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Alexandre Karpov, David Miller, Rice, F. R., Stern, J. A., Bruce Bumble, LeDuc, H. G., et al. (2004). Low-noise SIS mixer for far-infrared radio astronomy. In Proc. SPIE (Vol. 5498, pp. 616–621). Glasgow, Scotland, UK.
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Vachtomin, Y. B., Antipov, S. V., Kaurova, N. S., Maslennikov, S. N., Smirnov, K. V., Polyakov, S. L., et al. (2004). Noise temperature, gain bandwidth and local oscillator power of NbN phonon-cooled HEB mixer at terahertz frequenciess. In Proc. 29th IRMMW / 12th THz (pp. 329–330). Karlsruhe, Germany.
Abstract: We present the performances of HEB mixers based on 3.5 nm thick NbN film integrated with log-periodic spiral antenna. The double side-band receiver noise temperature values are 1300 K and 3100 K at 2.5 THz and at 3.8 THz, respectively. The gain bandwidth of the mixer is 4.2 GHz and the noise bandwidth is 5 GHz. The local oscillator power is 1-3 /spl mu/W for mixers with different active area.
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Kaurova, N. S., Finkel, M. I., Maslennikov, S. N., Vahtomin, Y. B., Antipov, S. V., Smirnov, K. V., et al. (2004). Submillimeter mixer based on YBa2Cu3O7-x thin film. In Proc. 1-st conf. Fundamental problems of high temperature superconductivity (291). Moscow-Zvenigorod.
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Каурова, Н. С., Финкель, М. И., Масленников, С. Н., Вахтомин, Ю. Б., Антипов, С. В., Смирнов, К. В., et al. (2004). Смеситель субмиллиметрового диапазона длин волн на основе тонкой пленки YBa2Cu3O7-x. In 1-я международная конференция Фундаментальные проблемы высокотемпературной сверхпроводимости (291). Москва-Звенигород.
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Semenov, A., Richter, H., Smirnov, K., Voronov, B., Gol'tsman, G., & Hübers, H. - W. (2004). The development of terahertz superconducting hot-electron bolometric mixers. Supercond. Sci. Technol., 17(5), 436–439.
Abstract: We present recent advances in the development of NbN hot-electron bolometric (HEB) mixers for flying terahertz heterodyne receivers. Three important issues have been addressed: the quality of the source NbN films, the effect of the bolometer size on the spectral properties of different planar feed antennas, and the local oscillator (LO) power required for optimal operation of the mixer. Studies of the NbN films with an atomic force microscope indicated a surface structure that may affect the performance of the smallest mixers. Measured spectral gain and noise temperature suggest that at frequencies above 2.5 THz the spiral feed provides better overall performance than the double-slot feed. Direct measurements of the optimal LO power support earlier estimates made in the framework of the uniform mixer model.
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Pan, S. K., A. R. Kerr, M. W. P., Lauria, E. F., Crady, W. K., Horner, N., Srikanth, J. S., et al. (2004). A fixed-tuned integrated SIS mixer with ultra-wideband IF and quantum-limited sensitivity for ALMA band 3 (84-116 GHz) receivers. In Proc. 15th Int. Symp. Space Terahertz Technol. (pp. 55–61). Northampton, MA.
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Martin슠Harwit. (2004). The Herschel mission. Advances in Space Research, 34(3), 568–572.
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Moore, D. P., Remedios, J. J., Waterfall, A. M., & Burgess, A. (2004). Measuring halocarbons from the MIPAS instrument.
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Yu, B., Zeng, F., Yang, Y., Xing, Q., Chechin, A., Xin, X., et al. (2004). Torsional vibrational modes of tryptophan studied by terahertz time-domain spectroscopy. Biophys. J., 86(3), 1649–1654.
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Ciulin, V., Carter, S. G., & Sherwin, M. S. (2004). Terahertz optical mixing in biased GaAs single quantum wells. Phys. Rev. B, 70(11), 115312–(1–6).
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