Monte Carlo population synthesis of young massive star clusters matches the combined H.E.S.S. Galactic Plane Survey and LHAASO first catalog for five parameter combinations, strongly disfavoring Bohm diffusion.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Abeona is confirmed as a faint ~30 arcmin bilateral radio SNR shell with synchrotron polarization, flux density 1.5 Jy, and a spatially coincident 5.7-sigma GeV gamma-ray source.
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Young Massive Star Clusters as TeV Emitters: Constraints from H.E.S.S. and LHAASO
Monte Carlo population synthesis of young massive star clusters matches the combined H.E.S.S. Galactic Plane Survey and LHAASO first catalog for five parameter combinations, strongly disfavoring Bohm diffusion.
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Radio detection of supernova remnant G310.7-5.4 with $\gamma$-ray counterpart: Abeona SNR
Abeona is confirmed as a faint ~30 arcmin bilateral radio SNR shell with synchrotron polarization, flux density 1.5 Jy, and a spatially coincident 5.7-sigma GeV gamma-ray source.