Presentation
13 December 2020 GRAVITY+: towards faint science, all sky milli arcsecond optical interferometric imaging
Author Affiliations +
Abstract
GRAVITY and the VLTI have transformed optical interferometry with ground-breaking results on the Galactic Center, Active Galactic Nuclei, and Exoplanets. With modest upgrades to GRAVITY+, the Paranal Observatory will open up the extragalactic sky for milli-arcsec resolution interferometric imaging, and give access to galactic targets as faint as 22 mag. GRAVITY+ will measure the black hole masses of active galactic nuclei across cosmic times, establish whether globular clusters harbor intermediate-mass black holes, and obtain high-quality exoplanet spectra and orbits. The straightforward upgrade consists of implementing off-axis fringe tracking, an improved throughput, and laser-guide star adaptive optics for all 8m telescopes and can be divided up into several phases. Most of the upgrades will be beneficial to all VLTI instruments. Here we present a few selected science cases and outline the project, which could be implemented within a few years.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stefan Gillessen "GRAVITY+: towards faint science, all sky milli arcsecond optical interferometric imaging", Proc. SPIE 11446, Optical and Infrared Interferometry and Imaging VII, 114460Z (13 December 2020); https://doi.org/10.1117/12.2562557
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KEYWORDS
Interferometry

Optical imaging

Active galactic nuclei

Exoplanets

Adaptive optics

Image resolution

Laser optics

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