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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 308674.0, MPI für Astronomie / Publikationen_mpia
MATISSE: A four beams combiner in the mid-infrared for the VLTI
Authors:Lagarde, S.; Lopez, B.; Antonelli, P.; Beckman, U.; Behrend, J.; Bresson, Y.; Chesneau, O.; Dugué, M.; Glazenborg, A.; Graser, U.; Hofmann, K. H.; Jaffe, W.; Leinert, C.; Millour, F.; Menut, J. L.; Petrov, R. G.; Ratzka, T.; Weigelt, G.; Wolf, S.; Abraham, P.; Connot, C.; Henning, T.; Heininger, M.; Hugues, Y.; Kraus, S.; Laun, W.; Matter, A.; Neumann, U.; Nussbaum, E.; Niedzielski, A.; Mosoni, L.; Robbe-Dubois, S.; Roussel, A.; Schertl, D.; Vakili, F.; Wagner, K.; Waters, L. B. F. M.
Publisher:SPIE
Date of Publication (YYYY-MM-DD):2006
Title of Proceedings:Advances in Stellar Interferometry
Start Page:62683M-1
End Page:10
Volume (in Series):6268
Name of Conference/Meeting:Advances in Stellar Interferometry
Audience:Not Specified
Abstract / Description:A first generation of VLTI (Very Large Telescopes Interferometer) focal instruments, AMBER in the near-infrared and MIDI in the mid-infrared, has been already integrated and tested. New and important science results have been obtained. These instruments combine two (for MIDI) or three (for AMBER) beams coming from the eight telescopes installed at Cerro Paranal (four 8-meters and four 1.8-meters telescopes). In order to improve the capabilities of the interferometer and to engage a new scientific prospective, the second generation of VLTI instruments is currently under study. MATISSE belongs to this second generation. MATISSE objective is the image reconstruction. It will extend the astrophysical potential of the VLTI by overcoming the ambiguities existing in the interpretation of simple visibility measurements. It is a spectro-interferometer combining up to four beams with a large spectral coverage ranging from 3 to 25 mum (L, M, N and Q bands). Different spectral resolutions (between 30 and 1500) are foreseen. MATISSE will measure closure phase relations thus offering an efficient capability for image reconstruction. The concept of MATISSE is presented in this paper. The recombination mode of MATISSE is similar to the AMBER beam combination, but has been adapted to the constraints specific to the mid-infrared domain.
Comment of the Author/Creator:Date: 2006, July 1, 2006
External Publication Status:published
Document Type:Conference-Paper
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bi...
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