Publication data of Shelton, Robin L.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20002005201020152020202502004006008001000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications20002005201020152020202501224364860012345
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestSupernova remnants in the Magellanic Clouds. 4. X-ray emission from the largest SNR in the LMCSupernova remnants in the Magellanic Clouds. 4. X-ray emission from the lar…The Galactic Halo's O VI Resonance Line IntensitySimulations of supernova remnants in diffuse media. 2. Three remnants and their x-ray emissionSimulations of supernova remnants in diffuse media. 2. Three remnants and …Surprisingly little O VI emission arises in the Local BubbleSimulations of High-Velocity Clouds. I. Hydrodynamics and High-Velocity High IonsSimulations of High-Velocity Clouds. I. Hydrodynamics and High-Velocity High…An XMM-Newton Observation of the Local Bubble Using a Shadowing Filament in the Southern Galactic HemisphereAn XMM-Newton Observation of the Local Bubble Using a Shadowing Filamen…An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l=120 and l=240An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII …The Trouble with the Local BubbleMultifidelity emulation for the matter power spectrum using Gaussian processesMultifidelity emulation for the matter power spectrum using Gaussian proces…Numerical Study of Turbulent Mixing Layers with Non-Equilibrium Ionization CalculationsNumerical Study of Turbulent Mixing Layers with Non-Equilibrium Ionization …Chandra observations and models of the mixed-morphology supernova remnant W44: Global trendsChandra observations and models of the mixed-morphology supernova remn…An XMM-Newton Survey of the Soft X-ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission IntensitiesAn XMM-Newton Survey of the Soft X-ray Background. II. An All-Sky Catalog o…Comparing Suzaku and XMM-Newton Observations of the Soft X-ray Background: Evidence for Solar Wind Charge Exchange EmissionComparing Suzaku and XMM-Newton Observations of the Soft X-ray Backgrou…A Survey of OVI absorption in the local interstellar mediumThe Origin of the Hot Gas in the Galactic Halo: Confronting Models with XMM-Newton ObservationsThe Origin of the Hot Gas in the Galactic Halo: Confronting Models with XMM-…The X-ray structure and spectrum of the pulsar wind nebula surrounding PSR B1853+01 in W44The X-ray structure and spectrum of the pulsar wind nebula surrounding PS…The ionization of the local interstellar medium, as revealed by fuse observations of n, o and ar toward white dwarf starsThe ionization of the local interstellar medium, as revealed by fuse observatio…An XMM-Newton Survey of the Soft X-ray Background. III. The Galactic Halo X-ray EmissionAn XMM-Newton Survey of the Soft X-ray Background. III. The Galactic Halo X…Modeling w44 as a supernova remnant in a density gradient, with a partially formed dense shell and thermal conduction in the hot interiorModeling w44 as a supernova remnant in a density gradient, with a partially …20002005201020152020202502004006008001000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Supernova remnants in the Magellanic Clouds. 4. X-ray emission from the largest SNR in the LMCSupernova remnants in the Magellanic Clouds. 4. X-ray emission from the lar…The Galactic Halo's O VI Resonance Line IntensitySimulations of supernova remnants in diffuse media. 2. Three remnants and their x-ray emissionSimulations of supernova remnants in diffuse media. 2. Three remnants and …Surprisingly little O VI emission arises in the Local BubbleSimulations of High-Velocity Clouds. I. Hydrodynamics and High-Velocity High IonsSimulations of High-Velocity Clouds. I. Hydrodynamics and High-Velocity High…An XMM-Newton Observation of the Local Bubble Using a Shadowing Filament in the Southern Galactic HemisphereAn XMM-Newton Observation of the Local Bubble Using a Shadowing Filamen…An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l=120 and l=240An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII …The Trouble with the Local BubbleMultifidelity emulation for the matter power spectrum using Gaussian processesMultifidelity emulation for the matter power spectrum using Gaussian proces…Numerical Study of Turbulent Mixing Layers with Non-Equilibrium Ionization CalculationsNumerical Study of Turbulent Mixing Layers with Non-Equilibrium Ionization …Chandra observations and models of the mixed-morphology supernova remnant W44: Global trendsChandra observations and models of the mixed-morphology supernova remn…An XMM-Newton Survey of the Soft X-ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission IntensitiesAn XMM-Newton Survey of the Soft X-ray Background. II. An All-Sky Catalog o…Comparing Suzaku and XMM-Newton Observations of the Soft X-ray Background: Evidence for Solar Wind Charge Exchange EmissionComparing Suzaku and XMM-Newton Observations of the Soft X-ray Backgrou…A Survey of OVI absorption in the local interstellar mediumThe Origin of the Hot Gas in the Galactic Halo: Confronting Models with XMM-Newton ObservationsThe Origin of the Hot Gas in the Galactic Halo: Confronting Models with XMM-…The X-ray structure and spectrum of the pulsar wind nebula surrounding PSR B1853+01 in W44The X-ray structure and spectrum of the pulsar wind nebula surrounding PS…The ionization of the local interstellar medium, as revealed by fuse observations of n, o and ar toward white dwarf starsThe ionization of the local interstellar medium, as revealed by fuse observatio…An XMM-Newton Survey of the Soft X-ray Background. III. The Galactic Halo X-ray EmissionAn XMM-Newton Survey of the Soft X-ray Background. III. The Galactic Halo X…Modeling w44 as a supernova remnant in a density gradient, with a partially formed dense shell and thermal conduction in the hot interiorModeling w44 as a supernova remnant in a density gradient, with a partially …2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025020406080