Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Raquel, Bjorn Jasper"'
Autor:
Lin, Leah Ya-Ling, Hashimoto, Tetsuya, Goto, Tomotsugu, Raquel, Bjorn Jasper, Ho, Simon C. -C., Chen, Bo-Han, Kim, Seong Jin, Ling, Chih-Teng
Fast radio bursts (FRBs) are millisecond-duration radio waves from the Universe. Even though more than 50 physical models have been proposed, the origin and physical mechanism of FRB emissions are still unknown. The classification of FRBs is one of t
Externí odkaz:
http://arxiv.org/abs/2410.00576
Autor:
Chien, Tom C. -C., Ling, Chih-Teng, Goto, Tomotsugu, Wu, Cossas K. -W., Kim, Seong Jin, Hashimoto, Tetsuya, Lin, Yu-Wei, Kilerci, Ece, Ho, Simon C. -C., Wang, Po-Ya, Raquel, Bjorn Jasper R.
The nature of the interaction between active galactic nuclei (AGNs) and their host galaxies remains an unsolved question. Therefore, conducting an AGN census is valuable to AGN research. Nevertheless, a significant fraction of AGNs are obscured by th
Externí odkaz:
http://arxiv.org/abs/2406.14888
Autor:
Lin, Yu-Wei, Wu, Cossas K. -W., Ling, Chih-Teng, Goto, Tomotsugu, Kim, Seong Jin, Kilerci, Ece, Hashimoto, Tetsuya, Wang, Po-Ya, Ho, Simon C. -C., Hsiao, Tiger Yu-Yang, Raquel, Bjorn Jasper R., Uno, Yuri
It has been an unanswered question how many dusty galaxies have been undetected from the state-of-the-art observational surveys. JWST enables us to detect faint IR galaxies that have prominent polycyclic aromatic hydrocarbon (PAH) features in the mid
Externí odkaz:
http://arxiv.org/abs/2401.01043
Autor:
Raquel, Bjorn Jasper R., Hashimoto, Tetsuya, Goto, Tomotsugu, Chen, Bo Han, Uno, Yuri, Hsiao, Tiger Yu-Yang, Kim, Seong Jin, Ho, Simon C. -C.
Fast Radio Bursts (FRBs) are mysterious bursts in the millisecond timescale at radio wavelengths. Currently, there is little understanding about the classification of repeating FRBs, based on difference in physics, which is of great importance in und
Externí odkaz:
http://arxiv.org/abs/2307.02811
Autor:
Chen, Bo Han, Hashimoto, Tetsuya, Goto, Tomotsugu, Raquel, Bjorn Jasper R., Uno, Yuri, Kim, Seong Jin, Hsiao, Tiger Y. -Y., Ho, Simon C. -C.
Fast radio bursts (FRBs) are astronomical transients with millisecond timescales. Although most of the FRBs are not observed to repeat, a few of them are detected to repeat more than hundreds of times. There exist a large variety of physical properti
Externí odkaz:
http://arxiv.org/abs/2303.17133
Autor:
Hsiao, Tiger Yu-Yang, Goto, Tomotsugu, Hashimoto, Tetsuya, Santos, Daryl Joe D., Wong, Yi Hang Valerie, Kim, Seong Jin, Raquel, Bjorn Jasper R., Ho, Simon C. -C., Chen, Bo-Han, Kilerci, Ece, Lu, Ting-Yi, On, Alvina Y. L., Lin, Yu-Wei, Wu, Cossas K. -W.
The Hubble constant ($H_{0}$) is a measurement to describe the expansion rate of the Universe in the current era. However, there is a $4.4\sigma$ discrepancy between the measurements from the early Universe and the late Universe. In this research, we
Externí odkaz:
http://arxiv.org/abs/2209.05008
Autor:
Lin, Hsiu-Hsien, Lin, Kai-yang, Li, Chao-Te, Tseng, Yao-Huan, Jiang, Homin, Wang, Jen-Hung, Cheng, Jen-Chieh, Pen, Ue-Li, Chen, Ming-Tang, Chen, Pisin, Chen, Yaocheng, Goto, Tomotsugu, Hashimoto, Tetsuya, Hwang, Yuh-Jing, King, Sun-Kun, Kubo, Derek, Kuo, Chung-Yun, Mills, Adam, Nam, Jiwoo, Oshiro, Peter, Shen, Chang-Shao, Tseng, Hsien-Chun, Wang, Shih-Hao, Wu, Vigo Feng-Shun, Bower, Geoffrey, Chang, Shu-Hao, Chen, Pai-An, Chen, Ying-Chih, Chiang, Yi-Kuan, Fedynitch, Anatoli, Gusinskaia, Nina, Ho, Simon C. -C., Hsiao, Tiger Y. -Y., Hu, Chin-Ping, De Huang, Yau, Garcia, Jose Miguel Jauregui, Kim, Seong Jin, Kuo, Cheng-Yu, Ling, Decmend Fang-Jie, On, Alvina Y. L., Peterson, Jeffrey B., Raquel, Bjorn Jasper R., Su, Shih-Chieh, Uno, Yuri, Wu, Cossas K. -W., Yamasaki, Shotaro, Zhu, Hong-Ming
Publikováno v:
PASP 134 094106 (2022)
Fast Radio Bursts (FRBs) are bright millisecond-duration radio transients that appear about 1,000 times per day, all-sky, for a fluence threshold 5 Jy ms at 600 MHz. The FRB radio-emission physics and the compact objects involved in these events are
Externí odkaz:
http://arxiv.org/abs/2206.08983
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Lin, Yu-Wei, Wu, Cossas K-W, Ling, Chih-Teng, Goto, Tomotsugu, Kim, Seong Jin, Kilerci, Ece, Hashimoto, Tetsuya, Wang, Po-Ya, Ho, Simon C-C, Hsiao, Tiger Yu-Yang, Raquel, Bjorn Jasper R, Uno, Yuri
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Feb2024, Vol. 527 Issue 4, p11882-11892, 11p
