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Fig. 4.
The 6 spectra fitted in this work. We used a doubly absorbed NTHCOMP continuum model plus 2 Gaussian emission lines according to Table 4. Observation #74 was split onto 3 time periods: #74a (eclipse), #74b (egress), and #74c (out-of-eclipse). Orbital phases (ϕ) are indicated in each panel.
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