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I think the reason neither Andy nor I have responded is that you didn’t provide the necessary log data. You have posted questions dozens of times on the forum so I’m surprised you didn’t understand that. We’re not going to explain all the entries that appear in the debug log file but if you submit the correct data and identify a specific event that concerns you, we will explain what happened.
Bruce
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Thank you, Bruce, for your reply. Of course, you may have the log data. I did think you might want to request the log data, but I waited to hear what, if anything, you specifically wanted because I thought perhaps it would save you work if I provided background information and pointed to specific entries in the log that could allow you to address those specific issues versus sending you log files and asking, "What went wrong?" In other words, I thought I was being helpful, but it appears not.
Perhaps it is a matter of perspective. In any case, I identified the events of concern in my original post. I look forward to your explanations of what happened.
I have uploaded the Debug and Guide Logs. Here is the link.
https://openphdguiding.org/logs/dl/PHD2_logs_abv4.zip
I don't know if you
also want the PHD Broker Log, or any other logs. Please advise if
you do.
Thank you,
Manning B
Hi Manning. You’re using sub-frames on your camera exposures with a size of 35x35 pixels. The auto-select algorithm uses the full frame to locate the stars, but the sub-frame rectangle is always relative to the primary guide star. There’s no choice about that, the camera will only return a single, rectangular region of interest. So all the secondary stars will be “lost” because they don’t reside in that region. If you want to use multiple stars for guiding, you will have to discontinue use of sub-frames.
Regards,
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Hi Manning. Yes, the documentation should make this point explicit. In the initial implementation of multi-star, I automatically disabled the feature if sub-frames were used. But disabling the option confused a lot of people so I removed that. I hoped that the interaction with sub-frames would be somewhat obvious but I guess it’s not. With sub-frames enabled, the real-time display is showing only a very small rectangle somewhere in the image display window – so any stars that don’t lie within that rectangle are never seen by PHD2.
The debug log file is a developer tool so it may contain all sorts of things that only make sense if you’re familiar with the code. You were looking at a number of internal exception messages that are useful to us but not to the casual reader. That’s why we don’t push users toward looking at the debug log file in most cases. I understand your desire to be independent but you will be significantly constrained in understanding things at the debug log level unless you are familiar with the code. We *always* want to see log files when people have questions. If it turns out that we don’t need the log data, it doesn’t matter, it’s no-harm-no-foul. That’s why we implemented the upload and log storage facility on our web site. In general, I think it’s best if you pose the question – at a user and operational level - along with the log files and let us do the analysis first.
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Here are some short answers so I don’t have to get into the innards of the algorithm
1. Secondary stars are populated only as a result of an Auto-select, and they are subject to the same qualification conditions as the primary star – SNR, min-HFD, etc. Auto-select is a fairly expensive action with some side-effects so it isn’t done automatically unless you have manually changed the multi-star option from false to true while guiding is active.
2. Secondary stars can be dropped for many reasons, including low-SNR. In most cases, their removal occurs only after multiple consecutive failures to meet the qualification conditions.
3. Auto exposure is still useful but you have to use a more sensible minimum exposure time. Even with an AO, sub-second exposure times are more likely to chase seeing than to mitigate it. If you set a lower boundary of 1 second, you will probably see fewer dropped secondary stars. You have to make your own trade-offs between having multiple stars and letting the mount go too long between guide corrections.
4. Loss of the primary star is handled the same as always. The list of guide stars is sorted by SNR and the primary star is nearly always the “best” star.
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