about
Discovery of a galaxy cluster with a violently starbursting core at z = 2.506GOODS-Herschel: ultra-deep XMM-Newton observations reveal AGN/star-formation connectionThe impact of galaxy interactions on active galactic nucleus activity in zCOSMOSThe XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nucleiUltraluminous X-ray sources out to z ~ 0.3 in the COSMOS fieldThe X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOSOngoing and co-evolving star formation in zCOSMOS galaxies hosting active galactic nucleiThe environments of active galactic nuclei within the zCOSMOS density fieldThe spatial clustering of X-ray selected AGN in the XMM-COSMOS fieldOn R-W1 as a diagnostic to discover obscured active galactic nuclei in wide-area X-ray surveysGalaxy clusters in the Swift/BAT era. II. 10 more clusters detected above 15 keVGalaxy clusters in the Swift/Burst Alert Telescope era: hard X-rays in the intracluster mediumA weak lensing study of X-ray groups in the COSMOS survey: form and evolution of the mass-luminosity relationThe XMM‐Newton Wide‐Field Survey in the COSMOS Field. III. Optical Identification and Multiwavelength Properties of a Large Sample of X‐Ray–Selected SourcesTheXMM‐NewtonWide‐Field Survey in the COSMOS Field: Statistical Properties of Clusters of GalaxiesErratum: Finding rare AGN:XMM–NewtonandChandraobservations of SDSS Stripe 82The Chandra Cosmos Legacy survey: overview and point source catalogThe 31 deg^2^ release of the Stripe 82 X-ray survey: the point source catalogThe Chandra COSMOS legacy survey: optical/IR identificationsThe incidence of obscuration in active galactic nucleiFinding rare AGN: XMM–Newton and Chandra observations of SDSS Stripe 82Finding rare AGN: X-ray number counts of Chandra sources in Stripe 82Detailed shape and evolutionary behavior of the X-ray luminosity function of active galactic nucleiSpectral energy distributions of type 1 active galactic nuclei in the COSMOS survey. I. The XMM-COSMOS sampleThe Chandra COSMOS survey. III. Optical and infrared identification of X-ray point sourcesExtended X-ray emission from non-thermal sources in the COSMOS field: a detailed study of a large radio galaxy atz= 1.168Fe K emission from active galaxies in the COSMOS fieldThe bulk of the black hole growth since z ~ 1 occurs in a secular universe: no Major Merger-AGN connectionPKS 0537-286, carrying the information of the environment of SMBHs in the early UniverseA runaway black hole in COSMOS: gravitational wave or slingshot recoil?The VLA-COSMOS perspective on the infrared-radio relation. I. New constraints on selection biases and the non-evolution of the Infrared/Radio properties of star-forming and active galactic nucleus galaxies at intermediate and high redshiftMassive galaxies in COSMOS: evolution of black hole versus bulge mass but not versus total stellar mass over the last 9 gyr?The Chandra survey of the COSMOS field. II. Source detection and photometryThe Chandra COSMOS survey. I. Overview and point source catalogObservational limits on type 1 active galactic nucleus accretion rate in COSMOSThe XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogueChasing highly obscured QSOs in the COSMOS fieldActive galactic nucleus host galaxy morphologies in COSMOSTheXMM‐NewtonWide‐Field Survey in the COSMOS Field. IV. X‐Ray Spectral Properties of Active Galactic NucleiNon-linearity and environmental dependence of the star-forming galaxies main sequence
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description
researcher, ORCID id # 0000-0002-1697-186X
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wetenschapper
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name
Nico Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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N. Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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Nico Cappelluti
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0000-0002-1697-186X