VLTI-AMBER velocity-resolved aperture-synthesis imaging of η Carinae with a spectral resolution of 12 000 - Studies of the primary star wind and innermost wind-wind collision zone

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Fig. E.1

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Comparison of the measured visibilities, differential phases, and closure phases shown in Fig. 2 (curves with error bars) with the visibilities and phases derived from the images in Fig. 4 reconstructed with the differential-phase method (crosses).

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