Adaptive Optics for Extremely Large Telescopes 4 – Conference Proceedings
Parent: UC Observatories
eScholarship stats: Breakdown by Item for December, 2024 through March, 2025
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 70 | 15 | 55 | 21.4% |
| 217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 63 | 9 | 54 | 14.3% |
| 2vj6w3gm | The use of CPU, GPU and FPGA in real-time control of adaptive optics systems | 61 | 7 | 54 | 11.5% |
| 3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 58 | 10 | 48 | 17.2% |
| 4gr3p2pf | Adaptive Optics Program at TMT | 58 | 14 | 44 | 24.1% |
| 7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 57 | 10 | 47 | 17.5% |
| 93x3m220 | Non common path aberration correction with non linear WFSs | 57 | 7 | 50 | 12.3% |
| 1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 55 | 7 | 48 | 12.7% |
| 4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 53 | 11 | 42 | 20.8% |
| 015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 52 | 9 | 43 | 17.3% |
| 5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 52 | 16 | 36 | 30.8% |
| 10b151nz | A New Slow Focus Sensor for GeMS | 51 | 5 | 46 | 9.8% |
| 56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 51 | 6 | 45 | 11.8% |
| 8cg2r2p8 | PSF reconstruction for AO photometry and astrometry | 51 | 5 | 46 | 9.8% |
| 910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 51 | 10 | 41 | 19.6% |
| 8nb0n5jf | Progress report on the ESO 4LGSF | 48 | 6 | 42 | 12.5% |
| 2zm625jk | Selex infrared sensors for astronomy – present and future | 47 | 3 | 44 | 6.4% |
| 3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 46 | 4 | 42 | 8.7% |
| 80j280rv | Filtering the interaction matrix in an adaptive optics system | 46 | 6 | 40 | 13.0% |
| 81f1f8pt | Prototyping the GMT phasing camera with the Magellan AO system | 46 | 8 | 38 | 17.4% |
| 1x2266wp | Optical design of the Post Focal Relay of MAORY | 44 | 12 | 32 | 27.3% |
| 3cq132qm | Pyramid versus Shack-Hartmann: Trade Study Results for the NFIRAOS NGS WFS | 44 | 4 | 40 | 9.1% |
| 6r38q9vb | Performance assessment for the linear control of adaptive optics systems: noise propagation and temporal errors | 44 | 9 | 35 | 20.5% |
| 7t06254q | GeMS, the path toward AO facility | 44 | 10 | 34 | 22.7% |
| 87f6s2zv | The GMT Dynamic Optical Simulation | 44 | 4 | 40 | 9.1% |
| 0479k8m1 | Observations of the dynamic turbulence above La Palma using Stereo-SCIDAR | 43 | 11 | 32 | 25.6% |
| 2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 43 | 7 | 36 | 16.3% |
| 1df66431 | Resolving the low-mass content of Westerlund 1 using MCAO | 42 | 5 | 37 | 11.9% |
| 7019b6vc | AO for MOSAIC, the E-ELT Multiple Object Spectrograph | 42 | 7 | 35 | 16.7% |
| 5q66922d | E-ELT M4 Unit updated design and prototype results | 41 | 9 | 32 | 22.0% |
| 62p140z1 | Measuring Segment Piston with a Non-Redundant Pupil Mask on the Giant Magellan Telescope | 41 | 3 | 38 | 7.3% |
| 7774b5p6 | GMCAO for E-ELT: a feasibility study | 41 | 3 | 38 | 7.3% |
| 1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 40 | 3 | 37 | 7.5% |
| 20s3w2j6 | Laser guide star adaptive optics at Lick Observatory | 40 | 6 | 34 | 15.0% |
| 4h03k92b | Analysis of GeMS tip-tilt on-sky data: LQG implementation for vibration rejections | 40 | 9 | 31 | 22.5% |
| 5dg67931 | Analytical study of high altitude turbulence wide-field wavefront sensing: impact on the design and reconstruction quality of future solar AO systems | 40 | 5 | 35 | 12.5% |
| 6317r29b | Near-infrared tip-tilt sensing at Keck: System architecture and on-sky performance | 40 | 5 | 35 | 12.5% |
| 0bz8t4mv | Commissioning of ARGOS at LBT: adaptive optics procedures | 39 | 5 | 34 | 12.8% |
| 29g816zb | SPHERE extreme AO system On-sky operation, final performance and future improvements | 39 | 8 | 31 | 20.5% |
| 2mn1w74z | Point spread function determination for Keck adaptive optics: overview | 39 | 11 | 28 | 28.2% |
| 5t0211tn | SCExAO: the first high contrast exoplanet imager on an ELT? | 39 | 4 | 35 | 10.3% |
| 8d79v3t0 | XAO at LBT: current performances in the visible and upcoming upgrade | 39 | 5 | 34 | 12.8% |
| 8w80k9sp | An Integrated MASS/DIMM Monitor Based on a Low-Noise CCD Detector | 39 | 5 | 34 | 12.8% |
| 2mq8n4d4 | First Results of the Ground Layer Adaptive Optics System ARGOS | 38 | 3 | 35 | 7.9% |
| 4jh5c19s | Laboratory tests on HeNOS, the MCAO test bench for NFIRAOS | 38 | 2 | 36 | 5.3% |
| 087701qh | Development of multi time-step tomographic reconstruction with RAVEN | 37 | 3 | 34 | 8.1% |
| 20x7p7qb | Recent Improvements to the Keck II Laser Guide Star Facility | 37 | 10 | 27 | 27.0% |
| 56p467d6 | Astrometry with MCAO at Gemini and at ELTs | 37 | 7 | 30 | 18.9% |
| 6809n74d | Durham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs) | 37 | 6 | 31 | 16.2% |
| 8979r2d9 | Preliminary performance analysis of a LGS system for GTC | 37 | 7 | 30 | 18.9% |
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