| Item | Title | Total requests | 2024-09 | 2024-08 | 2024-07 | 2024-06 |
|---|---|---|---|---|---|---|
| 0479k8m1 | Observations of the dynamic turbulence above La Palma using Stereo-SCIDAR | 70 | 17 | 23 | 19 | 11 |
| 80j280rv | Filtering the interaction matrix in an adaptive optics system | 65 | 6 | 19 | 18 | 22 |
| 8nb0n5jf | Progress report on the ESO 4LGSF | 62 | 8 | 25 | 21 | 8 |
| 4gr3p2pf | Adaptive Optics Program at TMT | 60 | 5 | 28 | 16 | 11 |
| 2mn1w74z | Point spread function determination for Keck adaptive optics: overview | 59 | 10 | 16 | 20 | 13 |
| 015808kc | Measuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope | 57 | 9 | 17 | 21 | 10 |
| 4s5364qp | A Fresnel propagation analysis for SPEED (Segmented Pupil Experiment for Exoplanet Detection) | 56 | 2 | 18 | 13 | 23 |
| 51x9d368 | Calibrating the Non-Common Path Aberrations on the MOAO system RAVEN and | 55 | 1 | 30 | 17 | 7 |
| 5cf394wh | Adaptive Optics for Extremely Large Telescopes 4 - Program Booklet | 53 | 8 | 15 | 15 | 15 |
| 16b4h26g | Use of Laser Guide Star with Pyramid Wavefront Sensor | 52 | 6 | 8 | 19 | 19 |
| 93x3m220 | Non common path aberration correction with non linear WFSs | 52 | 3 | 21 | 13 | 15 |
| 1qh5b3v0 | Commissioning ShARCS: the Shane Adaptive optics infraRed Camera-Spectrograph for the Lick Observatory 3-m telescope | 51 | 2 | 24 | 15 | 10 |
| 20x7p7qb | Recent Improvements to the Keck II Laser Guide Star Facility | 51 | 4 | 10 | 23 | 14 |
| 56v9924z | Experimental implementation of a Pyramid WFS: Towards the | 51 | 7 | 19 | 14 | 11 |
| 7019b6vc | AO for MOSAIC, the E-ELT Multiple Object Spectrograph | 51 | 2 | 29 | 12 | 8 |
| 1367c5xw | Anti-aliasing wave-front reconstruction with Shack-Hartmann sensors | 50 | 4 | 18 | 17 | 11 |
| 6cr4288r | Preliminary design of the MICADO calibration unit | 50 | 4 | 10 | 21 | 15 |
| 8w80k9sp | An Integrated MASS/DIMM Monitor Based on a Low-Noise CCD Detector | 49 | 3 | 18 | 19 | 9 |
| 2cr972kt | Aligning the LINC-NIRVANA Natural Guide Stars MCAO system | 48 | 5 | 19 | 18 | 6 |
| 2mq7f7k6 | OCAM2S: an integral shutter ultrafast and low noise wavefront sensor camera for laser guide stars adaptive optics systems | 48 | 6 | 21 | 15 | 6 |
| 4jh5c19s | Laboratory tests on HeNOS, the MCAO test bench for NFIRAOS | 48 | 4 | 22 | 15 | 7 |
| 758421jz | Laser Pointing Camera: a valuable tool for the LGS-AO operations | 48 | 8 | 18 | 19 | 3 |
| 3wq362xn | Adaptive Optics Point Spread Function Reconstruction at W. M. Keck Observatory in Laser & Natural Guide Star Modes : Final Developments | 47 | 2 | 20 | 17 | 8 |
| 5n84b2z0 | Multi-conjugate Adaptive Optics at Big Bear Solar Observatory | 47 | 8 | 16 | 15 | 8 |
| 3416j3cb | Effects of reconstruction layer profiles on atmospheric tomography in E-ELT AO systems | 46 | 1 | 16 | 17 | 12 |
| 7kh262xf | Simulations of AO for the E-ELT and its instruments | 46 | 1 | 19 | 18 | 8 |
| 0bz8t4mv | Commissioning of ARGOS at LBT: adaptive optics procedures | 45 | 1 | 17 | 17 | 10 |
| 3gp3k4kg | Retrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems | 45 | 7 | 10 | 18 | 10 |
| 6317r29b | Near-infrared tip-tilt sensing at Keck: System architecture and on-sky performance | 45 | 3 | 13 | 14 | 15 |
| 8ft440wn | Optimizing LGS WFS Pixel Processing in the Context of Evolving Turbulence and Sodium Profile | 45 | 4 | 16 | 17 | 8 |
| 8x09340m | Dissecting Star-forming regions with the GeMS MCAO instrument: lessons learned for optimal post-processing of WFAO data | 44 | 2 | 17 | 17 | 8 |
| 1h5301vq | Coupling of WFS with a segmented DM “Test of different concepts: SH, Pyramid, Zernike phase sensor” | 43 | 2 | 20 | 15 | 6 |
| 7t52h1r1 | Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs | 43 | 11 | 11 | 12 | 9 |
| 0gt3876k | SPHERE extreme AO system On-sky operation, final performance and future improvements | 42 | 1 | 18 | 15 | 8 |
| 2mq8n4d4 | First Results of the Ground Layer Adaptive Optics System ARGOS | 42 | 2 | 19 | 15 | 6 |
| 5q66922d | E-ELT M4 Unit updated design and prototype results | 42 | 6 | 17 | 14 | 5 |
| 910646qf | Low Wind Effect, the main limitation of the SPHERE instrument | 41 | 7 | 8 | 12 | 14 |
| 2zm625jk | Selex infrared sensors for astronomy – present and future | 39 | 5 | 7 | 9 | 18 |
| 666710ff | Science operation of the SOAR Adaptive Module (SAM) | 39 | 7 | 7 | 19 | 6 |
| 6h92z4q4 | Development of an ELT XAO testbed using a self referenced Mach-Zehnder wavefront sensor | 39 | 3 | 15 | 16 | 5 |
| 9q7259nn | Non Boltzmann Modeling of Sodium Guidestar Returns and Implications for Guidestar Linewidth | 39 | 1 | 20 | 11 | 7 |
| 217686nz | Design and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging | 38 | 5 | 7 | 14 | 12 |
| 42h0n70s | Implementation of SLODAR atmospheric turbulence profiling to the ARGOS system | 38 | 4 | 12 | 15 | 7 |
| 6js4k5m5 | Commissioning of ARGOS at LBT: adaptive optics procedures | 38 | 2 | 17 | 13 | 6 |
| 087701qh | Development of multi time-step tomographic reconstruction with RAVEN | 37 | 4 | 9 | 18 | 6 |
| 1k41x51n | INO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope | 37 | 4 | 8 | 18 | 7 |
| 20s3w2j6 | Laser guide star adaptive optics at Lick Observatory | 37 | 3 | 11 | 12 | 11 |
| 3cq132qm | Pyramid versus Shack-Hartmann: Trade Study Results for the NFIRAOS NGS WFS | 37 | 2 | 9 | 16 | 10 |
| 4p4339x0 | State of the art IR cameras for wavefront sensing using e-APD MCT arrays | 36 | 3 | 9 | 14 | 10 |
| 5gz5j6jm | Precise and deep photometry from the ground: on-sky science performance of MCAO | 36 | 16 | 14 | 6 |
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