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Mann, C. M., Matheson, D. N., Ellison, B. N., Oldfield, M. L., Moyna, B. P., Spencer, J. J., et al. (1998). On the design and measurement of a 2.5 THz waveguide mixer. In Proc. 9th Int. Symp. Space Terahertz Technol. (161).
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Tetsu Suzuki, Chris Mann, Takanari Yasui, Hirotomo Fujishima, & Koji Mizuno. (1998). Quasi–integrated planar Schottky barrier diodes for 2.5 THz receivers. In Proc. 9th Int. Symp. Space Terahertz Technol. (187).
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Maddison, B. J., Martin, R. J., Oldfield, M. L., Mann, C. M., Matheson, D. N., Ellison, B. N., et al. (1998). A compact 500 GHz planar schottky siode receiver with a wide instantaneous bandwidth. In Proc. 9th Int. Symp. Space Terahertz Technol. (367).
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Brown, R. L. (1998). Technical specification of the Millimeter Array. In T. G. Phillips (Ed.), Proc. SPIE, Advanced Technology MMW, Radio, and Terahertz Telescopes, vol. 3357 (pp. 231–237).
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Dahl, H., Metz, H. J., & Wriedt, T. (1998). Light scattering of silver halide crystals. In Proc. 3rd Workshop on Electromagnetic and Light Scattering (pp. 51–58). Universität Bremen.
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Dieleman, P. (1998). Fundamental limitations of THz niobium and niobiumnitride SIS mixers. Ph.D. thesis, , Rijksuniversiteit, Groningen.
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Il’in, K. S., Milostnaya, I. I., Verevkin, A. A., Gol’tsman, G. N., Gershenzon, E. M., & Sobolewski, R. (1998). Ultimate quantum efficiency of a superconducting hot-electron photodetector. Appl. Phys. Lett., 73(26), 3938–3940.
Abstract: The quantum efficiency and current and voltage responsivities of fast hot-electron photodetectors, fabricated from superconducting NbN thin films and biased in the resistive state, have been shown to reach values of 340, 220 A/W, and 4×104 V/W,
respectively, for infrared radiation with a wavelength of 0.79 μm. The characteristics of the photodetectors are presented within the general model, based on relaxation processes in the nonequilibrium electron heating of a superconducting thin film. The observed, very high efficiency and sensitivity of the superconductor absorbing the photon are explained by the high multiplication rate of quasiparticles during the avalanche breaking of Cooper pairs.
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Floet, D. W., Baselmans, J. J. A., Klapwijk, T. M., & Gao, J. R. (1998). Resistive transition of niobium superconducting hot-electron bolometer mixers. Appl. Phys. Lett., 73(19), 2826.
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Burke, P. J., Schoelkopf, R. J., Prober, D. E., Skalare, A., Karasik, B. S., Gaidis, M. C., et al. (1998). Spectrum of thermal fluctuation noise in diffusion and phonon cooled hot-electron mixers. Appl. Phys. Lett., 72(12), 1516–1518.
Abstract: A systematic study of the intermediate frequency noise bandwidth of Nb thin-film superconducting hot-electron bolometers is presented. We have measured the spectrum of the output noise as well as the conversion efficiency over a very broad intermediate frequency range (from 0.1 to 7.5 GHz) for devices varying in length from 0.08 μm to 3 μm. Local oscillator and rf signals from 8 to 40 GHz were used. For a device of a given length, the spectrum of the output noise and the conversion efficiency behave similarly for intermediate frequencies less than the gain bandwidth, in accordance with a simple thermal model for both the mixing and thermal fluctuation noise. For higher intermediate frequencies the conversion efficiency decreases; in contrast, the noise decreases but has a second contribution which dominates at higher frequency. The noise bandwidth is larger than the gain bandwidth, and the mixer noise is low, between 120 and 530 K (double side band).
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Yagoubov, P., Kroug, M., Merkel, H., Kollberg, E., Gol'tsman, G., Svechnikov, S., et al. (1998). Noise temperature and local oscillator power requirement of NbN phonon-cooled hot electron bolometric mixers at terahertz frequencies. Appl. Phys. Lett., 73(19), 2814–2816.
Abstract: In this letter, the noise performance of NbN-based phonon-cooled hot electron bolometric quasioptical mixers is investigated in the 0.55–1.1 THz frequency range. The best results of the double-sideband <cd><2018>DSB<cd><2019> noise temperature are: 500 K at 640 GHz, 600 K at 750 GHz, 850 K at 910 GHz, and 1250 K at 1.1 THz. The water vapor in the signal path causes significant contribution to the measured receiver noise temperature around 1.1 THz. The devices are made from 3-nm-thick NbN film on high-resistivity Si and integrated with a planar spiral antenna on the same substrate. The in-plane dimensions of the bolometer strip are typically 0.2Ï«2 um. The amount of local oscillator power absorbed in the bolometer is less than 100 nW.
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