Unlocking the radio- γ spectrum of the pulsar wind nebula around PSR J1124–5916 in SNR G292.0+1.8

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Table 4

Models parameters.

Parameters	Values
Electrons spectrum

E_min	1 GeV
E_max	500 TeV
γ₁	1.024
γ₂	∼2.9
γ_cool	∼3.9
$E_{b_{inj}, j}$ ${E_{{{\rm{b}}_{{\rm{inj}}}},{\rm{j}}}}$	∼40GeV
$E_{b_{cool}, e}$ ${{\rm{E}}_{{{\rm{b}}_{{\rm{cool}}}},{\rm{e}}}}$	∼25TeV

Model 1

FIR energy density	0.2 eV cm^-3
NIR energy density	0.1 eV cm^-3
Magnetic field	∼15 μG
We(>1GeV)	∼5.3 × 10⁴⁸ erg

Model 2

FIR energy density	1.0 eV cm^-3
NIR energy density	0.7 eV cm^-3
Magnetic field	∼25 μG
We(>1GeV)	∼2.2 × 10⁴⁸ erg

Notes. Details of model parameters presented in the SED Fig. 7. Model 1 and 2 use the same electron spectrum shape.

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