  Virgo III is a newly discovered ultra-faint dwarf (UFD) candidate, and
finding RR Lyrae associated with this galaxy is important to constrain its
distance. In this work, we present a search of RR Lyrae in the vicinity of
Virgo III based on the time-series $r$-band images taken from the Lulin
One-meter Telescope (LOT). We have identified three RR Lyrae from our LOT data,
including two fundamental mode (ab-type) and a first-overtone (c-type) RR
Lyrae. Assuming these three RR Lyrae are members of Virgo III, we derived the
distance to this UFD as $154\pm25$ kpc, fully consistent with the independent
measurements given in the literature. We have also revisited the relation
between absolute $V$-band magnitude ($M_V$) and the number of RR Lyrae (of all
types, $N_{RRL}$) found in local galaxies, demonstrating that the
$M_V$-$N_{RRL}$ relation is better described with the specific RR Lyrae
frequency.
