My new little scope..
I did identify one of the big issues with little scope, that being internal reflection inside the tube behind the corrector plate, so it took surgery to fix it, remove corrector and apply flock to inside of tube, replace corrector exactly where it was. the result is nothing short of astounding.
I have attached the flats, and here is an AI snippet of what flats are, if your interested.
In astrophotography,
flats (or flat field frames) are calibration images used to correct uneven illumination and optical path imperfections in your final image. They are essential for removing "dust donuts" (shadows from dust on the sensor or filters) and vignetting (the darkening of image edges).
Key Purposes of Flat Frames
- Correcting Vignetting: Evenly distributes light across the frame to eliminate darker corners caused by the telescope's optical design.
- Removing Dust Artifacts: Subtracts shadows cast by dust particles on the sensor, filters, or lenses.
- Normalizing Sensor Response: Accounts for small variations in sensitivity between individual pixels (Pixel Response Non-Uniformity or PRNU).
My images should improve, when I get to see the sky again.
Before Modification top, after modification bottom.
