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Cited article:

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Outflow–Cloud Interaction as the Possible Origin of the Peculiar Radio Emission in the Tidal Disruption Event AT2018cqh

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A Partitioned Global Address Space Parallel Code for Numerical Modeling in Special Relativistic Hydrodynamics

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The remarkable microquasar S26: A super-Eddington PeVatron

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Adaptive Mesh Refinement with a “Garden” Technique for Solving the Special Relativistic Hydrodynamics Equations

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Upper limit on the coronal cosmic ray energy budget in Seyfert galaxies

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Using Piecewise Parabolic Reconstruction of Physical Variables in the Rusanov Solver. I. The Special Relativistic Hydrodynamics Equations

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