Star formation characteristics of galaxies hosting AGN

We present an analysis of the ultra-violet (UV) observations of two Seyfert type active galactic nuclei (AGN), namely NGC$$4051 and NGC$$4151. These observations aimed at studying the star formation in the hosts of these AGN were carried out with the ultra-violet imaging telescope on board AstroSat in far-UV. A total of 193 and 328 star-forming regions (SF) were identified using SExtractor in NGC$$4051 and NGC$$4151, respectively. Using aperture photometry of the identified SF regions, we estimated the star formation rates (SFRs). We found NGC$$4051 to have the lowest SFR with a median value of 3.16 $\times$ 10${}^{-5}$ M${}_{\odot }$ yr${}^{-1}$ while for NGC$$4151, we found a median SFR of 0.012 M${}_{\odot }$ yr${}^{-1}$.