Phase Referencing in Optical Interferometry
Mercedes E. Filho, Paulo Garcia, Gilles Duvert, Gaspard Duchene, Eric, Thiebaut, John Young, Olivier Absil, Jean-Phillipe Berger, Thomas Beckert,, Sebastian Hoenig, Dieter Schertl, Gerd Weigelt, Leonardo Testi, Eric Tatuli,, Virginie Borkowski, Michael de Becker, Jean Surdej

TL;DR
This paper explores the potential of phase referencing techniques in optical interferometry, using simulations and radio algorithms to improve high-resolution imaging beyond traditional closure phase methods.
Contribution
It demonstrates the feasibility of applying radio interferometry image reconstruction algorithms to optical data for enhanced imaging capabilities.
Findings
Successful image reconstruction in simulated optical data
Achieved 4 milliarcsecond resolution in K band images
Phase referencing shows promise for future optical interferometry
Abstract
One of the aims of next generation optical interferometric instrumentation is to be able to make use of information contained in the visibility phase to construct high dynamic range images. Radio and optical interferometry are at the two extremes of phase corruption by the atmosphere. While in radio it is possible to obtain calibrated phases for the science objects, in the optical this is currently not possible. Instead, optical interferometry has relied on closure phase techniques to produce images. Such techniques allow only to achieve modest dynamic ranges. However, with high contrast objects, for faint targets or when structure detail is needed, phase referencing techniques as used in radio interferometry, should theoretically achieve higher dynamic ranges for the same number of telescopes. Our approach is not to provide evidence either for or against the hypothesis that phase…
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