The miniJPAS Survey: The Radial Distribution of Star Formation Rate in Faint X-ray AGN

<p>Figures show the AGN host galaxies accompanied by their observed J-spectra within their Kron radii and the fitted spectrum with \texttt{CIGALE} to determine their physical properties. We note that \texttt{CIGALE} does not fit AGN emission for 1 source with miniJPAS object ID 2241-18160. This object fell in the composite area in the BPT diagram, and in the LINER area in the WHAN diagram. This could represent a case where the AGN is obscured due to dust and \texttt{CIGALE} fails to fit optical AGN emission for this case. This further emphasizes the importance of X-ray emission to identify AGN systems that are optically obscured and are seen as normal galaxies without X-ray detections. We report that the inclusion or emission of this object from our AGN sample does not produce any differences in the results obtained in this paper.</p>