Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Albert M. Fowler"'
Autor:
Wendy Mays, Matthieu Bec, Everett M. Irwin, Klaus W. Hodapp, Randolph Chung, Joseph L. Hora, Robert Nolan, Louis Robertson, Michael Merrill, Hubert Yamada, Joseph B. Jensen, Albert M. Fowler, Kent Fletcher, Douglas A. Simons
Publikováno v:
Publications of the Astronomical Society of the Pacific. 115:1388-1406
This paper presents the basic design of the Gemini Near‐Infrared Imager (NIRI) and discusses its capabilities. NIRI offers three different pixel scales to match different operating modes of the Gemini telescope and allows polarimetric and spectrosc
Autor:
Albert M. Fowler, K. Michael Merrill, Craig R. McCreight, Fred Vrba, William J. Ball, Arne Henden
Publikováno v:
Experimental Astronomy. 14:61-68
The Orion program is a project to develop a 2K × 2K infrared focal plane using InSb p-on-n diodes for detectors. It is the natural follow-up to the successful Aladdin 1K × 1K program started in the early 90's. The work is being done at the Raytheon
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:
William J. Ball, Arne Henden, Kenneth Michael Merrill, Craig R. McCreight, Albert M. Fowler, Fred Vrba
Publikováno v:
SPIE Proceedings.
The Orion program developed a 2048x2048 infrared focal plane using InSb PV diodes for detectors. Several of these focal planes have been produced. However, the yield of the original readout multiplexer was not up to expectations owing to unanticipate
Autor:
K. Michael Merrill, Albert M. Fowler, William J. Ball, Arne Henden, Fred Vrba, Craig R. McCreight
Publikováno v:
Scientific Detectors for Astronomy ISBN: 9781402017889
The Orion program is a project to develop a 2K×2K infrared focal plane using InSb p-on-n diodes for detectors. It is the natural follow-up to the successful Aladdin 1K×1K program started in the early 90’s. The work is being done at the Raytheon I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bd16637919386a524e7537ac070daca1
https://doi.org/10.1007/1-4020-2527-0_7
https://doi.org/10.1007/1-4020-2527-0_7
Publikováno v:
SPIE Proceedings.
The Abu infrared imager consists of an ALADDIN 1024x1024 InSB array mounted in a cold-head cooled dewar capable of pumping down to operational temperature without cryogens, equipped with one-to-one transfer optics and an eight-position filter wheel.
Autor:
William J. Ball, Albert M. Fowler, Michael Merrill, Craig R. McCreight, Arne Henden, Frederick J. Vrba
Publikováno v:
SPIE Proceedings.
Orion is a program to develop a 2048x2048 infrared focal plane using InSb PV detectors. It is the natural follow-on to the successful Aladdin 1024x1024 program, which was the largest IR focal plane of the 90's. Although the pixels are somewhat smalle
Autor:
Robert J. Martineau, Albert M. Fowler, John W. MacKenty, Knox S. Long, Matthew A. Greenhouse, Thomas P. Greene, Judith L. Pipher, Craig R. McCreight, Michael E. Ressler, Donald N. B. Hall, Erick T. Young
Publikováno v:
SPIE Proceedings.
This paper summarizes the findings of the Next Generation Space Telescope (NGST) Detector Requirements Review Panel. This panel was comprised of NGST Integrated Science Instrument Module study representatives, detector specialists, and members of the
Autor:
Albert M. Fowler
Publikováno v:
SPIE Proceedings.
Autor:
Albert M. Fowler, Rodney Marks, John W. V. Storey, Antony Schinckel, Darren L. DePoy, Maxime Boccas, Doyal A. Harper, Nigel Sharp, Michael C. B. Ashley, William J. Ball, Paul Martini
Publikováno v:
SPIE Proceedings.
ABU is a NOAO IR imaging camera designed for evaluating the performance of the 1024x1024 Aladdth InSb array. For this experiment, it was outfitted with five filters (see Figure 9) m the 3-5 micron range to exploit the low water vapor and lower air te