GRAVITY: Microarcsecond Astrometry and Deep Interferometric Imaging with the VLT View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

2009

AUTHORS

F. Eisenhauer , G. Perrin , W. Brandner , C. Straubmeier , A. Böhm , H. Baumeister , F. Cassaing , Y. Clénet , K. Dodds-Eden , A. Eckart , E. Gendron , R. Genzel , S. Gillessen , A. Gräter , C. Gueriau , N. Hamaus , X. Haubois , M. Haug , T. Henning , S. Hippler , R. Hofmann , F. Hormuth , K. Houairi , S. Kellner , P. Kervella , R. Klein , J. Kolmeder , W. Laun , P. Léna , R. Lenzen , M. Marteaud , V. Naranjo , U. Neumann , T. Paumard , S. Rabien , J. R. Ramos , J. M. Reess , R.-R. Rohloff , D. Rouan , G. Rousset , B. Ruyet , A. Sevin , M. Thiel , J. Ziegleder , D. Ziegler

ABSTRACT

We present the AO assisted, near-infrared VLTI instrument GRAVITY for precision narrow-angle astrometry and interferometric phase referenced imaging of faint objects. With its two fibers per telescope beam, its internal wavefront sensors and fringe tracker, and a novel metrology concept, GRAVITY will not only push the sensitivity far beyond what is offered today, but will also advance the astrometric accuracy for UTs to 10 μas. GRAVITY is designed to work with four telescopes, thus providing phase referenced imaging and astrometry for 6 baselines simultaneously. Its unique capabilities and sensitivity will open a new window for the observation of a wide range of objects, and—amongst others—will allow the study of motions within a few times the event horizon size of the Galactic Center black hole. More... »

PAGES

361-365

Book

TITLE

Science with the VLT in the ELT Era

ISBN

978-1-4020-9189-6
978-1-4020-9190-2

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-1-4020-9190-2_61

DOI

http://dx.doi.org/10.1007/978-1-4020-9190-2_61

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1024124546


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