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The metrology system of the VLTI instrument GRAVITY

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arxiv 1608.04888 v1 pith:E42WVELJ submitted 2016-08-17 astro-ph.IM

The metrology system of the VLTI instrument GRAVITY

classification astro-ph.IM
keywords metrologysystemdopdsgravityinstrumentthree-beamvltiamplifiers
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The VLTI instrument GRAVITY combines the beams from four telescopes and provides phase-referenced imaging as well as precision-astrometry of order 10 microarcseconds by observing two celestial objects in dual-field mode. Their angular separation can be determined from their differential OPD (dOPD) when the internal dOPDs in the interferometer are known. Here, we present the general overview of the novel metrology system which performs these measurements. The metrology consists of a three-beam laser system and a homodyne detection scheme for three-beam interference using phase-shifting interferometry in combination with lock-in amplifiers. Via this approach the metrology system measures dOPDs on a nanometer-level.

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