scholarly article | Q13442814 |
P818 | arXiv ID | 1201.3920 |
P356 | DOI | 10.1155/2012/853701 |
P50 | author | Nico Cappelluti | Q58373971 |
Alexis Finoguenov | Q58375746 | ||
Viola Allevato | Q58375748 | ||
P2860 | cites work | Host galaxy morphologies of X-ray selected AGN: assessing the significance of different black hole fuelling mechanisms to the accretion density of the Universe atz∼ 1 | Q58908876 |
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AGN Host Galaxies atz ~ 0.4-1.3: Bulge-dominated and Lacking Merger-AGN Connection | Q58909017 | ||
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The real-space clustering of luminous red galaxies aroundz< 0.6 quasars in the Sloan Digital Sky Survey | Q57630798 | ||
The Mass‐to‐Light Function of Virialized Systems and the Relationship between Their Optical and X‐Ray Properties | Q57651834 | ||
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The environments of active galactic nuclei within the zCOSMOS density field | Q58035683 | ||
The spatial clustering of X-ray selected AGN in the XMM-COSMOS field | Q58035695 | ||
The Masses, Ancestors, and Descendants of Extremely Red Objects: Constraints from Spatial Clustering | Q58474560 | ||
Evidence for three accreting black holes in a galaxy at z ~ 1.35: a snapshot of recently formed black hole seeds? | Q58786378 | ||
Heavily obscured active galactic nuclei in high-redshift luminous infrared galaxies | Q58786476 | ||
CANDELS: constraining the AGN-merger connection with host morphologies at z ~ 2 | Q58908662 | ||
The bulk of the black hole growth since z ~ 1 occurs in a secular universe: no Major Merger-AGN connection | Q58908754 | ||
P275 | copyright license | Creative Commons Attribution 3.0 Unported | Q14947546 |
P6216 | copyright status | copyrighted | Q50423863 |
P304 | page(s) | 1-19 | |
P577 | publication date | 2012-01-01 | |
P1433 | published in | Advances in Astronomy | Q15757184 |
P1476 | title | Clustering of X-Ray-Selected AGN | |
P478 | volume | 2012 |
Q105582766 | Host galaxies and large-scale structures of active galactic nuclei |
Q58981836 | The XXL Survey |
Q58910712 | The nature of the unresolved extragalactic cosmic soft X-ray background |
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