Each pixel's photoelectrons become a voltage at an amplifier, and the ADC turns that voltage into a whole number: a count, also called a gray level or ADU. In an sCMOS camera the conversion runs in parallel. Every column has its own amplifiers and converters, so many pixels are digitized at once, which is a large part of why these sensors are fast. A CCD, by contrast, passes its pixels one after another through a readout amplifier and converter.
Two settings decide what a count means. The bit count N sets how many levels exist, 2N: 4,096 at 12 bits and 65,536 at 16. The gain, in electrons per count, sets how much charge one step represents. Scientific cameras typically offer 12- and 16-bit modes, and many add an 8-bit speed mode. A common rule, from Pawley, sets the gain so that one count equals between half and all of the read noise, a kind of Nyquist sampling in intensity. Steps finer than that describe the noise in more detail without adding information; steps much coarser start to merge values the sensor could tell apart.
The ADC then needs enough levels to span the full well at that gain: roughly one to two levels for every read-noise unit, or one to two times the dynamic rangeLoading... (full well divided by read noiseLoading...). With fewer levels, either the top of the well is cut off or each count spans more than the read noise, and the converter rather than the sensor becomes the limit. Rounding to whole counts adds a small noise of its own, one step divided by √12 (rms); at the half-to-all gain that is at most about 0.29 of the read noise.