Publication data of Schleicher, Dominik R.G.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion200620082010201220142016201820202022202401000200030004000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications20062008201020122014201620182020202220240306090120150048121620
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion2006200820102012201420162018202020222024010203040
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestHigh resolution studies of massive primordial haloesThe Turbulent Dynamo in Highly Compressible Supersonic PlasmasFormation of massive seed black holes via collisions and accretionBlack hole formation in primordial galaxies: chemical and radiative conditionsA UV flux constraint on the formation of direct collapse black holesReionization - A probe for the stellar population and the physics of the early universeReionization - A probe for the stellar population and the physics of the early u…How realistic UV spectra and X-rays suppress the abundance of direct collapse black holesHow realistic UV spectra and X-rays suppress the abundance of direct collaps…KROME – a package to embed chemistry in astrophysical simulationsThe Small-Scale Dynamo and Non-Ideal MHD in Primordial Star FormationSmall-scale dynamo action during the formation of the first stars and galaxies. I. The ideal MHD limitSmall-scale dynamo action during the formation of the first stars and galaxie…Mach Number Dependence of Turbulent Magnetic Field Amplification: Solenoidal versus Compressive FlowsMach Number Dependence of Turbulent Magnetic Field Amplification: Solenoi…Massive black hole factories: Supermassive and quasi-star formation in primordial halosMassive black hole factories: Supermassive and quasi-star formation in primo…The characteristic black hole mass resulting from direct collapse in the early universeThe characteristic black hole mass resulting from direct collapse in the early …The generation of strong magnetic fields during the formation of the first starsThe generation of strong magnetic fields during the formation of the first sta…Initial mass function of intermediate mass black hole seedsMagnetic fields in the Large-Scale Structure of the UniverseA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulenceA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: …Black hole formation in the early universeThe First Magnetic Fields200620082010201220142016201820202022202401000200030004000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)High resolution studies of massive primordial haloesThe Turbulent Dynamo in Highly Compressible Supersonic PlasmasFormation of massive seed black holes via collisions and accretionBlack hole formation in primordial galaxies: chemical and radiative conditionsA UV flux constraint on the formation of direct collapse black holesReionization - A probe for the stellar population and the physics of the early universeReionization - A probe for the stellar population and the physics of the early u…How realistic UV spectra and X-rays suppress the abundance of direct collapse black holesHow realistic UV spectra and X-rays suppress the abundance of direct collaps…KROME – a package to embed chemistry in astrophysical simulationsThe Small-Scale Dynamo and Non-Ideal MHD in Primordial Star FormationSmall-scale dynamo action during the formation of the first stars and galaxies. I. The ideal MHD limitSmall-scale dynamo action during the formation of the first stars and galaxie…Mach Number Dependence of Turbulent Magnetic Field Amplification: Solenoidal versus Compressive FlowsMach Number Dependence of Turbulent Magnetic Field Amplification: Solenoi…Massive black hole factories: Supermassive and quasi-star formation in primordial halosMassive black hole factories: Supermassive and quasi-star formation in primo…The characteristic black hole mass resulting from direct collapse in the early universeThe characteristic black hole mass resulting from direct collapse in the early …The generation of strong magnetic fields during the formation of the first starsThe generation of strong magnetic fields during the formation of the first sta…Initial mass function of intermediate mass black hole seedsMagnetic fields in the Large-Scale Structure of the UniverseA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulenceA new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: …Black hole formation in the early universeThe First Magnetic Fields20062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average20062008201020122014201620182020202220240100200300400