I frequently use drizzle integration on images downloaded from Telescope Live. Can Mure Denoise be used on Drizzle Integrated images? If so what are the considerations with the Mure Denoise parameters on drizzled data?
Also, I download flats, biases, and flat darks to calculate the Mure Denoise Detector Settings. I also download image bundles imaged over time from Telescope Live. My thinking is that the read noise and gain is fairly stable over time. Therefore frequent downloading recalculating gain and read noise to coincide with the image bundle is not necessary. Is my thinking correct here?
Finally, is Mure Denoise applicable to both CCD and CMOS detectors?
I apologize if you already addressed this in your videos. What I did get from your videos is the value of Mure Denoise.
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