19 July 2016 The calibration of PIXIE
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The FIRAS instrument demonstrated the use of an external calibrator to compare the sky to an instrumented blackbody. The PIXIE calibrator is improved from -35 dB to -65 dB. Another significant improvement is the ability to insert the calibrator into either input of the FTS. This allows detection and correction of additional errors, reduces the effective calibration noise by a factor of 2, eliminates an entire class of systematics and allows continuous observations. This paper presents the design and use of the PIXIE calibrator.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
D. J. Fixsen, D. J. Fixsen, D. T. Chuss, D. T. Chuss, Alan Kogut, Alan Kogut, Paul Mirel, Paul Mirel, E. J. Wollack, E. J. Wollack, } "The calibration of PIXIE", Proc. SPIE 9914, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, 991439 (19 July 2016); doi: 10.1117/12.2232836; https://doi.org/10.1117/12.2232836


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