Publication data of McDonald, Michael A.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19801985199019952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19801990200020102020030609012015002.557.51012.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1980198519901995200020052010201520202025051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestEvolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Red…An HST/WFC3-UVIS View of the Starburst in the Cool Core of the Phoenix ClusterAn HST/WFC3-UVIS View of the Starburst in the Cool Core of the Phoenix Clus…Optical Spectroscopy of Halpha Filaments in Cool Core Clusters: Kinematics, Reddening, and Sources of IonizationOptical Spectroscopy of Halpha Filaments in Cool Core Clusters: Kinematics, R…A Robust Quantification of Galaxy Cluster Morphology Using Asymmetry and Central ConcentrationA Robust Quantification of Galaxy Cluster Morphology Using Asymmetry and …Testing for X-ray-SZ Differences and Redshift Evolution in the X-ray Morphology of Galaxy ClustersTesting for X-ray-SZ Differences and Redshift Evolution in the X-ray Morpholog…ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix clusterALMA observations of massive molecular gas filaments encasing radio bubble…Star Formation Efficiency in the Cool Cores of Galaxy ClustersThe Effect of Environment on the Formation of Halpha Filaments and Cool Cores in Galaxy Groups and ClustersThe Effect of Environment on the Formation of Halpha Filaments and Cool Co…Cosmological constraints from gas mass fractions of massive, relaxed galaxy clustersCosmological constraints from gas mass fractions of massive, relaxed galaxy …Constraints on the optical depth of galaxy groups and clustersRadial Profile of the 3.55 keV line out to $R_{200}$ in the Perseus ClusterThe Evolution of the Intracluster Medium Metallicity in Sunyaev-Zel'dovich-Selected Galaxy Clusters at 0 $< z <$ 1.5The Evolution of the Intracluster Medium Metallicity in Sunyaev-Zel'dovich-Se…Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of GalaxiesRevisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galax…The Luminosity Profile and Structural Parameters of the Andromeda GalaxyA census of cool core galaxy clusters in IllustrisTNGShaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and ClustersShaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Casc…A Very Deep Chandra Observation of Abell 2052: Bubbles, Shocks, and SloshingA Very Deep Chandra Observation of Abell 2052: Bubbles, Shocks, and Sloshi…On the Origin of the Extended Halpha Filaments in Cooling Flow ClustersThe Remarkable Similarity of Massive Galaxy Clusters from z ∼ 0 to z ∼ 1.919801985199019952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Red…An HST/WFC3-UVIS View of the Starburst in the Cool Core of the Phoenix ClusterAn HST/WFC3-UVIS View of the Starburst in the Cool Core of the Phoenix Clus…Optical Spectroscopy of Halpha Filaments in Cool Core Clusters: Kinematics, Reddening, and Sources of IonizationOptical Spectroscopy of Halpha Filaments in Cool Core Clusters: Kinematics, R…A Robust Quantification of Galaxy Cluster Morphology Using Asymmetry and Central ConcentrationA Robust Quantification of Galaxy Cluster Morphology Using Asymmetry and …Testing for X-ray-SZ Differences and Redshift Evolution in the X-ray Morphology of Galaxy ClustersTesting for X-ray-SZ Differences and Redshift Evolution in the X-ray Morpholog…ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix clusterALMA observations of massive molecular gas filaments encasing radio bubble…Star Formation Efficiency in the Cool Cores of Galaxy ClustersThe Effect of Environment on the Formation of Halpha Filaments and Cool Cores in Galaxy Groups and ClustersThe Effect of Environment on the Formation of Halpha Filaments and Cool Co…Cosmological constraints from gas mass fractions of massive, relaxed galaxy clustersCosmological constraints from gas mass fractions of massive, relaxed galaxy …Constraints on the optical depth of galaxy groups and clustersRadial Profile of the 3.55 keV line out to $R_{200}$ in the Perseus ClusterThe Evolution of the Intracluster Medium Metallicity in Sunyaev-Zel'dovich-Selected Galaxy Clusters at 0 $< z <$ 1.5The Evolution of the Intracluster Medium Metallicity in Sunyaev-Zel'dovich-Se…Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of GalaxiesRevisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galax…The Luminosity Profile and Structural Parameters of the Andromeda GalaxyA census of cool core galaxy clusters in IllustrisTNGShaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and ClustersShaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Casc…A Very Deep Chandra Observation of Abell 2052: Bubbles, Shocks, and SloshingA Very Deep Chandra Observation of Abell 2052: Bubbles, Shocks, and Sloshi…On the Origin of the Extended Halpha Filaments in Cooling Flow ClustersThe Remarkable Similarity of Massive Galaxy Clusters from z ∼ 0 to z ∼ 1.919801985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1980198519901995200020052010201520202025050100150200250