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POSSIBLE SUPERNOVA IN NGC 5430 – XM10AD

POSSIBLE SUPERNOVA IN NGC 5430

Guoyou Sun(Wenzhou, Zhejiang, China) and Xing Gao (Urumqi, Xinjiang, China),report the discovery of a possible supernova (mag approximately 17.2) on several 60-s survey images (limiting mag about 19.5)taken by Xing Gao in Xingming Observation Sky Survey(C42) around Oct. 3.60524 UT using a unfilled CCD Camera ( + Celestron C14 Schmidt-Cassegrain telescope D=350-mm @f/6.9 ). the new object approximately located at R.A. =14h 00m 47s.14 Dec:=+59°20’16”.8 (equinox 2000.0). Nothing was visible at this position on DSS on Apr 8,1997(limiting mag about 19.5).

All images can be seen from: http://www.xjltp.com/XOSS/XM10AD/XM10AD.htm

C42 Xingming Observatory, Mt. Nanshan. Observers G.Sun,X.Gao ,Measurers G.Sun. 0.35-m f/6.9 Schmidt-Cassegrain telescope and CCD.

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continued observation of “POSSIBLE SUPERNOVA IN NGC 5430″

we extend the observation of this object ,followed the reduction below
NET USNO-A2.0
XM10AD C2010 10 03.60524 14 00 47.14 +59 20 16.8 17.2 V C42
XM10AD C2010 10 04.57821 14 00 47.10 +59 20 17.2 17.2 V C42
XM10AD C2010 10 05.58779 14 00 47.12 +59 20 16.8 16.9 V C42
XM10AD C2010 10 06.58351 14 00 47.14 +59 20 16.9 16.7 V C42

bolow is the prime report

Guoyou Sun(Wenzhou, Zhejiang, China) and Xing Gao (Urumqi, Xinjiang, China),
report the discovery of a possible supernova (mag approximately 17.2) on several
60-s survey images (limiting mag about 19.5)taken by Xing Gao in Xingming
Observation Sky Survey(C42) around Oct. 3.60524 UT using a unfilled CCD( +
Celestron C14 Schmidt-Cassegrain telescope D=350-mm @f/6.9 ). the new object
approximately located at R.A. =14h 00m 47s.14 Decl.=+59°20’16”.8 (equinox
2000.0).Located 13″.7 east and 33″.5 north of the nucleus of NGC 5430. Nothing
was visible at this position on DSS on Apr 8,1997(limiting mag about 19.5).

All images can be seen from: http://www.xjltp.com/XOSS/XM10AD/XM10AD.htm

C42 Xingming Observatory, Mt. Nanshan. Observers G.Sun,X.Gao ,Measurers G.Sun.
0.35-m f/6.9 Schmidt-Cassegrain telescope and CCD.

 

 

SDSS

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