Fig. 10.
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Predicted γ-photon count maps and smoothed significance maps for energies exceeding 25 TeV in the multiple traveling PWNe modeling attempt. Panels (a)–(b) show the γ-photon count map and significance map calculated with the model including PSR J0218+4232 and a hypothetical pulsar. The blue arrow indicates the proper motion direction of the hypothetical pulsar. Panels (c)–(d) show the γ-photon count map and significance map calculated with the model including two hypothetical pulsars. Here, the γ-ray emission from PSR J0218+4232 has been excluded.
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