Matisse

Autor(en)

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, W. D. Cotton

Abstrakt

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.

Organisation(en)

Institut für Astrophysik

Seiten

353-357

DOI

https://doi.org/10.1007/978-1-4020-9190-2_59

Publikationsdatum

2009

ÖFOS 2012

1030 Physik, Astronomie

Link zum Portal

https://ucrisportal.univie.ac.at/de/publications/e5e27df9-f4e9-4d8c-a794-07953bef9714