Simulations show CTAO southern array observations at multi-TeV energies, combined with X-ray data, can likely constrain magnetic field and electron distributions in PWNe such as HESS J1813-178 and MSH 15-52, with gains from better resolution offset by photon statistics limits.
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High-Resolution Measurements with the CTAO Southern Array: The Case for Pulsar Wind Nebulae
Simulations show CTAO southern array observations at multi-TeV energies, combined with X-ray data, can likely constrain magnetic field and electron distributions in PWNe such as HESS J1813-178 and MSH 15-52, with gains from better resolution offset by photon statistics limits.