Publication data of Hamilton, Andrew J.S.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19851990199520002005201020152020202501000200030004000500060007000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications198519901995200020052010201520202025030609012015002.557.51012.5
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestA Scheme to deal accurately and efficiently with complex angular masks in galaxy surveysA Scheme to deal accurately and efficiently with complex angular masks in g…Information content of the non-linear matter power spectrumZero-Energy Modes from Coalescing Andreev States in a Two-Dimensional Semiconductor-Superconductor Hybrid PlatformZero-Energy Modes from Coalescing Andreev States in a Two-Dimensional Se…The River model of black holesThe Real space power spectrum of the PSCz survey from 0.01 to 300 h Mpc**-1The Real space power spectrum of the PSCz survey from 0.01 to 300 h Mpc*…Nonlinear cosmological power spectra in real and redshift spaceTowards a refined cosmic concordance model: Joint 11 parameter constraints from CMB and large scale structureTowards a refined cosmic concordance model: Joint 11 parameter constraint…On measuring the covariance matrix of the nonlinear power spectrum from simulationsOn measuring the covariance matrix of the nonlinear power spectrum from s…Matter power spectrum from the Lyman-alpha forest: Myth or reality?Methods for Rapidly Processing Angular Masks of Next-Generation Galaxy SurveysMethods for Rapidly Processing Angular Masks of Next-Generation Galaxy Sur…The Power spectrum of galaxies in the 2dF 100k redshift surveyMeasuring the galaxy power spectrum with future redshift surveysUncorrelated modes of the nonlinear power spectrumLinear redshift distortions: A ReviewReconstructing the primordial spectrum of fluctuations of the universe from the observed nonlinear clustering of galaxiesReconstructing the primordial spectrum of fluctuations of the universe from …Toward Better Ways to Measure the Galaxy Correlation FunctionMeasuring Omega and the real correlation function from the redshift correlation functionMeasuring Omega and the real correlation function from the redshift correlati…A high resolution foreground cleaned CMB map from WMAPThe Significance of the largest scale CMB fluctuations in WMAP19851990199520002005201020152020202501000200030004000500060007000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)A Scheme to deal accurately and efficiently with complex angular masks in galaxy surveysA Scheme to deal accurately and efficiently with complex angular masks in g…Information content of the non-linear matter power spectrumZero-Energy Modes from Coalescing Andreev States in a Two-Dimensional Semiconductor-Superconductor Hybrid PlatformZero-Energy Modes from Coalescing Andreev States in a Two-Dimensional Se…The River model of black holesThe Real space power spectrum of the PSCz survey from 0.01 to 300 h Mpc**-1The Real space power spectrum of the PSCz survey from 0.01 to 300 h Mpc*…Nonlinear cosmological power spectra in real and redshift spaceTowards a refined cosmic concordance model: Joint 11 parameter constraints from CMB and large scale structureTowards a refined cosmic concordance model: Joint 11 parameter constraint…On measuring the covariance matrix of the nonlinear power spectrum from simulationsOn measuring the covariance matrix of the nonlinear power spectrum from s…Matter power spectrum from the Lyman-alpha forest: Myth or reality?Methods for Rapidly Processing Angular Masks of Next-Generation Galaxy SurveysMethods for Rapidly Processing Angular Masks of Next-Generation Galaxy Sur…The Power spectrum of galaxies in the 2dF 100k redshift surveyMeasuring the galaxy power spectrum with future redshift surveysUncorrelated modes of the nonlinear power spectrumLinear redshift distortions: A ReviewReconstructing the primordial spectrum of fluctuations of the universe from the observed nonlinear clustering of galaxiesReconstructing the primordial spectrum of fluctuations of the universe from …Toward Better Ways to Measure the Galaxy Correlation FunctionMeasuring Omega and the real correlation function from the redshift correlation functionMeasuring Omega and the real correlation function from the redshift correlati…A high resolution foreground cleaned CMB map from WMAPThe Significance of the largest scale CMB fluctuations in WMAP1985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1985199019952000200520102015202020250100200300400500600