Fig. 6.
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Deconvolved EF(E) spectra of IXPE (I, Q, U) and NuSTAR of Cyg X-2 (upper panel) and GX 9+9 (lower panel) with the best-fit model reported in Table 2 superposed and residuals between data and the model in units of σ. The greater rolling angle of Cyg X-2 makes visible the U component of the bldisk spectrum in the IXPE detector reference frame.
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