
Proceedings Paper
Infrared absolute calibrations down to 10 fW in low-temperature environments at NISTFormat | Member Price | Non-Member Price |
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Paper Abstract
The Low Background Infrared (LBIR) facility at the National Institute of Standards and Technology (NIST) is
responsible for absolute IR radiometric calibrations (SI traceable) in low-background temperature (below 80 K)
environments. IR radiometric test hardware that needs to be operated in cryogenic environments is calibrated in
cryogenic vacuum chambers maintained by the facility to create environments that simulate the low-temperature
background of space. Transfer radiometers have also been developed to calibrate IR radiometric test hardware this is too
large to ship to NIST from their own IR test facilities. The first generation transfer radiometer, the BXR, is a filter-based
radiometer that uses an As-doped Si Blocked Impurity Band detector, and can calibrate IR test chambers to a total
uncertainty of less than 3 % (1 σ ) at powers as low as to 10-14 W/cm2. The BXR has evaluated 9 chambers and the
performance of a subset of these chambers will be discussed to a limited extent to demonstrate the need for calibrating
IR test chambers. The second generation transfer radiometer, the MDXR, and new primary standards allowing absolute
calibrations as low as 10-15 W/cm2 are in the final stages of development. The MDXR will have all the functionality of
the BXR and it will have a cryogenic Fourier transform spectrometer (FTS) for high resolution spectral capability.
Performance specifications and test results from development activity on the new primary standards will be discussed.
Paper Details
Date Published: 22 July 2008
PDF: 7 pages
Proc. SPIE 7021, High Energy, Optical, and Infrared Detectors for Astronomy III, 70210S (22 July 2008); doi: 10.1117/12.789845
Published in SPIE Proceedings Vol. 7021:
High Energy, Optical, and Infrared Detectors for Astronomy III
David A. Dorn; Andrew D. Holland, Editor(s)
PDF: 7 pages
Proc. SPIE 7021, High Energy, Optical, and Infrared Detectors for Astronomy III, 70210S (22 July 2008); doi: 10.1117/12.789845
Show Author Affiliations
Adriaan C. Carter, National Institute of Standards and Technology (United States)
Raju U. Datla, National Institute of Standards and Technology (United States)
Raju U. Datla, National Institute of Standards and Technology (United States)
Solomon I. Woods, Jung Research and Development Corp. (United States)
Timothy M. Jung, Jung Research and Development Corp. (United States)
Timothy M. Jung, Jung Research and Development Corp. (United States)
Published in SPIE Proceedings Vol. 7021:
High Energy, Optical, and Infrared Detectors for Astronomy III
David A. Dorn; Andrew D. Holland, Editor(s)
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