2023-03-15: APP 2.0.0-beta14 has been released !
IMPROVED FRAME LIST, sorting on column header click and you can move the columns now which will be preserved between restarts.
We are very close now to releasing APP 2.0.0 stable with a complete printable manual...
Astro Pixel Processor Windows 64-bit
Astro Pixel Processor macOS Intel 64-bit
Astro Pixel Processor macOS Apple M Silicon 64-bit
Astro Pixel Processor Linux DEB 64-bit
Astro Pixel Processor Linux RPM 64-bit
Hi,
I usually use all calibration frames (Flats, Dark Flats, Darks, Bias) in pre-processing but I have a good CCD and image at -20C so in theory I shouldn't need to use Darks.
So tonight I tried using all of the above except Darks and ended up with hot pixels still showing after Calibration. I was using Average weighting and tried Windsor/Mad/Sigma rejection to no avail.
Then tried again with Darks and hot pixels are gone.
Any thoughts, do I need Darks to get rid of hot pixels?
BTW, I created a bad pixel map and it turned out looking like a grey image without the Darks - with the Darks the hot pixels show up fine. Is that expected?
Any thoughts?
Apologies, the week has been very busy overhere.
So yes, the purpose of a dark is exactly that, to identify hot pixels. And amp-glow, if that would be the case. You can create a BPM with a proper, long dark and if you have no amp-glow, you can use just a BPM. Having this grey background is normal indeed.
No worries, thanks for your patience. 😉