Zobrazeno 1 - 10
of 906
pro vyhledávání: '"MIYATA,Takashi"'
Autor:
Uno, Kohki, Maeda, Keiichi, Nagao, Takashi, Nakaoka, Tatsuya, Motohara, Kentaro, Tajitsu, Akito, Konishi, Masahito, Koyama, Shuhei, Takahashi, Hidenori, Tanaka, Masaomi, Kuncarayakti, Hanindyo, Kawabata, Miho, Yamanaka, Masayuki, Aoki, Kentaro, Isogai, Keisuke, Taguchi, Kenta, Ogawa, Mao, Kawabata, Koji S., Yoshii, Yuzuru, Miyata, Takashi, Imazawa, Ryo
We have performed intensive follow-up observations of a Type IIn/Ia-CSM SN (SN IIn/Ia-CSM), 2020uem, with photometry, spectroscopy, and polarimetry. In this paper, we report on the results of our observations focusing on optical/near-infrared (NIR) p
Externí odkaz:
http://arxiv.org/abs/2301.09901
Autor:
Sasaki, Tomoyuki, Sugiyama, Mariko, Kuno, Mitsuhiro, Miyata, Takashi, Kobayashi, Tomoko, Yasuda, Yoshinori, Onoue, Takeshi, Takagi, Hiroshi, Hagiwara, Daisuke, Iwama, Shintaro, Suga, Hidetaka, Banno, Ryoichi, Arima, Hiroshi
Publikováno v:
In Physiology & Behavior 1 December 2024 287
Autor:
Matsumoto, Akinori, Ouchi, Masami, Nakajima, Kimihiko, Kawasaki, Masahiro, Murai, Kai, Motohara, Kentaro, Harikane, Yuichi, Ono, Yoshiaki, Kushibiki, Kosuke, Koyama, Shuhei, Aoyama, Shohei, Konishi, Masahiro, Takahashi, Hidenori, Isobe, Yuki, Umeda, Hiroya, Sugahara, Yuma, Onodera, Masato, Nagamine, Kentaro, Kusakabe, Haruka, Hirai, Yutaka, Moriya, Takashi J., Shibuya, Takatoshi, Komiyama, Yutaka, Fukushima, Keita, Fujimoto, Seiji, Hattori, Takashi, Hayashi, Kohei, Inoue, Akio K., Kikuchihara, Shotaro, Kojima, Takashi, Koyama, Yusei, Lee, Chien-Hsiu, Mawatari, Ken, Miyata, Takashi, Nagao, Tohru, Ozaki, Shinobu, Rauch, Michael, Saito, Tomoki, Suzuki, Akihiro, Takeuchi, Tsutomu T., Umemura, Masayuki, Xu, Yi, Yabe, Kiyoto, Zhang, Yechi, Yoshii, Yuzuru
The primordial He abundance $Y_\mathrm{P}$ is a powerful probe of cosmology. Currently, $Y_\mathrm{P}$ is best determined by observations of metal-poor galaxies, while there are only a few known local extremely metal-poor ($<0.1 Z_\odot$) galaxies (E
Externí odkaz:
http://arxiv.org/abs/2203.09617
Autor:
Miwata, Tsutomu, Suga, Hidetaka, Mitsumoto, Kazuki, Zhang, Jun, Hamada, Yoshimasa, Sakakibara, Mayu, Soen, Mika, Ozaki, Hajime, Asano, Tomoyoshi, Miyata, Takashi, Kawaguchi, Yohei, Yasuda, Yoshinori, Kobayashi, Tomoko, Sugiyama, Mariko, Onoue, Takeshi, Hagiwara, Daisuke, Iwama, Shintaro, Oyadomari, Seiichi, Arima, Hiroshi
Publikováno v:
In Peptides March 2024 173
Autor:
Ohsawa, Ryou, Hirota, Akira, Morita, Kohei, Abe, Shinsuke, Kastinen, Daniel, Kero, Johan, Szasz, Csilla, Fujiwara, Yasunori, Nakamura, Takuji, Nishimura, Koji, Sako, Shigeyuki, Watanabe, Jun-ichi, Aoki, Tsutomu, Arima, Noriaki, Arimatsu, Ko, Doi, Mamoru, Ichiki, Makoto, Ikeda, Shiro, Ita, Yoshifusa, Kasuga, Toshihiro, Kobayashi, Naoto, Kokubo, Mitsuru, Konishi, Masahiro, Maehara, Hiroyuki, Miyata, Takashi, Mori, Yuki, Morii, Mikio, Morokuma, Tomoki, Motohara, Kentaro, Nakada, Yoshikazu, Okumura, Shin-ichiro, Sarugaku, Yuki, Sato, Mikiya, Shigeyama, Toshikazu, Soyano, Takao, Takahashi, Hidenori, Tanaka, Masaomi, Tarusawa, Ken'ichi, Tominaga, Nozomu, Urakawa, Seitaro, Usui, Fumihiko, Yamashita, Takuya, Yoshikawa, Makoto
Publikováno v:
Planetary and Space Science 194 (2020) 10511
