ChandraCOSMOS Legacy Survey: Clustering dependence of Type 2 active galactic nuclei on host galaxy properties

@article{Allevato2019ChandraCOSMOSLS,
  title={ChandraCOSMOS Legacy Survey: Clustering dependence of Type 2 active galactic nuclei on host galaxy properties},
  author={V. Allevato and A. Viitanen and Alexis Finoguenov and Francesca Maria Civano and Hyewon Suh and Francesco Shankar and Angelo Bongiorno and Andrea Ferrara and Roberto Gilli and Takamitsu Miyaji and Stefano Marchesi and Nico Cappelluti and Mara Salvato},
  journal={Astronomy \& Astrophysics},
  year={2019}
}
Aims.We perform clustering measurements of 800 X-ray selectedChandraCOSMOS Legacy (CCL) Type 2 active galactic nuclei (AGN) with known spectroscopic redshift to probe the halo mass dependence on AGN host galaxy properties, such as galaxy stellar massMstar, star formation rate (SFR), and specific black hole accretion rate (BHAR;λBHAR) in the redshift rangez = [0−3].Methods.We split the sample of AGN with known spectroscopic redshits according toMstar, SFR andλBHAR, while matching the… 

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References

SHOWING 1-10 OF 98 REFERENCES
The XMM-Newton wide field survey in the COSMOS field: Clustering dependence of X-ray selected AGN on host galaxy properties
Aims. We study the spatial clustering of 632 (1130) XMM-COSMOS active galactic nuclei (AGNs) with known spectroscopic or photometric redshifts in the range z = [0.1–2.5] in order to measure the AGN
Accreting supermassive black holes in the COSMOS field and the connection to their host galaxies
Using the wide multiband photometry available in the Cosmic Evolution Survey (COSMOS) field, we explore the host galaxy properties of a large sample of active galactic nuclei (AGNs; ∼1700 objects)
Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching
We investigate the star formation properties of a large sample of ~2300 X-ray-selected Type 2 Active Galactic Nuclei (AGNs) host galaxies out to z ~ 3 in the Chandra COSMOS Legacy Survey in order to
The galaxy-halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS field
We present new constraints on the relationship between galaxies and their host dark matter haloes, measured from the location of the peak of the stellar-to-halo mass ratio (SHMR), up to the most
Multi-wavelength Properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
We investigate the multi-wavelength properties of host galaxies of 3701 X-ray-selected active galactic nuclei (AGNs) out to z~5 in the Chandra-COSMOS Legacy Survey. Thanks to the extensive
The Swift/BAT AGN Spectroscopic Survey. IX: The Clustering Environments of an Unbiased Sample of Local AGNs
We characterize the environments of local accreting supermassive black holes by measuring the clustering of AGN in the Swift/BAT Spectroscopic Survey (BASS). With 548 AGN in the redshift range
AGN host galaxy mass function in COSMOS: is AGN feedback responsible for the mass-quenching of galaxies?
We investigate the role of supermassive black holes in the global context of galaxy evolution by measuring the host galaxy stellar mass function (HGMF) and the specific accretion rate i.e.,
Large-scale clustering measurements with photometric redshifts: comparing the dark matter haloes of X-ray AGN, star-forming and passive galaxies at z ≈ 1
We combine multi-wavelength data in the AEGIS-XD and C-COSMOS surveys to measure the typical dark matter halo mass of X-ray selected active galactic nuclei (AGN) [LX(2-10 keV) > 1042 erg s-1] in
The zCOSMOS Survey. The dependence of clustering on luminosity and stellar mass at z=0.2-1
We study the dependence of galaxy clustering on luminosity and stellar mass at redshifts z ~ [0.2-1] using the first zCOSMOS 10K sample. We measure the redshift-space correlation functions xi(rp,pi)
Measuring the dark matter halo mass of X-ray AGN at z ∼ 1 using photometric redshifts
Data from the AEGIS, COSMOS and ECDFS surveys are combined to infer the bias and dark matter halo mass of moderate luminosity [LX(2-10 keV) = 42.9 erg s-1] X-ray AGN at z~1 via their
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