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Tuesday, December 25, 2012

Info Post






Have planned to shoot this detail for years. A pillar like formation at the North East corner of the IC 1805, the Heart Nebula. This is a very dim target, there is 8h of h-alpha emission captured and it's at a limit to be enough to show this object. 






An unnamed object in IC 1805


Ra 02h 39m 43s Dec +61° 54′ 04″ Image is shot at 21.12.2012






Colors are mapped to a HST-palette, R=Sulfur, G=Hydrogen and B=Oxygen






An experimental starless image






This image shows just the nebulosity








Image in visual colors





Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum.






Orientation in IC 1805





Area of interest is marked with a white rectangle. The angular size is about 0,5 degrees. (Same as a Moon)








A two frame mosaic






This target was partly overlapping with my previous imaging project in IC 1805,


  the Melotte 15so I was able to build a two frame mosaic.








Technical details





Processing work flow:


Image acquisition, MaxiDL v5.07.


Stacked and calibrated in CCDStack2.


Levels, curves and color combine in PS CS3.





Optics, Meade LX200 GPS 12" @ f5


Camera, QHY9


Guiding, SXV-AO, an active optics unit, and Lodestar guide camera 8Hz


Image Scale, ~0,8 arc-seconds/pixel


24 x 1200s exposures for the H-alpha, emission of ionized Hydrogen = 8h


Narrowband cahnnels for ionized Oxygen and Sulfur are taken from an older wide field image.







A single 20 min. exposure


Image is just calibrated, linearly stretched and scaled down.





 As can be seen here, this is a very dim target! The pillar like object is barely visible at the image center above.















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