Radar and optical simultaneous observations of meteors are important to understand the size distribution of the interplanetary dust. However, faint meteors detected by high power large aperture radar observations, which are typically as faint as 10 m
Externí odkaz:
http://arxiv.org/abs/2008.08942
Autor:
Kamizuka, Takafumi, Nakada, Yoshikazu, Yanagisawa, Kenshi, Ohsawa, Ryou, Ita, Yoshifusa, Izumiura, Hideyuki, Mito, Hiroyuki, Onozato, Hiroki, Asano, Kentaro, Ueta, Toshiya, Miyata, Takashi
Publikováno v:
The Astrophysical Journal, Volume 897, Issue 1, id.42, 20 pp. (2020)
Non-variable OH/IR stars are thought to have just left the asymptotic giant branch (AGB) phase. In this conventional picture, they must still show strong circumstellar extinction caused by the dust ejected during the AGB phase, and the extinction is
Externí odkaz:
http://arxiv.org/abs/2008.06897
Akademický článek
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Autor:
Hayase, Ayaka, Onoue, Takeshi, Kobayashi, Tomoko, Wada, Eri, Handa, Tomoko, Kinoshita, Tamaki, Yamagami, Ayana, Yasuda, Yoshinori, Iwama, Shintaro, Kawaguchi, Yohei, Miyata, Takashi, Sugiyama, Mariko, Takagi, Hiroshi, Hagiwara, Daisuke, Suga, Hidetaka, Banno, Ryoichi, Kuwatsuka, Yachiyo, Ando, Masahiko, Goto, Motomitsu, Arima, Hiroshi
Publikováno v:
In Primary Care Diabetes December 2023 17(6):575-580
Autor:
Richmond, Michael W., Tanaka, Masaomi, Morokuma, Tomoki, Sako, Shigeyuki, Ohsawa, Ryou, Arima, Noriaki, Tominaga, Nozomu, Doi, Mamoru, Aoki, Tsutomu, Arimatsu, Ko, Ichiki, Makoto, Ikeda, Shiro, Ita, Yoshifusa, Kasuga, Toshihiro, Kawabata, Koji S., Kawakita, Hideyo, Kobayashi, Naoto, Kokubo, Mitsuru, Konishi, Masahiro, Maehara, Hiroyuki, Mito, Hiroyuki, Miyata, Takashi, Mori, Yuki, Morii, Mikio, Motohara, Kentaro, Nakada, Yoshikazu, Shin-Ich, Onozato, Hiroki, Sarugaku, Yuki, Sato, Mikiya, Shigeyama, Toshikazu, Soyano, Takao, Takahashi, Hidenori, Tanikawa, Ataru, Tarusawa, Ken'ichi, Urakawa, Seitaro, Usui, Fumihiko, Watanabe, Junichi, Yamashita, Takuya, Yoshikawa, Makoto
Using a prototype of the Tomo-e Gozen wide-field CMOS mosaic camera, we acquire wide-field optical images at a cadence of 2 Hz and search them for transient sources of duration 1.5 to 11.5 seconds. Over the course of eight nights, our survey encompas
Externí odkaz:
http://arxiv.org/abs/1910.11343
Autor:
Arimatsu, Ko, Ohsawa, Ryou, Hashimoto, George L., Urakawa, Seitaro, Takahashi, Jun, Tozuka, Miyako, Itoh, Yoichi, Yamashita, Misato, Usui, Fumihiko, Aoki, Tsutomu, Arima, Noriaki, Doi, Mamoru, Ichiki, Makoto, Ikeda, Shiro, Ita, Yoshifusa, Kasuga, Toshihiro, Kobayashi, Naoto, Kokubo, Mitsuru, Konishi, Masahiro, Maehara, Hiroyuki, Matsunaga, Noriyuki, Miyata, Takashi, Morii, Mikio, Morokuma, Tomoki, Motohara, Kentaro, Nakada, Yoshikazu, Okumura, Shin-ichiro, Sako, Shigeyuki, Sarugaku, Yuki, Sato, Mikiya, Shigeyama, Toshikazu, Soyano, Takao, Takahashi, Hidenori, Tarusawa, Ken'ichi, Tominaga, Nozomu, Watanabe, Jun-ichi, Yamashita, Takuya, Yoshikawa, Makoto
We report observations of a stellar occultation by the classical Kuiper belt object (50000) Quaoar occurred on 28 June 2019. A single-chord high-cadence (2 Hz) photometry dataset was obtained with the Tomo-e Gozen CMOS camera mounted on the 1.05 m Sc
Externí odkaz:
http://arxiv.org/abs/1910.09988