English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

Bringing the new adaptive optics module for interferometry (NAOMI) into operation

MPS-Authors
/persons/resource/persons4766

Eisenhauer,  Frank
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

/persons/resource/persons4782

Pfuhl,  Oliver
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)
There are no public fulltexts stored in PuRe
Supplementary Material (public)
There is no public supplementary material available
Citation

Gonté, F., Abad, J. A., Abuter, R., Carpentier, E. A., Alonso, J., Andofalto, L., et al. (2019). Bringing the new adaptive optics module for interferometry (NAOMI) into operation. The Messenger, 177, 19-23. doi:10.18727/0722-6691/5149.


Cite as: https://hdl.handle.net/21.11116/0000-0005-1FA0-4
Abstract
NAOMI was developed by a consortium
composed of IPAG and ESO. Its Provisional
Acceptance Chile review was
held in April 2019. The NAOMI systems
that have been installed on the Auxiliary
Telescopes make the Very Large Telescope
Interferometer (VLTI) and its
instruments much less dependent on
the atmospheric and dome seeing
conditions.
NAOMI increases the interferometer’s
operability and improves the
performance of its instruments and,
very early on, was identified as being
critical to the VLTI. In this article,
we
review the project, describe its principles
and architecture, and offer a preview
of the improvements it brings to
VLTI instruments.