SN2010gv

Вспышка сверхновой в безымянной галактике была открыта 10 августа 2010г. охотником на сверхновые Koichi Itagaki (Япония). В момент открытия блеск звезды оценивался 16.0m, тип - Ia. Сверхновая наблюдалась на дату открытия в Витебской Обсерватории, блеск звезды оценен 15.8m (CR).


Текст циркуляра об открытии:

POSSIBLE SUPERNOVA IN GALAXY IN DRACO
>     S. Nakano, Sumoto, Japan, reports the discovery by Koichi Itagaki
> (Teppo-cho, Yamagata) of an apparent supernova (mag 16.4) on unfiltered
> CCD frames (limiting magnitude 19.0) taken on Aug. 9.705 UT using a 0.60-m
> f/5.7 reflector (+ Bitran BT-214E camera).  The new object is located at
> R.A. = 17h58m22s.56 +/- 0s.02, Decl. = +50o47'34".0 +/- 0".4 (equinox
> 2000.0), near a small and faint galaxy.  Toru Yusa (Osaki, Japan) reports
> his confirming images (limiting mag 18-19) of the new object taken remotely
> at the RAS Observatory near Mayhill, NM, U.S.A., on Aug. 10.148 and 10.169,
> providing position end figures 22s.56 +/0 0s.01, 34".6 +/- 0".1.  Additional
> unfiltered CCD magnitudes for the variable, including pre-discovery images
> found by Itagaki from his archive:  2008 Aug. 31.50, [19.5 (Itagaki); 2010
> Aug. 3.614, 17.5 (Itagaki); 6.576, 16.9 (Itagaki); 10.148, 16.0 (Yusa,
> 0.30-m f/12 reflector + FLI IMG1024-DM camera); 10.169, 16.0 (Yusa, 0.25-m
> f/3.4 reflector + SBIG ST-10XME camera); 10.446, 16.2 (Itagaki); 10.527,
> 16.3 (Yusa, 0.30-m f/12 Cassegrain reflector + SBIG STL-1001E camera at
> Osaki, Japan).  Itagaki's pre- and discovery images of the new variable are
> posted at website URL http://www.k-itagaki.jp/images/psn-anon-2.jpg.  Also,
> Yusa has posted an image of the variable at the following website URL:
> http://www.palette.furukawa.miyagi.jp/space/images/PSN_100810.jpg.  The
> faint presumed host galaxy is SDSS J175822.33+504733.1.
>     Following posting on the Central Bureau's unconfirmed-objects webpage,
> Vitali Nevski (Vitebsk, Belarus) writes that he obtained CCD images on Aug.
> 10.880 with a 0.3-m reflector that yield magnitude 15.8 and position end
> figures 22s.58, 34".7 (USNO-B1.0 catalogue) for the possible supernova,
> adding that nothing is visible at this position on a Palomar Sky Survey
> image obtained on 1993 Aug. 16 (via the Digitized Sky Survey; limiting red
> mag 21).
>
>
> NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
>      superseded by text appearing later in the printed IAU Circulars.
>
>                         (C) Copyright 2010 CBAT
> 2010 August 11                   (CBET 2404)              Daniel W. E. Green 
 

Снимок галактики из архива DSS, в которой вспыхнула сверхновая:



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