M
Marcos A. van Dam
Researcher at W.M. Keck Observatory
Publications - 36
Citations - 606
Marcos A. van Dam is an academic researcher from W.M. Keck Observatory. The author has contributed to research in topics: Adaptive optics & Wavefront. The author has an hindex of 11, co-authored 36 publications receiving 537 citations. Previous affiliations of Marcos A. van Dam include University of Canterbury.
Papers
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Journal ArticleDOI
A low density of 0.8 g cm(-3) for the Trojan binary asteroid 617 Patroclus.
Franck Marchis,Daniel Hestroffer,P. Descamps,Jérôme Berthier,A. H. Bouchez,Randall D. Campbell,Jason C. Y. Chin,Marcos A. van Dam,S. K. Hartman,Erik M. Johansson,R. Lafon,David Le Mignant,Imke de Pater,Paul J. Stomski,Doug Summers,Frédéric Vachier,Peter L. Wizinovich,Michael H. Wong +17 more
TL;DR: It is reported that the components of 617 Patroclus move around the system's centre of mass, describing a roughly circular orbit, and a very low density is derived, suggesting that they could have been formed in the outer part of the Solar System.
Journal ArticleDOI
Experimental verification of the frozen flow atmospheric turbulence assumption with use of astronomical adaptive optics telemetry
TL;DR: Open-loop deformable mirror telemetry from Altair and Keck adaptive optics is used to determine whether atmospheric turbulence follows the frozen flow hypothesis, indicating that the atmosphere is stable enough for predictive control to measure and adapt to prevailing atmospheric conditions before they change.
Journal ArticleDOI
Dispersed fringe sensor for the Giant Magellan Telescope.
TL;DR: This paper shows that using four off-axis DFSs operating at J-band with 10 ms exposures, this paper is able to measure segment piston to the required 50 nm accuracy every 30 s with over 90% sky coverage.
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Wave-front sensing from defocused images by use of wave-front slopes
TL;DR: A novel technique for deriving wave-front aberrations from two defocused intensity measurements based on the evolution of the cumulative density function of the intensity with light propagation, which requires use of a Radon transform.
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Modeling low order aberrations in laser guide star adaptive optics systems
TL;DR: This paper uses a model to characterize the LGS aberrations as a function of pupil angle, elevation, sodium structure, uplink tip/tilt error, detector field of view, the number of detector pixels, and seeing, and employs the model to estimate the L GSAberrations for the Palomar LGS AO system, the planned Keck I and the Thirty Meter Telescope AO systems.