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[vsnet-alert 7575] Re: SGR 1900+14 / bright optical counterpart
- Date: Wed, 06 Nov 2002 17:56:52 -0700
- To: B Monard <BMonard@mweb.co.za>
- From: Arne Henden <aah@nofs.navy.mil>
- Subject: [vsnet-alert 7575] Re: SGR 1900+14 / bright optical counterpart
- Cc: grb@aavso.org, vsnet-alert@kusastro.kyoto-u.ac.jp, Joe Patterson <jop@astro.columbia.edu>, Dan Green <dgreen@cfa.harvard.edu>, Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>, Berto Monard <LAGMonar@csir.co.za>
- Delivered-To: vsnet-alert@kusastro.kyoto-u.ac.jp
- References: <003001c285cb$917ae1c0$24b91fc4@berto>
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
- User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:0.9.9) Gecko/20020408
Please don't get too anxious about this observation. If you
look at the literature on SGR1900+14 (especially Vrba et al.
2000, ApJ 533, 17 and Vrba et al. 1996, ApJ 468, 225), you
will find that there is a close pair of highly reddened M stars located
at approximately
19:07:15.2 +9:19:21.3 J2000
Since this location matches Berto's coordinates, I am sure that
he is just seeing these two stars blended, especially since he is observing
unfiltered. You must be very careful in reddened regions.
Arne
B Monard wrote:
> Hi,
>
> In response to alerts from several GCN circulars, the starfield of the
> suspected active transient and gamma ray burster SGR 1900+14 was imaged this
> evening at the Bronberg Observatory (South Africa), using the 12" f/4.2 SCT
> with CCD camera ST-7E.
>
> More than 30 images with exposures of 45 sec were taken (in extremely windy
> conditions) and the best images were inspected.
>
> By comparison to images of the Digitized Sky Survey of generation 2 / red
> and blue, a new and bright object was visible at position 19 07 15.18 +09 19
> 22.6, astrometrically traceable to the USNO-A2.0 frame.
>
> The brightness of this new object and its neareness to the published
> coordinates (19 07 14.33 +09 19 21.1 from radio interferometry) make this
> object the probable optical counterpart of the active gamma ray burster.
>
> Photometry of the object showed no obvious fluctuations of the brightness.
> The unfiltered CCD observation:
> SGR 1900+14 20021106.737 15.0CR
>
> Note: on most images the object looked distinctly elongated in the E-W
> direction.
>
> If the weather allows, follow-up observations will be done at the Bronberg
> Observatory tomorrow.
> However, the longer nights in the Northern hemisphere ought to enable
> timeseries of much longer duration on this Northern target.
>
> This notice may be cited and communicated to the GCN network.
>
> Berto Monard / MLF
> Bronberg Observatory / CBA Pretoria
>
>
>
>
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