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      The GRAVITY fringe tracker: correlation between optical path residuals and atmospheric parameters

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          Abstract

          After the first year of observations with the GRAVITY fringe tracker, we compute correlations between the optical path residuals and atmospheric and astronomical parameters. The median residuals of the optical path residuals are 180 nm on the ATs and 270 nm on the UTs. The residuals are uncorrelated with the target magnitudes for Kmag below 5.5 on ATs (9 on UTs). The correlation with the coherence time is however extremely clear, with a drop-off in fringe tracking performance below 3 ms.

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          Author and article information

          Journal
          28 June 2018
          Article
          1806.10858
          48a3f1d2-1013-447e-834c-0191f7faf1b4

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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          Custom metadata
          submitted to SPIE Astronomical Telescopes & Instrumentation 2018
          astro-ph.IM

          Instrumentation & Methods for astrophysics
          Instrumentation & Methods for astrophysics

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