  Broad H$\alpha$ and H$\beta$ emission lines (FWHM > 1,000 km s$^{-1}$) are
incredibly efficient tracers of the high-velocity clouds encircling Active
Galactic Nuclei (AGN). As a result, we search for these broad line AGN in the
Sloan Digital Sky Survey's Mapping Nearby Galaxies at Apache Point Observatory
(MaNGA) catalog. We identify 301 broad-line H$\alpha$ galaxies and 801
broad-line H$\beta$ galaxies in the catalog. In total, we detect 1,042 unique
broad-line galaxies with luminosities between 10$^{37}$ - 10$^{43}$ erg
s$^{-1}$; 60 feature both broad H$\alpha$ and broad H$\beta$ emission. We also
determine that the broad line region radius ranges between 0.01 - 46 light
days, with a median radius of 0.1 light days (0.02 pc) for our broad H$\beta$
sample. In addition, we find that both samples feature a higher fraction of
galaxy mergers (44% for the broad H$\alpha$ sample and 43% for the broad
H$\beta$ sample), compared to the full MaNGA galaxy sample (26%), which
suggests that merger-driven fueling is strongly active in our sample.
