Publication data of Pen, Ue-Li: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion199520002005201020152020202502500500075001000012500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1995200020052010201520202025060120180240300048121620
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1995200020052010201520202025010203040506070
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestLow-amplitude clustering in low-redshift 21-cm intensity maps cross-correlated with 2dF galaxy densitiesLow-amplitude clustering in low-redshift 21-cm intensity maps cross-correlat…Self-Regulated ReionizationNon-Cosmological FRBs from Young Supernova Remnant PulsarsThe GMRT Epoch of Reionization experiment: A New upper limit on the neutral hydrogen power spectrum at z~8.6The GMRT Epoch of Reionization experiment: A New upper limit on the neutra…All-Sky Interferometry with Spherical Harmonic Transit TelescopesSimulating cosmic reionization: How large a volume is large enough?Cosmic shear from galaxy spinsSimulating cosmic reionization at large scales. 2. the 21-cm emission features and statistical signalsSimulating cosmic reionization at large scales. 2. the 21-cm emission feature…Discriminating weak lensing from intrinsic spin correlations using the curl-gradient decompositionDiscriminating weak lensing from intrinsic spin correlations using the curl-gr…Determination of z~0.8 neutral hydrogen fluctuations using the 21 cm intensity mapping auto-correlationDetermination of z~0.8 neutral hydrogen fluctuations using the 21 cm inten…Spin induced galaxy alignments and their implications for weak lensing measurementsSpin induced galaxy alignments and their implications for weak lensing meas…Power spectra in global defect theories of cosmic structure formationA refined foreground-corrected limit on the HI power spectrum at z=8.6 from the GMRT Epoch of Reionization ExperimentA refined foreground-corrected limit on the HI power spectrum at z=8.6 fro…Cosmological parameters from Cosmic Background Imager observations and comparisons with BOOMERANG, DASI, and MAXIMACosmological parameters from Cosmic Background Imager observations and …Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlationSimulating cosmic reionization at large scales. 1. the geometry of reionizationHydrogen 21-cm Intensity Mapping at redshift 0.8Dense magnetized plasma associated with a fast radio burstBaryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy199520002005201020152020202502500500075001000012500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Low-amplitude clustering in low-redshift 21-cm intensity maps cross-correlated with 2dF galaxy densitiesLow-amplitude clustering in low-redshift 21-cm intensity maps cross-correlat…Self-Regulated ReionizationNon-Cosmological FRBs from Young Supernova Remnant PulsarsThe GMRT Epoch of Reionization experiment: A New upper limit on the neutral hydrogen power spectrum at z~8.6The GMRT Epoch of Reionization experiment: A New upper limit on the neutra…All-Sky Interferometry with Spherical Harmonic Transit TelescopesSimulating cosmic reionization: How large a volume is large enough?Cosmic shear from galaxy spinsSimulating cosmic reionization at large scales. 2. the 21-cm emission features and statistical signalsSimulating cosmic reionization at large scales. 2. the 21-cm emission feature…Discriminating weak lensing from intrinsic spin correlations using the curl-gradient decompositionDiscriminating weak lensing from intrinsic spin correlations using the curl-gr…Determination of z~0.8 neutral hydrogen fluctuations using the 21 cm intensity mapping auto-correlationDetermination of z~0.8 neutral hydrogen fluctuations using the 21 cm inten…Spin induced galaxy alignments and their implications for weak lensing measurementsSpin induced galaxy alignments and their implications for weak lensing meas…Power spectra in global defect theories of cosmic structure formationA refined foreground-corrected limit on the HI power spectrum at z=8.6 from the GMRT Epoch of Reionization ExperimentA refined foreground-corrected limit on the HI power spectrum at z=8.6 fro…Cosmological parameters from Cosmic Background Imager observations and comparisons with BOOMERANG, DASI, and MAXIMACosmological parameters from Cosmic Background Imager observations and …Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlationSimulating cosmic reionization at large scales. 1. the geometry of reionizationHydrogen 21-cm Intensity Mapping at redshift 0.8Dense magnetized plasma associated with a fast radio burstBaryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1995200020052010201520202025025050075010001250