Publication data of Scharf, Caleb A.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250122436486001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe warps survey -. 4. the x-ray luminosity-temperature relation of high redshift galaxy clustersThe warps survey -. 4. the x-ray luminosity-temperature relation of high reds…A statistical detection of gamma-ray emission from galaxy clusters: Implications for the gamma-ray background and structure formationA statistical detection of gamma-ray emission from galaxy clusters: Implicatio…Distant cluster hunting I: a comparison between the optical and x-ray luminosity functions from an optical/x-ray surveyDistant cluster hunting I: a comparison between the optical and x-ray lumino…Extended x-ray emission around 4C41.17 at z=3.8Discovery of a very x-ray luminous galaxy cluster at z=0.89 in the warps surveyDiscovery of a very x-ray luminous galaxy cluster at z=0.89 in the warps sur…The 2-10 kev xrb dipole and its cosmological implicationsThe Chandra Deep Protocluster Survey: Evidence for an Enhancement in the AGN Activity in the SSA22 Protocluster at z = 3.09The Chandra Deep Protocluster Survey: Evidence for an Enhancement in the …Distant cluster hunting. 2. A comparison of x-ray and optical cluster detection techniques and catalogs from the rox surveyDistant cluster hunting. 2. A comparison of x-ray and optical cluster detectio…Evidence for x-ray emission from a large scale filament of galaxies ?The warps survey. 3. The discovery of an x-ray luminous galaxy cluster at z=0.833 and the evolution of x-ray luminous clusters at z<1The warps survey. 3. The discovery of an x-ray luminous galaxy cluster at z=…Wiener reconstruction of galaxy surveys in spherical harmonicsThe Evolution of the cluster x-ray scaling relations in the WARPS sample at 0.6 < z < 1.0The Evolution of the cluster x-ray scaling relations in the WARPS sample at 0.…The Chandra Deep Protocluster Survey: Ly-alpha Blobs are powered by heating, not coolingThe Chandra Deep Protocluster Survey: Ly-alpha Blobs are powered by heatin…The WARPS survey. 6. Galaxy cluster and source identifications from phase 1The warps survey. 2. The log(n)-log(s) relation and the x-ray evolution of low luminosity clusters of galaxiesThe warps survey. 2. The log(n)-log(s) relation and the x-ray evolution of low l…The warps x-ray survey of galaxies, groups and clusters I: method and first resultsThe warps x-ray survey of galaxies, groups and clusters I: method and first r…Observational tests of the mass-temperature relation for galaxy clustersA Spherical Harmonic Approach to Redshift Distortion and a Measurement of Omega from the 1.2 Jy IRAS Redshift SurveyA Spherical Harmonic Approach to Redshift Distortion and a Measurement of …The Luminosity-temperature relation at z = 0.4 for clusters of galaxies19952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The warps survey -. 4. the x-ray luminosity-temperature relation of high redshift galaxy clustersThe warps survey -. 4. the x-ray luminosity-temperature relation of high reds…A statistical detection of gamma-ray emission from galaxy clusters: Implications for the gamma-ray background and structure formationA statistical detection of gamma-ray emission from galaxy clusters: Implicatio…Distant cluster hunting I: a comparison between the optical and x-ray luminosity functions from an optical/x-ray surveyDistant cluster hunting I: a comparison between the optical and x-ray lumino…Extended x-ray emission around 4C41.17 at z=3.8Discovery of a very x-ray luminous galaxy cluster at z=0.89 in the warps surveyDiscovery of a very x-ray luminous galaxy cluster at z=0.89 in the warps sur…The 2-10 kev xrb dipole and its cosmological implicationsThe Chandra Deep Protocluster Survey: Evidence for an Enhancement in the AGN Activity in the SSA22 Protocluster at z = 3.09The Chandra Deep Protocluster Survey: Evidence for an Enhancement in the …Distant cluster hunting. 2. A comparison of x-ray and optical cluster detection techniques and catalogs from the rox surveyDistant cluster hunting. 2. A comparison of x-ray and optical cluster detectio…Evidence for x-ray emission from a large scale filament of galaxies ?The warps survey. 3. The discovery of an x-ray luminous galaxy cluster at z=0.833 and the evolution of x-ray luminous clusters at z<1The warps survey. 3. The discovery of an x-ray luminous galaxy cluster at z=…Wiener reconstruction of galaxy surveys in spherical harmonicsThe Evolution of the cluster x-ray scaling relations in the WARPS sample at 0.6 < z < 1.0The Evolution of the cluster x-ray scaling relations in the WARPS sample at 0.…The Chandra Deep Protocluster Survey: Ly-alpha Blobs are powered by heating, not coolingThe Chandra Deep Protocluster Survey: Ly-alpha Blobs are powered by heatin…The WARPS survey. 6. Galaxy cluster and source identifications from phase 1The warps survey. 2. The log(n)-log(s) relation and the x-ray evolution of low luminosity clusters of galaxiesThe warps survey. 2. The log(n)-log(s) relation and the x-ray evolution of low l…The warps x-ray survey of galaxies, groups and clusters I: method and first resultsThe warps x-ray survey of galaxies, groups and clusters I: method and first r…Observational tests of the mass-temperature relation for galaxy clustersA Spherical Harmonic Approach to Redshift Distortion and a Measurement of Omega from the 1.2 Jy IRAS Redshift SurveyA Spherical Harmonic Approach to Redshift Distortion and a Measurement of …The Luminosity-temperature relation at z = 0.4 for clusters of galaxies19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250255075100125150175