Zobrazeno 1 - 10
of 13
pro vyhledávání: '"Kimberly R. Slavis"'
Autor:
Fred Duttweiler, Gerald J. Visser, Emrah Kalemci, Tumay O. Tumer, Richard E. Rothschild, James L. Matteson, P. F. Dowkontt, Kimberly R. Slavis, Edwin A. Stephan, J. W. Epstein, George L. Huszar, Paul L. Hink, Philippe Leblanc, Michael R. Pelling
Publikováno v:
X-Ray and Gamma-Ray Instrumentation for Astronomy XI.
Our collaboration is characterizing a prototype detector module designed for high energy X-ray astrophysics research covering the 20 - 250 keV energy range. The module consists of a three dimensional position sensitive CdZnTe detector, 25 mm X 25 mm
Autor:
Derrick C. Mancini, Michael E. Graham, Yong S. Chu, Ruediger Staubert, James R. Wilson, James L. Matteson, Paul L. Hink, Melville P. Ulmer, William A. Heindl, Anita Madan, Robert I. Altkorn, Kimberly R. Slavis, Allen S. Krieger, Duane Gruber, Richard E. Rothschild
Publikováno v:
SPIE Proceedings.
The FAR.XITE is a proposed balloon payload. After a test flight, our initial goal is to fly 10 nested mirror modules, but then even more modules can be added until the mass limit of the pointing system and balloon gondola are reached. These limits ar
High altitude balloon flights of position sensitive CdZnTe detectors for high energy X-ray astronomy
Autor:
Paul Dowkontt, J.W. Epstein, Kimberly R. Slavis, Ed Stephan, Paul L. Hink, Robert T. Skelton, Fred Duttweiler, George L. Huszar, Philippe Leblanc, James L. Matteson
Publikováno v:
AIP Conference Proceedings.
Cadmium Zinc Telluride (CZT) is a semiconductor detector well suited for high energy X-ray astronomy. The High-Energy X-ray Imaging Spectrometer (HEXIS) program is developing this technology for use in a hard X-ray all-sky survey and as a focal plane
Autor:
J. R. Macri, Allen D. Zych, T. Gregory Guzik, James L. Matteson, David L. Band, S. Cheenu Kappadath, J. Gregory Stacy, Paul L. Hink, Mark L. McConnell, Terrence J. O'Neill, Michael Cherry, P. Parker Altice, Kimberly R. Slavis, James Buckley, James M. Ryan
Publikováno v:
SPIE Proceedings.
MARGIE will be a large-area, wide field-of-view, hard x- ray/gamma-ray imaging telescope capable of providing accurate positions for faint gamma-ray bursts in near-real- time and of performing a sensitive survey of both steady and transient cosmic so
Autor:
Robert T. Skelton, Fred Duttweiller, George L. Huszar, James L. Matteson, Edwin A. Stephan, J. W. Epstein, P. F. Dowkontt, Paul L. Hink, Philippe Leblanc, Kimberly R. Slavis
Publikováno v:
SPIE Proceedings.
Cadmium Zinc Telluride (CZT) is a room temperature semiconductor detector well suited for high energy x-ray astronomy. We have developed a CZT detector with 500 micron crossed strip readout and an advanced electrode design that greatly improves energ
Publikováno v:
Hard X-Ray, Gamma-Ray, and Neutron Detector Physics.
Position-sensitive CZT detectors for research in astrophysics in the five - several hundred keV range are being developed by several groups. These are very promising for large area detector arrays in coded mask imagers and small-area focal plane dete
Autor:
Robert T. Skelton, Laurence E. Peterson, Richard E. Rothschild, Duane Gruber, James L. Matteson, Michael R. Pelling, William A. Heindl, Kimberly R. Slavis, Paul L. Hink, W. Robert Binns
Publikováno v:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX.
HEXIS is a MIDEX-class mission concept for x-ray astronomy. Its objectives are to improve our knowledge of the high energy x-ray sky by increasing the number of sources above 20 keV to > 2,000, discovering transient sources such as x-ray novae and ga
Autor:
Kimberly R. Slavis, Paul F. Dowkontt, Fred Duttweiller, John W. Epstein, Paul L. Hink, George L. Huszar, Philippe C. Leblanc, James L. Matteson, Robert T. Skelton, Edwin A. Stephan
Publikováno v:
EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy IX.
Autor:
Edwin A. Stephan, Tumay O. Tumer, Robert T. Skelton, James L. Matteson, George L. Huszar, Fred Duttweiller, P. F. Dowkontt, Paul L. Hink, Kimberly R. Slavis, Scott D. Kravis, Philippe Leblanc
Publikováno v:
SPIE Proceedings.
Coded mask imagers for future high energy x-ray astronomy missions will require detector planes with areas of hundreds to thousands of cm2 and position resolutions < 1 mm. Such detectors will enable coded mask imagers to discover and study thousands
Conference
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.