Hello John,
I think I didn't make myself clear regarding the use of ASTAP to calculate the backfocus. I use it as the plate solver in my capture software (I use the AstroPhotography Tools - APT) with some of Star databases in the ASTAP. Some of the libraries are H18, H17, D50, D05, etc. Hope this helps:
https://sourceforge.net/projects/astap-program/files/star_databasesI'll leave two prints of my software in how I do it:


I have in 1 the ASTAP configured in the first image, as you can check. In the software calculator (point 2 at the right), I have the the manufacture camera and telescope settings, as you can see, mainly the camera's chip size and pixel size. The telescope in this situation is an RC with a native focal lenght of 1624mm and 203mm of aperture.
When I calculate using the software tool combined with ASTAP, it gives me after the camera shot the focal lenght as you can see in the point 3. In this case I need to readjust the optical train in order to have the proper and correct backfocus. The ASTAP solved in the software 1648.76mm, meaning that I need to reduce the focal lenght to the manufacture specifications of 1624mm.
If you where using a SCT C8, is the same thing. But insted of the 1624mm, is would be the 1280mm gaved by the focal reducer/flattner of the Celestron.
In the case of the SCT C8 + Celestron 0.63x reducer/flatnner, you adjust the backfocus until the software gives you the 1280mm or something really really close to that value. In my case I'm around 112.1mm of backfocus from the last element of the reducer/flatnner up to the camera's sensor, insted of the 105mm of backfocus given by Celestron.
I don't know if this helps to understand it.
You also can do it manually. Just upload the fit file from the camera, to the nova astrometry website (
https://nova.astrometry.net/upload) and after the image is been solved, search for the pixel scale in Arc/Sec.
Then you do this math 206.265 x the camera pixel size / by the value of the pixel scale in Arc/Sec. given by the Astrometry website and you'll have the focal lenght. You can check in this image:

In this image particularly will be this way: 206.265 x 3.80um / 0.476 arcsec/pixel = 1646.65mm
The value 206.265 is fixed. The variables are the pixel size and the resolution in the fits file shooted by the camera in Arc/Sec. per pixel. But this is if you don't have any other way of doing it, you can do it manually.
Well If you have more questions, or you need further help, just let me know.
Regards,
Cesar