Publication data of Bahcall, Neta A.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1970198019902000201020200250050007500100001250015000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications197019801990200020102020030609012015002.557.51012.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion197019801990200020102020010203040506070
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe mass function of clusters of galaxiesConstraining omega with cluster evolutionThe C4 clustering algorithm: Clusters of galaxies in the Sloan Digital Sky SurveyThe C4 clustering algorithm: Clusters of galaxies in the Sloan Digital Sky Surv…The Baryonic Acoustic Feature and Large-Scale Clustering in the SDSS LRG SampleThe Baryonic Acoustic Feature and Large-Scale Clustering in the SDSS LRG S…Detection of cosmic magnification with the Sloan Digital Sky SurveyThe Dependence on environment of the color - magnitude relation of galaxiesClustering of High Redshift (Z >= 2.9) Quasars from the Sloan Digital Sky SurveyClustering of High Redshift (Z >= 2.9) Quasars from the Sloan Digital Sky Su…Cosmic homogeneity demonstrated with luminous red galaxiesThe Galaxy - mass correlation function measured from weak lensing in the SDSSThe Galaxy - mass correlation function measured from weak lensing in the S…The shape of the SDSS DR5 galaxy power spectrumPresent status of the theoretical predictions for the Cl-36 solar neutrino experimentPresent status of the theoretical predictions for the Cl-36 solar neutrino expe…A map of the universeThe Spatial correlation function of RICH clusters of galaxiesThe Most massive distant clusters: Determining omega and sigma_8Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological ImplicationsCorrelation of CMB with large-scale structure: I. ISW Tomography and Cosmol…The Linear theory power spectrum from the Lyman-alpha forest in the Sloan Digital Sky SurveyThe Linear theory power spectrum from the Lyman-alpha forest in the Sloan …Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and LuminosityGalaxy Clustering in the Completed SDSS Redshift Survey: The Dependence …The Galaxy luminosity function and luminosity density at redshift z = 0.1The Cosmic triangle: Assessing the state of the universe1970198019902000201020200250050007500100001250015000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The mass function of clusters of galaxiesConstraining omega with cluster evolutionThe C4 clustering algorithm: Clusters of galaxies in the Sloan Digital Sky SurveyThe C4 clustering algorithm: Clusters of galaxies in the Sloan Digital Sky Surv…The Baryonic Acoustic Feature and Large-Scale Clustering in the SDSS LRG SampleThe Baryonic Acoustic Feature and Large-Scale Clustering in the SDSS LRG S…Detection of cosmic magnification with the Sloan Digital Sky SurveyThe Dependence on environment of the color - magnitude relation of galaxiesClustering of High Redshift (Z >= 2.9) Quasars from the Sloan Digital Sky SurveyClustering of High Redshift (Z >= 2.9) Quasars from the Sloan Digital Sky Su…Cosmic homogeneity demonstrated with luminous red galaxiesThe Galaxy - mass correlation function measured from weak lensing in the SDSSThe Galaxy - mass correlation function measured from weak lensing in the S…The shape of the SDSS DR5 galaxy power spectrumPresent status of the theoretical predictions for the Cl-36 solar neutrino experimentPresent status of the theoretical predictions for the Cl-36 solar neutrino expe…A map of the universeThe Spatial correlation function of RICH clusters of galaxiesThe Most massive distant clusters: Determining omega and sigma_8Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological ImplicationsCorrelation of CMB with large-scale structure: I. ISW Tomography and Cosmol…The Linear theory power spectrum from the Lyman-alpha forest in the Sloan Digital Sky SurveyThe Linear theory power spectrum from the Lyman-alpha forest in the Sloan …Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and LuminosityGalaxy Clustering in the Completed SDSS Redshift Survey: The Dependence …The Galaxy luminosity function and luminosity density at redshift z = 0.1The Cosmic triangle: Assessing the state of the universe1970198019902000201020200255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1970198019902000201020200200400600800