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[vsnet-newvar 572] New variable star MisV0998

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0998).

MisV0998
  R.A.  20h03m03s.94
  Decl. +30o51'08".8  (2000.0)
  Mag.  12.5C-13.3C
  Type  SR?
= USNO-A2.0_1200.14288457  20 03 03.824  +30 51 10.09  15.6R  19.4B
= IRAS 20010+3042  R.A.=20 03 05.34  Decl.=+30 51 14.0  (57 x 7", p.a.=74)  flux(12)=0.55  flux(25)=0.27  flux(60)=<4.53  flux(100)=<72.60  0% variable
= 2MASS 200303.832 +305109.44 (2000.0)  7.693  6.397  5.824

  http://vsnet.aerith.net/misao/data/MisV/MisV0998.gif

MisV0998 19990430.69883 133C Mis image="KenIchi Kadota"
MisV0998 19990430.69927 133C Mis image="KenIchi Kadota"
MisV0998 19990707.68539 132C Mis image="KenIchi Kadota"
MisV0998 19990707.68582 132C Mis image="KenIchi Kadota"
MisV0998 19990801.60360 133C Mis image="KenIchi Kadota"
MisV0998 19990801.60403 132C Mis image="KenIchi Kadota"
MisV0998 19990831.63742 130C Mis image="KenIchi Kadota"
MisV0998 19990831.63866 132C Mis image="KenIchi Kadota"
MisV0998 20000708.56302 126C Mis image="Nobuo Ohkura"
MisV0998 20000708.56487 126C Mis image="Nobuo Ohkura"
MisV0998 20000708.56671 125C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0998.

It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.

The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".

The identification with the 2MASS data is by Taichi Kato and John
Greaves.

Please see the URL below for the MISAO Project and the PIXY system.

  http://vsnet.aerith.net/misao/

--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/

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