How this stuff works all depends on the camera drivers and how they choose to scale the data. It makes the most sense to have the saturation value reflect the actual max value that can be returned by the camera driver. Otherwise, you will allow PHD2 to unnecessarily select a saturated star and that can work against you.
Regards,
Bruce
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Yes, as long as you’re pointed at something that ought to saturate the sensor – for example, a first magnitude star using a 2-second exposure, something like that. If you’re going to do it this way, *temporarily* stop using the dark library because that can affect what’s displayed. It’s probably going to be close to 4096 from what you’ve described, there’s no need for great precision.
Bruce
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You can probably ignore the square-top appearance, I would just go with the measured saturation level. You can always back off a bit on that – for example, I use a saturation value of 65000 on my 16-bit camera. Particularly if you’re doing multi-star guiding, you are probably in good shape.
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