Publication data of White, Martin J.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion199019952000200520102015202020250500010000150002000025000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19901995200020052010201520202025080160240320400048121620
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19901995200020052010201520202025020406080100
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestConvolution Lagrangian perturbation theory for biased tracersThe Effect of physical assumptions on the calculation of microwave background anisotropiesThe Effect of physical assumptions on the calculation of microwave backgrou…Mass Function Predictions Beyond LCDMHalo Assembly Bias in Hierarchical Structure FormationTowards an accurate model of the redshift space clustering of halos in the quasilinear regimeTowards an accurate model of the redshift space clustering of halos in the qu…Tensor perturbations in inflationary models as a probe of cosmologyThe Coyote Universe II: Cosmological Models and Precision Emulation of the Nonlinear Matter Power SpectrumThe Coyote Universe II: Cosmological Models and Precision Emulation of the N…Acoustic signatures in the cosmic microwave backgroundAnisotropies in the cosmic microwave backgroundTesting cosmological structure formation using redshift-space distortionsVirial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization CosmologyVirial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Norma…The Coyote Universe I: Precision Determination of the Nonlinear Matter Power SpectrumThe Coyote Universe I: Precision Determination of the Nonlinear Matter Power…The Four year COBE normalization and large scale structureA CMB polarization primerOn the Robustness of the Acoustic Scale in the Low-Redshift Clustering of MatterOn the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Ma…CMB anisotropies: Total angular momentum methodConstraining dark energy with SNe Ia and large scale structureCDM models with a smooth componentThe propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxiesThe propagation of uncertainties in stellar population synthesis modeling I: T…199019952000200520102015202020250500010000150002000025000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Convolution Lagrangian perturbation theory for biased tracersThe Effect of physical assumptions on the calculation of microwave background anisotropiesThe Effect of physical assumptions on the calculation of microwave backgrou…Mass Function Predictions Beyond LCDMHalo Assembly Bias in Hierarchical Structure FormationTowards an accurate model of the redshift space clustering of halos in the quasilinear regimeTowards an accurate model of the redshift space clustering of halos in the qu…Tensor perturbations in inflationary models as a probe of cosmologyThe Coyote Universe II: Cosmological Models and Precision Emulation of the Nonlinear Matter Power SpectrumThe Coyote Universe II: Cosmological Models and Precision Emulation of the N…Acoustic signatures in the cosmic microwave backgroundAnisotropies in the cosmic microwave backgroundTesting cosmological structure formation using redshift-space distortionsVirial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization CosmologyVirial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Norma…The Coyote Universe I: Precision Determination of the Nonlinear Matter Power SpectrumThe Coyote Universe I: Precision Determination of the Nonlinear Matter Power…The Four year COBE normalization and large scale structureA CMB polarization primerOn the Robustness of the Acoustic Scale in the Low-Redshift Clustering of MatterOn the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Ma…CMB anisotropies: Total angular momentum methodConstraining dark energy with SNe Ia and large scale structureCDM models with a smooth componentThe propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxiesThe propagation of uncertainties in stellar population synthesis modeling I: T…199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average199019952000200520102015202020250500100015002000