  For an observer, the Black Hole (BH) shadow is the BH's apparent image in the
sky due to the gravitational lensing of nearby radiation, emitted by an
external source. A recent class of solutions dubbed Kerr BHs with scalar hair
possess smaller shadows than the corresponding Kerr BHs and, under some
conditions, novel exotic shadow shapes can arise. Thus, these hairy BHs could
potentially provide new shadow templates for future experiments such as the
Event Horizon Telescope. In order to obtain the shadows, the backward
ray-tracing algorithm is briefly introduced, followed by numerical examples of
shadows of Kerr BHs with scalar hair contrasting with the Kerr analogues.
Additionally, an analytical solution for the Kerr shadow is derived in closed
form for a ZAMO observer at an arbitrary position.
