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We present the first spatially resolved analysis of rest-frame optical and UVimaging and spectroscopy for a lensed galaxy at z = 2.39 hosting a Seyfertactive galactic nucleus (AGN). Proximity to a natural guide star has enabledhigh signal-to-noise VLT SINFONI + adaptive optics observations of rest-frameoptical diagnostic emission lines, which exhibit an underlying broad componentwith FWHM ~ 700 km/s in both the Balmer and forbidden lines. Measured lineratios place the outflow robustly in the region of the ionization diagnosticdiagrams associated with AGN. This unique opportunity - combining gravitationallensing, AO guiding, redshift, and AGN activity - allows for a magnified viewof two main tracers of the physical conditions and structure of theinterstellar medium in a star-forming galaxy hosting a weak AGN at cosmic noon.By analyzing the spatial extent and morphology of the Ly-alpha anddust-corrected H-alpha emission, disentangling the effects of star formationand AGN ionization on each tracer, and comparing the AGN induced mass outflowrate to the host star formation rate, we find that the AGN does notsignificantly impact the star formation within its host galaxy.

Spatially Resolved Outflows in a Seyfert Galaxy at z = 2.39