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Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy. [PDF]
Klaassen P +40 more
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Shear Mechanics of Articular Cartilage and Cartilage-Inspired Materials. [PDF]
Michel J, Cohen I, Bonassar LJ, Das M.
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Submillimeter astronomy (heterodyne spectroscopy)
Proceedings of the IEEE, 1992Some of the aspects of submillimeter-wave astronomy which are relevant to the field of heterodyne spectroscopy are reviewed. Most of the discussion concerns the dense interstellar medium where stars are forming, with some work presented on nearby galaxies.
T G Phillips, J Keene
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Submillimeter receivers for radio astronomy
Proceedings of the IEEE, 1992The state of development of receivers for submillimeter-wave radio astronomy is reviewed. Bolometers for continuum observation, hot-electron mixer receivers for narrowband spectral line observation, and heterodyne receivers, both Schottky diode and superconducting tunnel junction, are presented.
R Blundell, C -Y E Tong
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Submillimeter astronomy and developments in China
2014 XXXIth URSI General Assembly and Scientific Symposium (URSI GASS), 2014Millimeter to submillimeter radio astronomy is one of the frontier areas in Chinese astronomy. The major research activities include molecular clouds, star formation, formation and evolutions of galaxies. Purple Mountain Observatory (PMO) is the major institute in China responsible for mm/submm astronomy and developments.
Sheng-Cai Shi, Ji Yang
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Low-pass interference filters for submillimeter astronomy
Applied Optics, 1980Low-pass (long-wave transmitting) interference filters, suitable for broadband photometric observations, previously have been constructed from series of capacitive grids stretched on thin Mylar. These filters have the desired optical properties of high transmission, sharp cut-ons, and good blocking at short wavelengths.
S E, Whitcomb, J, Keene
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Radio and Submillimeter Astronomy: Receivers and Spectrometers
2016This chapter presents the different radio receiver configurations used to achieve the high stability demanded by the high gains required for the detection. The radio spectrometers are discussed. The chapter is closed by a discussion of the measurements of the CMB.
R. Poggiani
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A low loss silicon optical diplexer for millimeter and submillimeter radio astronomy
Astronomical Telescopes + InstrumentationSimultaneous dual polarization observations at multiple frequencies are crucial for understanding time-varying astronomical phenomena. To achieve this, it is necessary to separate the main radio telescope beam into different frequency components to feed ...
K. Carter +4 more
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Techniques of Submillimeter Astronomy
1988This review discusses the relative merits of direct and heterodyne techniques for detection in the submillimeter band. A variety of astronomical observing conditions is examined, including those for mountain-top and space telescopes. The spectral resolution (Δν/ν) of the observation is shown to be an important factor in the decision between direct and ...
T. Phillips
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