O
Oswald H. W. Siegmund
Researcher at University of California, Berkeley
Publications - 241
Citations - 12585
Oswald H. W. Siegmund is an academic researcher from University of California, Berkeley. The author has contributed to research in topics: Microchannel plate detector & Detector. The author has an hindex of 45, co-authored 238 publications receiving 11858 citations. Previous affiliations of Oswald H. W. Siegmund include University of California, Los Angeles.
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Journal ArticleDOI
The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission
D. Christopher Martin,James L. Fanson,David Schiminovich,Patrick Morrissey,Peter G. Friedman,Tom A. Barlow,Tim Conrow,Robert Grange,Patrick N. Jelinsky,Bruno Milliard,Oswald H. W. Siegmund,Luciana Bianchi,Yong-Ik Byun,Jose Donas,Karl Forster,Timothy M. Heckman,Young-Wook Lee,Barry F. Madore,Barry F. Madore,Roger F. Malina,Susan G. Neff,R. Michael Rich,Todd Small,Frank Surber,Alexander S. Szalay,Barry Y. Welsh,Ted K. Wyder +26 more
TL;DR: Galaxy Evolution Explorer (GALEX) as mentioned in this paper performed the first space UV sky survey, including imaging and grism surveys in two bands (1350-1750 and 1750-2750?).
Journal ArticleDOI
The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission
D. Christopher Martin,James L. Fanson,David Schiminovich,Patrick Morrissey,Peter G. Friedman,Tom A. Barlow,Tim Conrow,Robert Grange,Patrick Jelinsky,Bruno Milliard,Oswald H. W. Siegmund,Luciana Bianchi,Yong-Ik Byun,Jose Donas,Karl Forster,Timothy M. Heckman,Young-Wook Lee,Barry F. Madore,Roger F. Malina,Susan G. Neff,R. Michael Rich,Todd Small,Alexander S. Szalay,Ted K. Wyder +23 more
TL;DR: Galaxy Evolution Explorer (GALEX) as discussed by the authors performed the first space UV sky survey, including imaging and grism surveys in two bands (1350-1750 Angstroms and 1750-2750 angstroms).
Journal ArticleDOI
The cosmic origins spectrograph
James C. Green,Cynthia S. Froning,Steve Osterman,Dennis Ebbets,Sara H. Heap,Claus Leitherer,Jeffrey L. Linsky,Blair D. Savage,Kenneth R. Sembach,J. Michael Shull,Oswald H. W. Siegmund,Theodore P. Snow,John R. Spencer,S. Alan Stern,John T. Stocke,Barry Y. Welsh,Stephane Beland,Eric B. Burgh,Charles W. Danforth,Brian A. Keeney,Jason B. McPhate,Steven V. Penton,J. Andrews,K. R. Brownsberger,Jon A. Morse,Erik Wilkinson +25 more
TL;DR: The Cosmic Origins Spectrograph (COS) as discussed by the authors is a moderate-resolution spectrograph with unprecedented sensitivity that was installed into the Hubble Space Telescope (HST) in May 2009, during HST Servicing Mission 4 (STS-125).
Journal ArticleDOI
The Cosmic Origins Spectrograph
James C. Green,Cynthia S. Froning,Steve Osterman,Dennis Ebbets,Sara H. Heap,Claus Leitherer Jeffrey L. Linsky,Blair D. Savage,Kenneth R. Sembach,J. Michael Shull,Oswald H. W. Siegmund,Theodore P. Snow,John R. Spencer,S. Alan Stern,John T. Stocke,Barry Y. Welsh,Stephane Beland,Eric B. Burgh,Charles W. Danforth,Brian A. Keeney,Jason B. McPhate,Steven V. Penton,John Paul Andrews,K. R. Brownsberger,Jon A. Morse,Erik Wilkinson +24 more
TL;DR: The Cosmic Origins Spectrograph (COS) as discussed by the authors is a moderate-resolution spectrograph with unprecedented sensitivity that was installed into the Hubble Space Telescope (HST) in May 2009, during HST Servicing Mission 4 (STS-125).
Journal ArticleDOI
The On-Orbit Performance of the Galaxy Evolution Explorer
Patrick Morrissey,David Schiminovich,Tom A. Barlow,D. Christopher Martin,B. Blakkolb,Tim Conrow,Brian Cooke,Kerry D. Erickson,James L. Fanson,Peter G. Friedman,Robert Grange,Patrick N. Jelinsky,Siu-Chun Lee,Dankai Liu,Alan S. Mazer,R. McLean,Bruno Milliard,David P. Randall,Wes Schmitigal,Amit Sen,Oswald H. W. Siegmund,Frank Surber,Arthur H. Vaughan,M. Viton,Barry Y. Welsh,Luciana Bianchi,Yong-Ik Byun,Jose Donas,Karl Forster,Timothy M. Heckman,Young-Wook Lee,Barry F. Madore,Barry F. Madore,Roger F. Malina,Susan G. Neff,R. Michael Rich,Todd Small,Alexander S. Szalay,Ted K. Wyder +38 more
TL;DR: The Galaxy Evolution Explorer (GALEX) as discussed by the authors is a NASA Small Explorer that is performing a survey of the sky in two ultraviolet bands, using a modified Ritchey-Chretien telescope with a 125 field of view, selectable imaging and objective-grism spectroscopic modes, and an innovative optical system with a thin-film multilayer dichroic beam splitter.