Publication data of Murphy, Michael T.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19851990199520002005201020152020202502000400060008000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19851990199520002005201020152020202504080120160200048121620
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestImpact of instrumental systematic errors on fine-structure constant measurements with quasar spectraImpact of instrumental systematic errors on fine-structure constant measure…The thermal history of the intergalactic medium down to redshift z = 1.5: a new curvature measurementThe thermal history of the intergalactic medium down to redshift z = 1.5: a …The UVES Large Program for Testing Fundamental Physics II: Constraints on a Change in {mu} Towards Quasar HE 0027-1836The UVES Large Program for Testing Fundamental Physics II: Constraints on a…Possible evidence for a variable fine structure constant from QSO absorption lines: Systematic errorsPossible evidence for a variable fine structure constant from QSO absorption …Stringent null constraint on cosmological evolution of the proton-to-electron mass ratioStringent null constraint on cosmological evolution of the proton-to-electron …The UVES Large Program for Testing Fundamental Physics: I Bounds on a change in alpha towards quasar HE 2217-2818The UVES Large Program for Testing Fundamental Physics: I Bounds on a cha…Improved constraints on possible variation of physical constants from H I 21cm and molecular QSO absorption linesImproved constraints on possible variation of physical constants from H I 21c…The neutral hydrogen cosmological mass density at z = 5Strong Limit on a Variable Proton-to-Electron Mass Ratio from Molecules in the Distant UniverseStrong Limit on a Variable Proton-to-Electron Mass Ratio from Molecules in th…Further constraints on variation of the fine structure constant from alkali doublet QSO absorption linesFurther constraints on variation of the fine structure constant from alkali dou…Revision of VLT/UVES constraints on a varying fine-structure constantThe Giant Gemini GMOS survey of $z_{em}$ > 4.4 quasars – I. Measuring the mean free path across cosmic timeThe Giant Gemini GMOS survey of $z_{em}$ > 4.4 quasars – I. Measuring th…Deuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: Converging on Omega_baryonsDeuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: …Spatial variation in the fine-structure constant -- new results from VLT/UVESPossible evidence for a variable fine structure constant from QSO absorption lines: Motivations, analysis and resultsPossible evidence for a variable fine structure constant from QSO absorption …Precision measures of the primordial abundance of deuteriumIndications of a spatial variation of the fine structure constantFurther evidence for a variable fine-structure constant from Keck/HIRES QSO absorption spectraFurther evidence for a variable fine-structure constant from Keck/HIRES QSO …Further evidence for cosmological evolution of the fine structure constant19851990199520002005201020152020202502000400060008000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Impact of instrumental systematic errors on fine-structure constant measurements with quasar spectraImpact of instrumental systematic errors on fine-structure constant measure…The thermal history of the intergalactic medium down to redshift z = 1.5: a new curvature measurementThe thermal history of the intergalactic medium down to redshift z = 1.5: a …The UVES Large Program for Testing Fundamental Physics II: Constraints on a Change in {mu} Towards Quasar HE 0027-1836The UVES Large Program for Testing Fundamental Physics II: Constraints on a…Possible evidence for a variable fine structure constant from QSO absorption lines: Systematic errorsPossible evidence for a variable fine structure constant from QSO absorption …Stringent null constraint on cosmological evolution of the proton-to-electron mass ratioStringent null constraint on cosmological evolution of the proton-to-electron …The UVES Large Program for Testing Fundamental Physics: I Bounds on a change in alpha towards quasar HE 2217-2818The UVES Large Program for Testing Fundamental Physics: I Bounds on a cha…Improved constraints on possible variation of physical constants from H I 21cm and molecular QSO absorption linesImproved constraints on possible variation of physical constants from H I 21c…The neutral hydrogen cosmological mass density at z = 5Strong Limit on a Variable Proton-to-Electron Mass Ratio from Molecules in the Distant UniverseStrong Limit on a Variable Proton-to-Electron Mass Ratio from Molecules in th…Further constraints on variation of the fine structure constant from alkali doublet QSO absorption linesFurther constraints on variation of the fine structure constant from alkali dou…Revision of VLT/UVES constraints on a varying fine-structure constantThe Giant Gemini GMOS survey of $z_{em}$ > 4.4 quasars – I. Measuring the mean free path across cosmic timeThe Giant Gemini GMOS survey of $z_{em}$ > 4.4 quasars – I. Measuring th…Deuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: Converging on Omega_baryonsDeuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: …Spatial variation in the fine-structure constant -- new results from VLT/UVESPossible evidence for a variable fine structure constant from QSO absorption lines: Motivations, analysis and resultsPossible evidence for a variable fine structure constant from QSO absorption …Precision measures of the primordial abundance of deuteriumIndications of a spatial variation of the fine structure constantFurther evidence for a variable fine-structure constant from Keck/HIRES QSO absorption spectraFurther evidence for a variable fine-structure constant from Keck/HIRES QSO …Further evidence for cosmological evolution of the fine structure constant1985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1985199019952000200520102015202020250100200300400500600