Fringe Tracker for the VLTI Spectro-Imager
L. Corcione, D. Bonino, D. F. Busher, M. Gai, S. Ligori, D. Loreggia,, G. Masssone, J. S. Young

TL;DR
This paper presents the design and implementation of a fringe tracker for the VLTI Spectro Imager, enabling high-resolution, stable interferometric imaging with multiple telescopes by compensating atmospheric disturbances.
Contribution
It introduces a scalable fringe tracker design for VSI that improves phase stability and is adaptable to different telescope configurations.
Findings
Designed a scalable fringe tracker for 4, 6, or 8 telescopes.
Achieves stable observations down to K=13 magnitude.
Enhances interferometric imaging resolution and efficiency.
Abstract
The implementation of the simultaneous combination of several telescopes (from four to eight) available at Very Large Telescope Interferometer (VLTI) will allow the new generation interferometric instrumentation to achieve interferometric image synthesis with unprecedented resolution and efficiency. The VLTI Spectro Imager (VSI) is the proposed second-generation near-infrared multi-beam instrument for the Very Large Telescope Interferometer, featuring three band operations (J, H and K), high angular resolutions (down to 1.1 milliarcsecond) and high spectral resolutions. VSI will be equipped with its own internal Fringe Tracker (FT), which will measure and compensate the atmospheric perturbations to the relative beam phase, and in turn will provide stable and prolonged observing conditions down to the magnitude K=13 for the scientific combiner. In its baseline configuration, VSI FT is…
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