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Voevodin EI, Gershenzon EM, Goltsman GN, Ptitsina NG. Energy-spectrum of shallow acceptors in Ge deformed strongly by a uniaxial pressure. Sov Phys and Technics of Semiconductors. 1989;23(8):843–6.
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Voevodin EI, Gershenzon EM, Goltsman GN, Ptitsina NG, Chulkova GM. Capture of free holes by charged acceptors in uniaxially deformed Ge. Fizika i Tekhnika Poluprovodnikov. 1988;22(3):540–3.
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Vorobyov VV, Kazakov AY, Soshenko VV, Korneev AA, Shalaginov MY, Bolshedvorskii SV, et al. Superconducting detector for visible and near-infrared quantum emitters [Invited]. Opt Mater Express. 2017;7(2):513–26.
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Wild W, Kardashev NS, Likhachev SF, Babakin NG, Arkhipov VY, Vinogradov IS, et al. Millimetron—a large Russian-European submillimeter space observatory. Exp Astron. 2009;23(1):221–44.
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Zhang W, Miao W, Li SL, Zhou KM, Shi SC, Gao JR, et al. Measurement of the spectral response of spiral-antenna coupled superconducting hot electron bolometers. IEEE Trans Appl Supercond. 2013;23(3):2300804.
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Zhang W, Miao W, Yao QJ, Lin ZH, Shi SC, Gao JR, et al. Spectral response and noise temperature of a 2.5 THz spiral antenna coupled NbN HEB mixer. Phys Procedia. 2012;36:334–7.
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Zhang W, Miao W, Zhong JQ, Shi SC, Hayton DJ, Vercruyssen N, et al. Temperature dependence of the receiver noise temperature and IF bandwidth of superconducting hot electron bolometer mixers. Supercond Sci Technol. 2014;27(8):085013 (1 to 5).
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Zhang W, Miao W, Zhong JQ, Shi SC, Hayton DJ, Vercruyssen N, et al. Temperature dependence of superconducting hot electron bolometers. In: Not published results: 24th international symposium on space terahertz technology.; 2013.
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Zolotov PI, Semenov AV, Divochiy AV, Goltsman GN, Romanov NR, Klapwijk TM. Dependence of photon detection efficiency on normal-state sheet resistance in marginally superconducting films of NbN. IEEE Trans Appl Supercond. 2021;31(5):1–5.
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Zvagelsky RD, Chubich DA, Kolymagin DA, Korostylev EV, Kovalyuk VV, Prokhodtsov AI, et al. Three-dimensional polymer wire bonds on a chip: morphology and functionality. J Phys D: Appl Phys. 2020;53(35):355102.
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