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[vsnet-newvar 1027] New variable star MisV1141

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1141).

MisV1141
  R.A.  00h01m21s.55
  Decl. +51o12'13".9  (2000.0)
  Mag.  13.0-14.2C
  Type  SR?
= USNO-A2.0 1350.00025578  00h01m21s.491 +51o12'13".98  Mag(R):14.0  Mag(B):16.5
= IRAS 23587+5055  00h01m20s.3 +51o11'58"  Ellipse:17x8"  P.A.:43  Flux(12):0.7632  Flux(25):0.4001  Flux(60):<0.4000  Flux(100):<1.595  Var:18%
= 2MASS 000121.468 +511213.76 (2000.0)  8.530  7.618  6.910

  http://vsnet.aerith.net/misao/data/MisV/MisV1141.gif

MisV1141 19990821.76440 13.18C Mis KAF-1600 - KenIchi_Kadota
MisV1141 19990821.76485 13.15C Mis KAF-1600 - KenIchi_Kadota
MisV1141 19990821.77180 13.02C Mis KAF-1600 - KenIchi_Kadota
MisV1141 19990821.77225 13.06C Mis KAF-1600 - KenIchi_Kadota
MisV1141 19991105.64057 14.20C Mis KAF-1600 - KenIchi_Kadota
MisV1141 19991105.64101 14.20C Mis KAF-1600 - KenIchi_Kadota
MisV1141 20000807.60357 13.83C Mis KAF-1600 - Nobuo_Ohkura

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1141.

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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