Euclid will measure the position and redshift of about millions of AGN in different environments, enabling us to compute accurately the 2-point correlation function. With almost one year to the first Euclid data, we need to forecast clustering properties of AGN in the Euclid Wide and Deep Surveys and probe our ability to retrieve the clustering signals a function of scale, AGN type and host galaxy properties. To this goal, we will use the official Euclid Flagship mock catalog of galaxies populated with AGN and any additional AGN mock catalog available within the Euclid Consortium to perform clustering measurements by using the official Euclid galaxy clustering code. This will allow us to evaluate the typical uncertainty in the correlation function and in the halo model parameters for the upcoming Euclid AGN sample.
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