20 October 2004 The wide-field imaging interferometry testbed: II. Characterization and calibration
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We discuss the procedure used to characterize the Wide-Field Imaging Interferometry Testbed (WIIT) components and system, including spectral transmission, throughput, wavefront quality, mechanical and thermal stability, and susceptibility to turbulence. The sources of uncertainty and visibility loss are identified and evaluated, and we briefly discuss measures taken to mitigate these effects. We further discuss calibration techniques which can be used to compensate for visibility loss factors, and describe the applicability of these calibration techniques to the future space-based far-IR interferometry missions SPIRIT (Space Infrared Interferometric Telescope) and SPECS (Submillimeter Probe of the Evolution of Cosmic Structure).
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephen A. Rinehart, Stephen A. Rinehart, J. Thomas Armstrong, J. Thomas Armstrong, Bradley J. Frey, Bradley J. Frey, Jeff Kirk, Jeff Kirk, David T. Leisawitz, David T. Leisawitz, Douglas B. Leviton, Douglas B. Leviton, Luke W. Lobsinger, Luke W. Lobsinger, Richard G. Lyon, Richard G. Lyon, Anthony J. Martino, Anthony J. Martino, Thomas A. Pauls, Thomas A. Pauls, Lee G. Mundy, Lee G. Mundy, E. Sears, E. Sears, } "The wide-field imaging interferometry testbed: II. Characterization and calibration", Proc. SPIE 5491, New Frontiers in Stellar Interferometry, (20 October 2004); doi: 10.1117/12.552076; https://doi.org/10.1117/12.552076


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