Far-infrared imaging array for SIRTF
— University of Arizona Skip to main navigation Skip to search Skip to main content University of Arizona Home Home Profiles Departments and Centers Scholarly Works Activities Grants Datasets Prizes Search by expertise, name or affiliation Far-infrared imaging array for SIRTF Erick T. Young, James T. Davis, Craig L. Thompson, George H. Rieke, G. Rivlis, Richard Schnurr, James Cadien, Lacinda Davidson, Gregory S. Winters, Karen A. Kormos Steward Observatory Lunar and Planetary Lab Planetary Sciences Research output: Contribution to journal › Conference article › peer-review 54 Scopus citations Overview Fingerprint Abstract We describe the design, construction, and performance of the 32 X 32 Ge:Ga imaging array being built at the University of Arizona for the Multiband Imaging Photometer for SIRTF (MIPS). The array will support a number of operational modes in the MIPS instrument including natural background-limited mapping at 70 micrometers , super-resolution observations at 70 micrometers , and spectral energy distribution measurements between 50 and 100 micrometers. The array is constructed in a modular manner using eight 4 X 32 pixel building blocks. To meet the sensitivity and stability requirements, the array must have excellent photometric repeatability, low noise, and robustness to the effects of the ionizing radiation environment in space. Key elements in attaining this level of performance are the Ge:Ga detectors materials and the cryogenic CRC-696 readout electronics. We present laboratory data for a 16 X 32 prototype of the array, and describe the plans for the construction of the qualification and flight units. Original language English (US) Pages (from-to) 57-65 Number of pages 9 Journal Proceedings of SPIE - The International Society for Optical Engineering Volume 3354 DOIs https://doi.org/10.1117/12.317315 State Published - 1998 Event Infrared Astronomical Instrumentation - Kona, HI, United States Duration: Mar 23 1998 → Mar 23 1998 ASJC Scopus subject areas Electronic, Optical and Magnetic Materials Condensed Matter Physics Computer Science Applications Applied Mathematics Electrical and Electronic Engineering Access to Document 10.1117/12.317315 Other files and links Link to publication in Scopus Fingerprint Dive into the research topics of 'Far-infrared imaging array for SIRTF'. Together they form a unique fingerprint. Infrared Imaging Mathematics 100% Far-infrared Mathematics 97% Space Infrared Telescope Facility Physics & Astronomy 65% Ionizing Radiation Chemical Compounds 60% Infrared imaging Engineering & Materials Science 58% Cryogenics Chemical Compounds 54% Photometers Engineering & Materials Science 52% Imaging techniques Engineering & Materials Science 37% View full fingerprint Cite this APA Standard Harvard Vancouver Author BIBTEX RIS Young, E. T., Davis, J. T., Thompson, C. L., Rieke, G. H., Rivlis, G., Schnurr, R., Cadien, J., Davidson, L., Winters, G. S., & Kormos, K. A. (1998). Far-infrared imaging array for SIRTF. Proceedings of SPIE - The International Society for Optical Engineering, 3354, 57-65. https://doi.org/10.1117/12.317315 Far-infrared imaging array for SIRTF. / Young, Erick T.; Davis, James T.; Thompson, Craig L.; Rieke, George H.; Rivlis, G.; Schnurr, Richard; Cadien, James; Davidson, Lacinda; Winters, Gregory S.; Kormos, Karen A. In: Proceedings of SPIE - The International Society for Optical Engineering, Vol. 3354, 1998, p. 57-65. Research output: Contribution to journal › Conference article › peer-review Young, ET, Davis, JT, Thompson, CL, Rieke, GH, Rivlis, G, Schnurr, R, Cadien, J, Davidson, L, Winters, GS & Kormos, KA 1998, 'Far-infrared imaging array for SIRTF', Proceedings of SPIE - The International Society for Optical Engineering, vol. 3354, pp. 57-65. https://doi.org/10.1117/12.317315 Young ET, Davis JT, Thompson CL, Rieke GH, Rivlis G, Schnurr R et al. Far-infrared imaging array for SIRTF. Proceedings of SPIE - The International Society for Optical Engineering. 1998;3354:57-65. https://doi.org/10.1117/12.317315 Young, Erick T. ; Davis, James T. ; Thompson, Craig L. ; Rieke, George H. ; Rivlis, G. ; Schnurr, Richard ; Cadien, James ; Davidson, Lacinda ; Winters, Gregory S. ; Kormos, Karen A. / Far-infrared imaging array for SIRTF. In: Proceedings of SPIE - The International Society for Optical Engineering. 