It was clear last night, quite warm, although seeing and transparency were poor. More testing and calibration, and some real progress was achieved.
Better PEC
Now that I have focus perfect, and given my suspicion that I may be doing unguided imaging with this short refractor, I decided to re-do my PEC calibration. This time I used the main camera to get cooling and higher resolution. I captured about six worm cycles of data and recalculated the model.
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PEC data gathering
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Computed PEC curve
Gathering data like this can be done before it is completely dark, so it was a good way to spend the hour of dusk while waiting for the sky to become completely dark. In the process, I noted two important things:
- Somehow, my TPoint model is off, even though it was near-perfect the other night. I needed to use a closed-loop slew to get to what should have been easy targets. I imagine I bumped something the other night while I was disconnecting and reconnecting the guide camera multiple times. Next testing evening, I will first try doing a re-synchronization and then, if necessary, a completely new TPoint model.
Also, in the process of doing full-frame images with the large QSI camera, I can clearly see the field curvature. The extreme edges of the field are badly distorted, confirming this as the likely cause of the distorted stars I’m seeing in the guide camera, which is even farther from the center of the field.
So, I think I’m not going to worry about correcting those guide camera stars now, but, rather, see what I can do with unguided imaging. After all, this is a very stable mount, and I’m presently using a very short focal-length imaging scope.
Testing Unguided Imaging Limits
So, I slewed to a nice test image – a spot midway between M81 and M82 – and took test images at 10, 60, 100, 200, 300, 400, 500, and 600 seconds, with PEC on but no guiding. Those images, calibrated, are here:
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10 seconds
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60 seconds
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100 seconds
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200 seconds
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300 seconds
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400 seconds
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500 seconds
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600 seconds
Ignore the badly distorted stars at the upper left edge of the field, and look at the center. While I think I may have a minor collimation issue with the camera, I can see no difference between the stars in the 10-second image and those in the 10-minute image. With this mount and scope, I clearly don’t need Autoguiding for exposures in the 5-10 minute range. So, I’m going to shelf my calibration of the Autoguider until later in the season when I switch back to a longer focal-length imaging scope.
It also occurs to me that I have a field flattener for short scopes in a drawer somewhere. If I come back to serious imaging with this scope later in the season (which I might want to do for a very wide field shot, such as M31) I’ll try that flattener.
Now, since I have a nice image framed anyway, I thought I would do some trial imaging of that M81 – M82 shot. I took 10 five-minute sub-exposures, unguided, and then a series of flat fields using the light panel mounted in the observatory. I already have a calibrated dark frame for use with this camera.
There sure are a lot of satellites in that part of the sky. Lots of satellite trails to be removed. Fortunately, the data rejection procedures in CCDStack make that fairly easy.
Here is the result, calibrated, combined, and cropped. (Still just a test – not a finished product, which would need better noise removal, scaling, etc.)
I would not have imagined I could get results like this unguided. This truly is a wonderful mount.
Static Electricity
A final note. I’ve had several major static electricity shocks over the last couple of days, and I don’t remember this being a big issue in the past. Twice tonight, a piece of equipment actually reset after a static spark.
What’s changed? I think the answer is the new vinyl cover on the dome – I used to have a woven polyethylene cover, but switched to this vinyl one last year. Maybe dragging the vinyl cover off the plastic dome is generating the charge. Running a ground wire to the dome is now on the to-do list.
