Adaptive Optics for Extremely Large Telescopes 4 – Conference Proceedings
Parent: UC Observatories
eScholarship stats: Breakdown by Item for January through April, 2025
| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 64 | 13 | 51 | 20.3% |
| 217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 62 | 11 | 51 | 17.7% |
| 2vj6w3gm | The use of CPU, GPU and FPGA in real-time control of adaptive optics systems | 58 | 6 | 52 | 10.3% |
| 3cq132qm | Pyramid versus Shack-Hartmann: Trade Study Results for the NFIRAOS NGS WFS | 58 | 6 | 52 | 10.3% |
| 4gr3p2pf | Adaptive Optics Program at TMT | 58 | 18 | 40 | 31.0% |
| 4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 57 | 9 | 48 | 15.8% |
| 8nb0n5jf | Progress report on the ESO 4LGSF | 55 | 9 | 46 | 16.4% |
| 1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 53 | 9 | 44 | 17.0% |
| 3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 51 | 7 | 44 | 13.7% |
| 015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 50 | 14 | 36 | 28.0% |
| 10b151nz | A New Slow Focus Sensor for GeMS | 49 | 5 | 44 | 10.2% |
| 1367c5xw | Anti-aliasing wave-front reconstruction with Shack-Hartmann sensors | 49 | 7 | 42 | 14.3% |
| 56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 49 | 5 | 44 | 10.2% |
| 5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 49 | 10 | 39 | 20.4% |
| 7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 48 | 10 | 38 | 20.8% |
| 9q7259nn | Non Boltzmann Modeling of Sodium Guidestar Returns and Implications for Guidestar Linewidth | 47 | 3 | 44 | 6.4% |
| 81f1f8pt | Prototyping the GMT phasing camera with the Magellan AO system | 45 | 8 | 37 | 17.8% |
| 93x3m220 | Non common path aberration correction with non linear WFSs | 45 | 9 | 36 | 20.0% |
| 2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 44 | 6 | 38 | 13.6% |
| 2zm625jk | Selex infrared sensors for astronomy – present and future | 44 | 3 | 41 | 6.8% |
| 5q66922d | E-ELT M4 Unit updated design and prototype results | 44 | 9 | 35 | 20.5% |
| 1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 43 | 5 | 38 | 11.6% |
| 20s3w2j6 | Laser guide star adaptive optics at Lick Observatory | 43 | 9 | 34 | 20.9% |
| 20x7p7qb | Recent Improvements to the Keck II Laser Guide Star Facility | 43 | 7 | 36 | 16.3% |
| 27q2v4s7 | Variation around the Pyramid theme: optical recombination and optimal use of photons | 43 | 8 | 35 | 18.6% |
| 910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 43 | 6 | 37 | 14.0% |
| 1x2266wp | Optical design of the Post Focal Relay of MAORY | 42 | 13 | 29 | 31.0% |
| 80j280rv | Filtering the interaction matrix in an adaptive optics system | 42 | 7 | 35 | 16.7% |
| 7t06254q | GeMS, the path toward AO facility | 41 | 6 | 35 | 14.6% |
| 29g816zb | SPHERE extreme AO system On-sky operation, final performance and future improvements | 40 | 10 | 30 | 25.0% |
| 3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 40 | 3 | 37 | 7.5% |
| 6js4k5m5 | Commissioning of ARGOS at LBT: adaptive optics procedures | 40 | 13 | 27 | 32.5% |
| 8cg2r2p8 | PSF reconstruction for AO photometry and astrometry | 40 | 5 | 35 | 12.5% |
| 8d79v3t0 | XAO at LBT: current performances in the visible and upcoming upgrade | 40 | 4 | 36 | 10.0% |
| 5t0211tn | SCExAO: the first high contrast exoplanet imager on an ELT? | 39 | 4 | 35 | 10.3% |
| 6809n74d | Durham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs) | 39 | 5 | 34 | 12.8% |
| 6r38q9vb | Performance assessment for the linear control of adaptive optics systems: noise propagation and temporal errors | 39 | 10 | 29 | 25.6% |
| 6sc7h6r2 | Optical calibration of the M4 prototype toward the final unit | 39 | 7 | 32 | 17.9% |
| 7019b6vc | AO for MOSAIC, the E-ELT Multiple Object Spectrograph | 39 | 5 | 34 | 12.8% |
| 0bz8t4mv | Commissioning of ARGOS at LBT: adaptive optics procedures | 38 | 5 | 33 | 13.2% |
| 2mq7f7k6 | OCAM2S: an integral shutter ultrafast and low noise wavefront sensor camera for laser guide stars adaptive optics systems | 38 | 11 | 27 | 28.9% |
| 56p467d6 | Astrometry with MCAO at Gemini and at ELTs | 38 | 8 | 30 | 21.1% |
| 8wj5p4cc | Modeling the pyramidal sensor by a ZEMAXTM user defined surface. | 38 | 7 | 31 | 18.4% |
| 2mq8n4d4 | First Results of the Ground Layer Adaptive Optics System ARGOS | 37 | 4 | 33 | 10.8% |
| 377606h0 | Statistical and morphological analysis of mock galactic fields in the Global-MCAO perspective | 37 | 7 | 30 | 18.9% |
| 5dg67931 | Analytical study of high altitude turbulence wide-field wavefront sensing: impact on the design and reconstruction quality of future solar AO systems | 37 | 7 | 30 | 18.9% |
| 8w80k9sp | An Integrated MASS/DIMM Monitor Based on a Low-Noise CCD Detector | 37 | 5 | 32 | 13.5% |
| 087701qh | Development of multi time-step tomographic reconstruction with RAVEN | 36 | 3 | 33 | 8.3% |
| 42h0n70s | Implementation of SLODAR atmospheric turbulence profiling to the ARGOS system | 36 | 8 | 28 | 22.2% |
| 6gk7874j | Tip-tilt modelling and control for GeMS: a performance comparison of identification techniques | 36 | 6 | 30 | 16.7% |
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