  We present here multi-band photometry for over 2000 Main-belt asteroids. For
each target we report the probabilistic taxonomy using the measured V-R and V-I
colors in combination with a machine-learning generated decision surface in
color-color space. Through this method we classify >85% of our targets as one
the four main Bus-DeMeo complexes: S-, C-, X-, or D-type. Roughly one third of
our targets have a known associated dynamic family with 69 families represented
in our data. Within uncertainty our results show no discernible difference in
taxonomic distribution between family members and non-family members. Nine of
the 69 families represented in our observed sample had 20 or more members
present and therefore we investigate the taxonomy of these families in more
detail and find excellent agreement with literature. Out of these 9
well-sampled families, our data show that the Themis, Koronis, Hygiea,
Massalia, and Eunomia families display a high degree of taxonomic homogeneity
and that the Vesta, Flora, Nysa-Polana, and Eos families show a significant
level of mixture in taxonomies. Using the taxonomic purity and the degree of
dispersion in observed colors for each of the 9 well-sampled collisional
families we also speculate which of these families potentially originated from
a differentiated parent body and/or is a family with a possible undetermined
nested family. Additionally, we obtained sufficient photometric data for 433 of
our targets to extract reliable rotation periods and observe no obvious
correlation between rotation properties and family membership.
