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de Graauw, T., Caux, E., Guesten, R., Helmich, F., Pearson, J., Phillips, T. G., et al. (2005). The Herschel-heterodyne instrument for the far-infrared (HIFI). In Bulletin of the American Astronomical Society (1219). Bulletin of the American Astronomical Society, 37.
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de Graauw, T., Whyborn, N., Caux, E., Phillips, T., Stutzki, J., Tielens, X., et al. (2006). The Herschel-heterodyne instrument for the far-infrared (HIFI). In Proc. SPIE. Orlando.
|
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de Lange, G., Hu, Q., Huang, H., & Lichtenberger, A. W. (1997). Development of a 170-210 GHz 3×3 micromachined SIS imaging array. In Proc. 8th Int. Symp. Space Terahertz Technol. (518).
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de Lange, G., Kuipers, J. J., Klapwijk, T. M., Panhuyzen, R. A., van de Stadt, H., & de Graauw, M. W. M. (1995). Superconducting resonator circuits at frequencies above the gap frequency. J. Appl. Phys., 77(4), 1795–1804.
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de Lange, G., Krieg, J. - M., Honingh, N., Karpov, A., & Cherednichenko, S. (2008). Performance of the HIFI flight mixers. In Proc. 19th Int. Symp. Space Terahertz Technol. (pp. 98–105).
Abstract: We summarize the technology and final results of the superconducting heterodyne SIS and HEB mixers that are developed for the HIFI instrument. Within HIFI 7 frequency bands cover the frequency range from 480 GHz to 1910 GHz. We describe the different device technologies and optical coupling schemes that are used to cover the frequency bands. The efforts of the different mixer teams that participate in HIFI have contributed to an instrument that will have unprecedented sensitivity and frequency coverage.
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