Fig. 14.
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Four closure phases obtained on a bright star, IRAS 10153-5540, as a function of the wavelength. The blue(+), red(⋆), green(▿), and orange(×) lines represent the CP for the different BCD position calibrated by VV396 Cen. The black(•) line represents the CP corrected by the BCDs only. The purple(⋄) line represents the CP of IRAS 10153-5540 calibrated by VV396 Cen and corrected by the BCDs.
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