2010
DOI: 10.1117/12.856698
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The fringe detection laser metrology for the GRAVITY interferometer at the VLTI

Abstract: Interferometric measurements of optical path length differences of stars over large baselines can deliver extremely accurate astrometric data. The interferometer GRAVITY will simultaneously measure two objects in the field of view of the Very Large Telescope Interferometer (VLTI) of the European Southern Observatory (ESO) and determine their angular separation to a precision of 10 µas in only 5 minutes. To perform the astrometric measurement with such a high accuracy, the differential path length through the V… Show more

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Cited by 9 publications
(5 citation statements)
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References 10 publications
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“…In the slow-rotation approximation, one can reexpand the ζ-expanded metric of Eq. (7). The Kerr metric, for example, can be expanded in the familiar form…”
Section: Rotating Black Hole Solutionsmentioning
confidence: 99%
See 1 more Smart Citation
“…In the slow-rotation approximation, one can reexpand the ζ-expanded metric of Eq. (7). The Kerr metric, for example, can be expanded in the familiar form…”
Section: Rotating Black Hole Solutionsmentioning
confidence: 99%
“…Due to past technological limitations, mass was the only property that could be inferred from the observation of the orbital motion of nearby stars. The next generation of upgrades to telescopes used in very long baseline interferometers will allow for the determination of other important properties, such as the location of the event horizon and the innermost stable circular orbit (ISCO) from observations of the black hole (BH) shadow and accretion disk, respectively [3][4][5][6][7][8][9][10][11][12][13][14]. One other property that we wish to infer is whether Sgr A* satisfies the so-called Kerr hypothesis, i.e.…”
Section: Introductionmentioning
confidence: 99%
“…The Fourier transform method has been widely used in optical interferometry for demodulation of carrier fringes. [5,6,7] However, this method has the drawback of poor ability to localize the signal properties, which also lead to a suppression of higher frequencies of the measurement. To overcome this shortcoming, Kemao Qian et al [8] proposed a new method for reconstructing phase and amplitude from a single carrier frequency interferogram by using Windowed Fourier transform method and combining it with localization of filtering.…”
Section: Reconstruction Methodsmentioning
confidence: 98%
“…the separation of 2 objects, at a level of the order of 10 micro-arcseconds on sky. To achieve this, a sophisticated metrology system has been designed [5]. The basic idea of the metrology system is to sample the optical path of the incoming telescope beams as complete as possible, with a precision of about 1nm (rms differential optical path difference of 2 objects separated by about 1" on sky).…”
Section: Introductionmentioning
confidence: 99%
“…The basic working principle is the same as described for the preliminary design 4,5 . A laser beam is injected backwards at the two beam combiners, in a way that one of the two paths includes a phase shifter by which the relative delay between the two beams can be adjusted.…”
Section: Working Principlementioning
confidence: 99%