Zobrazeno 1 - 10
of 345
pro vyhledávání: '"Yamada Kyohei"'
Autor:
Noriaki Kawano, Yamada Kyohei, Hiroaki Miyoshi, Noriaki Yoshida, Kouichi Ohshima, Fumiko Arakawa, Kazutaka Nakashima, Takuro Kameda, Yasunori Kogure, Yuta Ito, Shuro Yoshida, Takuro Kuriyama, Takashi Nakaike, Taro Tochigi, Ken Takigawa, Kiyoshi Yamashita, Atsushi Toyofuku, Tatsuya Manabe, Atsushi Doi, Soushi Terasaka, Kouske Marutsuka, Hidenobu Ochiai, Ikuo Kikuchi, Yasuo Mori, Keisuke Kataoka, Tomoharu Yoshizumi, Junji Yamauchi, Yoshihisa Yamano, Kazuya Shimoda
Publikováno v:
Renal Replacement Therapy, Vol 9, Iss 1, Pp 1-17 (2023)
Abstract Backgrounds Therefore, reports on the risk of HTLV-1-related diseases in organ transplantation have increased in recent years, and the management of HTLV in renal transplantation remains a challenge. Patients and methods We retrospectively a
Externí odkaz:
https://doaj.org/article/db83b28a408246b89cb019124a3a59df
Autor:
Koopman, Brian J., Bhimani, Sanah, Galitzki, Nicholas, Hasselfield, Matthew, Lashner, Jack, Nakata, Hironobu, Newburgh, Laura, Nguyen, David V., Sakuma, Tai, Yamada, Kyohei
The Simons Observatory (SO) is a cosmic microwave background (CMB) observatory consisting of three small aperture telescopes and one large aperture telescope. SO is located in the Atacama Desert in Chile at an elevation of 5180m. Distributed among th
Externí odkaz:
http://arxiv.org/abs/2406.15703
Autor:
Nguyen, David V., Bhimani, Sanah, Galitzki, Nicholas, Koopman, Brian J., Lashner, Jack, Newburgh, Laura, Silva-Feaver, Max, Yamada, Kyohei
The Simons Observatory (SO) is a group of modern telescopes dedicated to observing the polarized cosmic microwave background (CMB), transients, and more. The Observatory consists of four telescopes and instruments, with over 60,000 superconducting de
Externí odkaz:
http://arxiv.org/abs/2406.14089
Autor:
Galitzki, Nicholas, Tsan, Tran, Spisak, Jake, Randall, Michael, Silva-Feaver, Max, Seibert, Joseph, Lashner, Jacob, Adachi, Shunsuke, Adkins, Sean M., Alford, Thomas, Arnold, Kam, Ashton, Peter C., Austermann, Jason E., Baccigalupi, Carlo, Bazarko, Andrew, Beall, James A., Bhimani, Sanah, Bixler, Bryce, Coppi, Gabriele, Corbett, Lance, Crowley, Kevin D., Crowley, Kevin T., Day-Weiss, Samuel, Dicker, Simon, Dow, Peter N., Duell, Cody J., Duff, Shannon M., Gerras, Remington G., Groh, John C., Gudmundsson, Jon E., Harrington, Kathleen, Hasegawa, Masaya, Healy, Erin, Henderson, Shawn W., Hubmayr, Johannes, Iuliano, Jeffrey, Johnson, Bradley R., Keating, Brian, Keller, Ben, Kiuchi, Kenji, Kofman, Anna M., Koopman, Brian J., Kusaka, Akito, Lee, Adrian T., Lew, Richard A., Lin, Lawrence T., Link, Michael J, Lucas, Tammy J., Lungu, Marius, Mangu, Aashrita, McMahon, Jeffrey J, Miller, Amber D., Moore, Jenna E., Morshed, Magdy, Nakata, Hironobu, Nati, Federico, Newburgh, Laura B., Nguyen, David V., Niemack, Michael D., Page, Lyman A., Sakaguri, Kana, Sakurai, Yuki, Rao, Mayuri Sathyanarayana, Saunders, Lauren J., Shroyer, Jordan E., Sugiyama, Junna, Tajima, Osamu, Takeuchi, Atsuto, Bua, Refilwe Tanah, Teply, Grant, Terasaki, Tomoki, Ullom, Joel N., Van Lanen, Jeffrey L., Vavagiakis, Eve M., Vissers, Michael R, Walters, Liam, Wang, Yuhan, Xu, Zhilei, Yamada, Kyohei, Zheng, Kaiwen
The Simons Observatory (SO) is a cosmic microwave background (CMB) survey experiment that includes small-aperture telescopes (SATs) observing from an altitude of 5,200 m in the Atacama Desert in Chile. The SO SATs will cover six spectral bands betwee
Externí odkaz:
http://arxiv.org/abs/2405.05550
Autor:
