Publication data of Haas, Marcel R.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2006200820102012201420162018202020222024025050075010001250
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200620082010201220142016201820202022202404812162000.81.62.43.24
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion2006200820102012201420162018202020222024024681012
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersThe Maximum Mass of Star ClustersVariation of the cluster luminosity function across the disk of M51Galactic consequences of clustered star formationThe radii of thousands of star clusters in M51 with HST/ACSThe Origin of Extended Disk Galaxies at z=2Variations in Integrated Galactic Initial Mass Functions due to Sampling Method and Cluster Mass FunctionVariations in Integrated Galactic Initial Mass Functions due to Sampling Meth…Stellar Signatures of AGN Jet Triggered Star FormationJet interactions with a giant molecular cloud in the Galactic centre and ejection of hypervelocity starsJet interactions with a giant molecular cloud in the Galactic centre and ejecti…ACS imaging of star clusters in M51 II. The luminosity function and mass function across the diskACS imaging of star clusters in M51 II. The luminosity function and mass fun…Physical properties of simulated galaxy populations at z=2 -- II. Effects of physics ingredients other than cooling and outflowsPhysical properties of simulated galaxy populations at z=2 -- II. Effects of phy…Damped Lyα absorption systems in semi-analytic models with multiphase gasThe correlation structure of dark matter halo propertiesObservational evidence for a truncation of the star cluster initial mass function at the high mass endObservational evidence for a truncation of the star cluster initial mass functio…Physical properties of simulated galaxy populations at z=2 -- I. Effect of metal-line cooling and feedback from star formation and AGNPhysical properties of simulated galaxy populations at z=2 -- I. Effect of meta…ACS imaging of star clusters in M51. I. Identification and radius distributionDisentangling galaxy environment and host halo massThe rates and modes of gas accretion on to galaxies and their gaseous haloesThe physics driving the cosmic star formation history2006200820102012201420162018202020222024025050075010001250
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The Maximum Mass of Star ClustersVariation of the cluster luminosity function across the disk of M51Galactic consequences of clustered star formationThe radii of thousands of star clusters in M51 with HST/ACSThe Origin of Extended Disk Galaxies at z=2Variations in Integrated Galactic Initial Mass Functions due to Sampling Method and Cluster Mass FunctionVariations in Integrated Galactic Initial Mass Functions due to Sampling Meth…Stellar Signatures of AGN Jet Triggered Star FormationJet interactions with a giant molecular cloud in the Galactic centre and ejection of hypervelocity starsJet interactions with a giant molecular cloud in the Galactic centre and ejecti…ACS imaging of star clusters in M51 II. The luminosity function and mass function across the diskACS imaging of star clusters in M51 II. The luminosity function and mass fun…Physical properties of simulated galaxy populations at z=2 -- II. Effects of physics ingredients other than cooling and outflowsPhysical properties of simulated galaxy populations at z=2 -- II. Effects of phy…Damped Lyα absorption systems in semi-analytic models with multiphase gasThe correlation structure of dark matter halo propertiesObservational evidence for a truncation of the star cluster initial mass function at the high mass endObservational evidence for a truncation of the star cluster initial mass functio…Physical properties of simulated galaxy populations at z=2 -- I. Effect of metal-line cooling and feedback from star formation and AGNPhysical properties of simulated galaxy populations at z=2 -- I. Effect of meta…ACS imaging of star clusters in M51. I. Identification and radius distributionDisentangling galaxy environment and host halo massThe rates and modes of gas accretion on to galaxies and their gaseous haloesThe physics driving the cosmic star formation history20062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average20062008201020122014201620182020202220240255075100125150