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.
Papers
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Journal ArticleDOI
Detection of highly ionized CIV gas within the Local Cavity
TL;DR: In this article, high resolution ultraviolet measurements of the interstellar absorption line profiles of the CIV (1550 A) high ionization doublet recorded towards the nearby B2Ve star HD 158427 (d~74pc) were presented.
Journal ArticleDOI
UV photoemission efficiency of polycrystalline CVD diamond films
TL;DR: In this paper, the absolute quantum efficiency of polycrystalline diamond films grown on silicon substrates by chemical vapor deposition (CVD) was reported in the range of 25-200 nm.
Journal ArticleDOI
Ultraviolet and Far-Infrared-selected Star-forming Galaxies at z = 0: Differences and Overlaps
C. Kevin Xu,Veronique Buat,Jorge Iglesias-Páramo,Tsutomu T. Takeuchi,Tom A. Barlow,Luciana Bianchi,Jose Donas,Karl Forster,Peter G. Friedman,Timothy M. Heckman,Patrick N. Jelinsky,Young-Wook Lee,Barry F. Madore,Barry F. Madore,Roger F. Malina,D. Christopher Martin,Bruno Milliard,Patrick Morrissey,R. Michael Rich,Susan G. Neff,David Schiminovich,Oswald H. W. Siegmund,Todd Small,Alexander S. Szalay,Barry Y. Welsh,Ted K. Wyder,Sukyoung K. Yi +26 more
TL;DR: In this paper, two samples of local galaxies, one UV (GALEX) selected and the other FIR (IRAS) selected, to address the question of whether UV and FIR surveys see two sides ("bright" and "dark") of the star formation of the same population of galaxies or two different populations of star-forming galaxies is found.
Proceedings ArticleDOI
Calibration and flight qualification of FORTIS
Brian T. Fleming,Stephan R. McCandliss,K. Redwine,Mary Elizabeth Kaiser,J. W. Kruk,Paul D. Feldman,Alexander Kutyrev,Mary J. Li,Samuel H. Moseley,Oswald H. W. Siegmund,John V. Vallerga,Adrian Martin +11 more
TL;DR: The first flight of the Far Ultraviolet Off Rowland Circle Telescope for Imaging and Spectroscopy (FORTIS) was conducted by the Johns Hopkins University sounding rocket group on May 10, 2013 as mentioned in this paper.
Posted Content
A Brief Technical History of the Large-Area Picosecond Photodetector (LAPPD) Collaboration
Bernhard W. Adams,Klaus Attenkofer,Mircea Bogdan,Karen Byrum,A. Elagin,Jeffrey W. Elam,Henry J. Frisch,Jean-Francois Genat,H. M. X. Grabas,Joseph Gregar,Elaine Hahn,Mary K. Heintz,Zinetula Insepov,V. Ivanov,Sharon R. Jelinsky,Slade Jokely,Sun Wu Lee,Anil U. Mane,Jason B. McPhate,Michael J. Minot,P. Murat,Kurtis Nishimura,R. Northrop,Razib Obaid,Eric Oberla,Erik Ramberg,Anatoly Ronzhin,Oswald H. W. Siegmund,Gregory Sellberg,Neal T. Sullivan,Anton S. Tremsin,G. S. Varner,Igor V. Veryovkin,Alexei Vostrikov,Robert Wagner,Dean Walters,Hsien-Hau Wang,Matthew Wetstein,Junqi Xi,Zikri Yusov,A. V. Zinovev +40 more
TL;DR: The Large Area Picosecond PhotoDetector (LAPPD) Collaboration was formed in 2009 to develop large-area photodetectors capable of time resolutions measured in pico-seconds, with accompanying sub-millimeter spatial resolution.