Abstract:Studies indicate strong evidence of a scaling relation in the local Universe between the supermassive black hole mass (M BH ) and the stellar mass of their host galaxies (M ). They even show similar histories across cosmic times of their differential terms: star formation rate (SFR) and black hole accretion rate (BHAR). However, a clear picture of this coevolution is far from being understood. We select an X-ray sample of active galactic nuclei (AGN) up to z = 2.5 in the miniJPAS footprint. Their X-ray to infr… Show more
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