I'm not sure if there is a "quality" metric for bias and darks. I think you either did them correctly, or you didn't. Both are done with the lens cap on. Bias are taken at fastest exposure your camera supports (e.g. mine is 1/4000 for a Canon 450D). Darks use the exposure duration of your lights (e.g. 10 seconds, 30 seconds, 5 minutes, 10 minutes, etc. whatever they are). Both bias and darks, I'm told, are taken at the same ISO as your lights (ISO400, ISO800, ISO100, again whatever they are).
From there, then it is about quantity. Seems you may want at least 20 of both of those, 50 being better. The bias are easy to collect, the darks can be hard since in addition to all of the above, the darks should match the temperature of your lights. That's where it can get a little subjective: you might be 1 degree off, 3 degrees, 5 degrees. How far you can bend this rule might depend on the quantity and what software you end up using them with (I lack the experience here to really say).
Flats is where you do need some measure of quality, which basically comes down to getting the exposure right. Basically, as I understand it, you want the histogram of the light to be somewhere in the middle (just NOT on the left side). (1) The ISO matches your Lights, (2) the sensor should the same focus and orientation as your lights were taken. Then (3) finally, the sensor is also looking at a "flat" field like a blue sky, or a diffused light, an ipad white screen, etc.
I think to "see" the bias, dark, flat you'll need to stretch that raw image (but don't save it and used it in the stretch form, just use the stretch to preview the content). I don't have an example of a stretched dark... But here are examples of my stretched Flat and Bias, using a Canon 450D DSLR 12mp. Remember this is not the what these images look like normally, this is a screenshot of them while doing Auto STF in PI.