Hi Paul. If we ignore the big excursions – you really can’t be touching stuff when you’re guiding – your overall guiding RMS was about 1.3 arc-sec with similar results for both Dec and RA. I think you’re running with overly large minimum moves, which is probably limiting the guiding performance. This happened because your earlier GA run included a large excursion that was really an outlier. Since you’re just getting started, it would be best to do a fresh calibration each night, then run the GA to sample the seeing conditions. You should watch the guiding graph while this is being done to be sure there aren’t weird large excursions. I think a repeat run will produce lower recommendations for min-moves, probably less than 0.5 px.
We can’t really tell much from a compressed jpg image in terms of star shapes. Since you’re using a DSLR, you probably can’t produce FITs files, but an uncompressed TIFF version of a full-frame image will let us use some analysis tools to measure the star elongation. My expectation is that the stars are round enough but perhaps larger than they need to be.
Cheers,
Bruce
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Hi Paul, see below.
From: open-phd...@googlegroups.com [mailto:open-phd...@googlegroups.com] On Behalf Of Paul Porters
Sent: Saturday, June 22, 2019
12:54 AM
To: Open PHD Guiding
Subject: [open-phd-guiding] Re: Evaluation please
@Bryan: Thanks for the info on the FL subject, I already suspected that it might have to do with focussing, But the Bresser doesn't have a moving mirror, it has fixed mirrors and a 2.5" focuser: https://www.bresser.de/en/Astronomy/Telescopes/BRESSER-Messier-MC-152-Hexafoc-Optical-Tube-Assembly.html.
Does it also apply for this particular setup, I mean, the distance to the sensor is variable after all?
As I recall, you have a giant star-diagonal in the main imaging train, not something I’ve ever seen before. That increases the back-focus by a huge amount and thus changes the observed optical properties of the scope. I really think you need to get that out of there.
I shot the image last night on a clear night (90% Moon) with a Nikon D3200 at ISO3200 / 360s. Normally I snap RAW, but forgot to turn the camera back on that format ;-)
@ Bruce:
You're absolutely right, I did 2 GA runs yesterday, and the first one had much smaller values.
The culprit on the second one wasn't me by the way. My little dog Suzie decided it was time to come and join me, and her line snagged on the tripod ;-p (she's forgiven).
These GA runs are intended to be fairly precise. When something goes wrong during the data collection phase, you should just stop the run and certainly not apply any of the recommendations. Otherwise it’s likely to be garbage-in-garbage-out.
Bruce
I will take some RAW images next time I'm outside with the scope.
Thanks!
Paul
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Ok, I see. Even so, that looks like a considerable distance from the scope backplane to the camera sensor. The optical design may be like SCTs wherein the effective focal length/ focal ratio depends on the distance from the secondary to the focus position. With mass-produced SCTs, the quoted focal length is usually based on a nominal focus position, some value chosen by the factory. Of course, most of these SCTs have movable primary mirrors but yours may not. Bottom line, you can believe the plate solve results over the advertising. J
Bruce
From:
open-phd...@googlegroups.com [mailto:open-phd...@googlegroups.com] On Behalf Of Paul Porters
Sent: Saturday, June 22, 2019 8:32
AM
To: Open PHD Guiding
Subject: [open-phd-guiding] Re:
Evaluation please
Yeah, you're absolutely right there, garbage in = garbage out, that's a truth on almost every subject. Indeed, I should have discarded that one. All part of the learning curve I guess.
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