  Using the SARA 0.9 meter telescope at Kitt Peak National Observatory (KPNO)
we obtained R images during the summer of 2010 and V images during the summer
of 2012 of the globular cluster M14. These images were analyzed using the
DAOPHOT/ALLFRAME package of Stetson (1987,1994) to create a preliminary
color-magnitude diagram (CMD) of M14. We have positively identified the
positions of 64 of the 112 known RR Lyrae stars on the CMD. We find
considerable spread in both the magnitudes and color of the RR Lyrae stars
indicating a significant amount of differential reddening on relatively small
scales. This is also seen in the giant branch which shows up to ~0.15 magnitude
spread in V-R color. We also found the median magnitude of the RR Lyrae stars
and hence the horizontal branch to be V=17.2.
