Fig. 4
The colour map of the goodness of fit for the lightcurves, thermal data and combined data for all possible orientations of the spin axis given in ecliptic coordinates (λ,β). The top panel shows the rms residuals between the model and observed lightcurves, the middle plot shows the reduced χ2 for the thermal data and the bottom plot shows the total χ2 (Eq. (1)).
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