Publication data of Liu, Adrian: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20082010201220142016201820202022202401000200030004000
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-citaion200820102012201420162018202020222024010203040
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestA fast method for power spectrum and foreground analysis for 21 cm cosmologyA fast method for power spectrum and foreground analysis for 21 cm cosmol…Pulsar timing can constrain primordial black holes in the LIGO mass windowWill point sources spoil 21 cm tomography?The impact of modelling errors on interferometer calibration for 21 cm power spectraThe impact of modelling errors on interferometer calibration for 21 cm power…Multi-redshift limits on the 21cm power spectrum from PAPERPrecision Calibration of Radio Interferometers Using Redundant BaselinesDeep learning from 21-cm tomography of the Cosmic Dawn and ReionizationHow well can we measure and understand foregrounds with 21 cm experiments?How well can we measure and understand foregrounds with 21 cm experime…Emulating Simulations of Cosmic Dawn for 21 cm Power Spectrum Constraints on Cosmology, Reionization, and X-Ray HeatingEmulating Simulations of Cosmic Dawn for 21 cm Power Spectrum Constrain…An Improved Method for 21cm Foreground RemovalEliminating the optical depth nuisance from the CMB with 21 cm cosmologyAn improved model of diffuse galactic radio emission from 10 MHz to 5 THzOvercoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array dataOvercoming real-world obstacles in 21 cm power spectrum estimation: A me…A Method for 21cm Power Spectrum Estimation in the Presence of ForegroundsA Method for 21cm Power Spectrum Estimation in the Presence of Foregroun…Epoch of reionization window. II. Statistical methods for foreground wedge reductionEpoch of reionization window. II. Statistical methods for foreground wedge re…Data Analysis for Precision 21 cm CosmologyEpoch of reionization window. I. Mathematical formalismNew Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IGM at z=7.7New Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IG…What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of ReionizationWhat Next-Generation 21 cm Power Spectrum Measurements Can Teach Us …20082010201220142016201820202022202401000200030004000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)A fast method for power spectrum and foreground analysis for 21 cm cosmologyA fast method for power spectrum and foreground analysis for 21 cm cosmol…Pulsar timing can constrain primordial black holes in the LIGO mass windowWill point sources spoil 21 cm tomography?The impact of modelling errors on interferometer calibration for 21 cm power spectraThe impact of modelling errors on interferometer calibration for 21 cm power…Multi-redshift limits on the 21cm power spectrum from PAPERPrecision Calibration of Radio Interferometers Using Redundant BaselinesDeep learning from 21-cm tomography of the Cosmic Dawn and ReionizationHow well can we measure and understand foregrounds with 21 cm experiments?How well can we measure and understand foregrounds with 21 cm experime…Emulating Simulations of Cosmic Dawn for 21 cm Power Spectrum Constraints on Cosmology, Reionization, and X-Ray HeatingEmulating Simulations of Cosmic Dawn for 21 cm Power Spectrum Constrain…An Improved Method for 21cm Foreground RemovalEliminating the optical depth nuisance from the CMB with 21 cm cosmologyAn improved model of diffuse galactic radio emission from 10 MHz to 5 THzOvercoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array dataOvercoming real-world obstacles in 21 cm power spectrum estimation: A me…A Method for 21cm Power Spectrum Estimation in the Presence of ForegroundsA Method for 21cm Power Spectrum Estimation in the Presence of Foregroun…Epoch of reionization window. II. Statistical methods for foreground wedge reductionEpoch of reionization window. II. Statistical methods for foreground wedge re…Data Analysis for Precision 21 cm CosmologyEpoch of reionization window. I. Mathematical formalismNew Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IGM at z=7.7New Limits on 21cm EoR From PAPER-32 Consistent with an X-Ray Heated IG…What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of ReionizationWhat Next-Generation 21 cm Power Spectrum Measurements Can Teach Us …2008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2008201020122014201620182020202220240100200300400500600700