Publication data of Vito, Fabio: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20122014201620182020202220240200400600800
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications2012201420162018202020222024010203040500246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion201220142016201820202022202405101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe XMM Deep survey in the CDFS V. Iron K lines from active galactic nuclei in the distant UniverseThe XMM Deep survey in the CDFS V. Iron K lines from active galactic nuclei i…Sensitive Chandra coverage of a representative sample of weak-line quasars: revealing the full range of X-ray propertiesSensitive Chandra coverage of a representative sample of weak-line quasars: …Does black-hole growth depend on the cosmic environment?Evidence for feedback in action from the molecular gas content in the $z sim$ 1.6 outflowing QSO XID2028Evidence for feedback in action from the molecular gas content in the $z sim…Piercing Through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields: I. X-ray Spectral and Long-term Variability AnalysesPiercing Through Highly Obscured and Compton-thick AGNs in the Chandra …An Extreme X-ray Variability Event of a Weak-Line QuasarBlack hole accretion preferentially occurs in gas rich galaxiesCosmic radiation backgrounds from primordial black holesEvident black hole-bulge coevolution in the distant universeDeepest view of AGN X-ray variability with the 7 Ms Chandra Deep Field-South surveyDeepest view of AGN X-ray variability with the 7 Ms Chandra Deep Field-Sout…The high-redshift (z>3) AGN population in the 4 Ms Chandra Deep Field SouthBlack-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than Star Formation RateBlack-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than St…Linking black hole growth with host galaxies: the accretion–stellar mass relation and its cosmic evolutionLinking black hole growth with host galaxies: the accretion–stellar mass relati…The XMM deep survey in the CDF-S II. a 9-20 keV selection of heavily obscured active galaxies at z>1.7The XMM deep survey in the CDF-S II. a 9-20 keV selection of heavily obscure…Mock catalogs for the extragalactic X-ray sky: simulating AGN surveys with Athena and with the AXIS probeMock catalogs for the extragalactic X-ray sky: simulating AGN surveys with At…Tracing the accretion history of supermassive black holes through X-ray variability: results from the ChandraDeep Field-SouthTracing the accretion history of supermassive black holes through X-ray varia…The hard X-ray luminosity function of high-redshift (3 < $z lesssim$ 5) active galactic nucleiThe hard X-ray luminosity function of high-redshift (3 < $z lesssim$ 5) active…Long-Term X-ray Variability of Typical Active Galactic Nuclei in the Distant UniverseLong-Term X-ray Variability of Typical Active Galactic Nuclei in the Distant Uni…A magnetar-powered X-ray transient as the aftermath of a binary neutron-star mergerA magnetar-powered X-ray transient as the aftermath of a binary neutron-sta…20122014201620182020202220240200400600800
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The XMM Deep survey in the CDFS V. Iron K lines from active galactic nuclei in the distant UniverseThe XMM Deep survey in the CDFS V. Iron K lines from active galactic nuclei i…Sensitive Chandra coverage of a representative sample of weak-line quasars: revealing the full range of X-ray propertiesSensitive Chandra coverage of a representative sample of weak-line quasars: …Does black-hole growth depend on the cosmic environment?Evidence for feedback in action from the molecular gas content in the $z sim$ 1.6 outflowing QSO XID2028Evidence for feedback in action from the molecular gas content in the $z sim…Piercing Through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields: I. X-ray Spectral and Long-term Variability AnalysesPiercing Through Highly Obscured and Compton-thick AGNs in the Chandra …An Extreme X-ray Variability Event of a Weak-Line QuasarBlack hole accretion preferentially occurs in gas rich galaxiesCosmic radiation backgrounds from primordial black holesEvident black hole-bulge coevolution in the distant universeDeepest view of AGN X-ray variability with the 7 Ms Chandra Deep Field-South surveyDeepest view of AGN X-ray variability with the 7 Ms Chandra Deep Field-Sout…The high-redshift (z>3) AGN population in the 4 Ms Chandra Deep Field SouthBlack-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than Star Formation RateBlack-Hole Growth is Mainly Linked to Host-Galaxy Stellar Mass rather than St…Linking black hole growth with host galaxies: the accretion–stellar mass relation and its cosmic evolutionLinking black hole growth with host galaxies: the accretion–stellar mass relati…The XMM deep survey in the CDF-S II. a 9-20 keV selection of heavily obscured active galaxies at z>1.7The XMM deep survey in the CDF-S II. a 9-20 keV selection of heavily obscure…Mock catalogs for the extragalactic X-ray sky: simulating AGN surveys with Athena and with the AXIS probeMock catalogs for the extragalactic X-ray sky: simulating AGN surveys with At…Tracing the accretion history of supermassive black holes through X-ray variability: results from the ChandraDeep Field-SouthTracing the accretion history of supermassive black holes through X-ray varia…The hard X-ray luminosity function of high-redshift (3 < $z lesssim$ 5) active galactic nucleiThe hard X-ray luminosity function of high-redshift (3 < $z lesssim$ 5) active…Long-Term X-ray Variability of Typical Active Galactic Nuclei in the Distant UniverseLong-Term X-ray Variability of Typical Active Galactic Nuclei in the Distant Uni…A magnetar-powered X-ray transient as the aftermath of a binary neutron-star mergerA magnetar-powered X-ray transient as the aftermath of a binary neutron-sta…20122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2012201420162018202020222024050100150200