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Eclipsing binaries observed with the WIRE satellite I, Discovery and photometric analysis of the new bright A0 IV eclipsing binary ψ Centauri

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Figure

Fig. 1. Phased light curve of ψ Cen for a period of 38.81252 days. Data points from wire (black dots), smei (grey + symbols), and hipparcos(grey circles) are shown.
Table 1. wireeach source have been normalised so the outside-eclipse magnitudeis zero
Table 2. Photometric parameters and uncertainties foring ψ Cen found us- jktebop and Monte Carlo simulations
Fig. 3. Best-fitting parameter values for the 6000 synthetic light curvescreated for the Monte Carlo analysis.
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