Fétick et al., 2019 - Google Patents
Physics-based model of the adaptive-optics-corrected point spread function-applications to the sphere/zimpol and muse instrumentsFétick et al., 2019
View HTML- Document ID
- 1588850661298636366
- Author
- Fétick R
- Fusco T
- Neichel B
- Mugnier L
- Beltramo-Martin O
- Bonnefois A
- Petit C
- Milli J
- Vernet J
- Oberti S
- Bacon R
- Publication year
- Publication venue
- Astronomy & Astrophysics
External Links
Snippet
Context. Adaptive optics (AO) systems greatly increase the resolution of large telescopes, but produce complex point spread function (PSF) shapes, varying in time and across the field of view. The PSF must be accurately known since it provides crucial information about …
- 229940028444 Muse 0 title abstract description 26
Classifications
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colour
- G01J3/28—Investigating the spectrum
-
- G—PHYSICS
- G06—COMPUTING; CALCULATING; COUNTING
- G06F—ELECTRICAL DIGITAL DATA PROCESSING
- G06F17/00—Digital computing or data processing equipment or methods, specially adapted for specific functions
- G06F17/10—Complex mathematical operations
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N21/00—Investigating or analysing materials by the use of optical means, i.e. using infra-red, visible or ultra-violet light
- G01N21/17—Systems in which incident light is modified in accordance with the properties of the material investigated
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colour
- G01J3/02—Details
- G01J3/0205—Optical elements not provided otherwise, e.g. optical manifolds, diffusers, windows
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J1/00—Photometry, e.g. photographic exposure meter
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J9/00—Measuring optical phase difference; Determining degree of coherence; Measuring optical wavelength
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01S—RADIO DIRECTION-FINDING; RADIO NAVIGATION; DETERMINING DISTANCE OR VELOCITY BY USE OF RADIO WAVES; LOCATING OR PRESENCE-DETECTING BY USE OF THE REFLECTION OR RERADIATION OF RADIO WAVES; ANALOGOUS ARRANGEMENTS USING OTHER WAVES
- G01S13/00—Systems using the reflection or reradiation of radio waves, e.g. radar systems; Analogous systems using reflection or reradiation of waves whose nature or wavelength is irrelevant or unspecified
- G01S13/88—Radar or analogous systems specially adapted for specific applications
- G01S13/89—Radar or analogous systems specially adapted for specific applications for mapping or imaging
- G01S13/90—Radar or analogous systems specially adapted for specific applications for mapping or imaging using synthetic aperture techniques, e.g. correcting range migration errors
- G01S13/9035—Particular SAR processing techniques not provided for elsewhere, e.g. squint mode, doppler beam-sharpening mode, spotlight mode, bistatic SAR, inverse SAR
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N30/00—Investigating or analysing materials by separation into components using adsorption, absorption or similar phenomena or using ion-exchange, e.g. chromatography or field flow fractionation
- G01N30/02—Column chromatography
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01M—TESTING STATIC OR DYNAMIC BALANCE OF MACHINES OR STRUCTURES; TESTING STRUCTURES OR APPARATUS NOT OTHERWISE PROVIDED FOR
- G01M11/00—Testing of optical apparatus; Testing structures by optical methods not otherwise provided for
Similar Documents
| Publication | Publication Date | Title |
|---|---|---|
| Fétick et al. | Physics-based model of the adaptive-optics-corrected point spread function-applications to the sphere/zimpol and muse instruments | |
| Boucaud et al. | Convolution kernels for multi-wavelength imaging | |
| Neichel et al. | TIPTOP: a new tool to efficiently predict your favorite AO PSF | |
| Jensen-Clem et al. | Demonstrating predictive wavefront control with the Keck II near-infrared pyramid wavefront sensor | |
| Beltramo-Martin et al. | Review of PSF reconstruction methods and application to post-processing | |
| Kammerer et al. | The near infrared imager and slitless spectrograph for JWST. V. Kernel phase imaging and data analysis | |
| Meftah et al. | Solar radius determined from PICARD/SODISM observations and extremely weak wavelength dependence in the visible and the near-infrared | |
| Witzel et al. | The AIROPA software package: milestones for testing general relativity in the strong gravity regime with AO | |
| Berdeu et al. | PIC: a data reduction algorithm for integral field spectrographs-Application to the SPHERE instrument | |
| Groff et al. | Roman Space Telescope CGI: prism and polarizer characterization modes | |
| Beltramo-Martin et al. | Off-axis point spread function characterization in laser guide star adaptive optics systems | |
| Clermont et al. | Stray-light calibration and correction for the MetOp-SG 3MI mission | |
| Schöck et al. | Atmospheric turbulence characterization with the Keck adaptive optics systems. I. Open-loop data | |
| Clermont et al. | Out-of-field stray light correction in optical instruments: the case of Metop-3MI | |
| Orieux et al. | Super-resolution in map-making based on a physical instrument model and regularized inversion-Application to SPIRE/Herschel | |
| Schlichenmaier et al. | Effects of solar evolution on finite acquisition time of Fabry–Perot interferometers in high resolution solar physics | |
| Perrin et al. | Single-mode interferometric field of view in partial turbulence correction-Application to the observation of the environment of Sgr A* with GRAVITY | |
| Martin et al. | PSF reconstruction validated using on-sky CANARY data in MOAO mode | |
| Laugier et al. | Recovering saturated images for high dynamic kernel-phase analysis-Application to the determination of dynamical masses for the system Gl 494AB | |
| Simioni et al. | MICADO PSF-reconstruction work package description | |
| Cale et al. | Commissioning observations of HD 189733 with the PAlomar radial velocity instrument | |
| Irbah et al. | Solar seeing monitor MISOLFA: A new method for estimating atmospheric turbulence parameters | |
| Madurowicz et al. | GPI 2.0: Optimizing reconstructor performance in simulations and preliminary contrast estimates | |
| Martin et al. | Point spread function reconstruction validated using on-sky CANARY data in multiobject adaptive optics mode | |
| Pope | Kernel phase and kernel amplitude in Fizeau imaging |