MATISSE

B. Lopez, S. Lagarde, S. Wolf, W. Jaffe, G. Weigelt, P. Antonelli, P. Abraham, J.-Ch. Augereau, U. Beckman, J. Behrend, N. Berruyer, Y. Bresson, O. Chesneau, J. M. Clausse, C. Connot, W. C. Danchi, M. Delbo, K. Demyk, A. Domiciano, M. Dugué, A. Glazenborg, U. Graser, H. Hanenburg, Th. Henning, M. Heininger, K.-H. Hofmann, Y. Hugues, S. Jankov, S. Kraus, W. Laun, Ch. Leinert, H. Linz, A. Matter, Ph. Mathias, K. Meisenheimer, J.-L. Menut, F. Millour, L. Mosoni, U. Neumann, A. Niedzielski, E. Nussbaum, R. Petrov, Th. Ratzka, S. Robbe-Dubois, A. Roussel, D. Schertl, F.-X. Schmider, B. Stecklum, E. Thiebaut, F. Vakili, K. Wagner, L. B. F. M. Waters, O. Absil, J. Hron, N. Nardetto, J. Olofsson, B. Valat, M. Vannier, B. Goldman, S. Hönig and W. D. Cotton

Proceedings paper for the ESO workshop "The VLT in the ELT era"
Held in Garching from October 8-12, 2007.
Springer Astrophysics and Space Science Proceedings
"Science with the VLT in the ELT Era", pg.353-357 (2009)

Abstract
MATISSE is foreseen as a mid-infrared spectro-interferometer combining the beams of up to four UTs/ATs of the Very Large Telescope Interferometer (VLTI). MATISSE will measure closure phase relations and thus offer an efficient capability for image reconstruction in the L, M and N bands of the mid-infrared domain.

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