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14 new eclipsing white dwarf plus main-sequence binaries from the SDSS and Catalina surveys

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Figure

Table 1. Journal of photometric observations. The eclipse of the white dwarf occurs at phase 0, 1 etc.
Figure 1. BFOSC Spectrum of one of our newly identified PCEB systems(SDSS J2241+2536, gray line) with the best fit template spectrum over-plotted (black line)
Figure 2. Phase-folded CSS light curves of the 14 newly identified eclipsing PCEBs. SDSS J234035.84+185555.0 is a marginal detection and requires somefollow-up data to confirm the eclipse.
Figure 3. Follow-up light curves of 11 of the newly identified eclipsing systems, see Table 1 for the telescope+instrument+filter used for each observation
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