Publication data of Matsubara, Takahiko: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19801990200020102020010002000300040005000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1980199020002010202002550751001250246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19751980198519901995200020052010201520202025010203040
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestAnalytic expression of the genus in weakly non-gaussian field induced by gravityAnalytic expression of the genus in weakly non-gaussian field induced by gra…Analytic Minkowski Functionals of the Cosmic Microwave Background: Second-order Non-Gaussianity with Bispectrum and TrispectrumAnalytic Minkowski Functionals of the Cosmic Microwave Background: Secon…Stochasticity of bias and nonlocality of galaxy formation: Linear scalesRecursive Solutions of Lagrangian Perturbation TheorySignature of Primordial Non-Gaussianity on Matter Power SpectrumThe Correlation function in redshift space: General formula with wide angle effects and cosmological distortionsThe Correlation function in redshift space: General formula with wide angle ef…Limits on Primordial Non-Gaussianity from Minkowski Functionals of the WMAP Temperature AnisotropiesLimits on Primordial Non-Gaussianity from Minkowski Functionals of the WMA…Statistics of Smoothed Cosmic Fields in Perturbation Theory. 1. Formulation and Useful Formulae in Second Order Perturbation TheoryStatistics of Smoothed Cosmic Fields in Perturbation Theory. 1. Formulation a…Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of N-body Simulations and Analytic ModelsModeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Re…Simulations of Baryon Acoustic Oscillations II: Covariance matrix of the matter power spectrumSimulations of Baryon Acoustic Oscillations II: Covariance matrix of the matte…Primordial Non-Gaussianity and Analytical Formula for Minkowski Functionals of the Cosmic Microwave Background and Large-scale StructurePrimordial Non-Gaussianity and Analytical Formula for Minkowski Functionals …Cosmological redshift distortion of correlation functions as a probe of the density parameter and the cosmological constantCosmological redshift distortion of correlation functions as a probe of the den…Redshift space distortions of the correlation function in wide angle galaxy surveysRedshift space distortions of the correlation function in wide angle galaxy sur…Nonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space Distortions, and Primordial Non-GaussianityNonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space …Correlation function in deep redshift space as a cosmological probeSimulations of Wide-Field Weak Lensing Surveys I: Basic Statistics and Non-Gaussian EffectsSimulations of Wide-Field Weak Lensing Surveys I: Basic Statistics and Non-G…Large-Scale Anisotropic Correlation Function of SDSS Luminous Red GalaxiesNonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian pictureNonlinear perturbation theory with halo bias and redshift-space distortions vi…Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift SpaceResumming Cosmological Perturbations via the Lagrangian Picture: One-loop …19801990200020102020010002000300040005000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Analytic expression of the genus in weakly non-gaussian field induced by gravityAnalytic expression of the genus in weakly non-gaussian field induced by gra…Analytic Minkowski Functionals of the Cosmic Microwave Background: Second-order Non-Gaussianity with Bispectrum and TrispectrumAnalytic Minkowski Functionals of the Cosmic Microwave Background: Secon…Stochasticity of bias and nonlocality of galaxy formation: Linear scalesRecursive Solutions of Lagrangian Perturbation TheorySignature of Primordial Non-Gaussianity on Matter Power SpectrumThe Correlation function in redshift space: General formula with wide angle effects and cosmological distortionsThe Correlation function in redshift space: General formula with wide angle ef…Limits on Primordial Non-Gaussianity from Minkowski Functionals of the WMAP Temperature AnisotropiesLimits on Primordial Non-Gaussianity from Minkowski Functionals of the WMA…Statistics of Smoothed Cosmic Fields in Perturbation Theory. 1. Formulation and Useful Formulae in Second Order Perturbation TheoryStatistics of Smoothed Cosmic Fields in Perturbation Theory. 1. Formulation a…Modeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Regime of N-body Simulations and Analytic ModelsModeling Nonlinear Evolution of Baryon Acoustic Oscillations: Convergence Re…Simulations of Baryon Acoustic Oscillations II: Covariance matrix of the matter power spectrumSimulations of Baryon Acoustic Oscillations II: Covariance matrix of the matte…Primordial Non-Gaussianity and Analytical Formula for Minkowski Functionals of the Cosmic Microwave Background and Large-scale StructurePrimordial Non-Gaussianity and Analytical Formula for Minkowski Functionals …Cosmological redshift distortion of correlation functions as a probe of the density parameter and the cosmological constantCosmological redshift distortion of correlation functions as a probe of the den…Redshift space distortions of the correlation function in wide angle galaxy surveysRedshift space distortions of the correlation function in wide angle galaxy sur…Nonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space Distortions, and Primordial Non-GaussianityNonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space …Correlation function in deep redshift space as a cosmological probeSimulations of Wide-Field Weak Lensing Surveys I: Basic Statistics and Non-Gaussian EffectsSimulations of Wide-Field Weak Lensing Surveys I: Basic Statistics and Non-G…Large-Scale Anisotropic Correlation Function of SDSS Luminous Red GalaxiesNonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian pictureNonlinear perturbation theory with halo bias and redshift-space distortions vi…Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift SpaceResumming Cosmological Perturbations via the Lagrangian Picture: One-loop …197519801985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average197519801985199019952000200520102015202020250100200300400