Our 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
ESO's new Very Large Telescope will consist of four 8.2m telescopes and three moveable 1.8m telescop...
MATISSE is foreseen as a mid-infrared spectro-interferometric instrument combining the beams of up t...
Context. Optical interferometry is at a key development stage. The Very Large Telescope Interferomet...
Our objective is to develop of the mid-infrared imaging for the VLTI. Several areas of astrophysics ...
Our objective is to develop of the mid-infrared imaging for the VLTI. Several areas of astrophysics ...
International audienceMATISSE is foreseen as a mid-infrared spectro-interferometer combining the bea...
Our objective is the development of mid-infrared imaging at the VLTI. The related science case study...
A first generation of VLTI (Very Large Telescopes Interferometer) focal instruments, AMBER in the ne...
We report in this paper on the current status of the mid-infrared beam combiner of the VLTI: MIDI....
ESO's new Very Large Telescope will consist of four 8.2m telescopes and three moveable 1.8m telescop...
International audienceContext: Recently, an increasing number of scientific publications making use ...
After more than five years of preparation, the mid-infrared interferometric instrument MIDI has been...
Context. Recently, an increasing number of scientific publications making use of images obtained wit...
ESO's new Very Large Telescope will consist of four 8.2m telescopes and three moveable 1.8m telescop...
MATISSE is foreseen as a mid-infrared spectro-interferometric instrument combining the beams of up t...
Context. Optical interferometry is at a key development stage. The Very Large Telescope Interferomet...
Our objective is to develop of the mid-infrared imaging for the VLTI. Several areas of astrophysics ...
Our objective is to develop of the mid-infrared imaging for the VLTI. Several areas of astrophysics ...
International audienceMATISSE is foreseen as a mid-infrared spectro-interferometer combining the bea...
Our objective is the development of mid-infrared imaging at the VLTI. The related science case study...
A first generation of VLTI (Very Large Telescopes Interferometer) focal instruments, AMBER in the ne...
We report in this paper on the current status of the mid-infrared beam combiner of the VLTI: MIDI....
ESO's new Very Large Telescope will consist of four 8.2m telescopes and three moveable 1.8m telescop...
International audienceContext: Recently, an increasing number of scientific publications making use ...
After more than five years of preparation, the mid-infrared interferometric instrument MIDI has been...
Context. Recently, an increasing number of scientific publications making use of images obtained wit...
ESO's new Very Large Telescope will consist of four 8.2m telescopes and three moveable 1.8m telescop...
MATISSE is foreseen as a mid-infrared spectro-interferometric instrument combining the beams of up t...
Context. Optical interferometry is at a key development stage. The Very Large Telescope Interferomet...