oh but we do have those informations, we own these cameras, and we have lots of calibration (bias, dark, flat) frames.
For example, with a 15 pixel medium sample, I have the highest value in a bias field of around 360 ADU (yes, in the bottom left part of the frame), and the lowest around 330. 30 ADU might not seem a lot until you do some narrow band imaging and your nebula is just a few ADUs above the background noise.
matter of fact, I couldn't find any gradients in some friend's cameras with the same chip (QHY/FLI), though a fixed grid pattern does seem to exist.