Zobrazeno 1 - 10
of 199
pro vyhledávání: '"SAGAWA, Hideo"'
Autor:
Tamura, Yoichi, Sakai, Takeshi, Kawabe, Ryohei, Kojima, Takafumi, Taniguchi, Akio, Takekoshi, Tatsuya, Kang, Haoran, Shan, Wenlei, Hagimoto, Masato, Okauchi, Norika, Tetsuka, Airi, Inoue, Akio K., Kohno, Kotaro, Tanaka, Kunihiko, Bakx, Tom J. L. C., Fudamoto, Yoshinobu, Fujita, Kazuyuki, Harikane, Yuichi, Hashimoto, Takuya, Hatsukade, Bunyo, Hughes, David H., Iino, Takahiro, Kimura, Yuki, Maezawa, Hiroyuki, Matsuda, Yuichi, Mawatari, Ken, Nakajima, Taku, Nakatsubo, Shunichi, Oshima, Tai, Sagawa, Hideo, Schloerb, F. Peter, Takahashi, Shigeru, Taniguchi, Kotomi, Tsujita, Akiyoshi, Umehata, Hideki, Yonetsu, Teppei, Yun, Min S.
Unveiling the emergence and prevalence of massive/bright galaxies during the epoch of reionization and beyond, within the first 600 million years of the Universe, stands as a pivotal pursuit in astronomy. Remarkable progress has been made by JWST in
Externí odkaz:
http://arxiv.org/abs/2406.07975
Autor:
Gapp, Cyril, Rengel, Miriam, Hartogh, Paul, Sagawa, Hideo, Feuchtgruber, Helmut, Lellouch, Emmanuel, Villanueva, Geronimo L.
$Context.$ On October 31, 2009, the Photodetector Array Camera and Spectrometer (PACS) on board the Herschel Space Observatory observed far-infrared spectra of Jupiter between 50 and 220$\,\mu$m as part of the program "Water and Related Chemistry in
Externí odkaz:
http://arxiv.org/abs/2406.02179
Autor:
Team, GREX-PLUS Science, Inoue, Akio K., Harikane, Yuichi, Moriya, Takashi, Nomura, Hideko, Baba, Shunsuke, Fujii, Yuka, Gouda, Naoteru, Hirahara, Yasuhiro, Kawashima, Yui, Kodama, Tadayuki, Koyama, Yusei, Kurokawa, Hiroyuki, Matsuo, Taro, Matsuoka, Yoshiki, Matsuura, Shuji, Mawatari, Ken, Misawa, Toru, Nagamine, Kentaro, Nakajima, Kimihiko, Notsu, Shota, Ootsubo, Takafumi, Ohno, Kazumasa, Sagawa, Hideo, Shimonishi, Takashi, Tadaki, Ken-ichi, Takami, Michihiro, Terai, Tsuyoshi, Toba, Yoshiki, Yamashita, Takuji, Yasui, Chikako
GREX-PLUS (Galaxy Reionization EXplorer and PLanetary Universe Spectrometer) is a mission candidate for a JAXA's strategic L-class mission to be launched in the 2030s. Its primary sciences are two-fold: galaxy formation and evolution and planetary sy
Externí odkaz:
http://arxiv.org/abs/2304.08104
Autor:
Kimura, Tomoki, Fujii, Yuka, Kita, Hajime, Tsuchiya, Fuminori, Sagawa, Hideo, Team, the SKA-Japan Planetary Science
Bodies such as planets, moons, and asteroids in our solar system are the brightest objects in the low-frequency radio astronomy at $\lesssim$ 10 GHz. The low-frequency radio emissions from our solar system bodies exhibit various observed characterist
Externí odkaz:
http://arxiv.org/abs/2303.07579
We present the first determination of the abundance ratios of $^{13}$C substitutions of cyanoacetylene (HC$_{3}$N), [H$^{13}$CCCN]:[HC$^{13}$CCN]:[HCC$^{13}$CN] in Titan's atmosphere measured using millimeter-wave spectra obtained by the Atacama Larg
Externí odkaz:
http://arxiv.org/abs/2108.05019
We present a spatially resolved map of integrated-intensity and abundance of Neptune's stratospheric hydrogen cyanide (HCN). The analyzed data were obtained from the archived 2016 observation of the Atacama Large Millimeter/submillimeter Array. A 0.4
Externí odkaz:
http://arxiv.org/abs/2009.14072
Autor:
Greaves, Jane S., Richards, Anita M. S., Bains, William, Rimmer, Paul B., Sagawa, Hideo, Clements, David L., Seager, Sara, Petkowski, Janusz J., Sousa-Silva, Clara, Ranjan, Sukrit, Drabek-Maunder, Emily, Fraser, Helen J., Cartwright, Annabel, Mueller-Wodarg, Ingo, Zhan, Zhuchang, Friberg, Per, Coulson, Iain, Lee, E'lisa, Hoge, Jim
Publikováno v:
Greaves, J. S., Richards, A. M., Bains, W., Rimmer, P. B., Sagawa, H., Clements, D. L., ... & Hoge, J. (2020). Phosphine gas in the cloud decks of Venus. Nature Astronomy, 1-10
Measurements of trace-gases in planetary atmospheres help us explore chemical conditions different to those on Earth. Our nearest neighbor, Venus, has cloud decks that are temperate but hyper-acidic. We report the apparent presence of phosphine (PH3)
Externí odkaz:
http://arxiv.org/abs/2009.06593
Each of the nitriles present in the atmosphere of Titan can be expected to exhibit different \ce{^{14}N/^{15}N} values depending on their production processes, primarily because of the various \ce{N2} dissociation processes induced by different sourc
Externí odkaz:
http://arxiv.org/abs/2001.01484
Autor:
Peralta, Javier, Muto, Keishiro, Hueso, Ricardo, Horinouchi, Takeshi, Sánchez-Lavega, Agustín, Murakami, Shin-ya, Machado, Pedro, Young, Eliot F., Lee, Yeon Joo, Kouyama, Toru, Sagawa, Hideo, McGouldrick, Kevin, Satoh, Takehiko, Imamura, Takeshi, Limaye, Sanjay S., Sato, Takao M., Ogohara, Kazunori, Nakamura, Masato, Luz, David
Publikováno v:
The Astrophysical Journal Supplement Series, Volume 239, Number 2, id. 29 (2018)
We present measurements of the wind speeds at the nightside lower clouds of Venus from observations by JAXA's mission Akatsuki during 2016, complemented with new wind measurements from ground-based observations acquired with TNG/NICS in 2012 and IRTF
Externí odkaz:
http://arxiv.org/abs/1810.05418