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[vsnet-newvar 1379] New variable star MisV1161
- Date: Mon, 14 Jan 2002 22:02:57 -0600
- To: dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.ru, vsnet-newvar@kusastro.kyoto-u.ac.jp
- From: Seiichi Yoshida <comet@aerith.net>
- Subject: [vsnet-newvar 1379] New variable star MisV1161
- Delivered-To: vsnet-newvar@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1161).
MisV1161
R.A. 21h08m22s.39
Decl. +50o00'01".8 (2000.0)
Mag. 13.3-14.2C
Type ?
= MSX5C G090.8150+01.5734 21h08m22s.22 +49o59'53".9 InScanError:2.4" CrossScanError:1.8" Flux(A):0.31451
http://vsnet.aerith.net/misao/data/MisV/MisV1161.gif
MisV1161 20001013.44698 13.96C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1161 20001013.44883 14.16C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1161 20001013.45068 13.98C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1161 20011003.46622 13.46C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1161 20011003.46818 13.30C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1161 20011003.47015 13.39C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1161 20011025.40031 13.28C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1161 20011025.40228 13.25C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1161 20011025.40426 13.27C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, MISAO Project, discovered a new variable star
MisV1161.
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, 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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