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The goal of this work is to characterize the polarization effects of the VLTI and GRAVITY. This is needed to calibrate polarimetric observations with GRAVITY for instrumental effects and to understand the systematic error introduced to the…

GRAVITY+ is the upgrade of GRAVITY and the Very Large Telescope Interferometer (VLTI) with wide-separation fringe tracking, new adaptive optics, and laser guide stars on all four 8~m Unit Telescopes (UTs), for ever fainter, all-sky, high…

Instrumentation and Methods for Astrophysics · Physics 2022-09-14 GRAVITY+ Collaboration , : , R. Abuter , F. Allouche , A. Amorim , C. Bailet , M. Bauböck , J. -P. Berger , P. Berio , A. Bigioli , O. Boebion , M. L. Bolzer , H. Bonnet , G. Bourdarot , P. Bourget , W. Brandner , Y. Clénet , B. Courtney-Barrer , Y. Dallilar , R. Davies , D. Defrère , A. Delboulbé , F. Delplancke , R. Dembet , P. T. de Zeeuw , A. Drescher , A. Eckart , C. Édouard , F. Eisenhauer , M. Fabricius , H. Feuchtgruber , G. Finger , N. M. Förster Schreiber , E. Garcia , P. Garcia , F. Gao , E. Gendron , R. Genzel , J. P. Gil , S. Gillessen , T. Gomes , F. Gonté , C. Gouvret , P. Guajardo , S. Guieu , M. Hartl , X. Haubois , F. Haußmann , G. Heißel , Th. Henning , S. Hippler , S. Hönig , M. Horrobin , N. Hubin , E. Jacqmart , L. Jochum , L. Jocou , A. Kaufer , P. Kervella , H. Korhonen , L. Kreidberg , S. Lacour , S. Lagarde , O. Lai , V. Lapeyrère , R. Laugier , J. -B. Le Bouquin , J. Leftley , P. Léna , D. Lutz , F. Mang , A. Marcotto , D. Maurel , A. Mérand , F. Millour , N. More , H. Nowacki , M. Nowak , S. Oberti , T. Ott , L. Pallanca , T. Paumard , K. Perraut , G. Perrin , R. Petrov , O. Pfuhl , N. Pourré , S. Rabien , C. Rau , S. Robbe-Dubois , S. Rochat , M. Salman , M. Schöller , J. Schubert , N. Schuhler , J. Shangguan , T. Shimizu , S. Scheithauer , A. Sevin , F. Soulez , A. Spang , E. Stadler , J. Stadler , C. Straubmeier , E. Sturm , L. J. Tacconi , K. R. W. Tristram , F. Vincent , S. von Fellenberg , S. Uysal , F. Widmann , E. Wieprecht , E. Wiezorrek , J. Woillez , S. Yazici , A. Young , G. Zins

We present design results of the 2nd generation VLTI instrument GRAVITY beam stabilization and light injection subsystems. Designed to deliver micro-arcsecond astrometry, GRAVITY requires an unprecedented stability of the VLTI optical…

Instrumentation and Methods for Astrophysics · Physics 2012-12-21 O. Pfuhl , M. Haug , F. Eisenhauer , D. Penka , A. Amorim , S. Kellner , S. Gillessen , T. Ott , E. Wieprecht , E. Sturm , F. Haussmann , M. Lippa

We present significantly improved proper motion measurements of the Milky Way's central stellar cluster. These improvements are made possible by refining our astrometric reference frame with a new geometric optical distortion model for the…

Astrophysics of Galaxies · Physics 2015-05-20 Sylvana Yelda , Jessica R. Lu , Andrea M. Ghez , Will Clarkson , Jay Anderson , Tuan Do , Keith Matthews

Infrared interferometry is a new frontier for precision ground based observing, with new instrumentation achieving milliarcsecond (mas) spatial resolutions for faint sources, along with astrometry on the order of 10 microarcseconds. This…

We present the second-generation VLTI instrument GRAVITY, which currently is in the preliminary design phase. GRAVITY is specifically designed to observe highly relativistic motions of matter close to the event horizon of Sgr A*, the…

We present simulations of Keck Interferometer ASTRA and VLTI GRAVITY observations of mock star fields in orbit within ~50 milliarcseconds of Sgr A*. Dual-field phase referencing techniques, as implemented on ASTRA and planned for GRAVITY,…

