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Antipov SV, Svechnikov SI, Smirnov KV, Vakhtomin YB, Finkel MI, Goltsman GN, et al. Noise temperature of quasioptical NbN hot electron bolometer mixers at 900 GHz. Physics of Vibrations. 2001;9(4):242–5.
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Svechnikov SI, Antipov SV, Vakhtomin YB, Goltsman GN, Gershenzon EM, Cherednichenko SI, et al. Conversion and noise bandwidths of terahertz NbN hot-electron bolometer mixers. Physics of Vibrations. 2001;9(3):205–10.
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Tong CE, Blundell R, Papa DC, Smith M, Kawamura J, Gol'tsman G, et al. An all solid-state superconducting heterodyne receiver at terahertz frequencies. IEEE Microw Guid Wave Lett. 1999;9(9):366–8.
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Il'in KS, Currie M, Lindgren M, Milostnaya II, Verevkin AA, Gol'tsman GN, et al. Quantum efficiency and time-domain response of superconducting NbN hot-electron photodetectors. IEEE Trans Appl Supercond. 1999;9(2):3338–41.
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Semenov AD, Gol'tsman GN. Non-thermal response of a diffusion-cooled hot-electron bolometer. IEEE Trans Appl Supercond. 1999;9(2):4491–4.
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Gerecht E, Musante CF, Jian H, Yngvesson KS, Dickinson J, Waldman J, et al. New results for NbN phonon-cooled hot electron bolometric mixers above 1 THz. IEEE Trans Appl Supercond. 1999;9(2):4217–20.
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Yagoubov P, Kroug M, Merkel H, Kollberg E, Schubert J, Hubers H-W, et al. Heterodyne measurements of a NbN superconducting hot electron mixer at terahertz frequencies. IEEE Trans Appl Supercond. 1999;9(2):3757–60.
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Smirnov K, Vachtomin Y, Divochiy A, Antipov A, Goltsman G. Dependence of dark count rates in superconducting single photon detectors on the filtering effect of standard single mode optical fibers. Appl Phys Express. 2015;8(2):022501 (1 to 4).
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Pyatkov F, Khasminskaya S, Kovalyuk V, Hennrich F, Kappes MM, Goltsman GN, et al. Sub-nanosecond light-pulse generation with waveguide-coupled carbon nanotube transducers. Beilstein J Nanotechnol. 2017;8:38–44.
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Zorin M, Lindgren M, Danerud M, Karasik B, Winkler D, Gol'tsman G, et al. Nonequilibrium and bolometric responses of YBaCuO thin films to high-frequency modulated laser radiation. J Supercond. 1995;8(1):11–5.
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