Publication data of Padmanabhan, Hamsa: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion200820102012201420162018202020222024025050075010001250
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications2008201020122014201620182020202220240122436486001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion2008201020122014201620182020202220240510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestPhoton number conserving models of H ii bubbles during reionizationCosmic Information, the Cosmological Constant and the Amplitude of primordial perturbationsCosmic Information, the Cosmological Constant and the Amplitude of primor…Non-relativistic limit of quantum field theory in inertial and non-inertial frames and the Principle of EquivalenceNon-relativistic limit of quantum field theory in inertial and non-inertial frame…Constraints on the evolution of the relationship between H i mass and halo mass in the last 12 GyrConstraints on the evolution of the relationship between H i mass and halo m…Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI ResponseModelling the cosmic neutral hydrogen from DLAs and 21 cm observationsAlleviating the Need for Exponential Evolution of JWST Galaxies in 10$^{10}$ M $_{⊙}$ Haloes at z > 10 by a Modified ΛCDM Power SpectrumAlleviating the Need for Exponential Evolution of JWST Galaxies in 10$^{10}…Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy SurveysCross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic an…A new way to test the Cosmological Principle: measuring our peculiar velocity and the large-scale anisotropy independentlyA new way to test the Cosmological Principle: measuring our peculiar velocity…Constraining the evolution of [C II] intensity through the end stages of reionizationConstraining the evolution of [C II] intensity through the end stages of reioni…Constraining a halo model for cosmological neutral hydrogenCosMIn: The Solution to the Cosmological Constant ProblemTheoretical and observational constraints on the HI intensity power spectrumJoint power spectrum and voxel intensity distribution forecast on the CO luminosity function with COMAPJoint power spectrum and voxel intensity distribution forecast on the CO lumi…Intensity Mapping as a Probe of Axion Dark MatterConstraining the CO intensity mapping power spectrum at intermediate redshiftsConstraining the CO intensity mapping power spectrum at intermediate reds…Cosmological Constant from the Emergent Gravity PerspectiveA halo model for cosmological neutral hydrogen : abundances and clustering H i abundances and clusteringA halo model for cosmological neutral hydrogen : abundances and clustering…Astrophysics and Cosmology with Line-Intensity Mapping200820102012201420162018202020222024025050075010001250
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Photon number conserving models of H ii bubbles during reionizationCosmic Information, the Cosmological Constant and the Amplitude of primordial perturbationsCosmic Information, the Cosmological Constant and the Amplitude of primor…Non-relativistic limit of quantum field theory in inertial and non-inertial frames and the Principle of EquivalenceNon-relativistic limit of quantum field theory in inertial and non-inertial frame…Constraints on the evolution of the relationship between H i mass and halo mass in the last 12 GyrConstraints on the evolution of the relationship between H i mass and halo m…Packed Ultra-wideband Mapping Array (PUMA): Astro2020 RFI ResponseModelling the cosmic neutral hydrogen from DLAs and 21 cm observationsAlleviating the Need for Exponential Evolution of JWST Galaxies in 10$^{10}$ M $_{⊙}$ Haloes at z > 10 by a Modified ΛCDM Power SpectrumAlleviating the Need for Exponential Evolution of JWST Galaxies in 10$^{10}…Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy SurveysCross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic an…A new way to test the Cosmological Principle: measuring our peculiar velocity and the large-scale anisotropy independentlyA new way to test the Cosmological Principle: measuring our peculiar velocity…Constraining the evolution of [C II] intensity through the end stages of reionizationConstraining the evolution of [C II] intensity through the end stages of reioni…Constraining a halo model for cosmological neutral hydrogenCosMIn: The Solution to the Cosmological Constant ProblemTheoretical and observational constraints on the HI intensity power spectrumJoint power spectrum and voxel intensity distribution forecast on the CO luminosity function with COMAPJoint power spectrum and voxel intensity distribution forecast on the CO lumi…Intensity Mapping as a Probe of Axion Dark MatterConstraining the CO intensity mapping power spectrum at intermediate redshiftsConstraining the CO intensity mapping power spectrum at intermediate reds…Cosmological Constant from the Emergent Gravity PerspectiveA halo model for cosmological neutral hydrogen : abundances and clustering H i abundances and clusteringA halo model for cosmological neutral hydrogen : abundances and clustering…Astrophysics and Cosmology with Line-Intensity Mapping2008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200820102012201420162018202020222024050100150200250