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S-polarized KR (A) and RK emission spectra (B) of S101 and corresponding RhB emission (C and D, respectively) at different observation angles. 532 nm KR, P-polarized light illumination at 43° is used. The dashed blue lines in the top panels show the S101 emission from PVA layer on glass, and in the bottom panel is the corresponding RhB emission.
