VLTI status update: Three years into the second generation

Julien Woillez,Pascaline Darre,Sebastian Egner,Frederic Gonte,Xavier Haubois,Antoine Merand,Nicolas Schuhler,Jose Antonio Abad,Roberto Abuter,Emmanuel Aller-Carpentier,Jaime Alonso,Luigi Andolfato, Pablo Jose Barriga,Juan Beltran,Jean-Philippe Berger,Pierre Bourget,Roland Brast,Paul Bristow, Luis Caniguante, Ralf Conzelmann,Angela Cortes,Alain Delboulbe,Francoise Delplancke-Stroebele,Diego Del Valle,Roderick Dembet,Frederic Derie, Reinaldo Donoso,Philippe Duhoux,Christophe Dupuy, Andreas Foerster,Eloy Fuenteseca, Robert Frahm,Daniel Gaytan,Andreas Glindemann, Jaime Gonzales, Thibaut Guerlet,Sylvain Guieu,Stephane Guisard,Pablo Gutierrez,Pierre Haguenauer,Andreas Haimerl,Pierre van der Heyden,Stefan Huber,Norbert Hubin, Lieselotte Jochum,Laurent Jocou, Paul Jolley,Jean-Paul Kirchbauer,Johann Kolb, Johan Kosmalski, Peter Krempl,Jean-Baptiste Le Bouquin, Samuel Leveque,Paul Lilley, Jean Louis Lizon,Yves Magnard,Pedro Mardones,Alexander Meister,Thibaut Moulin,Juan Osorio,Juergen Ott,Laurent Pallanca,Jerome Paufique, Marcus Pavez,Luca Pasquini,Isabelle Percheron, Lorenzo Pettazzi,Thanh Phan Duc, Jean Francois Pirard,Andres Pino,Sebastien Poupar,Jutta Quentin,Andres Ramirez,Javier Reyes, Robert Ridings,Sylvain Rochat,Thomas Rivinius,Fernando Salgado,Markus Schoeller, Pavel Shchekaturov,Christian Stephan,Marcos Suarez, Richard Tamblay,Mario Tapia,Konrad Tristram, Guillermo Valdes,Christophe Verinaud,Willem-Jan de Wit,Gerard Zins

Proceedings of SPIE（2018）

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摘要

The near-infrared GRAVITY instrument has become a fully operational spectro-imager, while expanding its capability to support astrometry of the key Galactic Centre science. The mid-infrared MATISSE instrument has just arrived on Paranal and is starting its commissioning phase. NAOMI, the new adaptive optics for the Auxiliary Telescopes, is about to leave Europe for an installation in the fall of 2018. Meanwhile, the interferometer infrastructure has continuously improved in performance, in term of transmission and vibrations, when used with both the Unit Telescopes and Auxiliary Telescopes. These are the highlights of the last two years of the VLTI 2nd generation upgrade started in 2015.

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关键词

Stellar Interferometry,Very Large Telescope Interferometer

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