179 results on '"Fusco, Thierry"'
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2. Forecasting of turbulence impact on optical link from geostationary satellite
3. Towards robust deconvolution of hyperspectral data cubes
4. Prediction of AO corrected PSF for AOF NFM/SPHERE
5. Understand and correct for the low wind effect on the SPHERE and GRAVITY+ adaptive optics
6. Study of the LIFT focal-plane wavefront sensor for GALACSI NFM
7. HARMONI at ELT: Towards a final design for the natural guide star sensors system
8. Optimizing Fourier-filtering WFS to reach sensitivity close to the fundamental limit
9. Adapting the pyramid wavefront sensor for pupil fragmentation of the ELT class telescopes
10. Towards virtual access of adaptive optics telemetry data
11. HARMONI at ELT: designing a laser guide star wavefront sensors for the ELT
12. PSF nowcast using PASSATA simulations: towards a PSF forecast
13. HARMONI at ELT: wavefront control in SCAO mode
14. HARMONI at ELT: system analysis and performance estimation of the high-contrast module
15. HARMONI at ELT: prototyping for Single-Conjugate AO Sensor subsystem
16. The phase-shifted Zernike wave-front sensor
17. Laboratory demonstration of focal plane wavefront sensing using phase diversity: a way to tackle the problem of NCPA in SHARK-NIR. Part II: new characterization tests and alternative wavefront sensing strategies
18. HARMONI at ELT: adaptive optics calibration unit from design to prototyping
19. RISTRETTO: coronagraph and AO designs enabling High Dispersion Coronagraphy at 2 λ/D
20. HARMONI at ELT: full scale prototype of the laser guide star wavefront sensor
21. Deformable lens for testing the performance of focal plane wavefront sensing using phase diversity
22. Fourier filter LGS wavefront sensing for ELT size telescopes
23. MAVIS: preliminary design of the adaptive optics module
24. DEEPLOOP: DEEP Learning for an Optimized adaptive Optics Psf estimation
25. First light for PAPYRUS, the pyramid based adaptive optics system at LAM/OHP
26. HARMONI at ELT: overview of the capabilities and expected performance of the ELT's first light, adaptive optics assisted integral field spectrograph.
27. RISTRETTO: high-resolution spectroscopy at the diffraction limit of the VLT
28. HARMONI- the Extremely Large Telescope first light integral field spectrograph: a novel functional model based system engineering methodology for the design of an integrated instrument control system architecture
29. Current status of PAPYRUS : the pyramid based adaptive optics system at LAM/OHP
30. TIPTOP: a new tool to efficiently predict your favorite AO PSF
31. Maximum likelihood co-phasing of segmented mirrors with a pyramid in the visible: simulation vs. experiment
32. Laboratory demonstration of focal plane wavefront sensing using phase diversity: a way to tackle the problem of NCPA in SHARK-NIR
33. MAVIS adaptive optics module optical design
34. MAVIS: the adaptive optics module feasibility study
35. MOSAIC: the high multiplex and multi-IFU spectrograph for the ELT
36. MAVIS: science case, imager, and spectrograph
37. MAVIS: system modelling and performance prediction
38. Optimising tomographic reconstructor parameters for adaptive optics using real turbulence profiles
39. Injecting pupil binary intensity map into the laboratory adaptive optics bench using phase-only LCoS-SLM device
40. First results of laboratory tests of a three-sided pyramid wavefront sensor
41. MAVIS conceptual design
42. HARMONI: first light spectroscopy for the ELT: instrument final design and quantitative performance predictions
43. Precise photometry and astrometry in the core of the globular cluster NGC 6121 using PSF-R techniques
44. Operational forecast of the PSF figures of merit
45. The ORP on-sky community access program for adaptive optics instrumentation development
46. Ingot wavefront sensor: from the Fourier End2End numerical simulation to the LOOPS test bench
47. First error budget of a deployable CubeSat telescope
48. Review of PSF reconstruction methods and application to post-processing
49. GNAO: an MCAO facility for Gemini North
50. A possible VLT-SPHERE XAO upgrade: going faster, going fainter, going deeper (Conference Presentation)
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