Fig. 1
SuperWASP light curves for 12 eclipsing PCEBs phase-folded at periods given in Table 1, with binned mean curves overplotted in red (online only). The x axes indicate phase; the y axes SuperWASP flux in arbitrary units (pseudo-V magnitudes are given by 15 − 2.5log (flux). A typical point’s uncertainty is shown in the bottom right of each panel.
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