Publication data of Xu, Hao: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20102020200520152025025050075010001250
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200520102015202020250816243240012345
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20022004200620082010201220142016201820202022202405101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestX-ray Background at High Redshifts from Pop III Remnants: Results from Pop III star formation rates in the Renaissance SimulationsX-ray Background at High Redshifts from Pop III Remnants: Results from Pop I…Magnetohydrodynamic Turbulence and Cosmic-Ray Reacceleration in Galaxy ClustersMagnetohydrodynamic Turbulence and Cosmic-Ray Reacceleration in Galaxy …Scaling Relations for Galaxies Prior to ReionizationSpatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sources in the Early UniverseSpatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sour…The Two States of Star Forming CloudsComparisons of Cosmological MHD Galaxy Cluster Simulations to Radio ObservationsComparisons of Cosmological MHD Galaxy Cluster Simulations to Radio Obser…Polarization of cluster radio halos with upcoming radio interferometersEvolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters. I. The Effect of Injection Energy and RedshiftEvolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters. I. …Evolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters II. The Effects of Cluster Size and Dynamical StateEvolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters II. …Heating the Intergalactic medium by X-rays from Population III Binaries in High Redshift GalaxiesHeating the Intergalactic medium by X-rays from Population III Binaries in Hi…Supermassive Population III Supernovae and the Birth of the First QuasarsCosmological AMR MHD with EnzoThe Biermann Battery in Cosmological MHD Simulations of Population III Star FormationThe Biermann Battery in Cosmological MHD Simulations of Population III Star …Comparing Numerical Methods for Isothermal Magnetized Supersonic TurbulenceComparing Numerical Methods for Isothermal Magnetized Supersonic Turbule…Population III Stars and Remnants in High Redshift Galaxies$D D^{*}$ potentials in chiral perturbation theory and possible molecular states$D D^{*}$ potentials in chiral perturbation theory and possible molecular st…Turbulence and Dynamo in Galaxy Cluster Medium: Implications on the Origin of Cluster Magnetic FieldsTurbulence and Dynamo in Galaxy Cluster Medium: Implications on the Origi…Cosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and Warnings for ObservationsCosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and W…Classification and Ranking of Fermi LAT Gamma-ray Sources from the 3FGL Catalog using Machine Learning TechniquesClassification and Ranking of Fermi LAT Gamma-ray Sources from the 3FGL C…20102020200520152025025050075010001250
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)X-ray Background at High Redshifts from Pop III Remnants: Results from Pop III star formation rates in the Renaissance SimulationsX-ray Background at High Redshifts from Pop III Remnants: Results from Pop I…Magnetohydrodynamic Turbulence and Cosmic-Ray Reacceleration in Galaxy ClustersMagnetohydrodynamic Turbulence and Cosmic-Ray Reacceleration in Galaxy …Scaling Relations for Galaxies Prior to ReionizationSpatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sources in the Early UniverseSpatially Extended 21 cm Signal from Strongly Clustered UV and X-Ray Sour…The Two States of Star Forming CloudsComparisons of Cosmological MHD Galaxy Cluster Simulations to Radio ObservationsComparisons of Cosmological MHD Galaxy Cluster Simulations to Radio Obser…Polarization of cluster radio halos with upcoming radio interferometersEvolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters. I. The Effect of Injection Energy and RedshiftEvolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters. I. …Evolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters II. The Effects of Cluster Size and Dynamical StateEvolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters II. …Heating the Intergalactic medium by X-rays from Population III Binaries in High Redshift GalaxiesHeating the Intergalactic medium by X-rays from Population III Binaries in Hi…Supermassive Population III Supernovae and the Birth of the First QuasarsCosmological AMR MHD with EnzoThe Biermann Battery in Cosmological MHD Simulations of Population III Star FormationThe Biermann Battery in Cosmological MHD Simulations of Population III Star …Comparing Numerical Methods for Isothermal Magnetized Supersonic TurbulenceComparing Numerical Methods for Isothermal Magnetized Supersonic Turbule…Population III Stars and Remnants in High Redshift Galaxies$D D^{*}$ potentials in chiral perturbation theory and possible molecular states$D D^{*}$ potentials in chiral perturbation theory and possible molecular st…Turbulence and Dynamo in Galaxy Cluster Medium: Implications on the Origin of Cluster Magnetic FieldsTurbulence and Dynamo in Galaxy Cluster Medium: Implications on the Origi…Cosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and Warnings for ObservationsCosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and W…Classification and Ranking of Fermi LAT Gamma-ray Sources from the 3FGL Catalog using Machine Learning TechniquesClassification and Ranking of Fermi LAT Gamma-ray Sources from the 3FGL C…2002200420062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average20052010201520202025020406080100