Publication data of Eisenstein, Daniel: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1995200020052010201520202025050001000015000200002500030000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250601201802403000510152025
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025020406080100
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe shape of the SDSS DR5 galaxy power spectrumImproved forecasts for the baryon acoustic oscillations and cosmological distance scaleImproved forecasts for the baryon acoustic oscillations and cosmological dist…Solving Large Scale Structure in Ten Easy Steps with COLAThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipolesThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Su…Cosmic complementarity: Joint parameter estimation from CMB experiments and redshift surveysCosmic complementarity: Joint parameter estimation from CMB experiments …Relationship between environment and the broad - band optical properties of galaxies in the SDSSRelationship between environment and the broad - band optical properties of…Estimating fixed frame galaxy magnitudes in the SDSSThe Luminosity function of galaxies in SDSS commissioning dataOn 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…Weighing neutrinos with galaxy surveysImproving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic PeakImproving Cosmological Distance Measurements by Reconstruction of the Ba…Mid-infrared selection of active galaxiesThe DESI Experiment, a whitepaper for Snowmass 2013A 2 per cent distance to $z$=0.35 by reconstructing baryon acoustic oscillations - I. Methods and application to the Sloan Digital Sky SurveyA 2 per cent distance to $z$=0.35 by reconstructing baryon acoustic oscillat…Probing dark energy with baryonic acoustic oscillations from future large galaxy redshift surveysProbing dark energy with baryonic acoustic oscillations from future large gal…Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRSPower spectra for cold dark matter and its variantsObservational Probes of Cosmic AccelerationBaryonic features in the matter transfer function1995200020052010201520202025050001000015000200002500030000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The shape of the SDSS DR5 galaxy power spectrumImproved forecasts for the baryon acoustic oscillations and cosmological distance scaleImproved forecasts for the baryon acoustic oscillations and cosmological dist…Solving Large Scale Structure in Ten Easy Steps with COLAThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipolesThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Su…Cosmic complementarity: Joint parameter estimation from CMB experiments and redshift surveysCosmic complementarity: Joint parameter estimation from CMB experiments …Relationship between environment and the broad - band optical properties of galaxies in the SDSSRelationship between environment and the broad - band optical properties of…Estimating fixed frame galaxy magnitudes in the SDSSThe Luminosity function of galaxies in SDSS commissioning dataOn 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…Weighing neutrinos with galaxy surveysImproving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic PeakImproving Cosmological Distance Measurements by Reconstruction of the Ba…Mid-infrared selection of active galaxiesThe DESI Experiment, a whitepaper for Snowmass 2013A 2 per cent distance to $z$=0.35 by reconstructing baryon acoustic oscillations - I. Methods and application to the Sloan Digital Sky SurveyA 2 per cent distance to $z$=0.35 by reconstructing baryon acoustic oscillat…Probing dark energy with baryonic acoustic oscillations from future large galaxy redshift surveysProbing dark energy with baryonic acoustic oscillations from future large gal…Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRSPower spectra for cold dark matter and its variantsObservational Probes of Cosmic AccelerationBaryonic features in the matter transfer function19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average199520002005201020152020202505001000150020002500