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Cited article:

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A Spatially Resolved Study of Hard X-Ray Emission in Kepler’s Supernova Remnant: Indications of Different Regimes of Particle Acceleration

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Characterization of the Gamma-ray Emission from the Kepler Supernova Remnant with Fermi-LAT

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Efficiencies of Magnetic Field Amplification and Electron Acceleration in Young Supernova Remnants: Global Averages and Kepler’s Supernova Remnant

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Magnetic field estimates from the X-ray synchrotron emitting rims of the 30 Dor C superbubble and the implications for the nature of 30 Dor C’s TeV emission

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Spatio-temporal evolution of the non-resonant instability in shock precursors of young supernova remnants

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Transport of relativistic electrons at shocks in shell-type supernova remnants: diffusive and superdiffusive regimes

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A SPATIALLY RESOLVED STUDY OF THE SYNCHROTRON EMISSION AND TITANIUM IN TYCHO’S SUPERNOVA REMNANT USINGNuSTAR

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ENERGY DEPENDENCE OF SYNCHROTRON X-RAY RIMS IN TYCHO’S SUPERNOVA REMNANT

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MAGNETIC FIELD AMPLIFICATION IN THE THIN X-RAY RIMS OF SN 1006

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THREE-DIMENSIONAL SIMULATIONS OF THE NON-THERMAL BROADBAND EMISSION FROM YOUNG SUPERNOVA REMNANTS INCLUDING EFFICIENT PARTICLE ACCELERATION

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