Rezultaty - "Ministry of Education of the Republic of China"

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  1. 1
    Polarization Position Angle Swing and the Rotating Vector Model of Repeating Fast Radio Bursts

    Polarization Position Angle Swing and the Rotating Vector Model of Repeating Fast Radio Bursts od Xiaohui Liu, Heng Xu, Jiarui Niu, Yongkun Zhang, Jinchen Jiang, Dejiang Zhou, Jinlin Han, Weiwei Zhu, Kejia Lee, Di Li, Wei-Yang Wang, Bing Zhang, Xuelei Chen, Jia-Wei Luo, Rui Luo, Chenhui Niu, Yuanhong Qu, Bojun Wang, Fayin Wang, Pei Wang, Tiancong Wang, Qin Wu, Ziwei Wu, Jiangwei Xu, Yuan-Pei Yang, Jun-Shuo Zhang

    Wydane 2025-01-01

    Fast radio bursts (FRBs), typically highly polarized, usually have a nearly constant polarization position angle (PA) during each burst. Some bursts show significant PA variations, and one of them was claimed to have a PA variation pattern consistent with the prediction of the rotating vector model...

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  2. 2
    Softness Ratio of SWIFT Gamma-Ray Bursts and Relevant Correlations

    Softness Ratio of SWIFT Gamma-Ray Bursts and Relevant Correlations od Fan Xu, Yong-Feng Huang, Liang Li, Jin-Jun Geng, Xue-Feng Wu, Song-Bo Zhang, Chen Deng, Chen-Ran Hu, Xiao-Fei Dong, Hao-Xuan Gao

    Wydane 2025-01-01

    The properties of X-ray flashes (XRFs) and X-ray-rich gamma-ray bursts (XRRs) as compared with classical gamma-ray bursts (C-GRBs) have been widely discussed during the SWIFT era. It has been proposed that XRFs and XRRs are low-energy extensions of the gamma-ray burst (GRB) population, and therefore...

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  3. 3
    EP240801a/XRF 240801B: An X-Ray Flash Detected by the Einstein Probe and the Implications of Its Multiband Afterglow

    EP240801a/XRF 240801B: An X-Ray Flash Detected by the Einstein Probe and the Implications of Its Multiband Afterglow od Shuai-Qing Jiang, Dong Xu, Agnes P. C. van Hoof, Wei-Hua Lei, Yuan Liu, Hao Zhou, Yong Chen, Shao-Yu Fu, Jun Yang, Xing Liu, Zi-Pei Zhu, Alexei V. Filippenko, Peter G. Jonker, A. S. Pozanenko, He Gao, Xue-Feng Wu, Bing Zhang, Gavin P Lamb, Massimiliano De Pasquale, Shiho Kobayashi, Franz Erik Bauer, Hui Sun, Giovanna Pugliese, Jie An, Valerio D’Elia, Johan P. U. Fynbo, WeiKang Zheng, Alberto J. Castro-Tirado, Yi-Han Iris Yin, Yuan-Chuan Zou, Adam T. Deller, N. S. Pankov, A. A. Volnova, A. S. Moskvitin, O. I. Spiridonova, D. V. Oparin, V. Rumyantsev, O. A. Burkhonov, Sh. A. Egamberdiyev, V. Kim, M. Krugov, A. M. Tatarnikov, R. Inasaridze, Andrew J. Levan, Daniele Bjørn Malesani, Maria E. Ravasio, Jonathan Quirola-Vásquez, Joyce N. D. van Dalen, Javi Sánchez-Sierras, Daniel Mata Sánchez, Stuart P. Littlefair, Jennifer A. Chacón, Manuel A. P. Torres, Ashley A. Chrimes, Nikhil Sarin, Antonio Martin-Carrillo, Vik Dhillon, Yi Yang, Thomas G. Brink, Rebecca L. Davies, Sheng Yang, Amar Aryan, Ting-Wan Chen, Albert K. H. Kong, Wen-Xiong Li, Rui-Zhi Li, Jirong Mao, Ignacio Pérez-García, Emilio J. Fernández-García, Moira Andrews, Joseph Farah, Zhou Fan, Estefania Padilla Gonzalez, D. Andrew Howell, Dieter Hartmann, Jing-Wei Hu, Páll Jakobsson, Cheng-Kui Li, Zhi-Xing Ling, Curtis McCully, Megan Newsome, Benjamin Schneider, Kaew Samaporn Tinyanont, Ning-Chen Sun, Giacomo Terreran, Qing-Wen Tang, Wen-Xin Wang, Jing-Jing Xu, Wei-Min Yuan, Bin-Bin Zhang, Hai-Sheng Zhao, Juan Zhang

    Wydane 2025-01-01

    We present multiband observations and analysis of EP240801a, a low-energy, extremely soft gamma-ray burst (GRB) discovered on 2024 August 1 by the Einstein Probe (EP) satellite with a weak contemporaneous signal also detected by the Fermi Gamma-ray Burst Monitor (GBM). Optical spectroscopy of the af...

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  4. 4
    Multiwavelength Analysis of GRB 250101A: From Gamma-Ray Prompt Emission to Optical Afterglow

    Multiwavelength Analysis of GRB 250101A: From Gamma-Ray Prompt Emission to Optical Afterglow od Guowang Du, Yehao Cheng, Yuan-Pei Yang, Jun Yang, Jinghua Zhang, Dan Zhu, Yu Pan, Yuan Fang, Xingzhu Zou, Brajesh Kumar, Helong Guo, Xufeng Zhu, Yangwei Zhang, Fanchuan Kong, Chenxi Shang, Xinlei Chen, Xiangkun Liu, Xiaowei Liu

    Wydane 2025-01-01

    The interaction between the relativistic jet and the circumburst medium produces a multiwavelength afterglow of a gamma-ray burst (GRBs). In this work, we present multiwavelength properties of GRB 250101A based on the observations of Swift, Fermi, and Mephisto. The spectral analysis of Swift/Swift B...

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