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(2007). Radioastron space VLBI mission.
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Semenov, A., Haas, P., Ilin, K., Hubers, H., Siegel, M., Engel, A., et al. (2007). Energy resolution and sensitivity of a superconducting quantum detector. Phys. C: Supercond., 460-462, 1491–1492.
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(2007). Проект Радиоастрон.
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(2007). Проект Миллиметрон.
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Kardashev, N. S., Andreyanov, V. V., Gromov, V. D., Buyakas, V. I., Gvamichava, A. S., Kotik, A. N., et al. (2007). The Millimetron project. In N. S. Kardashev, & S. A. Dagkesamanskii (Eds.), Radioastronomical Tools and Techniques (111).
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Buyakas, V. I., & Rybakova, A. G. (2007). The Millimetron project: the unit of high-precision deployment of a space mirror. In N. S. Kardashev, & S. A. Dagkesamanskii (Eds.), Radioastronomical Tools and Techniques (127).
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(2007). Atacama large millimeter/submillimeter array.
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(2007). SOFIA – stratospheric observatory for infrared astronomy.
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(2007). SRON-TELIS.
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Jian Wei, David Olaya, Boris Karasik, Sergey Pereverzev, Andrei Sergeev, & Michael Gershenson. (2007). Ultra-sensitive hot-electron nanobolometers for terahertz astrophysics. ArXiv e-prints, 710.
Abstract: The background-limited spectral imaging of the early Universe requires spaceborne terahertz (THz) detectors with the sensitivity 2-3 orders of magnitude better than that of the state-of-the-art bolometers. To realize this sensitivity without sacrificing operating speed, novel detector designs should combine an ultrasmall heat capacity of a sensor with its unique thermal isolation. Quantum effects in thermal transport at nanoscale put strong limitations on the further improvement of traditional membrane-supported bolometers. Here we demonstrate an innovative approach by developing superconducting hot-electron nanobolometers in which the electrons are cooled only due to a weak electron-phonon interaction. At T<0.1K, the electron-phonon thermal conductance in these nanodevices becomes less than one percent of the quantum of thermal conductance. The hot-electron nanobolometers, sufficiently sensitive for registering single THz photons, are very promising for submillimeter astronomy and other applications based on quantum calorimetry and photon counting.
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