  We report results of VI time series photometry for the bright globular
cluster M5 taken between 2007-2011 using the 0.5-m telescope at Bowling Green
State Univ. and the PROMPT #4 telescope at Cerro Tololo. We used DAOPHOT to
obtain photometry to a limiting magnitude of V~19 mag. A search for variable
stars using the DAOMASTER variability index enabled us to recover the three
known bright variables (two Cepheids and one red, long period variable, or LPV)
and many known RR Lyrae stars, and to discover as many as thirteen new,
low-amplitude LPVs. We present light curves of several stars and analyze
periods and amplitudes where applicable.
