  We report the results of a sensitive search for water maser emission in the
Local Group Galaxy NGC 6822 with the Karl G. Jansky Very Large Array. The
observations provide tentative single-epoch detections of four candidates,
associated with two infrared-bright star formation regions (Hubble I/III and
Hubble IV). The candidate maser detections are all offset from the velocity
range where strong emission from HI neutral gas is observed toward NGC 6822,
with the closest offset by 40 kms$^{-1}$. Our observations include the location
of NL1K, a previous tentative water maser detection in NGC 6822. We do not
detect any emission from this location with a sensitivity limit approximately a
factor of 5 better than the original Sardina Radio Telescope observations.
