Fig. 10.
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Synthetic (solid lines) over observed (points) LCs (left plots) and RVs (right plots) for HM Pup (top panels), V632 Sco (middle panels), and TT Vel (bottom panels). Some LCs were vertically shifted for scaling reasons. The fit on the out-of-primary eclipse points of the B filter was re-scaled and plotted allowing for better viewing.
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