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M95 with SN 2012w (Leo)
Click on the image for a larger version
| Date/Site: |
March 21st, 2012, AAR-observatory in Presberg |
Exposure/
Filter |
L: 10 x 300 seconds (-20°C) |
| Camera: |
SBIG ST10XME, CFW9 with SBIG LRGB-Filters,
Guiding off-axis with Lodestar |
Optics/
Instrument: |
26cm f5-Newton on AP1200 |
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Focusing with Robofocus and MaximDL,
Calibration and deblooming: MaximDL 5,
processing in Photoshop |
The supernova is the brightest star within the galaxy.
The reflections were caused by the planet Mars just beyond the field of view.
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© Friedhelm Hübner, last revision: 09.12.2024