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20132019
most citedDetection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole

947 citations · 2.1k across the 21 of their papers we have counts for

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Showing 2014Show all

6 papers · 1 filter

astro-ph.IM2014★ 21 cited

The fiber coupler and beam stabilization system of the GRAVITY interferometer

O. Pfuhl, M. Haug, F. Eisenhauer +20

We present the installed and fully operational beam stabilization and fiber injection subsystem feeding the 2nd generation VLTI instrument GRAVITY. The interferometer GRAVITY requi…

astro-ph.IM2014

Alternative approach to precision narrow-angle astrometry for Antarctic long baseline interferometry

Y. Kok, M. J. Ireland, A. C. Rizzuto +4

The conventional approach to high-precision narrow-angle astrometry using a long baseline interferometer is to directly measure the fringe packet separation of a target and a nearb…

astro-ph.IM2014★ 1 cited

The GRAVITY metrology system: modeling a metrology in optical fibers

N. Blind, H. Huber, F. Eisenhauer +20

GRAVITY is the second generation VLT Interferometer (VLTI) instrument for high-precision narrow-angle astrometry and phase-referenced interferometric imaging. The laser metrology s…

astro-ph.IM2014★ 13 cited

GRAVITY: the Calibration Unit

N. Blind, F. Eisenhauer, M. Haug +19

We present in this paper the design and characterisation of a new sub-system of the VLTI 2nd generation instrument GRAVITY: the Calibration Unit. The Calibration Unit provides all…

astro-ph.IM2014

The interferometric baselines and GRAVITY astrometric error budget

S. Lacour, F. Eisenhauer, S. Gillessen +9

GRAVITY is a new generation beam combination instrument for the VLTI. Its goal is to achieve microarsecond astrometric accuracy between objects separated by a few arcsec. This $10^…

astro-ph.IM2014★ 37 cited

Reaching micro-arcsecond astrometry with long baseline optical interferometry; application to the GRAVITY instrument

S. Lacour, F. Eisenhauer, S. Gillessen +10

A basic principle of long baseline interferometry is that an optical path difference (OPD) directly translates into an astrometric measurement. In the simplest case, the OPD is equ…