These galaxies prove to be a real challenge. I gathered data to make some details visible in these fluffy patches in the empty spaces around Leo. We ‘re looking deep into our universe. Picture taken with the C11 and Nikon D750
We all know the classic Bahtinov mask: it allows to focus a bit more objective compared to visual star focusing.
The Bahtinov will produce Cross-shaped stars, with one clear line that moves along the cross as you focus. When the line is centered in the cross, you should have achieved perfect focus.
So what is the tri-Bahtinov?
It essentially three Bahtinov masks in one, rotated over 120 degrees. It gives you three lines and three crosses to check collimation, along three axis simulteaneously.
In addition to focussing, the tri-Bahtinov so also indicates collimation status along three axis.
This is interesting for e.g. Schmidt-Cassegrain telescopes, where the collimation is done by push-pull screws of the secondary mirror along three axis.
A picture of a star using the tri-Bahtinov and the ASI174 Webcam. Very slight disalignement is visible.
You could basically do the same by turning your classic Bahtinov at 120° angles and check focus each time per individual axis.
Do i use the tri-Bahtinov very often? Not really. I believe it’s a great final check for a fixed SCT on a permanent mount. It will disclose the slightest error in collimation. But for every day use, with an SCT that is moved along and mounted for each session, it might be too cumbersome.
Since September the sun has barely appear in our skies and the same is true for stars. So there were only three clear nights without a Moon, all three of which I was so lucky to image the sky. On December 16th I could do this picture with the well-known Pleiades, in a wide field setup.
I used the EQ8 with the old Nikkor 180mm F2.8 ED unguided. An IDAS 2″ filter in front of the objective was used resulting in an effective F/ratio of 3.8.
20 frames of 300″ were stacked and processed by Jean Lammertyn in PI.