Abstract
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 a real astronomical OLBI data set.
© 2008 Optical Society of America
Full Article | PDF ArticleMore Like This
Christopher L. Carilli, Bojan Nikolic, and Nithyanandan Thyagarajan
J. Opt. Soc. Am. A 39(12) 2214-2223 (2022)
Antony Schutz, André Ferrari, David Mary, Ferréol Soulez, Éric Thiébaut, and Martin Vannier
J. Opt. Soc. Am. A 31(11) 2334-2345 (2014)
Éric Thiébaut and John Young
J. Opt. Soc. Am. A 34(6) 904-923 (2017)