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Found 5 papers, 1 papers with code
Prediction of soft proton intensities in the near-Earth space using machine learning
The average correlation between the observed and predicted data is about 56%, which is reasonable in light of the complex dynamics of fast-moving energetic protons in the magnetosphere.
Joint Suzaku and Chandra observations of the MKW4 galaxy group out to the virial radius
We measure an enclosed baryon fraction of 11% at R$_{200}$, remarkably smaller than the cosmic baryon fraction of 15%.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena
Analysis of the unconcentrated background of the EPIC-pn camera on board XMM-Newton
Through this relationship we quantify the contribution of cosmic ray interactions to the pn unconcentrated background and we find a second source which contributes to the pn unconcentrated background for a significant fraction (30%-70%), that does not vary with time and is roughly isotropic.
Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
Discovering the most elusive radio relic in the sky: Diffuse Shock Acceleration caught in the act?
The case of acceleration is challenged by the low predicted efficiency of low-Mach number merger shocks, unable to explain the power observed in most radio relics.
High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics
Atacama Compact Array Measurements of the Molecular Mass in the NGC 5044 Cooling Flow Group
This indicates that the two giant molecular clouds seen in absorption are most likely within the sphere of influence of the supermassive black hole.
Astrophysics of Galaxies
