Adaptive Optics for Extremely Large Telescopes 4 – Conference Proceedings
Parent: UC Observatories
eScholarship stats: Breakdown by Item for November, 2024 through February, 2025
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 69 | 11 | 58 | 15.9% |
| 4gr3p2pf | Adaptive Optics Program at TMT | 58 | 17 | 41 | 29.3% |
| 2vj6w3gm | The use of CPU, GPU and FPGA in real-time control of adaptive optics systems | 56 | 9 | 47 | 16.1% |
| 910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 53 | 11 | 42 | 20.8% |
| 3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 51 | 10 | 41 | 19.6% |
| 2zm625jk | Selex infrared sensors for astronomy – present and future | 47 | 3 | 44 | 6.4% |
| 56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 47 | 5 | 42 | 10.6% |
| 217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 45 | 11 | 34 | 24.4% |
| 8cg2r2p8 | PSF reconstruction for AO photometry and astrometry | 45 | 3 | 42 | 6.7% |
| 015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 44 | 9 | 35 | 20.5% |
| 10b151nz | A New Slow Focus Sensor for GeMS | 44 | 4 | 40 | 9.1% |
| 1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 44 | 5 | 39 | 11.4% |
| 3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 44 | 5 | 39 | 11.4% |
| 4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 44 | 12 | 32 | 27.3% |
| 5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 44 | 20 | 24 | 45.5% |
| 7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 44 | 8 | 36 | 18.2% |
| 93x3m220 | Non common path aberration correction with non linear WFSs | 43 | 5 | 38 | 11.6% |
| 1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 42 | 3 | 39 | 7.1% |
| 2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 42 | 7 | 35 | 16.7% |
| 2mq8n4d4 | First Results of the Ground Layer Adaptive Optics System ARGOS | 41 | 10 | 31 | 24.4% |
| 87f6s2zv | The GMT Dynamic Optical Simulation | 41 | 3 | 38 | 7.3% |
| 5dg67931 | Analytical study of high altitude turbulence wide-field wavefront sensing: impact on the design and reconstruction quality of future solar AO systems | 40 | 4 | 36 | 10.0% |
| 0479k8m1 | Observations of the dynamic turbulence above La Palma using Stereo-SCIDAR | 39 | 9 | 30 | 23.1% |
| 1x2266wp | Optical design of the Post Focal Relay of MAORY | 39 | 10 | 29 | 25.6% |
| 80j280rv | Filtering the interaction matrix in an adaptive optics system | 39 | 3 | 36 | 7.7% |
| 7t06254q | GeMS, the path toward AO facility | 38 | 7 | 31 | 18.4% |
| 23w5v4vv | New Cophasing and AO strategies for an extremely large telescope dedicated to extremely high contrast: The Colossus Project | 37 | 6 | 31 | 16.2% |
| 8d79v3t0 | XAO at LBT: current performances in the visible and upcoming upgrade | 37 | 5 | 32 | 13.5% |
| 4jh5c19s | Laboratory tests on HeNOS, the MCAO test bench for NFIRAOS | 36 | 2 | 34 | 5.6% |
| 62p140z1 | Measuring Segment Piston with a Non-Redundant Pupil Mask on the Giant Magellan Telescope | 36 | 3 | 33 | 8.3% |
| 6317r29b | Near-infrared tip-tilt sensing at Keck: System architecture and on-sky performance | 36 | 5 | 31 | 13.9% |
| 7019b6vc | AO for MOSAIC, the E-ELT Multiple Object Spectrograph | 36 | 6 | 30 | 16.7% |
| 8w80k9sp | An Integrated MASS/DIMM Monitor Based on a Low-Noise CCD Detector | 36 | 4 | 32 | 11.1% |
| 1367c5xw | Anti-aliasing wave-front reconstruction with Shack-Hartmann sensors | 35 | 4 | 31 | 11.4% |
| 1df66431 | Resolving the low-mass content of Westerlund 1 using MCAO | 35 | 4 | 31 | 11.4% |
| 2mn1w74z | Point spread function determination for Keck adaptive optics: overview | 35 | 11 | 24 | 31.4% |
| 3cq132qm | Pyramid versus Shack-Hartmann: Trade Study Results for the NFIRAOS NGS WFS | 35 | 4 | 31 | 11.4% |
| 29g816zb | SPHERE extreme AO system On-sky operation, final performance and future improvements | 34 | 8 | 26 | 23.5% |
| 2mq7f7k6 | OCAM2S: an integral shutter ultrafast and low noise wavefront sensor camera for laser guide stars adaptive optics systems | 34 | 10 | 24 | 29.4% |
| 4h03k92b | Analysis of GeMS tip-tilt on-sky data: LQG implementation for vibration rejections | 34 | 9 | 25 | 26.5% |
| 56p467d6 | Astrometry with MCAO at Gemini and at ELTs | 34 | 6 | 28 | 17.6% |
| 0gt3876k | SPHERE extreme AO system On-sky operation, final performance and future improvements | 33 | 8 | 25 | 24.2% |
| 6h92z4q4 | Development of an ELT XAO testbed using a self referenced Mach-Zehnder wavefront sensor | 33 | 3 | 30 | 9.1% |
| 7774b5p6 | GMCAO for E-ELT: a feasibility study | 33 | 3 | 30 | 9.1% |
| 81f1f8pt | Prototyping the GMT phasing camera with the Magellan AO system | 33 | 6 | 27 | 18.2% |
| 2dm1m7jq | MCAO numerical simulations for EST: analysis and parameter optimization | 32 | 7 | 25 | 21.9% |
| 42h0n70s | Implementation of SLODAR atmospheric turbulence profiling to the ARGOS system | 32 | 8 | 24 | 25.0% |
| 6809n74d | Durham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs) | 32 | 5 | 27 | 15.6% |
| 9q7259nn | Non Boltzmann Modeling of Sodium Guidestar Returns and Implications for Guidestar Linewidth | 32 | 2 | 30 | 6.3% |
| 5q66922d | E-ELT M4 Unit updated design and prototype results | 31 | 9 | 22 | 29.0% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.