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We analyse the integral-field spectroscopy data for the $\approx10,000$galaxies in final data release of the MaNGA survey. We identify 188 galaxiesfor 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 nobroad [OIII] $\lambda$5007 lines, and (3) 49 galaxies with double-peaked narrowemission lines. Most of the broad line galaxies are classified as ActiveGalactic Nuclei (AGN) from their line ratios. The catalogue helps us furtherunderstand the AGN-galaxy coevolution through the stellar population ofbroad-line region host galaxies and the relation between broad lines'properties and the host galaxies' dynamical properties. The stellar populationproperties (including mass, age and metallicity) of broad-line host galaxiessuggest there is no significant difference between narrow-line Seyfert-2galaxies 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 fromthe VLA FIRST survey. This sample may be useful for further studies on AGNactivities and feedback processes.

monthly notices of the royal astronomical society

A complete catalogue of broad-line AGNs and double-peaked emission lines  from MaNGA integral-field spectroscopy of 10K galaxies: stellar population of  AGNs, supermassive black holes, and dual AGNs