  A sidereal rotation counting approach is demonstrated by resolving an
ambiguity in the synodic rotation period of Koronis family member (3032) Evans,
whose rotation lightcurves' features did not easily distinguish between doubly-
and quadruply-periodic. It confirms that Evans's spin rate does not exceed the
rubble-pile spin barrier and thus presents no inconsistency with being a ~14-km
reaccumulated object. The full spin vector solution for Evans is comparable to
those for the known prograde low-obliquity comparably-fast rotators in the
Koronis family, consistent with having been spun up by YORP thermal radiation
torques.
