Astrophotographers use a Schwarzschild exponent to characterize reciprocity failure, but before we go there, be forewarned that most people who actually test films in the real world find that the manufacturers' published reciprocity adjustments are just a "shot in the dark" (to use an English idiom) as opposed to a real photograph shot in the dark and checked for speed loss.
Since you have a loss of 3 stops in 100 seconds, the standard calculation gives a Schwarzschild exponent of 0.55, extremely low by any standard. Even the worst of the now common films are about 0.65, with Acros being close to 1.0, which is no reciprocity failure.
To calculate a longer exposure corrected for reciprocity failure using the Schwarzschild exponent, designated as
p, use the following equation:
corrected exposure in seconds = (1+metered exposure)^(1/
p)-1
This is a Covington modified Schwarzschild formula to produce more accurate adjustments at shorter time exposures in the range of a few seconds to 60 seconds or so.
I'd bracket. Try exposures based on
p=0.55, but also use a couple of times in the range of
p=0.65 to 0.80 and compare the negative density to a standard fraction of a second exposure of the same object. Keep good notes. This will get you to the right correction range fairly quickly.
I'd also suggest trying Gainer's method, and testing to find the coefficient
a in his formula:
corrected time = metered time ^ 1.62 *
a + metered time
Instructions for that are here:
http://www.unblinkingeye.com/Articles/LIRF/lirf.html
a=0.6 might be a good place to start with the Gainer formula for APX 100.
You can easily make a spreadsheet table of adjusted times for yourself using the above formulae. If you don't have one, openoffice.org has an excellent free office suite with a spreadsheet that runs on pretty much any computing platform.
Lee