The GRAVITY metrology system: modeling a metrology in optical fibers
N. Blind, H. Huber, F. Eisenhauer, J. Weber, S. Gillessen, M. Lippa,, L. Burtscher, O. Hans, M. Haug, F. Haussmann, S. Huber, A. Janssen, S., Kellner, Y. Kok, T. Ott, O. Pfuhl, E. Sturm, E. Wieprecht, A. Amorim, W., Brandner, G. Perrin, K. Perraut, C. Straubmeier

TL;DR
This paper presents a semi-empirical model of the GRAVITY fibered metrology system to understand and improve its stability for high-precision astrometry, addressing non-common path errors affecting performance.
Contribution
It introduces a combined theoretical and experimental modeling approach to identify error sources and suggest design modifications for enhanced metrology stability.
Findings
Model successfully reproduces test measurements
Identifies key components contributing to errors
Proposes design improvements for 1 nm stability
Abstract
GRAVITY is the second generation VLT Interferometer (VLTI) instrument for high-precision narrow-angle astrometry and phase-referenced interferometric imaging. The laser metrology system of GRAVITY is at the heart of its astrometric mode, which must measure the distance of 2 stars with a precision of 10 micro-arcseconds. This means the metrology has to measure the optical path difference between the two beam combiners of GRAVITY to a level of 5 nm. The metrology design presents some non-common paths that have consequently to be stable at a level of 1 nm. Otherwise they would impact the performance of GRAVITY. The various tests we made in the past on the prototype give us hints on the components responsible for this error, and on their respective contribution to the total error. It is however difficult to assess their exact origin from only OPD measurements, and therefore, to propose a…
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