Astrophysics of Galaxies · Physics 2015-06-05 Jordan M. Stone , J. A. Eisner , J. D. Monnier , J. Woillez , P. Wizinowich , J. -U. Pott , A. M. Ghez

Since 2019, GRAVITY has provided direct observations of giant planets and brown dwarfs at separations of down to 95 mas from the host star. Some of these observations have provided the first direct confirmation of companions previously…

Instrumentation and Methods for Astrophysics · Physics 2024-06-07 N. Pourré , T. O. Winterhalder , J. -B. Le Bouquin , S. Lacour , A. Bidot , M. Nowak , A. -L. Maire , D. Mouillet , C. Babusiaux , J. Woillez , R. Abuter , A. Amorim , R. Asensio-Torres , W. O. Balmer , M. Benisty , J. -P. Berger , H. Beust , S. Blunt , A. Boccaletti , M. Bonnefoy , H. Bonnet , M. S. Bordoni , G. Bourdarot , W. Brandner , F. Cantalloube , P. Caselli , B. Charnay , G. Chauvin , A. Chavez , E. Choquet , V. Christiaens , Y. Clénet , V. Coudé du Foresto , A. Cridland , R. Davies , D. Defrère , R. Dembet , J. Dexter , A. Drescher , G. Duvert , A. Eckart , F. Eisenhauer , N. M. Föster Schreiber , P. Garcia , R. Garcia Lopez , E. Gendron , R. Genzel , S. Gillessen , J. H. Girard , F. Gonte , S. Grant , X. Haubois , G. Heißel , Th. Henning , S. Hinkley , S. Hippler , S. F. Hönig , M. Houllé , Z. Hubert , L. Jocou , J. Kammerer , M. Kenworthy , M. Keppler , P. Kervella , L. Kreidberg , N. T. Kurtovic , A. -M. Lagrange , V. Lapeyrère , D. Lutz , F. Mang , G. -D. Marleau , A. Mérand , F. Millour , P. Mollière , J. D. Monnier , C. Mordasini , E. Nasedkin , S. Oberti , T. Ott , G. P. L. Otten , C. Paladini , T. Paumard , K. Perraut , G. Perrin , O. Pfuhl , L. Pueyo , D. C. Ribeiro , E. Rickman , Z. Rustamkulov , J. Shangguan , T. Shimizu , D. Sing , F. Soulez , J. Stadler , T. Stolker , O. Straub , C. Straubmeier , E. Sturm , C. Sykes , L. J. Tacconi , E. F. van Dishoeck , A. Vigan , F. Vincent , S. D. von Fellenberg , J. Wang , F. Widmann , S. Yazici , the GRAVITY Collaboration , J. A. Abad , E. Aller Carpentier , J. Alonso , L. Andolfato , P. Barriga , J. -L. Beuzit , P. Bourget , R. Brast , L. Caniguante , E. Cottalorda , P. Darré , B. Delabre , A. Delboulbé , F. Delplancke-Ströbele , R. Donaldson , R. Dorn , C. Dupuy , S. Egner , G. Fischer , C. Frank , E. Fuenteseca , P. Gitton , T. Guerlet , S. Guieu , P. Gutierrez , P. Haguenauer , A. Haimerl , C. T. Heritier , S. Huber , N. Hubin , P. Jolley , J. -P. Kirchbauer , J. Kolb , J. Kosmalski , P. Krempl , M. Le Louarn , P. Lilley , B. Lopez , Y. Magnard , S. Mclay , A. Meilland , A. Meister , T. Moulin , L. Pasquini , J. Paufique , I. Percheron , L. Pettazzi , D. Phan , W. Pirani , J. Quentin , A. Rakich , R. Ridings , J. Reyes , S. Rochat , C. Schmid , N. Schuhler , P. Shchekaturov , M. Seidel , C. Soenke , E. Stadler , C. Stephan , M. Suárez , M. Todorovic , G. Valdes , C. Verinaud , G. Zins , S. Zúñiga-Fernández , the NAOMI Collaboration

Studying the orbital motion of stars around Sagittarius A* in the Galactic Center provides a unique opportunity to probe the gravitational potential near the supermassive black hole at the heart of our Galaxy. Interferometric data obtained…

Infrared interferometry has seen a revolution over the last few years. The advent of GRAVITY+ is about to enable high-contrast observations, all-sky coverage and faint science up to K=21, with the implementation on 8m-class telescope of…

