Speaker
Description
We will present a first study of the host galaxy stellar populations with the SDSS-V. For that objective, we will use optical spectra within a redshift range of 0.1 to 0.9 and retrieve a set of stellar population syntheses to disentangle the non-thermal component arising from the active nucleus from the host galaxy. The analysis tests the feasibility of recovering the stellar masses, star formation quantities, ages, synthetic colours, etc., for the AGN-hosting galaxies in the SDSS-V. Therefore, we explored a possible impact on the host galaxies' star formation efficiencies when a galaxy has or hasn't had a strong non-thermal component along the star formation main sequence. This work will generate data products such as stellar masses, star formation rates, star formation histories, and stellar free AGB emission.
