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Chinese Academy of Sciences Institutional Repositories Grid
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A New Solar Hard X-ray Image Reconstruction Algorithm for ASO-S/HXI Based on Deep Learning 期刊论文  OAI收割
SOLAR PHYSICS, 2024, 卷号: 299, 期号: 11
作者:  
Xia, Yuehan
  |  收藏  |  浏览/下载:11/0  |  提交时间:2024/11/25
Partial Disruption of a Planet around a White Dwarf: The Effect of Perturbations from the Remnant Planet on the Accretion 期刊论文  OAI收割
Astrophysical Journal, 2024, 卷号: 974, 期号: 1, 页码: 12100
作者:  
Abdusattar Kurban;  Xia Zhou;  Na Wang;  Yong-Feng Huang;  Yu-Bin Wang
  |  收藏  |  浏览/下载:2/0  |  提交时间:2025/06/05
Multiband analyses of the bright GRB 230812B and the associated SN2023pel 期刊论文  OAI收割
Monthly Notices of the Royal Astronomical Society, 2024, 卷号: 530, 期号: 1, 页码: 1-19
作者:  
T. Hussenot-Desenonges;  T. Wouters;  N. Guessoum;  I. Abdi;  A. Abulwf a
  |  收藏  |  浏览/下载:1/0  |  提交时间:2025/06/05
A burst storm from the repeating FRB 20200120E in an M81 globular cluster 期刊论文  OAI收割
Monthly Notices of the Royal Astronomical Society, 2023, 卷号: 520, 期号: 2, 页码: 2281-2305
作者:  
Nimmo, K.;  Hessels, J. W. T.;  Snelders, M. P.;  Karuppusamy, R.;  Hewitt, D. M.
  |  收藏  |  浏览/下载:1/0  |  提交时间:2024/06/23
The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP 期刊论文  OAI收割
SPACE TELESCOPES AND INSTRUMENTATION 2022: ULTRAVIOLET TO GAMMA RAY, 2022, 卷号: 12181, 页码: 121811Y
作者:  
eXTP
  |  收藏  |  浏览/下载:10/0  |  提交时间:2023/11/09
Periodicity Search on X-Ray Bursts of SGR J1935+2154 Using 8.5 yr of Fermi/GBM Data 期刊论文  OAI收割
The Astrophysical Journal, 2021, 卷号: 923, 页码: L30
作者:  
HXMT
  |  收藏  |  浏览/下载:25/0  |  提交时间:2022/02/08
Nondetection of the Gamma-Ray Burst X-Ray Emission Line: The Down-Comptonization Effect 期刊论文  OAI收割
ASTROPHYSICAL JOURNAL, 2020, 卷号: 900, 期号: 1, 页码: 5
作者:  
Liu JY(刘杰英);  Mao JR(毛基荣)
  |  收藏  |  浏览/下载:30/0  |  提交时间:2020/10/26
Overview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2020, 卷号: 63, 期号: 4, 页码: 18
作者:  
Zhang, Shuang-Nan;  Li, TiPei;  Lu, FangJun;  Song, LiMing;  Xu, YuPeng
  |  收藏  |  浏览/下载:87/0  |  提交时间:2021/12/06
Overview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2020, 卷号: 63, 期号: 4, 页码: 18
作者:  
Zhang, Shuang-Nan;  Li, TiPei;  Lu, FangJun;  Song, LiMing;  Xu, YuPeng
  |  收藏  |  浏览/下载:73/0  |  提交时间:2021/12/06
No pulsed radio emission during a bursting phase of a Galactic magnetar 期刊论文  OAI收割
Nature, 2020, 卷号: 587, 页码: 63-65
作者:  
HXMT
  |  收藏  |  浏览/下载:49/0  |  提交时间:2022/02/08
Astrophysics - High Energy Astrophysical Phenomena  Abstract: Fast radio bursts (FRBs) are millisecond-duration radio transients of unknown physical origin observed at extragalactic distances1-3. It has long been speculated that magnetars are the engine powering repeating bursts from FRB sources4-13, but no convincing evidence has been collected so far14. Recently, the Galactic magnetar SRG 1935+2154 entered an active phase by emitting intense soft íray bursts15. One FRB-like event with two peaks (FRB 200428) and a luminosity slightly lower than the faintest extragalactic FRBs was detected from the source, in association with a soft íray/hard-X-ray flare18-21. Here we report an eight-hour targeted radio observational campaign comprising four sessions and assisted by multi-wavelength (optical and hard-X-ray) data. During the third session, 29 soft-íray repeater (SGR) bursts were detected in íray energies. Throughout the observing period, we detected no single dispersed pulsed emission coincident with the arrivals of SGR bursts, but unfortunately we were not observing when the FRB was detected. The non-detection places a fluence upper limit that is eight orders of magnitude lower than the fluence of FRB 200428. Our results suggest that FRB-SGR burst associations are rare. FRBs may be highly relativistic and geometrically beamed, or FRB-like events associated with SGR bursts may have narrow spectra and characteristic frequencies outside the observed band. It is also possible that the physical conditions required to achieve coherent radiation in SGR bursts are difficult to satisfy, and that only under extreme conditions could an FRB be associated with an SGR burst.