Adaptive Optics for Extremely Large Telescopes 4 – Conference Proceedings
Parent: UC Observatories
eScholarship stats: Breakdown by Item for January through April, 2024
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 76 | 44 | 32 | 57.9% |
| 80j280rv | Filtering the interaction matrix in an adaptive optics system | 58 | 2 | 56 | 3.4% |
| 93x3m220 | Non common path aberration correction with non linear WFSs | 52 | 11 | 41 | 21.2% |
| 64r6t2cm | Coupling of WFS with a segmented DM “Test of different concepts: SH, Pyramid, Zernike phase sensor” | 51 | 5 | 46 | 9.8% |
| 015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 48 | 6 | 42 | 12.5% |
| 1367c5xw | Anti-aliasing wave-front reconstruction with Shack-Hartmann sensors | 46 | 5 | 41 | 10.9% |
| 7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 46 | 11 | 35 | 23.9% |
| 5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 45 | 20 | 25 | 44.4% |
| 6317r29b | Near-infrared tip-tilt sensing at Keck: System architecture and on-sky performance | 44 | 10 | 34 | 22.7% |
| 8nb0n5jf | Progress report on the ESO 4LGSF | 44 | 22 | 22 | 50.0% |
| 1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 42 | 4 | 38 | 9.5% |
| 56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 41 | 4 | 37 | 9.8% |
| 20x7p7qb | Recent Improvements to the Keck II Laser Guide Star Facility | 39 | 8 | 31 | 20.5% |
| 3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 39 | 7 | 32 | 17.9% |
| 2vj6w3gm | The use of CPU, GPU and FPGA in real-time control of adaptive optics systems | 38 | 6 | 32 | 15.8% |
| 20s3w2j6 | Laser guide star adaptive optics at Lick Observatory | 37 | 15 | 22 | 40.5% |
| 217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 37 | 8 | 29 | 21.6% |
| 2zm625jk | Selex infrared sensors for astronomy – present and future | 37 | 11 | 26 | 29.7% |
| 8cg2r2p8 | PSF reconstruction for AO photometry and astrometry | 36 | 7 | 29 | 19.4% |
| 2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 35 | 9 | 26 | 25.7% |
| 3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 35 | 3 | 32 | 8.6% |
| 4gr3p2pf | Adaptive Optics Program at TMT | 35 | 19 | 16 | 54.3% |
| 6809n74d | Durham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs) | 35 | 12 | 23 | 34.3% |
| 6gk7874j | Tip-tilt modelling and control for GeMS: a performance comparison of identification techniques | 35 | 6 | 29 | 17.1% |
| 910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 33 | 11 | 22 | 33.3% |
| 4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 32 | 8 | 24 | 25.0% |
| 8ft440wn | Optimizing LGS WFS Pixel Processing in the Context of Evolving Turbulence and Sodium Profile | 32 | 8 | 24 | 25.0% |
| 8d79v3t0 | XAO at LBT: current performances in the visible and upcoming upgrade | 31 | 6 | 25 | 19.4% |
| 8x09340m | Dissecting Star-forming regions with the GeMS MCAO instrument: lessons learned for optimal post-processing of WFAO data | 31 | 5 | 26 | 16.1% |
| 0gt3876k | SPHERE extreme AO system On-sky operation, final performance and future improvements | 30 | 12 | 18 | 40.0% |
| 9xx3208w | On-sky results of Raven, a MOAO science demonstrator at Subaru Telescope | 30 | 7 | 23 | 23.3% |
| 42h0n70s | Implementation of SLODAR atmospheric turbulence profiling to the ARGOS system | 29 | 7 | 22 | 24.1% |
| 6js4k5m5 | Commissioning of ARGOS at LBT: adaptive optics procedures | 29 | 4 | 25 | 13.8% |
| 8wj5p4cc | Modeling the pyramidal sensor by a ZEMAXTM user defined surface. | 29 | 2 | 27 | 6.9% |
| 1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 28 | 8 | 20 | 28.6% |
| 29g816zb | SPHERE extreme AO system On-sky operation, final performance and future improvements | 27 | 3 | 24 | 11.1% |
| 3416j3cb | Effects of reconstruction layer profiles on atmospheric tomography in E-ELT AO systems | 27 | 8 | 19 | 29.6% |
| 6r38q9vb | Performance assessment for the linear control of adaptive optics systems: noise propagation and temporal errors | 27 | 2 | 25 | 7.4% |
| 8sq053mx | Progress with the 4m high-order AO demonstrator, CHOUGH | 27 | 8 | 19 | 29.6% |
| 23w5v4vv | New Cophasing and AO strategies for an extremely large telescope dedicated to extremely high contrast: The Colossus Project | 26 | 6 | 20 | 23.1% |
| 51x9d368 | Calibrating the Non-Common Path Aberrations on the MOAO system RAVEN and | 26 | 6 | 20 | 23.1% |
| 6sc7h6r2 | Optical calibration of the M4 prototype toward the final unit | 26 | 6 | 20 | 23.1% |
| 7t06254q | GeMS, the path toward AO facility | 26 | 7 | 19 | 26.9% |
| 7bf187rg | Deformable Mirrors developments at ESO | 25 | 6 | 19 | 24.0% |
| 81f1f8pt | Prototyping the GMT phasing camera with the Magellan AO system | 25 | 3 | 22 | 12.0% |
| 2mn1w74z | Point spread function determination for Keck adaptive optics: overview | 24 | 2 | 22 | 8.3% |
| 3cq132qm | Pyramid versus Shack-Hartmann: Trade Study Results for the NFIRAOS NGS WFS | 24 | 2 | 22 | 8.3% |
| 5dg67931 | Analytical study of high altitude turbulence wide-field wavefront sensing: impact on the design and reconstruction quality of future solar AO systems | 24 | 5 | 19 | 20.8% |
| 5q66922d | E-ELT M4 Unit updated design and prototype results | 24 | 3 | 21 | 12.5% |
| 7f60s89n | Optimizing use of multiple stars for near-infrared tip-tilt compensation at the W. M. Keck Observatory | 24 | 4 | 20 | 16.7% |
Disclaimer: due to the evolving nature of the web traffic we receive and the methods we use to collate it, the data presented here should be considered approximate and subject to revision.