Laboratory characterization of Hierarchical Fringe Tracking

@misc{ligi2026laboratory,
  title = {{Laboratory characterization of Hierarchical Fringe Tracking}},
  author = {Roxanne Ligi and Stéphane Lagarde and Romain Petrov and Sylvie Robbe-Dubois and Julien Dejonghe and Fatmé Allouche and Teng Xu and Wei Wei and Massinissa Hadjara and Abdelkarim Boskri},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.05205},
  eprint = {2609.05205},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.05205},
  note = {CC BY-NC-ND 4.0},
}

TY  - UNPB
TI  - Laboratory characterization of Hierarchical Fringe Tracking
AU  - Roxanne Ligi
AU  - Stéphane Lagarde
AU  - Romain Petrov
AU  - Sylvie Robbe-Dubois
AU  - Julien Dejonghe
AU  - Fatmé Allouche
AU  - Teng Xu
AU  - Wei Wei
AU  - Massinissa Hadjara
AU  - Abdelkarim Boskri
PY  - 2026
DA  - 2026/09/28
PB  - arXiv
DO  - 10.48550/arxiv.2609.05205
UR  - https://arxiv.org/abs/2609.05205
AB  - One of the main limitations in long-baseline interferometry lies in its fringe tracking sensitivity. The challenge is therefore to maximize this sensitivity while minimizing the spreading of the signal on the detector. This is the goal at the core of the hierarchical fringe tracking (HFT) concept. We present the laboratory characterization of the 2^nd generation HFT chips operating in the near infrared (H band) for up to 4 telescopes with more linear phase and group delay estimators, allowing a strong simplification of the tracking algorithm. We show a comparison between theoretical intensity outputs for an optimized phase delay chip, and the laboratory measurements of two chips with different designs. The results do not reach the expectations but get close to them with the 10-outputs chip. Ultimately, this new chip is intended for implementation on the VLTI, CHARA or on the future Xuyi 100m-baseline Stellar Interferometer using three telescopes.
ER  -