Fig. 8.
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SED for the unabsorbed IR through γ-ray emission from J1741 and other well-studied middle-aged pulsars. The IR through X-ray fit parameters for B1055-52, Geminga, and B0656+14 are taken from Posselt et al. (2023), Kargaltsev et al. (2005), Mori et al. (2014), Durant et al. (2011), and Arumugasamy et al. (2018). The γ-ray fit parameters are taken from Fermi LAT 14-Year Point Source Catalog (4FGL-DR4) Abdollahi et al. (2020), Ballet et al. (2023)).
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