Resolving the hot dust around HD69830 and η Corvi with MIDI and VISIR

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Table 4:

Measuring the significance of the dip in visibility of $\eta$ Corvi at 10-11.5 $\mu$ m.
Baseline	Visibility
name	8-9 $\mu$ m	10-11.5 $\mu$ m	Ratio
A	1.016 $\pm$ 0.005	0.892 $\pm$ 0.004	0.877 $\pm$ 0.026
B	0.910 $\pm$ 0.003	0.818 $\pm$ 0.003	0.899 $\pm$ 0.027
D1	0.841 $\pm$ 0.003	0.739 $\pm$ 0.003	0.879 $\pm$ 0.026
D2	0.922 $\pm$ 0.003	0.801 $\pm$ 0.004	0.868 $\pm$ 0.026
$V_{\rm {res}}$	0.915	0.784	0.857

A description of the calculation of the visibilities and errors
is given in the caption to Table 3.

Source LaTeX | All tables | In the text

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