UC Observatories

Parent: UCLA

eScholarship stats: History by Item for March through June, 2026

ItemTitleTotal requests2026-062026-052026-042026-03
9j80t4m1The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra928262244199223
5cf394whAdaptive Optics for Extremely Large Telescopes 4 - Program Booklet3949011390101
5qs0n1bcInnovations and advances in instrumentation at the W. M. Keck Observatory, vol. III3838912010569
2qw2m22gThe Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data382109939684
4058w3z1Final Targeting Strategy for the Sloan Digital Sky Survey IV Apache Point Observatory Galactic Evolution Experiment 2 North Survey3111051076138
2vj6w3gmThe use of CPU, GPU and FPGA in real-time control of adaptive optics systems29081836858
11f44236THE DEEP2 GALAXY REDSHIFT SURVEY: DESIGN, OBSERVATIONS, DATA REDUCTION, AND REDSHIFTS**Based on observations taken at the W. M. Keck Observatory, which is operated jointly by the University of California and the California Institute of Technology, and on observations made with the NASA/ESO Hubble Space Telescope, obtained from the data archives at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555, and from the Canadian Astronomy Data Centre.284591036953
23w5v4vvNew Cophasing and AO strategies for an extremely large telescope dedicated to extremely high contrast: The Colossus Project283531047254
44b7j2bqThe Lick AGN Monitoring Project 2016: Velocity-resolved Hβ Lags in Luminous Seyfert Galaxies283285553147
7zs2q9fvInferring the intergalactic medium neutral fraction at z ∼ 6–8 with low-luminosity Lyman break galaxies277661007140
93x3m220Non common path aberration correction with non linear WFSs26686865836
1pm0r30zThe Keck/DEIMOS Stellar Archive. I. Uniform Velocities and Metallicities for 78 Milky Way Dwarf Galaxies and Globular Clusters265257756107
015808kcMeasuring Segment Piston with a Dispersed Fringe Sensor on the Giant Magellan Telescope26340984679
4d77d3hkThe HETDEX Instrumentation: Hobby–Eberly Telescope Wide-field Upgrade and VIRUS26366657062
9xx3208wOn-sky results of Raven, a MOAO science demonstrator at Subaru Telescope26260915952
9fp0m8s1The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA-derived Quantities, Data Visualization Tools, and Stellar Library25864855554
1k41x51nINO Pyramidal Wavefront Sensor Demonstrator: first closed-loop on-sky operation at Mont-Mégantic Telescope25363795754
77f6c5hqSDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass25181487151
0gt3876kSPHERE extreme AO system On-sky operation, final performance and future improvements24656816445
4gr3p2pfAdaptive Optics Program at TMT24060745452
1j62j00jPypeIt: The Python Spectroscopic Data Reduction Pipeline22833815658
7t52h1r1Miniaturized Shack-Hartmann Wavefront-Sensors for ELTs22761626638
7m06d2jpGTC Follow-up Observations of Very Metal-poor Star Candidates from DESI22645736642
6r38q9vbPerformance assessment for the linear control of adaptive optics systems: noise propagation and temporal errors22330887728
0479k8m1Observations of the dynamic turbulence above La Palma using Stereo-SCIDAR22034796146
1367c5xwAnti-aliasing wave-front reconstruction with Shack-Hartmann sensors22046735348
20x7p7qbRecent Improvements to the Keck II Laser Guide Star Facility21744686144
16b4h26gUse of Laser Guide Star with Pyramid Wavefront Sensor21634875144
217686nzDesign and Development Status of MKID Integral Field Spectrographs for High Contrast Imaging21648655548
2cr972ktAligning the LINC-NIRVANA Natural Guide Stars MCAO system21638775150
8646z73cImproved Cosmological Constraints from New, Old, and Combined Supernova Data Sets21359714835
5616n854The Draco Dwarf Spheroidal Galaxy in the First Year of Dark Energy Spectroscopic Instrument Data21124854953
8w80k9spAn Integrated MASS/DIMM Monitor Based on a Low-Noise CCD Detector21136795541
3cq132qmPyramid versus Shack-Hartmann: Trade Study Results for the NFIRAOS NGS WFS20945655148
5n84b2z0Multi-conjugate Adaptive Optics at Big Bear Solar Observatory20861545340
7h46n1q2Lick Observatory Supernova Search follow-up program: photometry data release of 93 Type Ia supernovae20868544739
38s3v07sThe Hobby–Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections* * Based on observations obtained with the Hobby–Eberly Telescope, which is a joint project of the University of Texas at Austin, the Pennsylvania State University, Ludwig-Maximilians-Universität München, and Georg-August-Universität Göttingen.20549536142
2mq7f7k6OCAM2S: an integral shutter ultrafast and low noise wavefront sensor camera for laser guide stars adaptive optics systems20437726035
80j280rvFiltering the interaction matrix in an adaptive optics system20451764532
3gp3k4kgRetrieving tip-tilt information from Tomographic Laser Guide Star Adaptive Optics Systems20336715046
4s5364qpA Fresnel propagation analysis for SPEED (Segmented Pupil Experiment for Exoplanet Detection)19941556637
5t0211tnSCExAO: the first high contrast exoplanet imager on an ELT?19940574953
9q7259nnNon Boltzmann Modeling of Sodium Guidestar Returns and Implications for Guidestar Linewidth19939774835
0v44n629Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe19841654547
6809n74dDurham AO Real-time Controller (DARC) running on Graphics Processing Units (GPUs)19837495854
5vv5p369Self-Coherent Camera as a focal plane phasing sensor - Overview and early comparison with the Zernike Phase Contrast Sensor19538536638
56v9924zExperimental implementation of a Pyramid WFS: Towards the19440694738
5q66922dE-ELT M4 Unit updated design and prototype results19430574958
62p140z1Measuring Segment Piston with a Non-Redundant Pupil Mask on the Giant Magellan Telescope19342555244
81f1f8ptPrototyping the GMT phasing camera with the Magellan AO system19349524646

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