EAS Publications Series : Radiative Transfer and Applications to Very Large Telescopes (Ph Stee ed.), v. 18, p. 251-271, 2006. http://dx.doi.org/10.1051/eas:2006016
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In long baseline interferometry, the raw fringe contrast must be calibrated to obtain the true visibility and then those observables that can be interpreted in terms of astrophysical parameters. The selection of suitable calibration stars is crucial for obtaining the ultimate precision of interferometric instruments like the VLTI. We have...
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Thanks to their large angular dimension and brightness, red giants and supergiants are privileged targets for optical long-baseline interferometers. Sixteen red giants and supergiants have been observed with the VLTI/AMBER facility over a two-years period, at medium spectral resolution (R=1500) in the K band. The limb-darkened angular diameters...
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Interferometry for Optical Astronomy II, SPIE Conference 4838, pp. 144-151 (2003)
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