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Friday, June 4, 2010

Info Post









HST-palette from the emission of ionized elements, R=Sulfur, G=Hydrogen and B=Oxygen









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.





Less compressed images here: 



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M8, the "Lagoon nebula" in Constellation Sagittarius.


Image field is about 30' x 30', half a degrees.


A new project, from Northern galactic remote telescope in Australia.


The Lagoon nebula, M8, in ionized light from the Three elements, H-alpha, O-III and S-II.





100% crop from the image of M8





The telescope and technical information:









16" RCOS ja Apogee U9000 camera. 


LRGB combo.


H-alpha 4x1200s, Dark and Flat calibrated.


O-III x1200s, Dark calibrated 


O-III x1200s, Dark calibrated


Raw data is shared with Petri Kehusmaa and J-P Metsavainio








Processing workflow:


Image acquisition, MaxiDL v4.xxx


Stacked and calibrated in CCDStack.


Deconvolution with a CCDSharp, 30 iterations


Levels, curves and color combine in PS CS3.



Edit 05.06.2010



Here is a Starless version of M8, I like to do some tricks with the images and the results are experimental in nature. Actual nebula can be seen better here.










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