Zobrazeno 1 - 10
of 57
pro vyhledávání: '"R, Dettmann"'
Publikováno v:
SPIE Proceedings.
The Giant Magellan Telescope (GMT) 1 is a 25 m telescope composed of seven 8.4 m “unit telescopes”, on a common mount. Each primary and conjugated secondary mirror segment will feed a common instrument interface, their focal planes co-aligned and
Autor:
Chan Park, Andrew Rakich, Lee R. Dettmann, Ueejeong Jeong, Chris Alongi, Yang Noh Yoon, Byeong-Gon Park, Ho Soon Yang, Sungho Lee, Il Kwon Moon, Paul Gardner, Robert Bernier, Wylie Rosenthal, Chang Jin Oh, Ho-Sang Kim, Je Heon Song, Jeong Yeol Han, Christoph Dribusch, Myung Cho, Kyoung Don Lee, Won Hyun Park, Youra Jun
Publikováno v:
SPIE Proceedings.
The Giant Magellan Telescope (GMT) will be featured with two Gregorian secondary mirrors, an adaptive secondary mirror (ASM) and a fast-steering secondary mirror (FSM). The FSM has an effective diameter of 3.2 m and built as seven 1.1 m diameter circ
Autor:
H. Hoffmann, H. Hillesheim, J. Güttner, K. Stade, Eva-Maria Merbt, K. Holle, M. Oettel, J. Strecke, G. Hesse, U. Horn, U. Valentin, H. Lemke, K. Chemnitius, I. Schimmel, J. Deufrains, V. Hesse, E. Keil, G. Klinger, A. Stelzner, R. Furcht, P. Gaida, M. Anke, R. Dettmann, B. Kramp, F. Robiller
Publikováno v:
Experimental and Clinical Endocrinology & Diabetes. 81:179-196
The toxicity of 17 alpha-cyanomethyl-17 beta-hydroxy-estra-4, 9-dien-3-one (STS 557) was studied by its oral administration of 0.1, 1.0 or 10.0 mg/kg/day to Wistar rats for six months, and of 0.01, 0.1 or 1.0 mg/kg/day to beagle dogs for six months,
Publikováno v:
Psychology and Marketing. 20:837-865
Firms spend considerable sums of money on marketing, and they continue to do so because marketing works. However, marketing can only work if marketers have a reasonably accurate view of human nature. It is argued that many consumer products and adver
Publikováno v:
SPIE Proceedings.
The Large Binocular Telescope consists of two 8.4m telescopes on a common mount. Its current active optics system uses measured mechanical deflections of its optics to compensate for misalignment due to changes in telescope elevation angle and analys
Autor:
Robert O. Reynolds, Lee R. Dettmann
Publikováno v:
SPIE Proceedings.
The Adaptively Corrected Echelle Spectrograph (ACES) high resolution echelle spectrograph was originally developed at Steward Observatory to couple adaptively-corrected stellar images to the instrument using a near single mode optical fiber to give R
Autor:
Michael J. Messerly, Andrea Arneson, Lee R. Dettmann, Ron Eng, Doug Leviton, W. Scott Smith, Adam Magruder, Robert Garfield, Bob Brown, Dave Chaney, Rob Bernier, John P. Schwenker, Koby Smith, James B. Hadaway, H. Philip Stahl, Patrick Johnson, Chris Alongi, Ben Gallagher, Ankit Patel, Martin Seilonen, Allen Lee, Patrick J. Reardon, Jay Daniel, Glen Cole
Publikováno v:
SPIE Proceedings.
JWST optical component in-process optical testing and cryogenic requirement compliance certification, verification & validation is probably the most difficult metrology job of our generation in astronomical optics. But, the challenge has been met: by
Autor:
Ankit Patel, Martin Seilonen, Ed Boese, Rob Bernier, Andrew McKay, John Kincade, Robert Garfield, Mark Bergeland, Lee R. Dettmann, Chris Alongi, Patrick Johnson, Adam Magruder, Andrea Arneson, Holger Glatzel, Jay Daniel, Lester M. Cohen, Benjamin B. Gallagher, Gary Surges, Robert J. Brown, Allen Lee
Publikováno v:
SPIE Proceedings.
During 2009, Tinsley finished most of the Configuration 1 pre-cryo test Computer Controlled Optical Surfacing (CCOS) operations on the James Webb Space Telescope primary mirror segments and in mid-2009 we began the Configuration 2 post-cryo test CCOS
Publikováno v:
SPIE Proceedings.
We developed a distortion measurement technique that works in snapshot mode. Distortion information across the full field of view can be captured in a single short exposure. To do this, a Ronchi ruling is placed in the object and image planes of the
Publikováno v:
SPIE Proceedings.
We describe the active support system for the 8.4 m LBT primary mirrors and the use of this system to optimize the mirror figure in the lab before installation in the telescope. We figured the mirror, mounted on passive supports, to an accuracy of 18