Zobrazeno 1 - 10
of 22
pro vyhledávání: '"D. S. Acton"'
Autor:
Claire E. Max, Peter Wizinowich, Andrea M. Ghez, Bruce Macintosh, Donald T. Gavel, Olivier Lai, D. S. Acton, Henry G. Roe, I. de Pater, Paul J. Stomski, Seran G. Gibbard
Publikováno v:
The Astronomical Journal. 125:364-375
We report on observations obtained with the adaptive optics system at the 10 m Keck II Telescope during engineering validation and early science observing time for the adaptive optics system. We observed Neptune at near-infrared wavelengths. Angular
Autor:
James E. Larkin, K. Ho, K. Tsubota, William Lupton, James M. Brase, C. Shelton, Claire E. Max, Paul J. Stomski, D. S. Acton, Donald T. Gavel, Andrea M. Ghez, Scot S. Olivier, Jong R. An, Kenneth Avicola, J. Gathright, Bruce Macintosh, Peter Wizinowich, Olivier Lai
Publikováno v:
Scopus-Elsevier
Adaptive optics (AO) is a technology that corrects in real time for the blurring effects of atmospheric turbulence, in principle allowing Earth‐bound telescopes to achieve their diffraction limit and to “see” as clearly as if they were in space
Autor:
Michelle Creech-Eakman, Charles Beichman, R. R. Thompson, B. C. Berkey, A. Tumminello, E. Hovland, Richard L. Johnson, T. Panteleeva, G. Hardy, A. Niessner, James Wallace, W. Dahl, J. Chin, J. Beletic, Eugene Serabyn, G. Eychaner, Andrew F. Boden, A. I. Sargent, Andy C. Rudeen, B. Parvin, R. Kendrick, Mark R. Swain, Dean L. Palmer, James D. Moore, Michael Shao, M. Mark Colavita, D. McBride, Peter Wizinowich, Christopher R. Neyman, E. R. Ligon, Rachel Akeson, H. A. Lewis, Erik M. Johansson, D. Chan, F. Vescelus, Christopher G. Paine, L. Reder, William Lupton, Christopher D. Koresko, Andrew Cooper, Michael Hess, G. Vasisht, C. Felizardo, Richard Cohen, M. Abajian, R. Smythe, Samuel L. Crawford, Jean Garcia-Gathright, T. Saloga, K. Summers, G. T. van Belle, Drew Medeiros, E. Appleby, C. Tyau, P. Kurpis, J. Walker, Rafael Millan-Gabet, J. Gathright, R. Boutell, Craig E. Nance, H. Henderson, K. Tsubota, J. Vause, A. J. Booth, J. Herstein, P. Swanson, Julien Woillez, B. Smith, J. Berlin, M. Papin, E. Wetherell, J. Kelley, D. Le Mignant, D. S. Acton, J. Bell, S. Ragland, David Morrison, U. Wehmeier, Paul J. Stomski, Frederic H. Chaffee, Bertrand Mennesson, J. Chock, M. Hrynevych, James L. Fanson
The Keck Interferometer (KI) combined the two 10 m W. M. Keck Observatory telescopes on Mauna Kea, Hawaii, as a long-baseline near- and mid-infrared interferometer. Funded by NASA, it operated from 2001 until 2012. KI used adaptive optics on the two
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bdd8b57d6cb764b47daf2946b2f0e7b2
https://resolver.caltech.edu/CaltechAUTHORS:20131203-090250079
https://resolver.caltech.edu/CaltechAUTHORS:20131203-090250079
Autor:
J. S. Knight, Bruce Hardy, P. Finley, D. S. Acton, Benjamin Gallagher, Allison Barto, Paul A. Lightsey
Publikováno v:
Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave.
The James Webb Space Telescope (JWST) telescope's secondary mirror and eighteen primary mirror segments are each actively controlled in rigid body position via six hexapod actuators. The mirrors are stowed to the mirror support structure to survive t
Autor:
J.W.B. de Groot, C. J. M. Lips, J. W. M. Hoppener, D. S. Acton, W. van Veelen, Thera P. Links, Robert M.W. Hofstra
Publikováno v:
Journal of internal medicine. 266(1)
The clinical management of patients with persistent or recurrent medullary thyroid carcinoma (MTC) is still under debate, because these patients either have a long-term survival, due to an indolent course of the disease, or develop rapidly progressin
Autor:
Sung-Soo Kim, Russel White, Peter Wizinowich, James E. Larkin, James R. Graham, Claire E. Max, James P. Lloyd, Jennifer Patience, Lisa Prato, Bruce Macintosh, Michael C. Liu, Ian S. McLean, D. S. Acton, C. McCabe, Brian J. Bauman, Scot S. Olivier, Andrea M. Ghez, D. Gavel
A combination of high-resolution and wide-field imaging reveals two binary stars and one triple star system among the sample of the first 11 stars with planets detected by radial velocity variations. High resolution speckle or adaptive optics (AO) da
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa9969ddb596657d86d8b623b6afb1b7
Autor:
Paul J. Stomski, Andrea M. Ghez, Peter Wizinowich, Olivier Lai, Robert K. Pina, D. S. Acton, Charles M. Telesco, Lisa Prato, R. S. Fisher
This paper presents diffraction-limited 1-18 micron images of the young quadruple star system HD 98800 obtained with the W. M. Keck 10-m telescopes using speckle and adaptive optics imaging at near-IR wavelengths and direct imaging at mid-IR waveleng
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ea40ffec5773f5a3c05680482d6ce08b
http://arxiv.org/abs/astro-ph/0011135
http://arxiv.org/abs/astro-ph/0011135
Autor:
Peter Wizinowich, D. S. Acton, James E. Larkin, Thomas Matheson, Alison L. Coil, Olivier Lai, Alexei V. Filippenko, T. M. Glassman
We report on the first observation of cosmologically distant field galaxies with an high order Adaptive Optics (AO) system on an 8-10 meter class telescope. Two galaxies were observed at 1.6 microns at an angular resolution as high as 50 milliarcsec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f9f27b3790e012b31590ec16ef2d388
http://arxiv.org/abs/astro-ph/0008411
http://arxiv.org/abs/astro-ph/0008411
Autor:
P. Stomski, P. Wizinowich, D. S. Acton, W. Lupton, J. Gathright, A. Conrad, H. Lewis, T. Gregory
Publikováno v:
Adaptive Optics.
The user interface and supervisory control subsystem (UISC) of the W. M. Keck Observatory Adaptive Optics (AO) system serves three main purposes. First, it is the single point of control for the AO system, the wavefront controller subsystem, the opti
Autor:
T. Gregory, P. Wizinowich, D. S. Acton, A. Gleckler, P. Stomski, S. Radau, J. Maute, M. Sirota
Publikováno v:
Adaptive Optics.
The W. M. Keck Observatory and Lawrence Livermore National Labs are currently developing an adaptive optics (AO) system for use on the 10-meter Keck II telescope. This paper will review the Optical Bench Subsystem, placing emphasis on the requirement