HIGHLIGHTS
SUMMARY
The combination of large area and low background allows Athena to characterize the spectral properties of faint X-ray sources, important e_g for constraining leptonic vs hadronic models in neutrino and VHE sources, or tracking the spectral evolution of afterglows of GRBs and GW mergers. If the path of the jet is blocked by a sufficiently large amount of material, consisting e_g of debris from the merger or NS wind, there will be jets that fail to emerge. The amount of debris in the polar region traversed by the jet is currently not known . . .
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