A two-band approach to n$\lambda$ phase error corrections with LBTI's PHASECam
E. R. Maier, P. M. Hinz, D. Defr\`ere, S. Ertel, and E. Downey

TL;DR
This paper introduces a two-band phase correction method for LBTI's PHASECam, improving the robustness of phase error correction by comparing H and K band telemetry to prevent fringe jumps during interferometry.
Contribution
The paper presents a novel multi-wavelength approach for phase error correction that enhances the reliability of fringe jump detection and correction in LBTI's PHASECam system.
Findings
Effective detection of fringe jumps using H and K band comparison
Improved phase correction stability during fast, large phase variations
Potential for automated, robust phase control in advanced interferometry modes
Abstract
PHASECam is the Large Binocular Telescope Interferometer's (LBTI) phase sensor, a near-infrared camera which is used to measure tip/tilt and phase variations between the two AO-corrected apertures of the Large Binocular Telescope (LBT). Tip/tilt and phase sensing are currently performed in the H (1.65 m) and K (2.2 m) bands at 1 kHz, and the K band phase telemetry is used to send tip/tilt and Optical Path Difference (OPD) corrections to the system. However, phase variations outside the range [-, ] are not sensed, and thus are not fully corrected during closed-loop operation. PHASECam's phase unwrapping algorithm, which attempts to mitigate this issue, still occasionally fails in the case of fast, large phase variations. This can cause a fringe jump, in which case the unwrapped phase will be incorrect by a wavelength or more. This can currently be manually corrected…
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