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[vsnet-newvar 989] New variable star MisV1128

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1128).

MisV1128
  R.A.  22h01m01s.34
  Decl. +42o02'12".3  (2000.0)
  Mag.  13.3-14.2C
  Type  ?
= USNO-A2.0 1275.16893048  22h01m01s.358 +42o02'12".36  Mag(R):14.1  Mag(B):14.8

  http://vsnet.aerith.net/misao/data/MisV/MisV1128.gif

MisV1128 19990520.75812 13.53C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990520.75855 13.52C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990817.74546 13.63C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990817.74612 13.55C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990821.71833 13.57C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990821.71878 13.71C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990831.66645 14.19C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990831.66688 14.00C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990912.71663 13.71C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990912.71707 13.30C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990923.52800 13.68C Mis KAF-1600 - KenIchi_Kadota
MisV1128 19990923.52844 13.54C Mis KAF-1600 - KenIchi_Kadota
MisV1128 20000907.53619 13.76C Mis KAF-1600 - Nobuo_Ohkura
MisV1128 20000907.53804 13.90C Mis KAF-1600 - Nobuo_Ohkura
MisV1128 20000926.49781 13.74C Mis KAF-1600 - Nobuo_Ohkura
MisV1128 20000926.49966 13.63C Mis KAF-1600 - Nobuo_Ohkura
MisV1128 20000926.50336 13.74C Mis KAF-1600 - Nobuo_Ohkura
MisV1128 20000926.51292 13.80C Mis KAF-1600 - Nobuo_Ohkura
MisV1128 20001106.41695 13.53C Mis KAF-1600 - Nobuo_Ohkura
MisV1128 20001106.41880 13.70C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1128.

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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