| Item | Title | Total requests | Download | View-only | %Dnld |
|---|---|---|---|---|---|
| 0479k8m1 | Observations of the dynamic turbulence above La Palma using Stereo-SCIDAR | 82 | 56 | 26 | 68.3% |
| 8nb0n5jf | Progress report on the ESO 4LGSF | 67 | 40 | 27 | 59.7% |
| 20x7p7qb | Recent Improvements to the Keck II Laser Guide Star Facility | 65 | 25 | 40 | 38.5% |
| 5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 64 | 20 | 44 | 31.3% |
| 015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 60 | 30 | 30 | 50.0% |
| 4gr3p2pf | Adaptive Optics Program at TMT | 60 | 31 | 29 | 51.7% |
| 2mn1w74z | Point spread function determination for Keck adaptive optics: overview | 58 | 21 | 37 | 36.2% |
| 2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 57 | 29 | 28 | 50.9% |
| 3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 57 | 22 | 35 | 38.6% |
| 758421jz | Laser Pointing Camera: a valuable tool for the LGS-AO operations | 57 | 34 | 23 | 59.6% |
| 51x9d368 | Calibrating the Non-Common Path Aberrations on the MOAO system RAVEN and | 55 | 33 | 22 | 60.0% |
| 56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 55 | 22 | 33 | 40.0% |
| 1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 53 | 24 | 29 | 45.3% |
| 7019b6vc | AO for MOSAIC, the E-ELT Multiple Object Spectrograph | 52 | 29 | 23 | 55.8% |
| 2mq7f7k6 | OCAM2S: an integral shutter ultrafast and low noise wavefront sensor camera for laser guide stars adaptive optics systems | 51 | 31 | 20 | 60.8% |
| 80j280rv | Filtering the interaction matrix in an adaptive optics system | 51 | 24 | 27 | 47.1% |
| 4jh5c19s | Laboratory tests on HeNOS, the MCAO test bench for NFIRAOS | 49 | 23 | 26 | 46.9% |
| 5q66922d | E-ELT M4 Unit updated design and prototype results | 49 | 26 | 23 | 53.1% |
| 93x3m220 | Non common path aberration correction with non linear WFSs | 48 | 17 | 31 | 35.4% |
| 5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 47 | 26 | 21 | 55.3% |
| 7kh262xf | Simulations of AO for the E-ELT and its instruments | 47 | 24 | 23 | 51.1% |
| 1367c5xw | Anti-aliasing wave-front reconstruction with Shack-Hartmann sensors | 46 | 13 | 33 | 28.3% |
| 8w80k9sp | An Integrated MASS/DIMM Monitor Based on a Low-Noise CCD Detector | 46 | 23 | 23 | 50.0% |
| 8x09340m | Dissecting Star-forming regions with the GeMS MCAO instrument: lessons learned for optimal post-processing of WFAO data | 45 | 20 | 25 | 44.4% |
| 0bz8t4mv | Commissioning of ARGOS at LBT: adaptive optics procedures | 44 | 24 | 20 | 54.5% |
| 0gt3876k | SPHERE extreme AO system On-sky operation, final performance and future improvements | 44 | 21 | 23 | 47.7% |
| 3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 44 | 13 | 31 | 29.5% |
| 7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 44 | 17 | 27 | 38.6% |
| 1h5301vq | Coupling of WFS with a segmented DM “Test of different concepts: SH, Pyramid, Zernike phase sensor” | 43 | 20 | 23 | 46.5% |
| 2mq8n4d4 | First Results of the Ground Layer Adaptive Optics System ARGOS | 43 | 20 | 23 | 46.5% |
| 3416j3cb | Effects of reconstruction layer profiles on atmospheric tomography in E-ELT AO systems | 43 | 21 | 22 | 48.8% |
| 6cr4288r | Preliminary design of the MICADO calibration unit | 43 | 21 | 22 | 48.8% |
| 8ft440wn | Optimizing LGS WFS Pixel Processing in the Context of Evolving Turbulence and Sodium Profile | 43 | 19 | 24 | 44.2% |
| 16b4h26g | Use of Laser Guide Star with Pyramid Wavefront Sensor | 42 | 16 | 26 | 38.1% |
| 217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 41 | 7 | 34 | 17.1% |
| 23w5v4vv | New Cophasing and AO strategies for an extremely large telescope dedicated to extremely high contrast: The Colossus Project | 41 | 17 | 24 | 41.5% |
| 6h92z4q4 | Development of an ELT XAO testbed using a self referenced Mach-Zehnder wavefront sensor | 41 | 24 | 17 | 58.5% |
| 4s5364qp | A Fresnel propagation analysis for SPEED (Segmented Pupil Experiment for Exoplanet Detection) | 40 | 19 | 21 | 47.5% |
| 6js4k5m5 | Commissioning of ARGOS at LBT: adaptive optics procedures | 40 | 20 | 20 | 50.0% |
| 087701qh | Development of multi time-step tomographic reconstruction with RAVEN | 39 | 14 | 25 | 35.9% |
| 5gz5j6jm | Precise and deep photometry from the ground: on-sky science performance of MCAO | 39 | 20 | 19 | 51.3% |
| 1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 38 | 9 | 29 | 23.7% |
| 2dm1m7jq | MCAO numerical simulations for EST: analysis and parameter optimization | 38 | 12 | 26 | 31.6% |
| 42h0n70s | Implementation of SLODAR atmospheric turbulence profiling to the ARGOS system | 38 | 14 | 24 | 36.8% |
| 4h03k92b | Analysis of GeMS tip-tilt on-sky data: LQG implementation for vibration rejections | 38 | 14 | 24 | 36.8% |
| 4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 38 | 15 | 23 | 39.5% |
| 87f6s2zv | The GMT Dynamic Optical Simulation | 38 | 9 | 29 | 23.7% |
| 910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 38 | 7 | 31 | 18.4% |
| 2vj6w3gm | The use of CPU, GPU and FPGA in real-time control of adaptive optics systems | 37 | 6 | 31 | 16.2% |
| 6809n74d | Durham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs) | 37 | 6 | 31 | 16.2% |
Note: Due to the evolving nature of web traffic, the data presented here should be considered approximate and subject to revision. Learn more.