  In preparation for observations with the $\textit{James Webb Space
Telescope}$ ($\textit{JWST}$), we have identified new members of the nearby,
young M dwarf sample and compiled an up to date list of these stars. Here we
summarize our efforts to identify young M dwarfs, describe the current sample,
and detail its demographics in the context of direct planet imaging. We also
describe our investigations of the unprecedented sensitivity of the
$\textit{JWST}$ when imaging nearby, young M dwarfs. The $\textit{JWST}$ is the
only near term facility capable of routinely pushing direct imaging
capabilities around M dwarfs to sub-Jovian masses and will provide key insight
into questions regarding low-mass gas-giant properties, frequency, formation,
and architectures.
