Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Gary L. Bostrup"'
Autor:
Gary L. Bostrup, Craig A. Cabelli, William E. Kleinhans, Lester J. Kozlowski, Klaus W. Hodapp, A. C. Chen, Donald E. Cooper, Kadri Vural, Scott A. Cabelli, Donald N. B. Hall
Publikováno v:
Le Journal de Physique IV. :Pr3-141
Autor:
Scott A. Cabelli, William E. Kleinhans, Gary L. Bostrup, Donald E. Cooper, Robert B. Bailey, Lester J. Kozlowski, M. Metzger, Kadri Vural, Klaus-Werner Hodapp, Lennox L. Cowie, C. Y. Chen, Donald N. B. Hall, Everett M. Irwin, Joseph L. Hora
Publikováno v:
New Astronomy. 1:177-196
Two generations of prototypes of a HgCdTe infrared detector array with 1024 × 1024 pixels developed by the Rockwell International Science Center have been tested in the new Quick Infrared Camera (QUIRC) and an upgraded version of KSPEC a cross-dispe
Autor:
Donald E. Cooper, Kadri Vural, Yibin Bai, Craig A. Cabelli, Lester J. Kozlowski, John T. Montroy, Klaus-Werner Hodapp, Gary L. Bostrup, A. C. Chen, Donald N. B. Hall
Publikováno v:
SPIE Proceedings.
Rockwell Space Center is developing low-noise visible and IR imaging sensors and systems for astronomy, high-end commercial, NASA, and advanced military applications. The first science grade 2048 by 2048 HAWAII-2 focal plane array (FPA) for astronomy
Autor:
Kadri Vural, Lester J. Kozlowski, C. A. Chen, Jose M. Arias, Jagmohan Bajaj, Donald E. Cooper, Donald N. B. Hall, J. A. Pinter, Klaus-Werner Hodapp, G. G. Price, Craig A. Cabelli, William E. Kleinhans, Gary L. Bostrup
Publikováno v:
SPIE Proceedings.
Rockwell is developing the world's largest HgCdTe IR focal plane array (FPA) for astronomy and low background applications. The format of the device is a hybrid 2048 X 2048 with a unit cell size of 18 micrometers X 18 micrometers . SWIR detectors wit
Autor:
Donald N. B. Hall, Klaus-Werner Hodapp, Kadri Vural, Scott A. Cabelli, A. C. Chen, Gary L. Bostrup, Lester J. Kozlowski, Craig A. Cabelli, William E. Kleinhans, Donald E. Cooper
Publikováno v:
SPIE Proceedings.
The HAWAII-2 is an IR 2048 2 focal plane array (FPA) that is being developed for next-generation IR astronomy. It will supplant our HAWAII 1024 2 as the largest high- performance imaging array available for IR astronomy. As with our prior IR sensor,
Autor:
Klaus-Werner Hodapp, G. G. Price, A. C. Chen, William E. Kleinhans, Scott A. Cabelli, Donald E. Cooper, Gary L. Bostrup, Dennis Edwall, Kadri Vural, Craig A. Cabelli, J. A. Pinter, Lester J. Kozlowski, Donald N. B. Hall, Jose M. Arias, G. A. Stanley, Robert B. Bailey
Publikováno v:
Infrared Detectors and Focal Plane Arrays V.
We have developed 1024 X 1024 HAWAII (HgCdTe Arrays for Wide-field Astronomical Infrared Imaging) focal plane arrays (FPAs) for use in astronomical applications. These devices have been delivered to various astronomy organizations around the world an
Autor:
D. M. Stephenson, William V. McLevige, Kadri Vural, Gary L. Bostrup, C. Y. Chen, Klaus-Werner Hodapp, Donald E. Cooper, William E. Kleinhans, Donald N. B. Hall, Robert B. Bailey, Lester J. Kozlowski, Scott A. Cabelli
Publikováno v:
SPIE Proceedings.
Rockwell Science Center and the University of Hawaii have developed a short wavelength infrared (SWIR) 1024 x 1024 focalplane array (EPA). The continuing project is funded by the U.S. Air Force Phillips Laboratory in connection with their AdvancedEle
Autor:
Gary L. Bostrup, Donald N. B. Hall, Kadri Vural, Donald E. Cooper, Scott A. Cabelli, Klaus-Werner Hodapp, William E. Kleinhans, Robert B. Bailey, Lester J. Kozlowski, Annie Chi-yi Chen
Publikováno v:
Instrumentation in Astronomy VIII.
The University of Hawaii and the Rockwell International Science Center are developing a large format SWIR detector array optimized for low background astronomical imaging and spectroscopic observations. This so called HgCdTe astronomical wide area IR
Autor:
Kadri Vural, Scott A. Cabelli, Isoris S. Gergis, Gary L. Bostrup, Philip E. Howard, Donald E. Cooper, Robert B. Bailey, Lester J. Kozlowski, William V. McLevige, W. E. Tennant, Annie Chi-yi Chen
Publikováno v:
Optical Engineering. 33:54
A high-performance 5-μm 640 X 480 HgCdTe/CdTe/Al2O3 infrared focal plane array (FPA) that offers full TV-compatible resolution with excellent sensitivity at temperatures below 120 K has been developed. Mean FPA D* at 95 K and background of 1014 phot