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[vsnet-newvar 851] New variable star MisV1072

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1072).

MisV1072
  R.A.  19h58m40s.06
  Decl. +49o16'05".5  (2000.0)
  Mag.  11.3-11.9C
  Type  ?
= USNO-A2.0 1350.11395403  19h58m40s.086 +49o16'05".36  Mag(R):12.9  Mag(B):15.6

  http://vsnet.aerith.net/misao/data/MisV/MisV1072.gif

MisV1072 19990430.67886 11.30C Mis KAF-1600 - KenIchi_Kadota
MisV1072 19990430.67930 11.32C Mis KAF-1600 - KenIchi_Kadota
MisV1072 19990724.60209 11.31C Mis KAF-1600 - KenIchi_Kadota
MisV1072 19990724.60253 11.33C Mis KAF-1600 - KenIchi_Kadota
MisV1072 20000918.43219 11.82C Mis KAF-1600 - Nobuo_Ohkura
MisV1072 20000918.43403 11.89C Mis KAF-1600 - Nobuo_Ohkura
MisV1072 20000918.43590 11.91C Mis KAF-1600 - Nobuo_Ohkura
MisV1072 20000919.43146 11.81C Mis KAF-1600 - Nobuo_Ohkura
MisV1072 20000919.43332 11.83C Mis KAF-1600 - Nobuo_Ohkura
MisV1072 20000919.43518 11.87C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1072.

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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