GRAVITY: The adaptive optics assisted, two object beam combiner for the VLTI
arXiv:astro-ph/0607372 · doi:10.1117/12.671431
Abstract
We present the adaptive optics assisted, near-infrared VLTI instrument - GRAVITY - for precision narrow-angle astrometry and interferometric phase referenced imaging of faint objects. Precision astrometry and phase-referenced interferometric imaging will realize the most advanced vision of optical/infrared interferometry with the VLT. Our most ambitious science goal is to study motions within a few times the event horizon size of the Galactic Center massive black hole and to test General Relativity in its strong field limit. We define the science reference cases for GRAVITY and derive the top level requirements for GRAVITY. The installation of the instrument at the VLTI is planned for 2012.
9 pages, Advances in Stellar Interferometry, SPIE Proc. Vol. 6268, 626811 (2006)
Cited by in corpus (10)
- Asteroseismology and Interferometry
- Detection of IMBHs with ground-based gravitational wave observatories: A biography of a binary of black holes, from birth to death
- Investigating the retention of intermediate-mass black holes in star clusters using N-body simulations
- The gravitational capture of compact objects by massive black holes
- An evolving hot spot orbiting around Sgr A*
- Estimating the phase in ground-based interferometry: performance comparison between single-mode and multimode schemes
- Polarized radiative transfer modeling of warped and clumpy dusty tori
- Disentangling Confused Stars at the Galactic Center with Long Baseline Infrared Interferometry
- The Galactic Center
- Fake plunges are very eccentric real EMRIs in disguise ... they dominate the rates and are blissfully ignorant of angular momentum barriers