Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Kevin W. Redman"'
Autor:
Susann Hummel, Andreas Roedel, Jason E. Hylan, Theodore Hadjimichael, Greg W. Wenzel, Maurice te Plate, Paul F. Schweiger, Joseph McMann, Markus Melf, Timothy J. Madison, Raymond G. Ohl, Jeffery S. Gum, Martyn Wells, Patrick Williams, Kevin W. Redman, Michael Maszkiewicz, David Lee, Alexander Beaton, Joseph E. Hayden, Phillip Coulter, Jerrod Young, Linda A. Miner, Kyle F. Mclean
Publikováno v:
Optical System Alignment, Tolerancing, and Verification VIII.
The James Webb Space Telescope science instruments are in the final stages of being integrated into the Integrated Science Instrument Module (ISIM) element. Each instrument is tied into a common coordinate system through mechanical references that ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6e3159b322ad9d712e0bac5a5903958d
https://doi.org/10.1117/12.2065017
https://doi.org/10.1117/12.2065017
Autor:
Kevin W. Redman, T. Scirpo, B. Hoffmann Eegholm, Joseph E. Hayden, Bradley J. Frey, J. Gill, M. Casas, Margaret Z. Dominguez, P. Morken, Babak Saif, V. Roberts, Raymond G. Ohl
Publikováno v:
SPIE Proceedings.
NASA's James Webb Space Telescope (JWST) will be a premier space science program for astrophysics following launch scheduled for 2014. JWST will observe the early universe, with emphasis on the time period during which the first stars and galaxies be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0f575ebce8e906743a72289bbd0717be
https://doi.org/10.1117/12.831303
https://doi.org/10.1117/12.831303
Publikováno v:
SPIE Proceedings.
The James Webb Space Telescope is a large infrared observatory with a segmented primary mirror, part of the Optical Telescope Element (OTE), and four science instruments supported by the Integrated Science Instrument Module (ISIM). We present the cal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::52416c4b1c29a2fa13c1e975f57c9245
https://doi.org/10.1117/12.824237
https://doi.org/10.1117/12.824237
Autor:
William L. Eichhorn, Pamela S. Davila, Joseph M. Stock, Kevin W. Redman, Joseph A. Connelly, Maria Nowak, James M. Marsh, Henry P. Sampler, Joe H. Sullivan, Gregory W. Wenzel, Derek Sabatke, Jason E. Hylan, Brent J. Bos, Philip Young, Geraldine A. Wright, Joseph McMann, Bradley J. Frey, John G. Hagopian, Raymond G. Ohl, Douglas B. McGuffey
Publikováno v:
Optical System Alignment and Tolerancing II.
The James Webb Space Telescope (JWST) is an infrared space telescope scheduled for launch in 2013. JWST has a 6.5 meter diameter deployable and segmented primary mirror, a deployable secondary mirror, and a deployable sun-shade. The optical train of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::29c2295be417f7d88886c6024507be46
https://doi.org/10.1117/12.798778
https://doi.org/10.1117/12.798778
Publikováno v:
Optical Spectroscopic Techniques, Remote Sensing, and Instrumentation for Atmospheric and Space Research IV.
The Cosmic Origins Spectrograph (COS) will be the most sensitive UV spectrograph to be flown aboard the Hubble Space Telescope. The COS FUV and NUV channels will provide high sensitivity at resolution greater than 20000 over wavelengths ranging from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::de560e25275713ae500c3f6039f49958
https://doi.org/10.1117/12.454270
https://doi.org/10.1117/12.454270
Publikováno v:
SPIE Proceedings.
The Cosmic Origins Spacecraft (COS) will be the most sensitive UV spectrograph to be flown aboard the Hubble Space Telescope. The COS FUV and NUV channels will provide high sensitivity at resolution greater than 20000 over wavelengths ranging from 11
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4583c54712f4e6c48e2a47fb82e0abd1
https://doi.org/10.1117/12.394019
https://doi.org/10.1117/12.394019
Autor:
Raymond G. Ohl, S. Smee, Robert H. Barkhouser, Douglas B. McGuffey, Gary D. Kushner, Steven J. Conard, Kevin W. Redman
Publikováno v:
SPIE Proceedings.
The Far Ultraviolet Spectroscopic Explorer (FUSE), currently being tested and scheduled for a 1999 launch, is an astrophysics satellite designed to provide high spectral resolving power (Lambda/(Delta)Lambda = 24,000-30,000) over the interval 90.5-11
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c809a22e172823a3528a282c0f489fef
https://doi.org/10.1117/12.366526
https://doi.org/10.1117/12.366526
Publikováno v:
SPIE Proceedings.
The FUSE, scheduled for a summer 1999 launch, is an astrophysics satellite designed to provide high spectral resolving power over the interval 90.5-118.7 nm. The FUSE optical path consists of four co-aligned, normal incidence, off-axis parabolic prim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f22af611f1174230f9cf226102d16f20
https://doi.org/10.1117/12.366541
https://doi.org/10.1117/12.366541
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Conference
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