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[vsnet-newvar 608] New variable star MisV1017

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1017).

MisV1017
  R.A.  21h01m37s.78
  Decl. +38o23'20".2  (2000.0)
  Mag.  9.9C-10.9C
  Type  SR:
= GSC3168.2337  21 01 37.83  +38 23 19.4  12.18
= USNO-A2.0_1275.14518550  21 01 37.781  +38 23 20.24  11.2R  14.1B
= IRAS 20597+3811  R.A.=21 01 39.33  Decl.=+38 23 24.8  (92 x 15", p.a.=64)  flux(12)=0.65  flux(25)=<0.33  flux(60)=<0.88  flux(100)=<8.38
= 2MASS 210137.800 +382319.02 (2000.0)  7.099  6.160  5.802

  http://vsnet.aerith.net/misao/data/MisV/MisV1017.gif

MisV1017 19990501.74777 104C Mis image="KenIchi Kadota"
MisV1017 19990501.74822 104C Mis image="KenIchi Kadota"
MisV1017 19990707.70216 108C Mis image="KenIchi Kadota"
MisV1017 19990817.72675 100C Mis image="KenIchi Kadota"
MisV1017 19990818.67789 99C Mis image="KenIchi Kadota"
MisV1017 19990818.67843 100C Mis image="KenIchi Kadota"
MisV1017 20000725.57933 109C Mis image="Nobuo Ohkura"
MisV1017 20000725.58119 109C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1017.

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.

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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