Fig. 6.
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Deconvolved energy spectrum of GX 5−1. The top panels show the deconvolved NICER (1.5–10 keV), NuSTAR (3.5–45 keV for Obs. 1 and 3.5–35 keV for Obs. 2), and IBIS/ISGRI (28–50 keV) spectra simultaneous with both IXPE observations, obtained from the best-fit model in Table 4. The IXPE (2–8 keV) energy spectrum is overplotted on the frozen model. The bottom panels show the residuals between data and model in units of σ.
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