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This online privacy policy describes the information CAF collects through the services available on our web site, (the “Site”) and how we use that information. It beats silently for eternity.The CAF name and reputation were built on a foundation of trust. Now this is the deepest heart of Orion - and a living heart as well. The balance of the Baader RGB is proprietory. The Baader UHC-L filter was used for 7.5 min. I have already taken pictures of the M42 at 2700mm with 11 and 6 micron, but the Marana is really extraordinary at this focal length when comparing my older results. The seeing was okay, because 3852mm focal length at -6 degrees Dec: is not a state were one could say : I'll take a quick picture now. Special mention should be made of the HDR of the Andor Marana. All usable datasets are within a range of 0.4 FWHM. I will still need to change this.īut still! This camera is a monster. The result is a proof that the mechanical backfocus of my setup is an ever so tiny bit too long (maybe 0.2/0.3 mm). UHC-L subframes are balanced between Blue/Green and Red. Countless subframes needed to be inspected/measured individually for best selection.įWHM weighting of Green and Blue are very similar, w. Fast changing air transparency really was my problem during these nights. This is true "Lucky-imaging"Įach subframe is just signal - no noise at all. RGB and an impeccable camera - what a dream come true. An ideal number of UHC-L frames, balanced w. Such kind of data set rested in my dreams since long.time.
Protoplanets made visible in the heart of Orion (Andor Marana w. More about Andor's cameras at Baader Planetarium> Resourceful amateurs will in future explore the interaction of smaller telescopes and ANDOR cameras even further and achieve previously unattained results. Surely the potential of the ANDOR Marana was used only rudimentarily in this test. It turned out that due to the sensitivity and the clean signal of the ANDOR cameras, excellent images can be obtained in a significantly reduced time.