001010.46344 12.31C Mis KAF-1600 - Nobuo_Ohkura
MisV1144 20001010.46528 12.36C Mis KAF-1600 - Nobuo_Ohkura
MisV1144 20001010.46713 12.35C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1144.

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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