ill be another bone in the 455
I found the bat mask got me close but not 100% and that the FWHM method was always dead on without any hint of error. you knew when you went past the sweet spot quickly. I am a very scientific kind of person, if i cannot repeat the value then i don't really like it.
For the bat mask you need programs to show you where the exact middle is of the central spike, and you can be off just by a little bit and be way out. Using nice reflectors that have f ratios up around the late 5s and on the bat mask works a charm. but when you start looking at sub F5 ratios your CFZ (critical focus zone) is under 50 micron... as you can see one small step off the line shoots everything. So this is my work flow.
Open up nebulosity (I find it has the best image reproduction of the progs i use)
take a 1 second preview, find the dimmest star. Fine focus
it will keep taking 1 sec photos for as long as you want it to
giving you a read out of Max intensity, and best FWHM to see when have
A. hit that sweet spot and
B. keeping a record so you know when you have gone past it and then back to it

Take a 10 second picture inspect it at 200% zoom and if you have a bright enough star, and your focus and collimation are good the diffraction spikes will have a rainbow effect. the sharper and brighter this is the better you are! (that's for the newt owners though

)
that generally takes me about 3 minutes from start to finish. and a wee bit longer if i want to fiddle a bit more.