Publication data of Bharadwaj, Somnath: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1995200020052010201520202025010002000300040005000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250408012016020003691215
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025010203040
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe Size of the longest filaments in the universeThe effect of non-Gaussianity on error predictions for the Epoch of Reionization (EoR) 21-cm power spectrumThe effect of non-Gaussianity on error predictions for the Epoch of Reionizatio…Estimation of Cosmological Parameters from HI Observations of Post-reionization EpochEstimation of Cosmological Parameters from HI Observations of Post-reionizati…Statistics of the epoch of reionization (EoR) 21-cm signal – II. The evolution of the power-spectrum error-covarianceStatistics of the epoch of reionization (EoR) 21-cm signal – II. The evolution o…The Evolution of correlation functions in the Zel'dovich approximation and its implications for the validity of perturbation theoryThe Evolution of correlation functions in the Zel'dovich approximation and its…Probing non-Gaussian features in the HI distribution at the epoch of reionizationProbing non-Gaussian features in the HI distribution at the epoch of reionizati…Improved foreground removal in GMRT 610 MHz observations towards redshifted 21-cm tomographyImproved foreground removal in GMRT 610 MHz observations towards redshif…Modeling galaxy halos using dark matter with pressureThe scale of homogeneity of the galaxy distribution in SDSS DR6On the use of seminumerical simulations in predicting the 21-cm signal from the epoch of reionizationOn the use of seminumerical simulations in predicting the 21-cm signal from…Characterizing Foreground for redshifted 21-cm radiation: 150 MHz GMRT observationsCharacterizing Foreground for redshifted 21-cm radiation: 150 MHz GMRT ob…Foregrounds for redshifted 21 cm studies of reionization: GMRT 153 MHz observationsForegrounds for redshifted 21 cm studies of reionization: GMRT 153 MHz obs…Quantifying the non-Gaussianity in the EoR 21-cm signal through bispectrumTesting homogeneity on large scales in the Sloan Digital Sky Survey Data Release OneTesting homogeneity on large scales in the Sloan Digital Sky Survey Data Rel…The multi-frequency angular power spectrum of the epoch of reionization 21 cm signalThe multi-frequency angular power spectrum of the epoch of reionization 21 …Using HI to probe large scale structures at z ~ 3HI Fluctuations at Large Redshifts. 1. Visibility correlationOn using visibility correlations to probe the HI distribution from the dark ages to the present epoch. 1. Formalism and the expected signalOn using visibility correlations to probe the HI distribution from the dark age…The CMBR fluctuations from HI perturbations prior to reionization1995200020052010201520202025010002000300040005000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The Size of the longest filaments in the universeThe effect of non-Gaussianity on error predictions for the Epoch of Reionization (EoR) 21-cm power spectrumThe effect of non-Gaussianity on error predictions for the Epoch of Reionizatio…Estimation of Cosmological Parameters from HI Observations of Post-reionization EpochEstimation of Cosmological Parameters from HI Observations of Post-reionizati…Statistics of the epoch of reionization (EoR) 21-cm signal – II. The evolution of the power-spectrum error-covarianceStatistics of the epoch of reionization (EoR) 21-cm signal – II. The evolution o…The Evolution of correlation functions in the Zel'dovich approximation and its implications for the validity of perturbation theoryThe Evolution of correlation functions in the Zel'dovich approximation and its…Probing non-Gaussian features in the HI distribution at the epoch of reionizationProbing non-Gaussian features in the HI distribution at the epoch of reionizati…Improved foreground removal in GMRT 610 MHz observations towards redshifted 21-cm tomographyImproved foreground removal in GMRT 610 MHz observations towards redshif…Modeling galaxy halos using dark matter with pressureThe scale of homogeneity of the galaxy distribution in SDSS DR6On the use of seminumerical simulations in predicting the 21-cm signal from the epoch of reionizationOn the use of seminumerical simulations in predicting the 21-cm signal from…Characterizing Foreground for redshifted 21-cm radiation: 150 MHz GMRT observationsCharacterizing Foreground for redshifted 21-cm radiation: 150 MHz GMRT ob…Foregrounds for redshifted 21 cm studies of reionization: GMRT 153 MHz observationsForegrounds for redshifted 21 cm studies of reionization: GMRT 153 MHz obs…Quantifying the non-Gaussianity in the EoR 21-cm signal through bispectrumTesting homogeneity on large scales in the Sloan Digital Sky Survey Data Release OneTesting homogeneity on large scales in the Sloan Digital Sky Survey Data Rel…The multi-frequency angular power spectrum of the epoch of reionization 21 cm signalThe multi-frequency angular power spectrum of the epoch of reionization 21 …Using HI to probe large scale structures at z ~ 3HI Fluctuations at Large Redshifts. 1. Visibility correlationOn using visibility correlations to probe the HI distribution from the dark ages to the present epoch. 1. Formalism and the expected signalOn using visibility correlations to probe the HI distribution from the dark age…The CMBR fluctuations from HI perturbations prior to reionization19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250100200300400500600