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[vsnet-newvar 1374] New variable star MisV1156
- Date: Mon, 14 Jan 2002 21:37:54 -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 1374] New variable star MisV1156
- 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 (MisV1156).
MisV1156
R.A. 20h38m36s.16
Decl. +48o58'06".9 (2000.0)
Mag. 13.0-13.5C
Type ?
= USNO-A2.0 1350.12683932 20h38m36s.285 +48o58'07".30 Mag(R):15.5 Mag(B):19.9
= MSX5C G086.9220+04.6247 20h38m36s.02 +48o58'05".9 InScanError:1.6" CrossScanError:1.3" Flux(A):0.24520
http://vsnet.aerith.net/misao/data/MisV/MisV1156.gif
MisV1156 19990709.75131 13.47C Mis KAF-1600 Tycho_Catalogue KenIchi_Kadota 0.16-m_f/3.3_hyperboloid_astro-camera_+_MUTOH_CV-16II
MisV1156 19990709.75177 13.36C Mis KAF-1600 Tycho_Catalogue KenIchi_Kadota 0.16-m_f/3.3_hyperboloid_astro-camera_+_MUTOH_CV-16II
MisV1156 19991121.46024 13.47C Mis KAF-1600 Tycho_Catalogue KenIchi_Kadota 0.16-m_f/3.3_hyperboloid_astro-camera_+_MUTOH_CV-16II
MisV1156 19991121.46068 13.45C Mis KAF-1600 Tycho_Catalogue KenIchi_Kadota 0.16-m_f/3.3_hyperboloid_astro-camera_+_MUTOH_CV-16II
MisV1156 20001011.43237 13.00C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
MisV1156 20001011.43422 13.00C Mis KAF-1600L Tycho_Catalogue Nobuo_Ohkura 0.16-m_f/3.8_Wright-Schmidt_reflector_+_SBIG_ST-8(ABG)
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1156.
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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