Current optical interferometers are affected by unknown turbulent phases on each telescope. In the field of radio-interferometry, the self-calibration technique is a powerful tool to process interferometric data with missing phase information. This paper intends to revisit the application of self-calibration to Optical Long Baseline Interferometry (OLBI). We cast rigorously the OLBI data processing problem into the self-calibration framework and demonstrate the efficiency of the method on real astronomical OLBI dataset.
@article{arxiv.0812.1178,
title = {A self-calibration approach for optical long baseline interferometry imaging},
author = {Serge Meimon and Laurent M. Mugnier and Guy Le Besnerais},
journal= {arXiv preprint arXiv:0812.1178},
year = {2009}
}