Hi Geoff, sorry you ran into trouble. Can you send me the debug log file from the failed attempt to find stars?
Thanks,
Bruce
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The debug log file should contain any sessions you ran “last night” regardless of release number. Just to be clear, I’m talking about the debug log, not the guide log.
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Yes, the log data you uploaded is what I want but I don’t quite understand the problem yet. Here is the list of guide stars that were found, including their HFD values:
19:12:07.094 00.000 5512 Star::Find(15, 59, 230, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.094 00.000 5512 Star::Find returns 1 (0), X=59.43, Y=229.85, Mass=74865, SNR=177.5, Peak=15750 HFD=2.1
19:12:07.094 00.000 5512 Star::Find(15, 219, 111, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.094 00.000 5512 Star::Find returns 1 (0), X=218.94, Y=110.88, Mass=28956, SNR=103.4, Peak=7681 HFD=2.2
19:12:07.094 00.000 5512 Star::Find(15, 335, 207, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.095 00.001 5512 Star::Find returns 1 (0), X=335.03, Y=206.69, Mass=22700, SNR=91.2, Peak=6223 HFD=2.2
19:12:07.095 00.000 5512 Star::Find(15, 259, 159, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.095 00.000 5512 Star::Find returns 1 (0), X=259.33, Y=159.31, Mass=23433, SNR=93.2, Peak=7161 HFD=1.7
19:12:07.095 00.000 5512 Star::Find(15, 315, 268, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.095 00.000 5512 Star::Find returns 1 (0), X=314.67, Y=267.63, Mass=20170, SNR=82.9, Peak=5852 HFD=1.8
19:12:07.095 00.000 5512 Star::Find(15, 126, 142, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.095 00.000 5512 Star::Find returns 1 (0), X=126.08, Y=141.44, Mass=8239, SNR=47.9, Peak=4117 HFD=2.1
19:12:07.095 00.000 5512 Star::Find(15, 110, 69, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.095 00.000 5512 Star::Find returns 1 (0), X=109.97, Y=69.23, Mass=9194, SNR=51.9, Peak=4259 HFD=2.3
19:12:07.095 00.000 5512 Star::Find(15, 151, 67, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.095 00.000 5512 Star::Find returns 1 (0), X=151.43, Y=67.11, Mass=8174, SNR=47.0, Peak=3923 HFD=2.1
19:12:07.096 00.001 5512 Star::Find(15, 243, 204, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.096 00.000 5512 Star::Find returns 1 (0), X=243.20, Y=203.42, Mass=5255, SNR=34.7, Peak=3548 HFD=1.9
19:12:07.096 00.000 5512 Star::Find(15, 329, 120, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.096 00.000 5512 Star::Find returns 1 (0), X=329.11, Y=119.63, Mass=2613, SNR=22.1, Peak=2939 HFD=2.3
19:12:07.096 00.000 5512 Star::Find(15, 261, 27, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.096 00.000 5512 Star::Find returns 1 (0), X=261.19, Y=26.80, Mass=1395, SNR=16.0, Peak=2929 HFD=1.7
19:12:07.096 00.000 5512 Star::Find(15, 308, 152, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.096 00.000 5512 Star::Find returns 1 (0), X=308.13, Y=152.26, Mass=1720, SNR=17.0, Peak=2878 HFD=2.3
19:12:07.096 00.000 5512 Star::Find(15, 348, 219, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.096 00.000 5512 Star::Find returns 1 (0), X=335.03, Y=206.69, Mass=22700, SNR=91.2, Peak=6223 HFD=2.2
19:12:07.096 00.000 5512 Star::Find(15, 36, 262, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.096 00.000 5512 Star::Find returns 1 (0), X=35.67, Y=261.63, Mass=1142, SNR=11.8, Peak=2821 HFD=1.7
19:12:07.096 00.000 5512 Star::Find(15, 63, 192, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.096 00.000 5512 Star::Find returns 1 (0), X=50.68, Y=207.13, Mass=11510, SNR=60.5, Peak=3290 HFD=2.2
19:12:07.097 00.001 5512 Star::Find(15, 81, 62, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.097 00.000 5512 Star::Find returns 1 (0), X=96.54, Y=47.95, Mass=8976, SNR=52.3, Peak=3856 HFD=2.2
19:12:07.097 00.000 5512 Star::Find(15, 307, 30, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.097 00.000 5512 Star::Find returns 1 (0), X=307.45, Y=29.93, Mass=1124, SNR=12.2, Peak=2823 HFD=2.3
19:12:07.097 00.000 5512 AutoFind: finding best star pass 1
19:12:07.097 00.000 5512 Star::Find(15, 59, 230, 0, (0,0,0,0), 1.5, 65000) frame 3
19:12:07.097 00.000 5512 Star::Find returns 1 (0), X=59.43, Y=229.85, Mass=74865, SNR=177.5, Peak=15750 HFD=2.1
So, 12 stars in the list with HFD values in the range of 1.7 to 2.3. But as guiding began, you started getting lost-star events because of HFD values that were much smaller as you say. Of course, you also got quite a number of lost star events running 2.6.10 right after that. It seems like there is a large amount of fluctuation here. Can I ask, do you really need to bin the camera? That’s giving you a very coarse image scale and the guiding results are not what I’d expect from an AP mount. I’m not opposed to making changes here but I’d like to understand the problem a little better.