1998 ; Vol. 3354. pp. 57-65. @article{d0ee845d383b4c1590933a746b192c90, title = "Far-infrared imaging array for SIRTF", abstract = "We describe the design, construction, and performance of the 32 X 32 Ge:Ga imaging array being built at the University of Arizona for the Multiband Imaging Photometer for SIRTF (MIPS). The array will support a number of operational modes in the MIPS instrument including natural background-limited mapping at 70 micrometers , super-resolution observations at 70 micrometers , and spectral energy distribution measurements between 50 and 100 micrometers. The array is constructed in a modular manner using eight 4 X 32 pixel building blocks. To meet the sensitivity and stability requirements, the array must have excellent photometric repeatability, low noise, and robustness to the effects of the ionizing radiation environment in space. Key elements in attaining this level of performance are the Ge:Ga detectors materials and the cryogenic CRC-696 readout electronics. We present laboratory data for a 16 X 32 prototype of the array, and describe the plans for the construction of the qualification and flight units.", author = "Young, {Erick T.} and Davis, {James T.} and Thompson, {Craig L.} and Rieke, {George H.} and G. Rivlis and Richard Schnurr and James Cadien and Lacinda Davidson and Winters, {Gregory S.} and Kormos, {Karen A.}", note = "Funding Information: This study was supported by grant C84-503 of the Dutch Kidney Foundation (Nierstichting Nederland). The authors thank Willy Bruins-van der Weij for secretarial support and Aly Drent-Bremer for technical assistance.; Infrared Astronomical Instrumentation ; Conference date: 23-03-1998 Through 23-03-1998", year = "1998", doi = "10.1117/12.317315", language = "English (US)", volume = "3354", pages = "57--65", journal = "Proceedings of SPIE - The International Society for Optical Engineering", issn = "0277-786X", publisher = "SPIE", } TY - JOUR T1 - Far-infrared imaging array for SIRTF AU - Young, Erick T. AU - Davis, James T. AU - Thompson, Craig L. AU - Rieke, George H. AU - Rivlis, G. AU - Schnurr, Richard AU - Cadien, James AU - Davidson, Lacinda AU - Winters, Gregory S. AU - Kormos, Karen A. N1 - Funding Information: This study was supported by grant C84-503 of the Dutch Kidney Foundation (Nierstichting Nederland). The authors thank Willy Bruins-van der Weij for secretarial support and Aly Drent-Bremer for technical assistance. PY - 1998 Y1 - 1998 N2 - We describe the design, construction, and performance of the 32 X 32 Ge:Ga imaging array being built at the University of Arizona for the Multiband Imaging Photometer for SIRTF (MIPS). The array will support a number of operational modes in the MIPS instrument including natural background-limited mapping at 70 micrometers , super-resolution observations at 70 micrometers , and spectral energy distribution measurements between 50 and 100 micrometers. The array is constructed in a modular manner using eight 4 X 32 pixel building blocks. To meet the sensitivity and stability requirements, the array must have excellent photometric repeatability, low noise, and robustness to the effects of the ionizing radiation environment in space. Key elements in attaining this level of performance are the Ge:Ga detectors materials and the cryogenic CRC-696 readout electronics. We present laboratory data for a 16 X 32 prototype of the array, and describe the plans for the construction of the qualification and flight units. AB - We describe the design, construction, and performance of the 32 X 32 Ge:Ga imaging array being built at the University of Arizona for the Multiband Imaging Photometer for SIRTF (MIPS). The array will support a number of operational modes in the MIPS instrument including natural background-limited mapping at 70 micrometers , super-resolution observations at 70 micrometers , and spectral energy distribution measurements between 50 and 100 micrometers. The array is constructed in a modular manner using eight 4 X 32 pixel building blocks. To meet the sensitivity and stability requirements, the array must have excellent photometric repeatability, low noise, and robustness to the effects of the ionizing radiation environment in space. Key elements in attaining this level of performance are the Ge:Ga detectors materials and the cryogenic CRC-696 readout electronics. We present laboratory data for a 16 X 32 prototype of the array, and describe the plans for the construction of the qualification and flight units. UR - http://www.scopus.com/inward/record.url?scp=0011809429&partnerID=8YFLogxK UR - http://www.scopus.com/inward/citedby.url?scp=0011809429&partnerID=8YFLogxK U2 - 10.1117/12.317315 DO - 10.1117/12.317315 M3 - Conference article AN - SCOPUS:0011809429 VL - 3354 SP - 57 EP - 65 JO - Proceedings of SPIE - The International Society for Optical Engineering JF - Proceedings of SPIE - The International Society for Optical Engineering SN - 0277-786X T2 - Infrared Astronomical Instrumentation Y2 - 23 March 1998 through 23 March 1998 ER - Powered by Pure, Scopus & Elsevier Fingerprint Engine™ © 2022 Elsevier B.V We use cookies to help provide and enhance our service and tailor content. 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