Presentation + Paper
26 August 2022 SPICA-FT: the new fringe tracker of the CHARA array
Author Affiliations +
Abstract
SPICA-FT is part of the CHARA/SPICA instrument which combines a visible 6T fibered instrument (SPICAVIS) with a H-band 6T fringe sensor. SPICA-FT is a pairwise ABCD integrated optics combiner. The chip is installed in the MIRC-X instrument. The MIRC-X spectrograph could be fed either by the classical 6T fibered combiner or by the SPICA-FT integrated optics combiner. SPICA-FT also integrates a dedicated fringe tracking software, called the opd-controller communicating with the main delay line through a dedicated channel. We present the design of the integrated optics chip, its implementation in MIRC-X and the software architecture of the group-delay and phase-delay control loops. The final integrated optics chip and the software have been fully characterized in the laboratory. First on-sky tests of the integrated optics combiner began in 2020. We continue the on-sky tests of the whole system (combiner + software) in Spring and Summer 2022. We present the main results, and we deduce the preliminary performance of SPICA-FT.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Cyril Pannetier, Philippe Bério, Denis Mourard, Sylvain Rousseau, Fatmé Allouche, Julien Dejonghe, Christophe Bailet, Daniel Lecron, Frédéric Cassaing, Jean-Baptiste Le Bouquin, Karine Perraut, John Monnier, Narsireddy Anugu, and Theo ten Brummelaar "SPICA-FT: the new fringe tracker of the CHARA array", Proc. SPIE 12183, Optical and Infrared Interferometry and Imaging VIII, 1218309 (26 August 2022); https://doi.org/10.1117/12.2628897
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KEYWORDS
Telescopes

Signal to noise ratio

Optical fibers

Integrated optics

Spectrographs

Manufacturing

Phase shifts

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