  We analyse the integral-field spectroscopy data for the $\approx10,000$
galaxies in final data release of the MaNGA survey. We identify 188 galaxies
for which the emission lines cannot be described by single Gaussian components.
These galaxies can be classified into (1) 38 galaxies with broad $H\alpha$ and
[OIII] $\lambda$5007 lines, (2) 101 galaxies with broad $H\alpha$ lines but no
broad [OIII] $\lambda$5007 lines, and (3) 49 galaxies with double-peaked narrow
emission lines. Most of the broad line galaxies are classified as Active
Galactic Nuclei (AGN) from their line ratios. The catalogue helps us further
understand the AGN-galaxy coevolution through the stellar population of
broad-line region host galaxies and the relation between broad lines'
properties and the host galaxies' dynamical properties. The stellar population
properties (including mass, age and metallicity) of broad-line host galaxies
suggest there is no significant difference between narrow-line Seyfert-2
galaxies and Type-1 AGN with broad $H\alpha$ lines. We use the broad-$H\alpha$
line width and luminosity to estimate masses of black hole in these galaxies,
and test the $M_{BH}-\sigma_{e}$ relation in Type-1 AGN host galaxies.
Furthermore we find three dual AGN candidates supported by radio images from
the VLA FIRST survey. This sample may be useful for further studies on AGN
activities and feedback processes.
