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Table 1

Best-fit power law indices for the diffuse stellar light inside of R< 0.5 pc.

Data Γin

Ks, wide field 0.32
Br γ 0.23
Ks deep field 0.25
H 0.29
Ks S13 0.26
IB227 0.19

Notes. All formal uncertainties are 0.01 after having been rescaled to a reduced χ2 = 1, i.e. we are dominated by systematics.

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