2009-01-01
AUTHORSS. Wolf , B. Lopez , W. Jaffe , G. Weigelt , J.-Ch. Augereau , N. Berruyer , O. Chesneau , W. C. Danchi , M. Delbo , K. Demyk , A. Domiciano , Th. Henning , K.-H. Hofmann , S. Kraus , Ch. Leinert , H. Linz , Ph. Mathias , K. Meisenheimer , J.-L. Menut , F. Millour , L. Mosoni , A. Niedzielski , R. Petrov , Th. Ratzka , B. Stecklum , E. Thiebaut , F. Vakili , L. B. F. M. Waters , O. Absil , J. Hron , S. Lagarde , A. Matter , N. Nardetto , J. Olofsson , B. Valat , M. Vannier , MATISSE Science team
ABSTRACTMATISSE is foreseen as a mid-infrared spectro-interferometric instrument 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 addition to this, MATISSE will open 2 new observing windows at the VLTI: the L and M band in addition to the N band. Furthermore, the instrument will offer the possibility to perform simultaneous observations in separate bands. MATISSE will also provide several spectroscopic modes. In summary, MATISSE can be seen as a successor of MIDI by providing imaging capabilities in the mid-infrared domain (for a more detailed description of MATISSE see Lopez et al., these proceedings). More... »
PAGES359-360
Science with the VLT in the ELT Era
ISBN
978-1-4020-9189-6
978-1-4020-9190-2
http://scigraph.springernature.com/pub.10.1007/978-1-4020-9190-2_60
DOIhttp://dx.doi.org/10.1007/978-1-4020-9190-2_60
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