Implementing multi-wavelength fringe tracking for the Large Binocular Telescope Interferometer's phase sensor, PHASECam
Erin R. Maier, Phil Hinz, Denis Defr\`ere, Paul Grenz, Elwood Downey,, Steve Ertel, Katie Morzinski, and Ewan S. Douglas

TL;DR
This paper introduces a multi-wavelength fringe jump detection and correction method for PHASECam at LBTI, enhancing the robustness of phase tracking in interferometry by comparing phase telemetry across bands.
Contribution
The paper presents a novel multi-wavelength approach for detecting and correcting fringe jumps, improving phase stability and data recovery in LBTI's fringe tracking system.
Findings
The method reliably detects fringe jumps using H- and K-band phase comparison.
It can recover a significant portion of data lost due to fringe jumps.
Archival telemetry demonstrates the method's effectiveness.
Abstract
PHASECam is the fringe tracker for the Large Binocular Telescope Interferometer (LBTI). It is a near-infrared camera which is used to measure both tip/tilt and fringe phase variations between the two adaptive optics (AO) corrected apertures of the Large Binocular Telescope (LBT). Tip/tilt and phase sensing are currently performed in the (1.65 m) and (2.2 m) bands at 1 kHz, but only the -band phase telemetry is used to send corrections to the system in order to maintain fringe coherence and visibility. However, due to the cyclic nature of the fringe phase, only the phase, modulo 360 deg, can be measured. PHASECam's phase unwrapping algorithm, which attempts to mitigate this issue, occasionally fails in the case of fast, large phase variations or low signal-to-noise ratio. This can cause a fringe jump, in which case the OPD correction will be incorrect by a…
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