Table 1: Photon luminosities for a neutron star with $T_{\rm core}=10^8$ K. The differences between isothermal crust and star-centered field are negligible but significant between them and crustal fields larger than 10¹³ G.
B[G] L[erg/s] L[erg/s] L[erg/s]

Isothermal Star-centered Crustal

crust field field

10¹² $3.32\times 10^{32}$ $3.28\times 10^{32}$ $3.26\times 10^{32}$

10^12.5 $3.70\times 10^{32}$ $3.66\times 10^{32}$ $3.36\times 10^{32}$

10¹³ $4.40\times 10^{32}$ $4.34\times 10^{32}$ $2.50\times 10^{32}$

**Table 1:** Photon luminosities for a neutron star with $T_{\rm core}=10^8$ K. The differences between isothermal crust and star-centered field are negligible but significant between them and crustal fields larger than 10¹³ G.
B[G]	L[erg/s]	L[erg/s]	L[erg/s]
	Isothermal	Star-centered	Crustal
	crust	field	field
10¹²	$3.32\times 10^{32}$	$3.28\times 10^{32}$	$3.26\times 10^{32}$
10^12.5	$3.70\times 10^{32}$	$3.66\times 10^{32}$	$3.36\times 10^{32}$
10¹³	$4.40\times 10^{32}$	$4.34\times 10^{32}$	$2.50\times 10^{32}$

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