Showing 21–40 of 47 results
/ Date/ Name
Jul 21, 2023Polarimetry and Astrometry of NIR Flares as Event Horizon Scale, Dynamical Probes for the Mass of Sgr A*Jul 25, 2018Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black holeOct 9, 2020Direct confirmation of the radial-velocity planet $β$ Pic cSep 22, 2021The mass of Beta Pictoris c from Beta Pictoris b orbital motionJun 15, 2021GRAVITY K-band spectroscopy of HD 206893 B: brown dwarf or exoplanetAug 9, 2022Direct discovery of the inner exoplanet in the HD206893 system. Evidence for deuterium burning in a planetary-mass companionNov 1, 2019The GRAVITY Young Stellar Object survey -- I. Probing the disks of Herbig Ae/Be stars in terrestrial orbitsMay 5, 2017First Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope InterferometerAug 8, 2016Making SPIFFI SPIFFIER: Upgrade of the SPIFFI instrument for use in ERIS and performance analysis from re-commissioningMay 12, 2023GMP-selected dual and lensed AGNs: selection function and classification based on near-IR colors and resolved spectra from VLT/ERIS, KECK/OSIRIS, and LBT/LUCIJan 28, 2021Improved GRAVITY astrometric accuracy from modeling of optical aberrationsJun 29, 2023Using the motion of S2 to constrain scalar clouds around SgrA*Dec 10, 2019Peering into the formation history of beta Pictoris b with VLTI/GRAVITY long baseline interferometryJan 11, 2021Constraining the Nature of the PDS 70 Protoplanets with VLTI/GRAVITYJan 18, 2021The ExoGRAVITY project: using single mode interferometry to characterize exoplanetsNov 11, 2020The GRAVITY Young Stellar Object survey IV. The CO overtone emission in 51 Oph at sub-au scalesJan 31, 2018Methods for multiple telescope beam imaging and guiding in the near infraredMay 5, 2017Sub-milliarcsecond Optical Interferometry of the HMXB BP Cru with VLTI/GRAVITYJun 1, 2022First Light for GRAVITY Wide: Large Separation Fringe Tracking for the Very Large Telescope InterferometerMay 7, 2010Far-infrared properties of submillimeter and optically faint radio galaxies