Publication data of Clowe, Douglas: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250200040006000800010000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250153045607501.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion199520002005201020152020202505101520253035
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestWeak lensing mass reconstructions of the eso distant cluster surveyFocusing Cosmic Telescopes: Exploring Redshift z~5-6 Galaxies with the Bullet Cluster 1E0657-56Focusing Cosmic Telescopes: Exploring Redshift z~5-6 Galaxies with the Bulle…The environments of starburst and post-starburst galaxies at z=0.4-0.8Effects of asphericity and substructure on the determination of cluster mass with weak gravitational lensingEffects of asphericity and substructure on the determination of cluster mass …On Dark Peaks and Missing Mass: A Weak Lensing Mass Reconstruction of the Merging Cluster System Abell 520On Dark Peaks and Missing Mass: A Weak Lensing Mass Reconstruction of the…Numerical simulations of weak lensing measurementsA New Look at Massive Clusters: weak lensing constraints on the triaxial dark matter halos of Abell 1689, Abell 1835, & Abell 2204A New Look at Massive Clusters: weak lensing constraints on the triaxial dark …Weak lensing by high-redshift clusters of galaxies. 1. Cluster mass reconstructionWeak lensing by high-redshift clusters of galaxies. 1. Cluster mass reconstruc…The Morphological Content of Ten EDisCS Clusters at 0.5 < z < 0.8A filament of dark matter between two clusters of galaxiesThe Build-up of the red-sequence in galaxy clusters since Z ~ 0.8The build-up of the colour-magnitude relation in galaxy clusters since z 0.8The evolution of the star formation activity in galaxies and its dependence on environmentThe evolution of the star formation activity in galaxies and its dependence on…Findings of the Joint Dark Energy Mission Figure of Merit Science Working GroupFindings of the Joint Dark Energy Mission Figure of Merit Science Working Gro…Strong and weak lensing united. 3. Measuring the mass distribution of the merging galaxy cluster 1E0657-56Strong and weak lensing united. 3. Measuring the mass distribution of the m…Weak lensing mass reconstruction of the interacting cluster 1E0657-558: Direct evidence for the existence of dark matterWeak lensing mass reconstruction of the interacting cluster 1E0657-558: Dir…Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-56Constraints on the Self-Interaction Cross-Section of Dark Matter from Numeri…Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56Direct constraints on the dark matter self-interaction cross-section from the …A direct empirical proof of the existence of dark matter19952000200520102015202020250200040006000800010000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Weak lensing mass reconstructions of the eso distant cluster surveyFocusing Cosmic Telescopes: Exploring Redshift z~5-6 Galaxies with the Bullet Cluster 1E0657-56Focusing Cosmic Telescopes: Exploring Redshift z~5-6 Galaxies with the Bulle…The environments of starburst and post-starburst galaxies at z=0.4-0.8Effects of asphericity and substructure on the determination of cluster mass with weak gravitational lensingEffects of asphericity and substructure on the determination of cluster mass …On Dark Peaks and Missing Mass: A Weak Lensing Mass Reconstruction of the Merging Cluster System Abell 520On Dark Peaks and Missing Mass: A Weak Lensing Mass Reconstruction of the…Numerical simulations of weak lensing measurementsA New Look at Massive Clusters: weak lensing constraints on the triaxial dark matter halos of Abell 1689, Abell 1835, & Abell 2204A New Look at Massive Clusters: weak lensing constraints on the triaxial dark …Weak lensing by high-redshift clusters of galaxies. 1. Cluster mass reconstructionWeak lensing by high-redshift clusters of galaxies. 1. Cluster mass reconstruc…The Morphological Content of Ten EDisCS Clusters at 0.5 < z < 0.8A filament of dark matter between two clusters of galaxiesThe Build-up of the red-sequence in galaxy clusters since Z ~ 0.8The build-up of the colour-magnitude relation in galaxy clusters since z 0.8The evolution of the star formation activity in galaxies and its dependence on environmentThe evolution of the star formation activity in galaxies and its dependence on…Findings of the Joint Dark Energy Mission Figure of Merit Science Working GroupFindings of the Joint Dark Energy Mission Figure of Merit Science Working Gro…Strong and weak lensing united. 3. Measuring the mass distribution of the merging galaxy cluster 1E0657-56Strong and weak lensing united. 3. Measuring the mass distribution of the m…Weak lensing mass reconstruction of the interacting cluster 1E0657-558: Direct evidence for the existence of dark matterWeak lensing mass reconstruction of the interacting cluster 1E0657-558: Dir…Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-56Constraints on the Self-Interaction Cross-Section of Dark Matter from Numeri…Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56Direct constraints on the dark matter self-interaction cross-section from the …A direct empirical proof of the existence of dark matter19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250200400600800