  Active Galactic Nuclei (AGN) are intensely accreting supermassive black holes
at the centers of massive galaxies. Though these objects occupy little spatial
extent of the galaxy itself, they are thought to have far reaching affects,
impacting the galaxy's star formation, and possibly it's lifespan until it
becomes 'red and dead'. Typical galaxies demonstrate that, over cosmic time,
they tend to separate into a bimodal distribution of 'red and dead' or blue and
star forming. We examine whether active galaxies evolve over cosmic time in a
similar way, and whether this can reveal anything about the complexities of the
relationship between an AGN and the host galaxy. We use the Stripe82X survey to
identify 3940 X-ray AGN spanning z=0-2.5, and we measure the rest-frame UVJ
colors of each galaxy. We classify AGN as star-forming or quiescent based on
their location in a UVJ color diagram. We find that there is not a clear
bimodal distribution between AGN in star forming and quiescent galaxies.
Furthermore, the most luminous X-ray sources tend to lie in the star forming
region, which may indicate a correlation between central engine activity and
increased rates of star formation.
