GRAVITY: observing the universe in motion

By F. Eisenhauer, G. Perrin, W. Brandner, C. Straubmeier, K. Perraut, A. Amorim, M. Schöller, S. Gillessen, Pierre Kervella, M. Benisty and 77 more. 2011

146 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/eb0465dba8bdac8333ddcdf5d7a108dc3e3f1a6b

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Citations in the corpus

First light for GRAVITY: Phase referencing optical interferometry for the Very Large Telescope Interferometer (2017, background): “…regions of active galactic nuclei (AGN), image circumstellar disks in young stellar objects and see their jets evolve in real time, and detect and characterize exo-planets especially around low mass stars and binaries – in short we will “Observe the Universe in motion” (Eisenhauer et al. 2011).”
Stellar Dynamics and Stellar Phenomena Near a Massive Black Hole (2017, methodology): “Already operating are the VLT/GRAVITY interferometer (Eisenhauer et al. 2011), which is looking for low-mass stars on relativistic orbits around Sgr A? with unprecedented astrometric precision, and large scale transient source surveys (Pan-STARRS (Kaiser et al. 2002), PTF/ZTF (Law et al. 2009;…”
THE ASTRALUX LARGE M-DWARF MULTIPLICITY SURVEY (2012, background): “The sample should also be useful for future planet-search projects, such as high-contrast imaging surveys, which typically seek to avoid close binaries as targets, or astrometry surveys with planned instruments such as GRAVITY (Eisenhauer et al. 2011), for which close binarity is highly desirable fo”
Detection of orbital motions near the last stable circular orbit of the massive black hole SgrA* (2018, methodology): “We have been observing the Galactic centre and SgrA* with the GRAVITY instrument (Gravity Collaboration et al. 2017, 2018; Eisenhauer et al. 2011, 2008; Paumard et al. 2008) during multiple campaigns in 2017/20181, with the aim of testing general relativity (GR) and the massive black hole paradigm…”
The nearby eclipsing stellar system δ Velorum - IV. Differential astrometry with VLT/NACO at the 100 microarcsecond level (2013, unknown): “The next generation interferometric instrumentation at near-infrared wavelengths, particularly the GRAVITY (Gillessen et al. 2010; Eisenhauer et al. 2011; Vincent et al. 2011) and ASTRA (Woillez et al. 2012; Stone et al. 2012) instruments, are expected to overcome this limit, down to an accuracy of…”