Table 3: Photon luminosity for a neutron star with $T_{\rm core}=10^6$ K.
B[G] L[erg/s] L[erg/s]
  Isothermal Crustal
  crust field
1012 $6.72\times 10^{28}$ $5.64\times 10^{28}$
1012.5 $9.08\times 10^{28}$ $5.42\times 10^{28}$
1013 $1.38\times 10^{29}$ $5.18\times 10^{28}$


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