Adaptive Optics for Extremely Large Telescopes 4 – Conference Proceedings
Parent: UC Observatories
eScholarship stats: Breakdown by Item for September through December, 2024
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 70 | 11 | 59 | 15.7% |
| 0479k8m1 | Observations of the dynamic turbulence above La Palma using Stereo-SCIDAR | 60 | 32 | 28 | 53.3% |
| 910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 50 | 6 | 44 | 12.0% |
| 4gr3p2pf | Adaptive Optics Program at TMT | 49 | 16 | 33 | 32.7% |
| 2vj6w3gm | The use of CPU, GPU and FPGA in real-time control of adaptive optics systems | 45 | 7 | 38 | 15.6% |
| 3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 44 | 4 | 40 | 9.1% |
| 56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 44 | 4 | 40 | 9.1% |
| 015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 43 | 18 | 25 | 41.9% |
| 20x7p7qb | Recent Improvements to the Keck II Laser Guide Star Facility | 42 | 20 | 22 | 47.6% |
| 217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 42 | 9 | 33 | 21.4% |
| 3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 42 | 10 | 32 | 23.8% |
| 7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 42 | 13 | 29 | 31.0% |
| 5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 41 | 23 | 18 | 56.1% |
| 23w5v4vv | New Cophasing and AO strategies for an extremely large telescope dedicated to extremely high contrast: The Colossus Project | 40 | 12 | 28 | 30.0% |
| 2mn1w74z | Point spread function determination for Keck adaptive optics: overview | 39 | 8 | 31 | 20.5% |
| 8cg2r2p8 | PSF reconstruction for AO photometry and astrometry | 39 | 5 | 34 | 12.8% |
| 8nb0n5jf | Progress report on the ESO 4LGSF | 38 | 17 | 21 | 44.7% |
| 93x3m220 | Non common path aberration correction with non linear WFSs | 38 | 0 | 38 | 0.0% |
| 1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 37 | 2 | 35 | 5.4% |
| 2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 37 | 8 | 29 | 21.6% |
| 87f6s2zv | The GMT Dynamic Optical Simulation | 37 | 4 | 33 | 10.8% |
| 2zm625jk | Selex infrared sensors for astronomy – present and future | 36 | 0 | 36 | 0.0% |
| 4jh5c19s | Laboratory tests on HeNOS, the MCAO test bench for NFIRAOS | 36 | 2 | 34 | 5.6% |
| 2dm1m7jq | MCAO numerical simulations for EST: analysis and parameter optimization | 35 | 12 | 23 | 34.3% |
| 4h03k92b | Analysis of GeMS tip-tilt on-sky data: LQG implementation for vibration rejections | 33 | 12 | 21 | 36.4% |
| 4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 33 | 10 | 23 | 30.3% |
| 62p140z1 | Measuring Segment Piston with a Non-Redundant Pupil Mask on the Giant Magellan Telescope | 33 | 3 | 30 | 9.1% |
| 758421jz | Laser Pointing Camera: a valuable tool for the LGS-AO operations | 32 | 12 | 20 | 37.5% |
| 5q66922d | E-ELT M4 Unit updated design and prototype results | 31 | 10 | 21 | 32.3% |
| 80j280rv | Filtering the interaction matrix in an adaptive optics system | 31 | 1 | 30 | 3.2% |
| 2mq8n4d4 | First Results of the Ground Layer Adaptive Optics System ARGOS | 30 | 9 | 21 | 30.0% |
| 10b151nz | A New Slow Focus Sensor for GeMS | 29 | 3 | 26 | 10.3% |
| 5dg67931 | Analytical study of high altitude turbulence wide-field wavefront sensing: impact on the design and reconstruction quality of future solar AO systems | 29 | 1 | 28 | 3.4% |
| 0gt3876k | SPHERE extreme AO system On-sky operation, final performance and future improvements | 28 | 7 | 21 | 25.0% |
| 1df66431 | Resolving the low-mass content of Westerlund 1 using MCAO | 28 | 2 | 26 | 7.1% |
| 1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 28 | 2 | 26 | 7.1% |
| 1x2266wp | Optical design of the Post Focal Relay of MAORY | 28 | 10 | 18 | 35.7% |
| 6809n74d | Durham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs) | 28 | 4 | 24 | 14.3% |
| 7t06254q | GeMS, the path toward AO facility | 28 | 5 | 23 | 17.9% |
| 2mq7f7k6 | OCAM2S: an integral shutter ultrafast and low noise wavefront sensor camera for laser guide stars adaptive optics systems | 27 | 9 | 18 | 33.3% |
| 7774b5p6 | GMCAO for E-ELT: a feasibility study | 27 | 1 | 26 | 3.7% |
| 7fr068zd | SHARK-NIR Channel: a high contrast imager with coronagraphic capabilities for the Large Binocular Telescope | 26 | 4 | 22 | 15.4% |
| 16b4h26g | Use of Laser Guide Star with Pyramid Wavefront Sensor | 25 | 0 | 25 | 0.0% |
| 29g816zb | SPHERE extreme AO system On-sky operation, final performance and future improvements | 25 | 7 | 18 | 28.0% |
| 6h92z4q4 | Development of an ELT XAO testbed using a self referenced Mach-Zehnder wavefront sensor | 25 | 6 | 19 | 24.0% |
| 8sq053mx | Progress with the 4m high-order AO demonstrator, CHOUGH | 25 | 9 | 16 | 36.0% |
| 56p467d6 | Astrometry with MCAO at Gemini and at ELTs | 24 | 3 | 21 | 12.5% |
| 6317r29b | Near-infrared tip-tilt sensing at Keck: System architecture and on-sky performance | 24 | 3 | 21 | 12.5% |
| 8d79v3t0 | XAO at LBT: current performances in the visible and upcoming upgrade | 24 | 2 | 22 | 8.3% |
| 8p13k3zc | Reducing adaptive optics latency using many-core processors | 24 | 3 | 21 | 12.5% |
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