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Table 8

Computed flux (F) and heating rate () L1 norms for the stellar component in test 3.

L1, F L1,

ϵmax = 5 × 10-3 0.004 0.035
ϵmax = 10-4 0.001 0.005
ϵmax = 5 × 10-3, UW 0.006 0.045
Mean 0.094 0.432

Notes. The correlated-k method is seen to introduce errors of about 4%.

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