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Cause of CHARA MIRC-X visibility discrepancies on E2 baseline

Determine the definitive cause of the intermittent discrepant uncalibrated visibilities observed on CHARA Array MIRC-X baselines including telescope E2 during the April 2021 observations of Polaris, discriminating between potential sources such as E2 delay line cart vibrations at very low tracking speeds and telescope oscillations while pointing near the pole.

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Background

During CHARA/MIRC-X observations, the authors observed occasional offsets and excess scatter in uncalibrated visibilities, especially on baselines involving telescope E2 in April 2021. These anomalies appeared between different calibrators and sometimes within a single target data set, often after a brief pause to realign starlight into the fibers.

Despite inspection of the transfer functions and rejection of clearly discrepant data, the root cause remained unidentified. The authors suggest possible instrumental or mechanical origins, including delay line cart vibrations or telescope oscillations near the pole, but emphasize that the definitive cause has not been established.

References

We could not find a definitive cause for the discrepant observations; it could be related to vibrations in the E2 delay line cart while tracking at very slow speeds in the north or telescope oscillations while pointing at the pole.

The Orbit and Dynamical Mass of Polaris: Observations with the CHARA Array (2407.09641 - Evans et al., 12 Jul 2024) in Section 2, Interferometric observations and data reduction (around Fig. 2)