55 results on '"Malbet, Fabien"'
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2. Theia: science cases and mission profiles for high precision astrometry in the future.
3. Toward a revival of stellar intensity interferometry.
4. Science case for 1 mas spectro-imagining in the near-infrared.
5. VLTI-AMBER observations of Eta Carinae with the FINITO fringe tracker and spectral resolution 12000.
6. Near-IR spectrograph of VSI (VLTI Spectro Imager): dispersing the light from an integrated optics beam-combiner.
7. Experiences from the first AMBER open time observations.
8. The VSI/VITRUV combiner: a phase-shifted four-beam integrated optics combiner.
9. VLTI-AMBER observations of Eta Carinae with high spatial resolution and spectral resolutions of 1,500 and 10,000.
10. Pupil Remapping Coronagraph (PRC): a high-performance coronagraph for a small-size visible Terrestrial Planet Finder.
11. The VLTI focal instrument Amber: results of the first phase of the alignment, integration, and verification in Paranal.
12. Imaging young stellar objects with AMBER on the VLTI.
13. Data reduction for the AMBER instrument.
14. A laboratory interferometer simulator for integrated optics combiners qualification.
15. Comparison of integrated optics concepts for a near-infrared multi-telescope beam combiner.
16. Characterizing closure-phase measurements at IOTA.
17. AMBER integration and laboratory performances.
18. Science program of the AMBER consortium.
19. VITRUV, a second-generation VLTI instrument for aperture synthesis imaging with eight telescopes.
20. Design and tests for the correction of atmospheric and instrumental effects on color-differential phase with AMBER/VLTI.
21. Integrated optics components in silica on silicon technology for stellar interferometry.
22. An integrated-optics 3-way beam combiner for IOTA.
23. System analysis of the AMBER instrument on VLTI.
24. High angular resolution in 2010-2020: a comparison between possible post-VLT/VLTI instruments.
25. OHANA and star formation: probing deep into the accretion/ejection mechanism.
26. OHANA: representative science objectives.
27. Jean-Marie Mariotti Center for Interferometry.
28. Increasing the imaging capabilities of the VLTI using integrated optics.
29. Interferometry with single mode waveguide.
30. New beam-combination Techniques at IOTA.
31. Young Stellar Objects science with interferometry.
32. Astrophysical potential of the AMBER/VLTI instrument.
33. Using the near infrared VLTI instrument AMBER.
34. ASPRO: a software to prepare observations with optical interferometers.
35. Qualification of IONIC (integrated optics near-infrared interferometric camera).
36. Infrared waveguides for interferometry applications.
37. Planar optics three-telescope beam combiners for astronomical interferometry.
38. AMBER: optical design and expected performance.
39. AMBER data simulator.
40. Probing the inner part of protoplanetary disks with the VLTI.
41. AMBER performances: signal-to-noise ratio analysis.
42. AMBER data structure, processing, and calibration.
43. Spatial filtering in AMBER.
44. Nulling interferometry for the DARWIN mission: experimental demonstration of the concept in the thermal infrared with high levels of rejection.
45. New insights into the nature of the circumstellar environment of FU Ori.
46. Combining up to eight telescope beams in a single chip.
47. Planar integrated optics contribution to instrumention for interferometry.
48. AMBER: the near-infrared focal instrument for the Very Large Telescope Interferometer.
49. Science opportunities with AMBER, the near-IR VLTI instrument.
50. Palomar Testbed Interferometer.
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