When you get lost-star events, PHD2 automatically saves the problem guide images in separate folders, all in the same directory as your normal log files. If you look at my response in this thread, you’ll find more info on how these folders are named. If possible, I’d like to see your lost-star images from the time period around 19:14 – 19:15 on 2/24.
https://groups.google.com/g/open-phd-guiding/c/2VWh3-UDnDI/m/9_gSKujdBQAJ
Thanks.
Bruce
From: open-phd...@googlegroups.com [mailto:open-phd...@googlegroups.com] On Behalf Of Geof Lewis
Sent: Thursday, February 24, 2022 2:35 PM
To: open-phd...@googlegroups.com
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Thanks, this is plenty of images. Let me stare at them awhile…
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Hi Geoff. I think it’s just a property of the guide camera, so that is what it is and we need to make a change that will let you do your thing. I need to talk to Andy and see how we want to handle this from a release update point of view. I assume you’re ok running on the prior release at this point but if not I can provide you with an updated binary that will avoid this problem. Just for grins, if you have time sometime down the road, I would be interested to see what happens if you try running the camera un-binned while using the native driver. If you decide to try that, be sure to create a new PHD2 profile so you don’t screw up what you have.
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Usually, you bin a guide camera for one of two reasons:
1. You are trying to improve the sensitivity because guide stars are scarce
2. You want to avoid over-sampling, in order words having a guider image scale that is too small
The first point would apply to you for the C14 and I think your star sizes there are probably larger than 1 pixel. On your refractor, binning results in an image scale of over 5 arc-sec/px which is pretty coarse, and it could be the limiting factor with your mount. So I’m suggesting you try running un-binned only on the refractor and, again, getting your star sizes up to a more normal range. It’s just a test, something we can perhaps learn from.
The recommendation to “always bin” doesn’t make much sense to me but I don’t know why the recommendation was made.
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Hi Geof. Yes, this is familiar ground for us. I didn’t want to take you into the weeds of interlaced sensors and the programming options for dealing with those. We don’t think those kinds of implementation details are important for users to know about. To cut to the chase, let’s go back to your final list of conclusions:
Bruce,
The 2 main takeaways for me were that...
· what I thought was unbinned in PHD2 (the default) is in fact 2x1 binning. Please can you confirm this.
Yes, that is correct. Most users aren’t familiar with asymmetric binning and we consider this an implementation detail that doesn’t belong in the UI.
· Terry states that the camera should work fine in any orientation using it's default 2x1 configuration, so this is how I will run the camera with the 4" TSAPO100Q in future.
Yes, you should ignore this hypothetical problem. In any case, it isn’t practical to think you can align the axes with an accuracy that is equivalent to computing star positions at the level of 0.05 to 0.1 px.
· Bin 2x2 is also a good solution and I will continue to use that when imaging through the C14 as it will more likely find suitable guide stars and will be a better match between guide camera and imaging camera image scales, plus is unlikely to run into the min HFD ,1px problems that I experienced with my 4" TSAPO100Q under v2.6.11.
Yes, you will almost certainly want to bin the camera 2x2 on the C14 for a variety of reasons.
I don’t think any of this “deep dive” changes the recommendations I gave you earlier and as long as you’re willing to try the un-binned approach on your refractor, you should be good to go with 2.6.11. But by all means report back if you run into problems.
Regards,
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No worries, Geof, I wasn’t trying to dissuade you from getting into the details. It’s all good, hope your imaging continues to go well.
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