Instrumentation and Methods for Astrophysics · Physics 2024-10-30 G. Bourdarot , F. Eisenhauer

One of the main endeavors of fundamental astrometry is to establish a practical realization of an inertial reference frame anchored to celestial objects whose positions are defined in the barycentric coordinates of the solar system. The…

Astrophysics · Physics 2008-11-26 Sergei M. Kopeikin , Valeri V. Makarov

The VLTI instrument GRAVITY combines the beams from four telescopes and provides phase-referenced imaging as well as precision-astrometry of order 10 microarcseconds by observing two celestial objects in dual-field mode. Their angular…

The 2nd generation VLTI instrument GRAVITY is a two-field infrared interferometer operating in the K band between 1.97 and 2.43 $\mu$m with either the four 8 m or the four 1.8 m telescopes of the Very Large Telescope (VLT). Beams collected…

GRAVITY+ improves by orders of magnitude the sensitivity, sky-coverage and contrast of the Very Large Telescope Interferometer (VLTI). A central part of this project is the development of Gravity Plus Adaptive Optics (GPAO), a dedicated…

Instrumentation and Methods for Astrophysics · Physics 2026-03-11 GRAVITY+ Collaboration , : , F. Allouche , C. Bailet , M. Benisty , A. Berdeu , J. -P. Berger , P. Berio , A. Bigioli , C. Blanchard , O. Boebion , H. Bonnet , G. Bourdarot , P. Bourget , W. Brandner , J. Brulé , P. Burgos , M. Carbillet , C. Correia , B. Courtney Barrer , S. Curaba , R. Davies , D. Defrère , A. Delboulbé , F. Delplancke , R. Dembet , A. Drescher , N. Dubost , A. Eckart , C. Édouard , F. Eisenhauer , L. Esteras Otal , M. Fabricius , H. Feuchtgruber , P. Fédou , G. Finger , N. M. Förster Schreiber , R. Frahm , E. Garcia , P. Garcia , R. Garcia Lopez , R. Genzel , J. P. Gil , S. Gillessen , T. Gomes , F. Gonté , V. Gopinath , C. Gouvret , J. Graf , P. Guajardo , S. Guieu , W. Hackenberg , M. Hartl , X. Haubois , F. Haußmann , T. Henning , P. Hibon , S. Hönig , M. Horrobin , M. Houllé , N. Hubin , I. Ibn Taieb , L. Jochum , L. Jocou , A. Jost , J. Kammerer , L. Karl , A. Kaufer , P. Kern , P. Kervella , J. Kolb , H. Korhonen , L. Kreidberg , P. Krempl , S. Lacour , S. Lagarde , O. Lai , V. Lapeyrère , R. Laugier , V. Leal , J. -B. Le Bouquin , J. Leftley , P. Léna , B. Lopez , D. Lutz , Y. Magnard , F. Mang , A. Marcotto , D. Maurel , A. Mérand , F. Millour , M. Montarges , N. More , N. Morujão , T. Moulin , H. Nowacki , M. Nowak , S. Oberti , T. Ott , L. Pallanca , F. Patru , T. Paumard , K. Perraut , G. Perrin , P. O. Petrucci , R. Petrov , O. Pfuhl , N. Pourré , S. Rabien , C. Rau , M. Riquelme , S. Robbe-Dubois , S. Rochat , M. Salman , J. Sánchez-Bermúdez , J. Schubert , J. Scigliuto , P. Shchekaturov , N. Schuhler , J. Shangguan , T. Shimizu , S. Scheithauer , C. Soenke , F. Soulez , E. Stadler , J. Stadler , C. Straubmeier , E. Sturm , M. Subroweit , C. Sykes , L. J. Tacconi , K. R. W. Tristram , S. Uysal , S. von Fellenberg , F. Widmann , E. Wieprecht , E. Wiezorrek , J. Woillez , S. Yazici , G. Zins

We systematically investigate the error sources for high-precision astrometry from adaptive optics based near-infrared imaging data. We focus on the application in the crowded stellar field in the Galactic Center. We show that at the level…

To evaluate a potential usually one analyzes trajectories of test particles. For the Galactic Center case astronomers use bright stars or photons, so there are two basic observational techniques to investigate a gravitational potential,…

General Relativity and Quantum Cosmology · Physics 2019-01-25 Alexander Zakharov

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 functions to test and calibrate the beam combiner…