Publication data of Shemmer, Ohad: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20002005201020152020202501000200030004000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications20002005201020152020202502040608010001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion200020052010201520202025010203040
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestBlack-Hole Mass and Growth Rate at z~4.8: A Short Episode of Fast Growth Followed by Short Duty Cycle ActivityBlack-Hole Mass and Growth Rate at z~4.8: A Short Episode of Fast Growth F…Complex optical-x-ray correlations in the narrow-line seyfert 1 galaxy ngc 4051Complex optical-x-ray correlations in the narrow-line seyfert 1 galaxy ngc 40…The X-ray spectral properties and variability of luminous high-redshift active galactic nucleiThe X-ray spectral properties and variability of luminous high-redshift active …A Population of X-ray Weak Quasars: PHL 1811 Analogs at High RedshiftNear infrared spectroscopy of high redshift active galactic nuclei. 2. Disappearing narrow line regions and the role of accretionNear infrared spectroscopy of high redshift active galactic nuclei. 2. Disappe…X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line …High-Redshift SDSS Quasars with Weak Emission LinesChandra observations of the highest redshift quasars from the sloan digital sky surveyChandra observations of the highest redshift quasars from the sloan digital s…Black-Hole Mass and Growth Rate at High RedshiftSupernova 2002ap - the first monthStar formation in the hosts of high-z QSOs: Evidence from Spitzer PAH detectionsStar formation in the hosts of high-z QSOs: Evidence from Spitzer PAH detect…Observational evidence of quasar feedback quenching star formation at high redshiftObservational evidence of quasar feedback quenching star formation at high…Dust covering factor, silicate emission and star formation in luminous QSOsNear infrared spectroscopy of high redshift active galactic nuclei. 1. A Metallicity-accretion rate relationshipNear infrared spectroscopy of high redshift active galactic nuclei. 1. A Metalli…The 4 Ms Chandra Deep Field-South Number Counts Apportioned by Source Class: Pervasive Active Galactic Nuclei and the Ascent of Normal GalaxiesThe 4 Ms Chandra Deep Field-South Number Counts Apportioned by Source …The Hard X-ray Spectral Slope as an Accretion-Rate Indicator in Radio-Quiet Active Galactic NucleiThe Hard X-ray Spectral Slope as an Accretion-Rate Indicator in Radio-Quiet A…The Hard X-ray Spectrum as a Probe for Black-Hole Growth in Radio-Quiet Active Galactic NucleiThe Hard X-ray Spectrum as a Probe for Black-Hole Growth in Radio-Quiet Act…The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky SurveyThe X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky…Reverberation Mapping of High-Luminosity Quasars: First Results20002005201020152020202501000200030004000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Black-Hole Mass and Growth Rate at z~4.8: A Short Episode of Fast Growth Followed by Short Duty Cycle ActivityBlack-Hole Mass and Growth Rate at z~4.8: A Short Episode of Fast Growth F…Complex optical-x-ray correlations in the narrow-line seyfert 1 galaxy ngc 4051Complex optical-x-ray correlations in the narrow-line seyfert 1 galaxy ngc 40…The X-ray spectral properties and variability of luminous high-redshift active galactic nucleiThe X-ray spectral properties and variability of luminous high-redshift active …A Population of X-ray Weak Quasars: PHL 1811 Analogs at High RedshiftNear infrared spectroscopy of high redshift active galactic nuclei. 2. Disappearing narrow line regions and the role of accretionNear infrared spectroscopy of high redshift active galactic nuclei. 2. Disappe…X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line Quasars: Unification with a Geometrically Thick Accretion Disk?X-ray Insights into the Nature of PHL 1811 Analogs and Weak Emission-Line …High-Redshift SDSS Quasars with Weak Emission LinesChandra observations of the highest redshift quasars from the sloan digital sky surveyChandra observations of the highest redshift quasars from the sloan digital s…Black-Hole Mass and Growth Rate at High RedshiftSupernova 2002ap - the first monthStar formation in the hosts of high-z QSOs: Evidence from Spitzer PAH detectionsStar formation in the hosts of high-z QSOs: Evidence from Spitzer PAH detect…Observational evidence of quasar feedback quenching star formation at high redshiftObservational evidence of quasar feedback quenching star formation at high…Dust covering factor, silicate emission and star formation in luminous QSOsNear infrared spectroscopy of high redshift active galactic nuclei. 1. A Metallicity-accretion rate relationshipNear infrared spectroscopy of high redshift active galactic nuclei. 1. A Metalli…The 4 Ms Chandra Deep Field-South Number Counts Apportioned by Source Class: Pervasive Active Galactic Nuclei and the Ascent of Normal GalaxiesThe 4 Ms Chandra Deep Field-South Number Counts Apportioned by Source …The Hard X-ray Spectral Slope as an Accretion-Rate Indicator in Radio-Quiet Active Galactic NucleiThe Hard X-ray Spectral Slope as an Accretion-Rate Indicator in Radio-Quiet A…The Hard X-ray Spectrum as a Probe for Black-Hole Growth in Radio-Quiet Active Galactic NucleiThe Hard X-ray Spectrum as a Probe for Black-Hole Growth in Radio-Quiet Act…The X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky SurveyThe X-ray Properties of the Most-Luminous Quasars from the Sloan Digital Sky…Reverberation Mapping of High-Luminosity Quasars: First Results2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025050100150200250300