Adachi, Shunsuke, Adkins, Tylor, Baccigalupi, Carlo, Chinone, Yuji, Crowley, Kevin T., Errard, Josquin, Fabbian, Giulio, Feng, Chang, Fujino, Takuro, Hasegawa, Masaya, Hazumi, Masashi, Jeong, Oliver, Kaneko, Daisuke, Keating, Brian, Kusaka, Akito, Lee, Adrian T., Lonappan, Anto I., Minami, Yuto, Murata, Masaaki, Piccirillo, Lucio, Reichardt, Christian L., Siritanasak, Praween, Spisak, Jacob, Takakura, Satoru, Teply, Grant P., Yamada, Kyohei
The Crab Nebula, also known as Tau A, is a polarized astronomical source at millimeter wavelengths. It has been used as a stable light source for polarization angle calibration in millimeter-wave astronomy. However, it is known that its intensity and
Externí odkaz:
http://arxiv.org/abs/2403.02096
Autor:
Sugiyama, Junna, Terasaki, Tomoki, Sakaguri, Kana, Bixler, Bryce, Sakurai, Yuki, Arnold, Kam, Crowley, Kevin T., Datta, Rahul, Galitzki, Nicholas, Hasegawa, Masaya, Johnson, Bradley R., Keating, Brian, Kusaka, Akito, Lee, Adrian, Matsumura, Tomotake, Mcmahon, Jeffrey, Silva-Feaver, Maximiliano, Wang, Yuhan, Yamada, Kyohei
Publikováno v:
J Low Temp Phys (2024)
The Simons Observatory (SO) experiment is a cosmic microwave background (CMB) experiment located in the Atacama Desert, Chile. The SO' s small aperture telescopes (SATs) consist of three telescopes designed for precise CMB polarimetry at large angula
Externí odkaz:
http://arxiv.org/abs/2402.09620
Autor:
Murata, Masaaki, Nakata, Hironobu, Iijima, Kengo, Adachi, Shunsuke, Seino, Yudai, Kiuchi, Kenji, Matsuda, Frederick, Randall, Michael J., Arnold, Kam, Galitzki, Nicholas, Johnson, Bradley R., Keating, Brian, Kusaka, Akito, Lloyd, John B., Seibert, Joseph, Silva-Feaver, Maximiliano, Tajima, Osamu, Terasaki, Tomoki, Yamada, Kyohei
Publikováno v:
Rev. Sci. Instrum. 94, 124502 (2023)
For cosmic microwave background (CMB) polarization observations, calibration of detector polarization angles is essential. We have developed a fully remote controlled calibration system with a sparse wire grid that reflects linearly polarized light a
Externí odkaz:
http://arxiv.org/abs/2309.02035
Autor:
The POLARBEAR Collaboration, Adachi, Shunsuke, Adkins, Tylor, Arnold, Kam, Baccigalupi, Carlo, Barron, Darcy, Cheung, Kolen, Chinone, Yuji, Crowley, Kevin T., Errard, Josquin, Fabbian, Giulio, Feng, Chang, Flauger, Raphael, Fujino, Takuro, Green, Daniel, Hasegawa, Masaya, Hazumi, Masashi, Kaneko, Daisuke, Katayama, Nobuhiko, Keating, Brian, Kusaka, Akito, Lee, Adrian T., Minami, Yuto, Nishino, Haruki, Reichardt, Christian L., Siritanasak, Praween, Spisak, Jacob, Tajima, Osamu, Takakura, Satoru, Takatori, Sayuri, Teply, Grant Paul, Yamada, Kyohei
Publikováno v:
Phys. Rev. D 108, 043017 (2023)
Very light pseudoscalar fields, often referred to as axions, are compelling dark matter candidates and can potentially be detected through their coupling to the electromagnetic field. Recently a novel detection technique using the cosmic microwave ba
Externí odkaz:
http://arxiv.org/abs/2303.08410
Autor:
Iyono Atsushi, Yamamoto Saya, Aoki Shigeki, Hara Toshio, Kuretsubo Kenji, Marushima Toshitsugu, Matsumoto Haruka, Mizutani Fukashi, Ozaki Keita, Shibayama Emi, Suzuki Atsumu, Takahashi Satoru, Tateishi Yurie, Yabu Misato, Yamada Kyohei, Kodama Koichi, Hamada Kaname, Kawahara Hiroaki, Komatani Ryosuke, Komatsu Masahiro, Miyanishi Motoaki, Morishita Misaki, Morishima Kunihiro, Nakamura Mitsuhiro, Naganawa Naotaka, Nanano Toshiyuki, Nishio Akira, Niwa Kimio, Otsuka Naoto, Rokujo Hiroki, Sato Osamu, Yoshimoto Masahiro
Publikováno v:
EPJ Web of Conferences, Vol 145, p 06003 (2017)
Nuclear emulsion plates for studying elementary particle physics as well as cosmic ray physics are very powerful tracking tools with sub-micron spatial resolutions of charged particle trajectories. Even if gamma rays have to be detected, electron-pos
Externí odkaz:
https://doaj.org/article/7e57f18c35ef423c913d0b5402998a1b
Publikováno v:
In Sensors and Actuators: A. Physical 1 May 2024 370