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The Very Large Telescope, being build by the European Southern Observatory, has an
interferoetric node in which the light of the four 8 eter aperture telescopes, and of
a number of smaller telescopes, will be combined coherently to give iilliarcsecond level
angular resolution at optical wavelengths on very faint objects. This paper describes
current plans to impleMent this mode.
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Jacques Maurice Beckers, "Interferometry with ESO's Very Large Telescope," Proc. SPIE 1319, Optics in Complex Systems, (1 July 1990); https://doi.org/10.1117/12.34794