Figure 1. X-Ray lightcurve plotted against orbital phase. The pulsar is eclipsed by the companion between orbital phases 0.8 and 0.2.
Figure 2. Delays in pulse arrival times fitted to a sinusoid. Errors in orbital parameters are for 90% confidence in one interesting parameter.
Figure 3. Orbital variation of pulse profile.
Figure 4. Pulse-phase averaged spectrum fitted to a model with narrow Gaussians at 6.4, 6.56, 6.67, and 6.93 keV.
Figure 5. Iron line intensities versus pulse phase.
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