UC Observatories
Parent: UCLA
eScholarship stats: Breakdown by Item for October, 2024 through January, 2025
Item | Title | Total requests | Download | View-only | %Dnld |
---|---|---|---|---|---|
5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 82 | 11 | 71 | 13.4% |
0479k8m1 | Observations of the dynamic turbulence above La Palma using Stereo-SCIDAR | 56 | 22 | 34 | 39.3% |
910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 55 | 10 | 45 | 18.2% |
2vj6w3gm | The use of CPU, GPU and FPGA in real-time control of adaptive optics systems | 54 | 10 | 44 | 18.5% |
3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 52 | 6 | 46 | 11.5% |
56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 52 | 5 | 47 | 9.6% |
4gr3p2pf | Adaptive Optics Program at TMT | 51 | 15 | 36 | 29.4% |
2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 49 | 9 | 40 | 18.4% |
20x7p7qb | Recent Improvements to the Keck II Laser Guide Star Facility | 46 | 22 | 24 | 47.8% |
23w5v4vv | New Cophasing and AO strategies for an extremely large telescope dedicated to extremely high contrast: The Colossus Project | 46 | 13 | 33 | 28.3% |
217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 45 | 11 | 34 | 24.4% |
2zm625jk | Selex infrared sensors for astronomy – present and future | 45 | 3 | 42 | 6.7% |
3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 45 | 11 | 34 | 24.4% |
015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 44 | 12 | 32 | 27.3% |
7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 44 | 8 | 36 | 18.2% |
87f6s2zv | The GMT Dynamic Optical Simulation | 43 | 3 | 40 | 7.0% |
93x3m220 | Non common path aberration correction with non linear WFSs | 43 | 2 | 41 | 4.7% |
10b151nz | A New Slow Focus Sensor for GeMS | 42 | 4 | 38 | 9.5% |
8cg2r2p8 | PSF reconstruction for AO photometry and astrometry | 42 | 4 | 38 | 9.5% |
2mn1w74z | Point spread function determination for Keck adaptive optics: overview | 41 | 10 | 31 | 24.4% |
1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 40 | 3 | 37 | 7.5% |
1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 40 | 2 | 38 | 5.0% |
4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 40 | 14 | 26 | 35.0% |
5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 40 | 20 | 20 | 50.0% |
5q66922d | E-ELT M4 Unit updated design and prototype results | 39 | 13 | 26 | 33.3% |
6809n74d | Durham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs) | 38 | 6 | 32 | 15.8% |
2mq8n4d4 | First Results of the Ground Layer Adaptive Optics System ARGOS | 37 | 10 | 27 | 27.0% |
4h03k92b | Analysis of GeMS tip-tilt on-sky data: LQG implementation for vibration rejections | 37 | 11 | 26 | 29.7% |
4jh5c19s | Laboratory tests on HeNOS, the MCAO test bench for NFIRAOS | 37 | 2 | 35 | 5.4% |
5dg67931 | Analytical study of high altitude turbulence wide-field wavefront sensing: impact on the design and reconstruction quality of future solar AO systems | 37 | 3 | 34 | 8.1% |
62p140z1 | Measuring Segment Piston with a Non-Redundant Pupil Mask on the Giant Magellan Telescope | 37 | 3 | 34 | 8.1% |
80j280rv | Filtering the interaction matrix in an adaptive optics system | 37 | 3 | 34 | 8.1% |
7t06254q | GeMS, the path toward AO facility | 36 | 7 | 29 | 19.4% |
0gt3876k | SPHERE extreme AO system On-sky operation, final performance and future improvements | 35 | 9 | 26 | 25.7% |
2dm1m7jq | MCAO numerical simulations for EST: analysis and parameter optimization | 35 | 11 | 24 | 31.4% |
56p467d6 | Astrometry with MCAO at Gemini and at ELTs | 35 | 7 | 28 | 20.0% |
8nb0n5jf | Progress report on the ESO 4LGSF | 35 | 12 | 23 | 34.3% |
29g816zb | SPHERE extreme AO system On-sky operation, final performance and future improvements | 34 | 11 | 23 | 32.4% |
0bz8t4mv | Commissioning of ARGOS at LBT: adaptive optics procedures | 33 | 5 | 28 | 15.2% |
2mq7f7k6 | OCAM2S: an integral shutter ultrafast and low noise wavefront sensor camera for laser guide stars adaptive optics systems | 33 | 10 | 23 | 30.3% |
7774b5p6 | GMCAO for E-ELT: a feasibility study | 33 | 2 | 31 | 6.1% |
8p13k3zc | Reducing adaptive optics latency using many-core processors | 33 | 6 | 27 | 18.2% |
39h072gr | System analysis of the Segmented Pupil Experiment for Exoplanet Detection - SPEED - in view of the ELTs | 32 | 8 | 24 | 25.0% |
6h92z4q4 | Development of an ELT XAO testbed using a self referenced Mach-Zehnder wavefront sensor | 32 | 5 | 27 | 15.6% |
8d79v3t0 | XAO at LBT: current performances in the visible and upcoming upgrade | 32 | 4 | 28 | 12.5% |
3416j3cb | Effects of reconstruction layer profiles on atmospheric tomography in E-ELT AO systems | 31 | 5 | 26 | 16.1% |
42h0n70s | Implementation of SLODAR atmospheric turbulence profiling to the ARGOS system | 31 | 8 | 23 | 25.8% |
6317r29b | Near-infrared tip-tilt sensing at Keck: System architecture and on-sky performance | 31 | 3 | 28 | 9.7% |
7fr068zd | SHARK-NIR Channel: a high contrast imager with coronagraphic capabilities for the Large Binocular Telescope | 31 | 6 | 25 | 19.4% |
1df66431 | Resolving the low-mass content of Westerlund 1 using MCAO | 30 | 2 | 28 | 6.7% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.