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APerture Synthesis in the MID-Infrared with the VLTI

hal.structure.identifierLaboratoire Gemini [LG]
hal.structure.identifierDépartement Fresnel [FRESNEL]
hal.structure.identifierLaboratoire d'étude des Mécanismes de la recombinaison [LMR]
dc.contributor.authorLOPEZ, B.
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
hal.structure.identifierInstitute of Plant Sciences, Faculty of Agricultural, Food, and Environmental Quality Sciences
hal.structure.identifierLaboratoire de Géophysique Interne et Tectonophysique [LGIT]
hal.structure.identifierLaboratoire de Mathématiques [LAMA]
dc.contributor.authorWOLF, S.
dc.contributor.authorDUGUÉE, M.
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorGRASER, U.
hal.structure.identifierLaboratoire Gemini [LG]
hal.structure.identifierLaboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides [CASSIOPEE]
dc.contributor.authorMATHIAS, Ph.
hal.structure.identifierLaboratoire Gemini [LG]
hal.structure.identifierDépartement Fresnel [FRESNEL]
dc.contributor.authorANTONELLI, P.
hal.structure.identifierLaboratoire d'Astrophysique de Grenoble [LAOG]
hal.structure.identifierLaboratoire de l'intégration, du matériau au système [IMS]
hal.structure.identifierDépartement d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA]
dc.contributor.authorAUGEREAU, J.-C.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorDUTREY, Anne
dc.contributor.authorCOAUTHORS, And
dc.date.issued2008
dc.description.abstractEnOur objective is to develop of the mid-infrared imaging for the VLTI. Several areas of astrophysics will benefit of this new capability. APreS-MIDI comprises a beam combiner which interfaces with the current MIDI instrument. It thus constitutes an extension to the two-beam interferometric instrument MIDI by increasing the number of recombined beams up to four. This extension provides better uv-coverage (6 visibility points measured in one set) and moreover will allow measurement of 4 closure phase relations thus providing for the first time aperture synthesis images in the mid-infrared spectral regime.
dc.language.isoen
dc.publisherSpringer Berlin / Heidelberg
dc.source.titleThe Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation - Proceedings of the ESO Workshop
dc.title.enAPerture Synthesis in the MID-Infrared with the VLTI
dc.typeChapitre d'ouvrage
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
bordeaux.page345
bordeaux.title.proceedingThe Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation - Proceedings of the ESO Workshop
hal.identifierhal-00320183
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00320183v1
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