Publication data of Nagamine, Kentaro: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20002005201020152020202505001000150020002500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications2000200520102015202020250204060801000246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion200020052010201520202025051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestLuminosity density and star formation rate from lambda-cdm hydrodynamical simulationLuminosity density and star formation rate from lambda-cdm hydrodynamic…Multiphase, non-spherical gas accretion onto a black holePairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matter Model using the Bullet ClusterPairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matt…Photometric properties of Lyman - break galaxies at z=3 in cosmological SPH simulationsPhotometric properties of Lyman - break galaxies at z=3 in cosmological SPH …Star formation history and stellar metallicity distribution in a cold dark matter UniverseStar formation history and stellar metallicity distribution in a cold dark matte…Massive galaxies in cosmological simulations: UV-selected sample at redshift z = 2Massive galaxies in cosmological simulations: UV-selected sample at redshift z…Gamma-ray burst rate: high-redshift excess and its possible originsSteep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z>=6 and the Implications for ReionisationSteep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z>=6 an…Is there a missing galaxy problem?Future evolution of nearby large scale structure in a universe dominated by a cosmological constantFuture evolution of nearby large scale structure in a universe dominated by a…Massive galaxies and EROs at z = 1-3 in cosmological hydrodynamic simulations: Near-IR propertiesMassive galaxies and EROs at z = 1-3 in cosmological hydrodynamic simulati…Distribution of damped lyman-alpha absorbers in a lambda cold dark matter universeDistribution of damped lyman-alpha absorbers in a lambda cold dark matter …Lyman-alpha Emitters and Lyman-break Galaxies at z=3-6 in Cosmological SPH SimulationsLyman-alpha Emitters and Lyman-break Galaxies at z=3-6 in Cosmological SP…Star formation rate and metallicity of damped lyman-alpha absorbers in cosmological sph simulationsStar formation rate and metallicity of damped lyman-alpha absorbers in cos…Signatures of galactic superwinds. Inhomogeneous metal enrichment of the Lyman-alpha forestSignatures of galactic superwinds. Inhomogeneous metal enrichment of the …Abundance of damped Lyman-alpha absorbers in cosmological SPH simulationsAbundance of damped Lyman-alpha absorbers in cosmological SPH simulatio…The history of cosmological star formation: three independent approaches and a critical test using the extragalactic background lightThe history of cosmological star formation: three independent approaches an…Escape fraction of ionizing photons from high-redshift galaxies in cosmological SPH simulationsEscape fraction of ionizing photons from high-redshift galaxies in cosmologic…Comparing AMR and SPH cosmological simulations: 1. Dark matter and adiabatic simulationsComparing AMR and SPH cosmological simulations: 1. Dark matter and adiab…20002005201020152020202505001000150020002500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Luminosity density and star formation rate from lambda-cdm hydrodynamical simulationLuminosity density and star formation rate from lambda-cdm hydrodynamic…Multiphase, non-spherical gas accretion onto a black holePairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matter Model using the Bullet ClusterPairwise Velocities of Dark Matter Halos: a Test for the Lambda Cold Dark Matt…Photometric properties of Lyman - break galaxies at z=3 in cosmological SPH simulationsPhotometric properties of Lyman - break galaxies at z=3 in cosmological SPH …Star formation history and stellar metallicity distribution in a cold dark matter UniverseStar formation history and stellar metallicity distribution in a cold dark matte…Massive galaxies in cosmological simulations: UV-selected sample at redshift z = 2Massive galaxies in cosmological simulations: UV-selected sample at redshift z…Gamma-ray burst rate: high-redshift excess and its possible originsSteep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z>=6 and the Implications for ReionisationSteep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z>=6 an…Is there a missing galaxy problem?Future evolution of nearby large scale structure in a universe dominated by a cosmological constantFuture evolution of nearby large scale structure in a universe dominated by a…Massive galaxies and EROs at z = 1-3 in cosmological hydrodynamic simulations: Near-IR propertiesMassive galaxies and EROs at z = 1-3 in cosmological hydrodynamic simulati…Distribution of damped lyman-alpha absorbers in a lambda cold dark matter universeDistribution of damped lyman-alpha absorbers in a lambda cold dark matter …Lyman-alpha Emitters and Lyman-break Galaxies at z=3-6 in Cosmological SPH SimulationsLyman-alpha Emitters and Lyman-break Galaxies at z=3-6 in Cosmological SP…Star formation rate and metallicity of damped lyman-alpha absorbers in cosmological sph simulationsStar formation rate and metallicity of damped lyman-alpha absorbers in cos…Signatures of galactic superwinds. Inhomogeneous metal enrichment of the Lyman-alpha forestSignatures of galactic superwinds. Inhomogeneous metal enrichment of the …Abundance of damped Lyman-alpha absorbers in cosmological SPH simulationsAbundance of damped Lyman-alpha absorbers in cosmological SPH simulatio…The history of cosmological star formation: three independent approaches and a critical test using the extragalactic background lightThe history of cosmological star formation: three independent approaches an…Escape fraction of ionizing photons from high-redshift galaxies in cosmological SPH simulationsEscape fraction of ionizing photons from high-redshift galaxies in cosmologic…Comparing AMR and SPH cosmological simulations: 1. Dark matter and adiabatic simulationsComparing AMR and SPH cosmological simulations: 1. Dark matter and adiab…2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2000200520102015202020250255075100125150175