Zobrazeno 1 - 10
of 13 875
pro vyhledávání: '"Kondo S."'
Autor:
Elgueta, S. S., Matsunaga, N., Jian, M., Taniguchi, D., Kobayashi, N., Fukue, K., Hamano, S., Sameshima, H., Kondo, S., Arai, A., Ikeda, Y., Kawakita, H., Otsubo, S., Sarugaku, Y., Yasui, C., Tsujimoto, T.
Newly-developed spectrographs with increased resolving powers, particularly those covering the near-IR range, allow the characterization of more and more absorption lines in stellar spectra. This includes the identification and confirmation of absorp
Externí odkaz:
http://arxiv.org/abs/2307.00158
In the field of WiFi sensing, as an alternative sensing source of the channel state information (CSI) matrix, the use of a beamforming feedback matrix (BFM)that is a right singular matrix of the CSI matrix has attracted significant interest owing to
Externí odkaz:
http://arxiv.org/abs/2112.06695
Publikováno v:
Proc. IEEE 19th Annual Consumer Communications & Networking Conference (CCNC 2022)
This paper presents a method that estimates the respiratory rate based on the frame capturing of wireless local area networks. The method uses beamforming feedback matrices (BFMs) contained in the captured frames, which is a rotation matrix of channe
Externí odkaz:
http://arxiv.org/abs/2108.03170
Autor:
Kubo, T., Sunami, K., Koyama, T., Kitami, M., Fujiwara, Y., Kondo, S., Yonemori, K., Noguchi, E., Morizane, C., Goto, Y., Maejima, A., Iwasa, S., Hamaguchi, T., Kawai, A., Namikawa, K., Arakawa, A., Sugiyama, M., Ohno, M., Yoshida, T., Hiraoka, N., Yoshida, A., Yoshida, M., Nishino, T., Furukawa, E., Narushima, D., Nagai, M., Kato, M., Ichikawa, H., Kohno, T., Yamamoto, N.
Publikováno v:
In ESMO Open April 2024 9(4)
Autor:
Fukue, K., Matsunaga, N., Kondo, S., Taniguchi, D., Ikeda, Y., Kobayashi, N., Sameshima, H., Hamano, S., Arai, A., Kawakita, H., Yasui, C., Mizumoto, M., Otsubo, S., Takenaka, K., Yoshikawa, T., Tsujimoto, T.
Red giants show a large number of absorption lines in both optical and near-infrared wavelengths. Still, the characteristics of the lines in different wave passbands are not necessarily the same. We searched for lines of Mg I, Si I, Ca I, Ti I, Cr I,
Externí odkaz:
http://arxiv.org/abs/2103.12478
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
The time-global existence of unique smooth positive solutions to the reaction diffusion equations of the Keener-Tyson model for the Belousov-Zhabotinsky reaction in the whole space is established with bounded non-negative initial data. Deriving estim
Externí odkaz:
http://arxiv.org/abs/1903.10715
Autor:
Sameshima, H., Ikeda, Y., Matsunaga, N., Fukue, K., Kobayashi, N., Kondo, S., Hamano, S., Kawakita, H., Yasui, C., Izumi, N., Mizumoto, M., Otsubo, S., Takenaka, K., Watase, A., Asano, A., Yoshikawa, T.
We present a catalog of absorption lines in the z', Y, and J bands that we identified in 21 Lyn, a slowly rotating A0.5 V star. We detected 155 absorption features in the high-resolution (0.90-1.35 um, R = 28,000) spectrum obtained with the WINERED s
Externí odkaz:
http://arxiv.org/abs/1810.07206
Autor:
D'Orazi, V., Magurno, D., Bono, G., Matsunaga, N., Braga, V. F., Elgueta, S. S., Fukue, K., Hamano, S., Inno, L., Kobayashi, N., Kondo, S., Monelli, M., Nonino, M., Przybilla, P. N., Sameshima, H., Saviane, I., Taniguchi, D., Thevenin, F., Urbaneja-Perez, M., Watase, A., Arai, A., Bergemann, M., Buonanno, R., Dall'Ora, M., Silva, R., Fabrizio, M., Ferraro, I., Fiorentino, G., Francois, P., Gilmozzi, R., Iannicola, G., Ikeda, Y., Jian, M., Kawakita, H., Kudritzki, R. -P., Lemasle, B., Marengo, M., Marinoni, S., Martinez-Vasquez, C., Minniti, D., Neeley, J., Otsubo, S., Prieto, J. L., Proxauf, B., Romaniello, M., Sanna, N., Sneden, C., Takenaka, K., Tsujimoto, T., Valenti, E., Yasui, C., Yoshikawa, T., Zoccali, M.
We present the first spectroscopic abundance determination of iron, alpha-elements (Si, Ca and Ti) and sodium for the Mira variable V1 in the metal-rich globular cluster NGC 5927. We use high-resolution (R~ 28,000), high signal-to-noise ratio (~200)
Externí odkaz:
http://arxiv.org/abs/1802.07314
Autor:
Elgueta, S S, Matsunaga, N, Jian, M, Taniguchi, D, Kobayashi, N, Fukue, K, Hamano, S, Sameshima, H, Kondo, S, Arai, A, Ikeda, Y, Kawakita, H, Otsubo, S, Yasui, C, Tsujimoto, T
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Aug2024, Vol. 532 Issue 4, p3694-3712, 19p