Zobrazeno 1 - 10
of 70
pro vyhledávání: '"superconducting spectrometer"'
Autor:
Akio Taniguchi, Tom J. L. C. Bakx, Jochem J. A. Baselmans, Robert Huiting, Kenichi Karatsu, Nuria Llombart, Matus Rybak, Tatsuya Takekoshi, Yoichi Tamura, Hiroki Akamatsu, Stefanie Brackenhoff, Juan Bueno, Bruno T. Buijtendorp, Shahab O. Dabironezare, Anne-Kee Doing, Yasunori Fujii, Kazuyuki Fujita, Matthijs Gouwerok, Sebastian Hähnle, Tsuyoshi Ishida, Shun Ishii, Ryohei Kawabe, Tetsu Kitayama, Kotaro Kohno, Akira Kouchi, Jun Maekawa, Keiichi Matsuda, Vignesh Murugesan, Shunichi Nakatsubo, Tai Oshima, Alejandro Pascual Laguna, David J. Thoen, Paul P. van der Werf, Stephen J. C. Yates, Akira Endo
Publikováno v:
Low Temperature Physics, 209, 278-286. AMER INST PHYSICS
Journal of Low Temperature Physics, 209(3-4), 278-286
Journal of Low Temperature Physics, 209(3-4), 278-286
Integrated superconducting spectrometer (ISS) technology will enable ultra-wideband, integral-field spectroscopy for (sub)millimeter-wave astronomy, in particular, for uncovering the dust-obscured cosmic star formation and galaxy evolution over cosmi
Autor:
Rybak, M., Bakx, T., Baselmans, J., Karatsu, K., Kohno, K., Takekoshi, T., Tamura, Y., Taniguchi, A., Werf, P.P. van der, Endo, A.
Publikováno v:
Journal of Low Temperature Physics, 209(5-6)
Journal of Low Temperature Physics, 209(5-6), 766-778
Journal of Low Temperature Physics, 209(5-6), 766-778
We present a feasibility study for the high-redshift galaxy part of the Science Verification Campaign with the 220-440 GHz DESHIMA 2.0 integrated superconducting spectrometer on the ASTE telescope. The first version of the DESHIMA 2.0 chip has been r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b3dd1c82b68895ca309aa83b0e150c3
https://hdl.handle.net/1887/3561342
https://hdl.handle.net/1887/3561342
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Koji Yoshimura, Mitsuaki Nozaki, T. Yoshida, Takuya Wada, K. T. Kim, R. E. Streitmatter, N. Thakur, T. Hams, Reiko Orito, K. Sakai, Akira Yamamoto, M. Hasegawa, J. F. Ormes, John W. Mitchell, Yasuhiro Makida, Eun-Suk Seo, Hideyuki Fuke, M. H. Lee, J. Nishimura, K. Abe, Sadakazu Haino, Masaya Sasaki
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The Balloon-borne Experiment with a Superconducting Spectrometer (BESS) has carried out precise observation of the low-energy cosmic rays. Using a tracking system (in a 0.8 T uniform magnetic field) with a rigidity resolution of ∼0.4% at 1GV and a
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Endo, A., Pascual Laguna, A., Hähnle, S.A., Karatsu, K., Thoen, David, Murugesan, V., Baselmans, J.J.A., Zmuidzinas, Jonas, Gao, Jian-Rong
Publikováno v:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X
Journal of Astronomical Telescopes, Instruments, and Systems, 8(3)
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, 11453
Journal of Astronomical Telescopes, Instruments, and Systems, 8(3)
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, 11453
Superconducting resonators and transmission lines are fundamental building blocks of integrated circuits for millimeter-submillimeter astronomy. Accurate simulation of radiation loss from the circuit is crucial for the design of these circuits becaus
Autor:
Kim, K. C., Hams, T., Lee, M. H., Mitchell, J. W., Ormes, J. F., Sasaki, M., Seo, E. S., Streitmatter, R. E., Abe, Koh, Fuke, Hideyuki, Makida, Y., Matsuda, S., Nishimura, Jun, Shikaze, Y., Suzuki, J., Tanaka, K., Yamagami, Takamasa, Yamamoto, A., Yoshida, Tetsuya, Yoshimura, K.
Publikováno v:
Advances in Space Research. 51(2):234-237
著者人数: 20名
Accepted: 2012-01-23
資料番号: SA1004101000
Accepted: 2012-01-23
資料番号: SA1004101000
Autor:
Dimitar Draganov, M. Buchvarova
Publikováno v:
Solar Physics. 284:599-614
We discuss a model which parameterizes the cosmic-ray (CR) spectrum at different physical conditions, which include the most important effects controlling the CR intensity, like convection–diffusion and energy losses. By a suitable choice of parame