Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Joseph P. Rosbeck"'
Autor:
Vaidya Nathan, J. E. Jensen, Joseph P. Rosbeck, Jeffrey M. Peterson, W. A. Radford, A. A. Buell, Edward P. Smith, J. B. Varesi, M. D. Newton, M. F. Vilela, G. M. Venzor, T. J. de Lyon, R. E. Bornfreund, Scott M. Johnson
Publikováno v:
Journal of Electronic Materials. 33:526-530
The heteroepitaxial growth of HgCdTe on large-area Si substrates is an enabling technology leading to the production of low-cost, large-format infrared focal plane arrays (FPAs). This approach will allow HgCdTe FPA technology to be scaled beyond the
Publikováno v:
SPIE Proceedings.
Large focal planes with InGaAs detector arrays have been developed that meet the demanding requirements of astronomy and other low background systems. With high quantum efficiency between 0.9 and 1.7 μm, the InGaAs detectors are ideally suited for m
Autor:
Joseph P. Rosbeck, Alan W. Hoffman, Albert M. Fowler, Peter J. Love, Elizabeth Corrales, Craig W. McMurtry, Michael Merrill
Publikováno v:
SPIE Proceedings.
Raytheon Vision Systems is under contract to develop 2K × 2K InSb Focal Plane Arrays (FPA) for the ORION and NEWFIRM projects teaming with NOAO, NASA, and USNO. This paper reviews the progress in the ORION, NEWFIRM, and the JWST projects, showing ba
Autor:
Peter J. Love, Alan W. Hoffman, Ken J. Ando, Elizabeth Corrales, William D. Ritchie, Neil J. Therrien, Joseph P. Rosbeck, Roger S. Holcombe, David J. Gulbransen
Publikováno v:
SPIE Proceedings.
Autor:
Joseph P. Rosbeck, Mark P. Murray, Roger S. Holcombe, David J. Gulbransen, Peter J. Love, Ken J. Ando, Neil J. Therrien, Alan W. Hoffman
Publikováno v:
SPIE Proceedings.
The demand for large-format NIR arrays has grown for both ground-based and space-based applications. These arrays are required for maintaining high resolution over very large fields of view for survey work. We describe results of the development of a
Publikováno v:
SPIE Proceedings.
Large infrared detector arrays are now available that meet the demanding requirements of the astronomy and civil space communities. This paper describes arrays with more than one million detector elements developed by Raytheon Vision Systems for thes
Autor:
Alan W. Hoffman, Joseph P. Rosbeck, Roger S. Holcombe, Craig W. McMurtry, John M. Durkee, Peter J. Love, Ken J. Ando, Nancy A. Lum
Publikováno v:
SPIE Proceedings.
Raytheon Infrared Operations is under contract to develop 2K x 2K InSb arrays for the NGST NIRcam instrument and 1K x 1K Si:As IBC arrays for the NGST MIRI instrument. This paper reviews the progress in the NIR, showing NGST bare mux readout noise at
Autor:
Andy Hutchinson, Michael D. Jack, Raymond S. Balcerak, P. E. Herning, James F. Asbrock, C. Anderson, William L. Johnson, Murray H. Kalisher, B. Walker, V. Liquori, K. Kosai, Joseph P. Rosbeck, Andrew T. Hunter, Maurice J. Halmos, Eli E. Gordon, Ward Trussel, P. Wetzel, Valerie Randall, John E. Jensen, George R. Chapman, Patrick A. Trotta, Sanghamitra Sen, Steven L. Bailey, Terence J. de Lyon
Publikováno v:
Materials for Infrared Detectors.
HgCdTe APDs and APD arrays offer unique advantages for high-performance eyesafe LADAR sensors. These include: operation at room temperature, low-excess noise, high gain, high-quantum efficiency at eyesafe wavelengths, GHz bandwidth, and high-packing
Autor:
Alan W. Hoffman, Judith L. Pipher, Joseph P. Rosbeck, D. Rapchun, W. Y. Lum, James D. Garnett, Danny J. Krebs, Murzy D. Jhabvala, R. Benson, William J. Forrest, G. Mark Cushman, George Domingo, W. J. Glaccum, Nancy A. Lum
Publikováno v:
Infrared Spaceborne Remote Sensing VIII.
SIRTF requires detector arrays with extremely high sensitivity, limited only by the background irradiance. Especially critical is the near infrared spectral region around 3 micrometers , where the detector current due to the zodiacal background is a
Autor:
Joseph P. Rosbeck, Peter J. Love, Ken J. Ando, Nancy A. Lum, James D. Garnett, Michael S. Smith, Kevin Sparkman
Publikováno v:
SPIE Proceedings.
This paper will review the state-of-the-art IR detectors at the Raytheon IR Center of Excellence for both grou8nd-based and space-based astronomy applications. Performance data will be presented on 0.5 to 5.0 micron Indium Antimonide (InSb) arrays an