Zobrazeno 1 - 10
of 70
pro vyhledávání: '"Thomas A. Sebring"'
Autor:
Constanza Araujo, Dale C. Zajac, Gregory N. Bogan, Michael Warner, Sandrine Thomas, Thomas A. Sebring, Jacques Sebag, Douglas R. Neill, Edward Hileman, Dave Mills, Joe DeVries, Oliver Wiecha, Paul J. Lotz, William J. Gressler
Publikováno v:
SPIE Proceedings.
The Large Synoptic Survey Telescope (LSST) has a 10 degrees square field of view which is achieved through a 3 mirror optical system comprised of an 8.4 meter primary, 3.5 meter secondary (M2) and a 5 meter tertiary mirror. The M2 is a 100mm thick me
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1f434c134db62c50ba3689c46ced5da8
https://doi.org/10.1117/12.2234021
https://doi.org/10.1117/12.2234021
Autor:
Jacques Sebag, Thomas A. Sebring, Oliver Wiecha, Constanza Araujo, Scott Kidney, Mickael Warner, Douglas R. Neill, Ryan C. Sneed, Dave Milles, Paul J. Lotz, William J. Gressler
Publikováno v:
SPIE Proceedings.
The Large Synoptic Survey Telescope (LSST) is a large (8.4 meter) wide-field (3.5 degree) survey telescope, which will be located on the Cerro Pachon summit in Chile. Both the Secondary Mirror (M2) Cell Assembly and Camera utilize hexapods to facilit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f827c44be67d609196524b91598adfe0
https://doi.org/10.1117/12.2231327
https://doi.org/10.1117/12.2231327
Autor:
R. Egerman, C. Stutzki, Stefi A. Baum, Nathan Loewen, G. Bonomi, Thomas A. Sebring, J. Teran, Christopher P. O'Dea
Publikováno v:
SPIE Proceedings.
Over the past two years, the New York Astronomical Corporation (NYAC), the business arm of the Astronomical Society of New York (ASNY), has continued planning and technical studies toward construction of a 12-meter class optical telescope for the use
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8484e0838a8c02585a38cdcf441c86ad
https://doi.org/10.1117/12.2062884
https://doi.org/10.1117/12.2062884
Publikováno v:
SPIE Proceedings.
The Astronomical Corporation of New York has commissioned a study of a 12-meter class telescope to be developed by a group of NY universities. The telescope concept builds on the basic principles established by the Keck telescopes; segmented primary
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7c807a8c2624ace954f6e62cbeb3d626
https://doi.org/10.1117/12.926998
https://doi.org/10.1117/12.926998
Autor:
Thomas A. Sebring
Publikováno v:
SPIE Proceedings.
The CCAT Project is an effort to construct a 25 meter aperture telescope above 5600 meters altitude operating down to wavelengths as short as 200 μm. CCAT has developed some new and innovative approaches to telescope and optics design, added new par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4e6d20e9856dcb28fad1cb0a49f87846
https://doi.org/10.1117/12.857334
https://doi.org/10.1117/12.857334
Publikováno v:
SPIE Proceedings.
CCAT will be a 25 m diameter submillimeter-wave telescope that will operate inside a dome located on Cerro Chajnantor in the Atacama Desert. The telescope must have high aperture efficiency at a wavelength of 350 microns and good performance out to a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c34c4f58a718ac0e1811a0d602c3bc0
https://doi.org/10.1117/12.856498
https://doi.org/10.1117/12.856498
Publikováno v:
SPIE Proceedings.
Technologies of modern optical telescopes with large primary mirror are based on adaptive optics. These telescopes operate with many small mirror segments, so that all the segments work as a large piece of a reflective curved plate, i.e. a paraboloid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::82e604e9503c9ae4e7ec3a17f8c374d8
https://doi.org/10.1117/12.787685
https://doi.org/10.1117/12.787685
Autor:
Paul F. Goldsmith, Thomas A. Sebring, R. A. Chamberlin, Mark Dragovan, Daniel R. Macdonald, J. Zmuidzinas, Simon J. E. Radford, C. Matt Bradford, David P. Woody
To meet the 10 µm RMS half wavefront error requirement for the 25 m diameter Cornell Caltech Atacama Telescope (CCAT), active control of the approximately 200 primary mirror panels is required. The CCAT baseline design includes carbon fiber aluminum
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d20a0e29a7a597bcfa23948ded2bc5a
https://resolver.caltech.edu/CaltechAUTHORS:20181113-084624022
https://resolver.caltech.edu/CaltechAUTHORS:20181113-084624022
Publikováno v:
Applied optics. 39(16)
The next century is knocking on our door, bringing with it the possibility of telescopes even bigger than the 8–10-m-class instruments that have proliferated over the past decade. The fixed spherical reflector is the most economical and pragmatic w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::feaa54c11c3dfae56eec82f54ebe9a48
https://pubmed.ncbi.nlm.nih.gov/18345204
https://pubmed.ncbi.nlm.nih.gov/18345204
Publikováno v:
SPIE Proceedings.
Cornell University and California Institute of Technology are currently studying the feasibility of constructing a 25 meter telescope to operate down to 200 micron wavelength to be sited on a high peak in the Atacama region of Chile. An enclosure dom
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d8bd505f84ee1b1209fd452749f2ecdc
https://doi.org/10.1117/12.670037
https://doi.org/10.1117/12.670037