Zobrazeno 1 - 10
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pro vyhledávání: '"Maeda A"'
Autor:
Yamaguchi F, Suzuki A, Hashiguchi M, Kondo E, Maeda A, Yokoe T, Sasaki J, Shikama Y, Hayashi M, Kobayashi S, Suzuki H
Publikováno v:
Infection and Drug Resistance, Vol Volume 17, Pp 161-170 (2024)
Fumihiro Yamaguchi,1 Ayako Suzuki,2 Miyuki Hashiguchi,3 Emiko Kondo,3 Atsuo Maeda,4 Takuya Yokoe,1 Jun Sasaki,4 Yusuke Shikama,1 Munetaka Hayashi,4 Sei Kobayashi,5 Hiroshi Suzuki6 1Department of Respiratory Medicine, Showa University Fujigaoka Hospit
Externí odkaz:
https://doaj.org/article/ab44bc7f40294866ada8b49e3ad9085d
Publikováno v:
South African Journal of Chemical Engineering, Vol 43, Iss , Pp 104-111 (2023)
Calcium sulfate scale occurrence is one of the major problems encountered on heat exchanger surfaces, membrane surfaces of reverse osmosis (RO) plants, and oilfield facilities. Scale prevention and treatment are extensively applied for confronting th
Externí odkaz:
https://doaj.org/article/2ebf1e51e06d4926bb31b0e9929451f5
Autor:
Reguitti, A., Dastidar, R., Pignata, G., Maeda, K., Moriya, T. J., Kuncarayakti, H., Rodríguez, Ó., Bersten, M., Anderson, J. P., Charalampopoulos, P., Fraser, M., Gromadzki, M., Young, D. R., Benetti, S., Cai, Y. -Z., Elias-Rosa, N., Lundqvist, P., Carini, R., Cosentino, S. P., Galbany, L., Gonzalez-Bañuelos, M., Gutiérrez, C. P., Kopsacheili, M., G., J. A. Pineda, Ramirez, M.
We present an analysis of the photometric and spectroscopic dataset of the Type II supernova (SN) 2018ivc in the nearby (10 Mpc) galaxy Messier 77. Thanks to the high cadence of the CHASE survey, we observed the SN rising very rapidly by nearly three
Externí odkaz:
http://arxiv.org/abs/2409.16890
Autor:
Maeda, Kento, Ikeda, Atsushi
The viscosity of supercooled liquids notably increases with decreasing temperature, leading to solidification through a glass transition. This process is accompanied by dynamic heterogeneity, characterized by persistent dynamic spatial correlations.
Externí odkaz:
http://arxiv.org/abs/2409.16725
The recent observations by the James Webb Space Telescope (JWST) have revealed a larger number of bright galaxies at $z\gtrsim10$ than was expected. The origin of this excess is still under debate, although several possibilities have been presented.
Externí odkaz:
http://arxiv.org/abs/2409.11468
Context. Supernova remnants (SNRs) are the late stages of supernovae before their merging into the surrounding medium. Oxygen-rich supernova remnants represent a rare subtype with strong visible light oxygen emission. Aims. We present a new method to
Externí odkaz:
http://arxiv.org/abs/2409.06504
Autor:
Fang, Qiliang, Moriya, Takashi J., Ferrari, Lucía, Maeda, Keiichi, Folatelli, Gaston, Ertini, Keila Y., Kuncarayakti, Hanindyo, Andrews, Jennifer E., Matsumoto, Tatsuya
SN 2023ixf is one of the most well-observed core-collapse supernova in recent decades, yet there is inconsistency in the inferred zero-age-main-sequence (ZAMS) mass $M_{\rm ZAMS}$ of its progenitor. Direct observations of the pre-SN red supergiant (R
Externí odkaz:
http://arxiv.org/abs/2409.03540
Autor:
Gangopadhyay, Anjasha, Dukiya, Naveen, Moriya, Takashi J, Tanaka, Masaomi, Maeda, Keiichi, Howell, D. Andrew, Singh, Mridweeka, Singh, Avinash, Sollerman, Jesper, Kawabata, Koji S, Brennan, Sean J, Pellegrino, Craig, Dastidar, Raya, Nakaoka, Tatsuya, Kawabata, Miho, Misra, Kuntal, Schulze, Steve, Chandra, Poonam, Taguchi, Kenta, Sahu, Devendra K, McCully, Curtis, Bostroem, K. Azalee, Gonzalez, Estefania Padilla, Newsome, Megan, Hiramatsu, Daichi, Takei, Yuki, Yamanaka, Masayuki, Tajitsu, Akito, Isogai, Keisuke
We present the long-term photometric and spectroscopic analysis of a transitioning SN~IIn/Ibn from $-$10.8 d to 150.7 d post $V$-band maximum. SN~2021foa shows prominent He {\sc i} lines comparable in strength to the H$\alpha$ line around peak, placi
Externí odkaz:
http://arxiv.org/abs/2409.02666
Autor:
Schulze, Steve, Gal-Yam, Avishay, Dessart, Luc, Miller, Adam A., Woosley, Stan E., Yang, Yi, Bulla, Mattia, Yaron, Ofer, Sollerman, Jesper, Filippenko, Alexei V., Hinds, K-Ryan, Perley, Daniel A., Tsuna, Daichi, Lunnan, Ragnhild, Sarin, Nikhil, Brennan, Sean J., Brink, Thomas G., Bruch, Rachel J., Chen, Ping, Das, Kaustav K., Dhawan, Suhail, Fransson, Claes, Fremling, Christoffer, Gangopadhyay, Anjasha, Irani, Ido, Jerkstrand, Anders, Knezevic, Nikola, Kushnir, Doron, Maeda, Keiichi, Maguire, Kate, Ofek, Eran, Omand, Conor M. B., Qin, Yu-Jing, Sharma, Yashvi, Sit, Tawny, Srinivasaragavan, Gokul P., Strothjohann, Nora L., Takei, Yuki, Waxman, Eli, Yan, Lin, Yao, Yuhan, Zheng, WeiKang, Zimmerman, Erez A., Bellm, Eric C., Coughlin, Michael W., Masci, Frank. J., Purdum, Josiah, Rigault, Mickael, Wold, Avery, Kulkarni, Shrinivas R.
The cores of stars are the cosmic furnaces where light elements are fused into heavier nuclei. The fusion of hydrogen to helium initially powers all stars. The ashes of the fusion reactions are then predicted to serve as fuel in a series of stages, e
Externí odkaz:
http://arxiv.org/abs/2409.02054
We propose a new strategy called think twice before recognizing to improve fine-grained traffic sign recognition (TSR). Fine-grained TSR in the wild is difficult due to the complex road conditions, and existing approaches particularly struggle with c
Externí odkaz:
http://arxiv.org/abs/2409.01534