[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-alert 7110] Re: Nova Oph 2002: astrometry by Kadota-san
- Date: Mon, 28 Jan 2002 09:45:03 +0100
- To: vsnet-alert@kusastro.kyoto-u.ac.jp
- From: Patrick Schmeer <extpasc@rz.uni-sb.de>
- Subject: [vsnet-alert 7110] Re: Nova Oph 2002: astrometry by Kadota-san
- Cc: cbat@cfa.harvard.edu, dgreen@cfa.harvard.edu
- Delivered-To: vsnet-alert@kusastro.kyoto-u.ac.jp
- In-Reply-To: <200201280750.QAA04773@ceres.kusastro.kyoto-u.ac.jp>
- References: <200201280750.QAA04773@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
- User-Agent: Mutt/1.3.25i
On Mon, Jan 28, 2002 at 04:50:18PM +0900, Taichi Kato wrote:
> Nova Oph 2002: astrometry by Kadota-san
>
> 2002 01 27.840 UT (4 frames)
> R.A. = 17h37m34s.36 Decl. = -16o23'18".4 (equinox 2000.0)
> 12 reference stars from GSC-ACT.
> Mean residuals: 0.14" in R.A., 0.15" in Decl.
> 0.18-m f/5.5 reflector.
> K. Kadota, Ageo, Saitama, Japan.
On the DSS image there is very close to this position (slightly north of it)
a mag 20-21 star (SW star in a triangle).
Please note that there is a relatively large difference (4.8" in declination)
between the positions obtained by West (vsnet-alert 7092) and by Kadota.
Regards,
Patrick
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp