Publication data of Barnes, T.G.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1980199020002010202002004006008001000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19801990200020102020081624324001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion198019851990199520002005201020152020202502468101214
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestResolving the Azimuthal Ambiguity in Vector Magnetogram Data with the Divergence-Free Condition: Application to Discrete DataResolving the Azimuthal Ambiguity in Vector Magnetogram Data with the Div…Effects of partitioning and extrapolation on the connectivity of potential magnetic fieldsEffects of partitioning and extrapolation on the connectivity of potential mag…The Near-IR surface brightness method applied to six Cepheids in the young LMC cluster NGC 1866The Near-IR surface brightness method applied to six Cepheids in the young …The accuracy of stellar atmospheric parameter determinations: a case study with HD 32115 and HD 37594The accuracy of stellar atmospheric parameter determinations: a case study …Hidden symmetries and large N factorisation for permutation invariant matrix observablesHidden symmetries and large N factorisation for permutation invariant matri…Infrared surface brightness distances to Cepheids: A Comparison of Bayesian and linear-bisector calculationsInfrared surface brightness distances to Cepheids: A Comparison of Bayesian …Permutation invariant Gaussian two-matrix modelsDistance Scale Zero-Points from Galactic RR Lyrae Star ParallaxesCalibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique II. The effect of metallicity, and the distance to the LMCCalibrating the Cepheid Period-Luminosity relation from the infrared surface …A Bayesian analysis of the cepheid distance scaleCalibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique I. The p-factor, the Milky Way relations, and a universal K-band relationCalibrating the Cepheid Period-Luminosity relation from the infrared surface …Stellar angular diameters and visual surface brightness. 3. An improved definition of the relationshipStellar angular diameters and visual surface brightness. 3. An improved defi…Non-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejectionNon-linear force-free field modeling of a solar active region around the time o…Direct distances to Cepheids in the Large Magellanic Cloud: Evidence for a universal slope of the period-luminosity relation up to solar abundanceDirect distances to Cepheids in the Large Magellanic Cloud: Evidence for a u…Stellar angular diameters and visual surface brightness. 1. Late spectral typesA Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Coro…A new calibration of Galactic Cepheid Period-Luminosity relations from B to K bands, and a comparison to LMC PL relationsA new calibration of Galactic Cepheid Period-Luminosity relations from B to K …Magellanic Cloud Cepheids - AbundancesHubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid Variable Stars: Period-Luminosity RelationsHubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid …1980199020002010202002004006008001000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Resolving the Azimuthal Ambiguity in Vector Magnetogram Data with the Divergence-Free Condition: Application to Discrete DataResolving the Azimuthal Ambiguity in Vector Magnetogram Data with the Div…Effects of partitioning and extrapolation on the connectivity of potential magnetic fieldsEffects of partitioning and extrapolation on the connectivity of potential mag…The Near-IR surface brightness method applied to six Cepheids in the young LMC cluster NGC 1866The Near-IR surface brightness method applied to six Cepheids in the young …The accuracy of stellar atmospheric parameter determinations: a case study with HD 32115 and HD 37594The accuracy of stellar atmospheric parameter determinations: a case study …Hidden symmetries and large N factorisation for permutation invariant matrix observablesHidden symmetries and large N factorisation for permutation invariant matri…Infrared surface brightness distances to Cepheids: A Comparison of Bayesian and linear-bisector calculationsInfrared surface brightness distances to Cepheids: A Comparison of Bayesian …Permutation invariant Gaussian two-matrix modelsDistance Scale Zero-Points from Galactic RR Lyrae Star ParallaxesCalibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique II. The effect of metallicity, and the distance to the LMCCalibrating the Cepheid Period-Luminosity relation from the infrared surface …A Bayesian analysis of the cepheid distance scaleCalibrating the Cepheid Period-Luminosity relation from the infrared surface brightness technique I. The p-factor, the Milky Way relations, and a universal K-band relationCalibrating the Cepheid Period-Luminosity relation from the infrared surface …Stellar angular diameters and visual surface brightness. 3. An improved definition of the relationshipStellar angular diameters and visual surface brightness. 3. An improved defi…Non-linear force-free field modeling of a solar active region around the time of a major flare and coronal mass ejectionNon-linear force-free field modeling of a solar active region around the time o…Direct distances to Cepheids in the Large Magellanic Cloud: Evidence for a universal slope of the period-luminosity relation up to solar abundanceDirect distances to Cepheids in the Large Magellanic Cloud: Evidence for a u…Stellar angular diameters and visual surface brightness. 1. Late spectral typesA Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Coro…A new calibration of Galactic Cepheid Period-Luminosity relations from B to K bands, and a comparison to LMC PL relationsA new calibration of Galactic Cepheid Period-Luminosity relations from B to K …Magellanic Cloud Cepheids - AbundancesHubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid Variable Stars: Period-Luminosity RelationsHubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid …19801985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19801985199019952000200520102015202020250255075100125150