K35 has now been used in about a dozen nights for photometric calibration, and so we have a pretty good handle on the transformation coefficients. They are:
Tv [B-V] = -0.008 +/- 0.010
Tbv = 0.983 +/- 0.016
Tvr = 1.024 +/- 0.023
Tri = 1.001 +/- 0.022
Tvi = 1.028 +/- 0.018
The mean extinction coefficients are:
Kv = 0.140 +/- 0.015
Kbv = 0.138 +/- 0.016
Kvr = 0.041 +/- 0.009
Kri = 0.035 +/- 0.008
Kvi = 0.076 +/- 0.009
These numbers are fairly typical of the Astrodon interference filters plus an STL-1001E camera.
Note: The Astrodon B filter has a red leak; you should not take data of objects that are redder than (B-I) = 5 without corrections.
Links:
[1] http://www.aavso.org/forums/variable-star-observing/aavsonet