Publication data of Kim, Jaisenung: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20062008201020122014201620182020202220240200400600800
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200620082010201220142016201820202022202408162432400246810
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestDirect reconstruction of spherical harmonics from interferometer observations of the CMB polarizationDirect reconstruction of spherical harmonics from interferometer observation…How accurately can we measure the hydrogen 2S->1S transition rate from the cosmological data?How accurately can we measure the hydrogen 2S->1S transition rate from t…The primordial 'f_NL' non-Gaussianity, and perturbations beyond the present horizonThe primordial 'f_NL' non-Gaussianity, and perturbations beyond the present …Parametric tension between even and odd multipole data of WMAP power spectrum: unaccounted contamination or missing parameters?Parametric tension between even and odd multipole data of WMAP power sp…The Accelerated Recombination, and the ACBAR and the WMAP dataSub-femtosecond synchronization of microwave oscillators with mode-locked Er-fiber lasersSub-femtosecond synchronization of microwave oscillators with mode-locked …Removing the ISW-lensing bias from the local-form primordial non-Gaussianity estimationRemoving the ISW-lensing bias from the local-form primordial non-Gaussianit…The Gauss-Legendre Sky Pixelization for the CMB polarization (GLESP-pol). Errors due to pixelization of the CMB skyThe Gauss-Legendre Sky Pixelization for the CMB polarization (GLESP-pol). Err…CMB polarization map derived from the WMAP 5 year data through Harmonic Internal Linear CombinationCMB polarization map derived from the WMAP 5 year data through Harmonic…Harmonic in-painting of CMB sky by constrained Gaussian realizationHow to make a clean separation between CMB E and B modes with proper foreground maskingHow to make a clean separation between CMB E and B modes with proper fo…Alfvén turbulence in the WMAP 5 year data and a forecast for the PLANCKLack of angular correlation and odd-parity preference in CMB dataCMB E/B decomposition of incomplete sky: a pixel space approachUnderstanding the WMAP Cold Spot mysteryCMB map derived from the WMAP data through harmonic internal linear combinationCMB map derived from the WMAP data through harmonic internal linear com…Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?Anomalous parity asymmetry of WMAP power spectrum data at low multpole…Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipolesAnomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe p…Limits on anisotropic inflation from the Planck data20062008201020122014201620182020202220240200400600800
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Direct reconstruction of spherical harmonics from interferometer observations of the CMB polarizationDirect reconstruction of spherical harmonics from interferometer observation…How accurately can we measure the hydrogen 2S->1S transition rate from the cosmological data?How accurately can we measure the hydrogen 2S->1S transition rate from t…The primordial 'f_NL' non-Gaussianity, and perturbations beyond the present horizonThe primordial 'f_NL' non-Gaussianity, and perturbations beyond the present …Parametric tension between even and odd multipole data of WMAP power spectrum: unaccounted contamination or missing parameters?Parametric tension between even and odd multipole data of WMAP power sp…The Accelerated Recombination, and the ACBAR and the WMAP dataSub-femtosecond synchronization of microwave oscillators with mode-locked Er-fiber lasersSub-femtosecond synchronization of microwave oscillators with mode-locked …Removing the ISW-lensing bias from the local-form primordial non-Gaussianity estimationRemoving the ISW-lensing bias from the local-form primordial non-Gaussianit…The Gauss-Legendre Sky Pixelization for the CMB polarization (GLESP-pol). Errors due to pixelization of the CMB skyThe Gauss-Legendre Sky Pixelization for the CMB polarization (GLESP-pol). Err…CMB polarization map derived from the WMAP 5 year data through Harmonic Internal Linear CombinationCMB polarization map derived from the WMAP 5 year data through Harmonic…Harmonic in-painting of CMB sky by constrained Gaussian realizationHow to make a clean separation between CMB E and B modes with proper foreground maskingHow to make a clean separation between CMB E and B modes with proper fo…Alfvén turbulence in the WMAP 5 year data and a forecast for the PLANCKLack of angular correlation and odd-parity preference in CMB dataCMB E/B decomposition of incomplete sky: a pixel space approachUnderstanding the WMAP Cold Spot mysteryCMB map derived from the WMAP data through harmonic internal linear combinationCMB map derived from the WMAP data through harmonic internal linear com…Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?Anomalous parity asymmetry of WMAP power spectrum data at low multpole…Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipolesAnomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe p…Limits on anisotropic inflation from the Planck data20062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2006200820102012201420162018202020222024020406080