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Fig. 2


Broadening functions close to the principal phases (counted from the primary eclipse, with the secondary occurring at phase 0.436): 0.142 (maximum separation of the components), 0.441 (end of the secondary eclipse), 0.800 (maximum separation of the components), and 0.997 (beginning of the primary eclipse). The radial velocity system is barycentric. Full mosaic showing all BFs including best fits is shown in Fig. 6.

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