Adaptive Optics for Extremely Large Telescopes 4 – Conference Proceedings
Parent: UC Observatories
eScholarship stats: History by Item for January through April, 2024
| Item | Title | Total requests | 2024-04 | 2024-03 | 2024-02 | 2024-01 |
|---|---|---|---|---|---|---|
| 5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 76 | 19 | 19 | 11 | 27 |
| 80j280rv | Filtering the interaction matrix in an adaptive optics system | 58 | 23 | 11 | 15 | 9 |
| 93x3m220 | Non common path aberration correction with non linear WFSs | 52 | 15 | 9 | 11 | 17 |
| 64r6t2cm | Coupling of WFS with a segmented DM “Test of different concepts: SH, Pyramid, Zernike phase sensor” | 51 | 40 | 2 | 5 | 4 |
| 015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 48 | 14 | 8 | 8 | 18 |
| 1367c5xw | Anti-aliasing wave-front reconstruction with Shack-Hartmann sensors | 46 | 19 | 7 | 10 | 10 |
| 7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 46 | 16 | 3 | 11 | 16 |
| 5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 45 | 13 | 9 | 8 | 15 |
| 6317r29b | Near-infrared tip-tilt sensing at Keck: System architecture and on-sky performance | 44 | 13 | 8 | 8 | 15 |
| 8nb0n5jf | Progress report on the ESO 4LGSF | 44 | 14 | 10 | 8 | 12 |
| 1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 42 | 17 | 7 | 5 | 13 |
| 56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 41 | 13 | 11 | 7 | 10 |
| 20x7p7qb | Recent Improvements to the Keck II Laser Guide Star Facility | 39 | 17 | 7 | 8 | 7 |
| 3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 39 | 18 | 4 | 8 | 9 |
| 2vj6w3gm | The use of CPU, GPU and FPGA in real-time control of adaptive optics systems | 38 | 14 | 10 | 8 | 6 |
| 20s3w2j6 | Laser guide star adaptive optics at Lick Observatory | 37 | 12 | 10 | 12 | 3 |
| 217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 37 | 17 | 5 | 8 | 7 |
| 2zm625jk | Selex infrared sensors for astronomy – present and future | 37 | 13 | 12 | 7 | 5 |
| 8cg2r2p8 | PSF reconstruction for AO photometry and astrometry | 36 | 10 | 10 | 6 | 10 |
| 2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 35 | 14 | 4 | 2 | 15 |
| 3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 35 | 12 | 10 | 5 | 8 |
| 4gr3p2pf | Adaptive Optics Program at TMT | 35 | 12 | 8 | 6 | 9 |
| 6809n74d | Durham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs) | 35 | 12 | 8 | 7 | 8 |
| 6gk7874j | Tip-tilt modelling and control for GeMS: a performance comparison of identification techniques | 35 | 17 | 2 | 4 | 12 |
| 910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 33 | 16 | 9 | 4 | 4 |
| 4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 32 | 11 | 6 | 7 | 8 |
| 8ft440wn | Optimizing LGS WFS Pixel Processing in the Context of Evolving Turbulence and Sodium Profile | 32 | 9 | 10 | 3 | 10 |
| 8d79v3t0 | XAO at LBT: current performances in the visible and upcoming upgrade | 31 | 12 | 1 | 3 | 15 |
| 8x09340m | Dissecting Star-forming regions with the GeMS MCAO instrument: lessons learned for optimal post-processing of WFAO data | 31 | 12 | 3 | 4 | 12 |
| 0gt3876k | SPHERE extreme AO system On-sky operation, final performance and future improvements | 30 | 15 | 3 | 5 | 7 |
| 9xx3208w | On-sky results of Raven, a MOAO science demonstrator at Subaru Telescope | 30 | 13 | 4 | 6 | 7 |
| 42h0n70s | Implementation of SLODAR atmospheric turbulence profiling to the ARGOS system | 29 | 10 | 2 | 6 | 11 |
| 6js4k5m5 | Commissioning of ARGOS at LBT: adaptive optics procedures | 29 | 9 | 4 | 10 | 6 |
| 8wj5p4cc | Modeling the pyramidal sensor by a ZEMAXTM user defined surface. | 29 | 13 | 2 | 5 | 9 |
| 1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 28 | 12 | 2 | 4 | 10 |
| 29g816zb | SPHERE extreme AO system On-sky operation, final performance and future improvements | 27 | 11 | 6 | 5 | 5 |
| 3416j3cb | Effects of reconstruction layer profiles on atmospheric tomography in E-ELT AO systems | 27 | 14 | 2 | 5 | 6 |
| 6r38q9vb | Performance assessment for the linear control of adaptive optics systems: noise propagation and temporal errors | 27 | 8 | 6 | 8 | 5 |
| 8sq053mx | Progress with the 4m high-order AO demonstrator, CHOUGH | 27 | 12 | 4 | 5 | 6 |
| 23w5v4vv | New Cophasing and AO strategies for an extremely large telescope dedicated to extremely high contrast: The Colossus Project | 26 | 15 | 4 | 3 | 4 |
| 51x9d368 | Calibrating the Non-Common Path Aberrations on the MOAO system RAVEN and | 26 | 14 | 2 | 3 | 7 |
| 6sc7h6r2 | Optical calibration of the M4 prototype toward the final unit | 26 | 9 | 2 | 5 | 10 |
| 7t06254q | GeMS, the path toward AO facility | 26 | 11 | 5 | 10 | |
| 7bf187rg | Deformable Mirrors developments at ESO | 25 | 10 | 3 | 4 | 8 |
| 81f1f8pt | Prototyping the GMT phasing camera with the Magellan AO system | 25 | 14 | 4 | 5 | 2 |
| 2mn1w74z | Point spread function determination for Keck adaptive optics: overview | 24 | 9 | 4 | 4 | 7 |
| 3cq132qm | Pyramid versus Shack-Hartmann: Trade Study Results for the NFIRAOS NGS WFS | 24 | 13 | 1 | 3 | 7 |
| 5dg67931 | Analytical study of high altitude turbulence wide-field wavefront sensing: impact on the design and reconstruction quality of future solar AO systems | 24 | 7 | 6 | 3 | 8 |
| 5q66922d | E-ELT M4 Unit updated design and prototype results | 24 | 10 | 4 | 6 | 4 |
| 7f60s89n | Optimizing use of multiple stars for near-infrared tip-tilt compensation at the W. M. Keck Observatory | 24 | 9 | 4 | 3 | 8 |
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