Yes exactly. One dark frame actually increase noise but removes unwanted signal. A program like deep sky stacker will work with stacks of different frames. I'm certainly no expert but a typical scenario would be you have 20 (or more) light frames of your deep sky object, then during the night you also grab some 20 dark frames with the same duration, then you take (next day perhaps) some flat field images to remove vignetting. And you also put a lens cap on, fastest shutter speed and grab a series of bias frames. 20+ or 256 in your case. These are averaged together and are used to calibrate all of the other types of frames, basically to remove read pattern noise. Then you end up with master dark and flat field images that you can reuse with different light frames. More serious astrophotographers will keep a library of master darks for different sensor temperatures.
So are you averaging dark frames? I don't know theory and math but I guess the result would be the same more or less. For shorter exposures it might be practical. Dark + bias frames might be used only because it is impractical to grab so many long exposure darks.