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Eclipsing post-common envelope binaries from the Catalina surveys

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Figure

Table 1. Identified eclipsing systems. The newly discovered systems are shown in bold and their parameters are taken fromscopically in SDSS J0745+2631, and SDSS J1307+2156 contains a featureless DC white dwarf, hence these systems have no parametersinformat
Figure 1. Phase-folded CSS light curves of the newly identified eclipsing PCEBs.
Figure 2. SDSS spectra of the newly identified eclipsing PCEBs. The hydrogen Balmer lines are indicated by red lines (absorptionfeatures are from the white dwarf, emission features indicate an active or irradiated main-sequence star) and the Na i lines are indicatedby the green lines (absorption from the main-sequence star).
Figure 3. Distribution of quasars (light gray dots), stars (darksystems, we identify 29 eclipsing PCEBs of which 17 were pre-viously known (magenta dots) and 12 are new discoveries (reddots)
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