Pixel
The discrete, photosensitive silicon physical detector element on a digital sensor that captures incoming cosmic photons and converts them into an electrical charge.
Each pixel acts as a micro-well with a finite Full Well Capacity (measured in electrons, e⁻). When photons strike the silicon substrate via the photoelectric effect, they generate electron-hole pairs that are digitized by the Analog-to-Digital Converter (ADC) into discrete ADU values. The physical size of the pixel (e.g., 3.76 µm) directly dictates the optical sampling rate of your telescope setup in arcseconds per pixel ("/px).
Pixel size must be matched to your telescope's focal length and local seeing conditions to prevent undersampling (blocky, pixelated stars) or oversampling (bloated stars with diluted signal). On mono sensors like the ASI2600MM, every pixel records raw, un-bayered narrowband or broadband signal across the entire array, maximizing spatial resolution and quantum efficiency.