Kepler magnitudes of host stars vs. the radii of associated planet candidates for the KOIs observed by Law et al. (2014) with Robo-AO (gray), Adams et al. (2012) with ARIES and PHARO (teal diamonds), Adams et al. (2013b) with ARIES (purple triangles), and in this paper with ARIES (orange stars). The symbols for the Law et al. (2014) targets indicate the photometric quality of the observations as described in their Table 5. The KOI radii were obtained from the cumulative planet candidate list at the NASA Exoplanet Archive (http://exoplanetarchive.ipac.caltech.edu/cgi-bin/ExoTables/nph-exotbls?dataset=cumulative) and have not been corrected for possible dilution due to the presence of nearby stars.