To plate solve, the software needs to know the plate scale (arc seconds per pixel) for the lens/sensor combination. "Plate" is the term from the old days of photographic plates.
I believe the ASIAIR is already set up with a database of DSLR that it supports to know the camera sensor's scale (micrometers per pixel), so that part is taken care of for you, and the only remaining unknown to solve for the plate scale is the focal length of the lens.
From their web page, the William Optics Zenithstar 61 APO has a native focal length of 360mm.
You also mentioned a flattener (but not which flattener). If you are using the FLAT61, it does not further change the focal length of the optical train, assuming that you have dialed in the correct back-focus. When you use a reducer or flattener, the back-focus is crucial not just to maintain the optimal field curvature, but it also affects the final focal length of the system.
Assuming that you have a FLAT61 set up properly, the focal length that you should tell ASIAIR to use is 360mm.
If 360mm did not work with the FLAT61, perhaps the flattener back focus is not perfectly dialed in (all is not lost, read further).
If you are using some other reducer, say, if the reducer is a 0.8x, you will need to multiply the native focal length by the reducer ratio (e.g., 0.8*360 = 288mm) to get the actual focal length of the lens.
If you are not sure what the true focal length is, enter 0 (yes, zero) into the focal length field of your main camera. When ASIAIR sees a 0, it will try more combinations to plate solve. It will take a little longer to do so, but when it succeeds, it will also change that zero in the focal length field to the actual focal length. This number is the precise focal length of your set up. You might note it down for future reference.
When unsure of the focal length (by entering zero), you might also adjust the exposure so that there are not too many stars detected. Try for perhaps no more than a hundred. Expose for more than 20, but less than 100. Also, reduce gain of camera and increase exposure to compensate, to get a cleaner plate.
You can read more about plate solving at astrometry.net.
Good luck,
Chen