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Aims. We perform clustering measurements of 800 X-ray selected Chandra COSMOSLegacy (CCL) Type 2 AGN with known spectroscopic redshift to probe the halomass dependence on AGN host galaxy properties, such as galaxy stellar massMstar, star formation rate (SFR) and specific black hole accretion rate (BHAR),in the redshift range z = [0 - 3].  Methods. We split the sample of AGN with known spectroscopic redshitsaccording to Mstar, SFR and specific BHAR, while matching the distributions interms of the other parameters, including redshift. We measure the projectedtwo-point correlation function wp(rp) and model it with the 2-halo term toderive the large-scale bias b and the corresponding typical mass of the hostinghalo, for the different subsamples.  Results. We found no significant dependence of the large-scale bias andtypical halo mass on galaxy stellar mass and specific BHAR for CCL Type 2 AGNat mean z~1, while a negative dependence on SFR is observed, with lower SFR AGNresiding in richer environment. Mock catalogs of AGN matched to have the sameX-ray luminosity, stellar mass, specific BHAR and SFR of CCL Type 2 AGN, almostreproduce the observed Mstar, specific BHAR and SFR-Mh relations, when assuminga fraction of satellite AGN of 15%, which corresponds to a ratio between theprobabilities of satellite and central AGN of being active Q = 2. Mock matchednormal galaxies follow a slightly steeper Mstar -Mh relation with low mass mockgalaxies residing in less massive halos than mock AGN of similar mass, and areless biased than mock AGN with similar specific BHAR and SFR, at least for Q >1.

The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties