Fig. 5.
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Total PA (upper panel), PD (middle panel), and normalized intensity (lower panel) of the BL as a function of the viewing angle with seed photons at the base of the slab (Case 1) for an optical depth of 2τ0 = 5, spin frequency of νbl = 500 Hz, and two values of the BL latitude. The PA is measured with respect to the projection on the sky of the NS spin axis.
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