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CORC

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Real-Time Monitoring of a Single Molecule in Sub-nanometer Space by Dynamic Surface-Enhanced Raman Spectroscopy 期刊论文
JOURNAL OF PHYSICAL CHEMISTRY LETTERS, 2023, 卷号: 14
作者:  Yan, Wuwen;  Chen, Siyu;  Li, Pan;  Dong, Ronglu;  Shin, Hyun-Hang
收藏  |  浏览/下载：7/0  |  提交时间：2023/11/10
Searching for the Nano-Hertz Stochastic Gravitational Wave Background with the Chinese Pulsar Timing Array Data Release I 期刊论文
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2023, 卷号: 23, 期号: 7
作者:  Xu, Heng;  Chen, Siyuan;  Guo, Yanjun;  Jiang, Jinchen;  Wang, Bojun
收藏  |  浏览/下载：17/0  |  提交时间：2023/07/31
Incremental Fermi Large Area Telescope Fourth Source Catalog 期刊论文
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2022, 卷号: 260, 期号: 2
作者:  Abdollahi, S.;  Acero, F.;  Baldini, L.;  Ballet, J.;  Bastieri, D.
收藏  |  浏览/下载：31/0  |  提交时间：2022/07/11
Compression rate of dynamic diamond anvil cells from room temperature to 10 K 期刊论文
REVIEW OF SCIENTIFIC INSTRUMENTS, 2022, 卷号: 93
作者:  Yan, Jinwei;  Liu, Xiaodi;  Gorelli, Federico Aiace;  Xu, Haian;  Zhang, Huichao
收藏  |  浏览/下载：7/0  |  提交时间：2022/12/23
Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white dwarfs 期刊论文
Monthly Notices of the Royal Astronomical Society, 2022, 卷号: 510, 期号: 4, 页码: 6011-6021
作者:  Wang B(王博);  Liu DD(刘栋栋);  Chen HL(陈海亮)
收藏  |  浏览/下载：81/0  |  提交时间：2022/03/07
The Maximum Accreted Mass of Recycled Pulsars 期刊论文
ASTROPHYSICAL JOURNAL, 2021, 卷号: 922, 期号: 2
作者:  Li ZW(李振威);  Chen XF(陈雪飞);  Chen HL(陈海亮);  Han ZW(韩占文)
收藏  |  浏览/下载：21/0  |  提交时间：2021/12/06
Formation of millisecond pulsars with helium white dwarfs, ultra-compact X-ray binaries, and gravitational wave sources 期刊论文
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 卷号: 503, 期号: 3, 页码: 3540-3551
作者:  Chen HL(陈海亮);  Tauris, Thomas M.;  Han ZW(韩占文);  Chen XF(陈雪飞)
收藏  |  浏览/下载：63/0  |  提交时间：2021/06/21
Gas Expansion Process in the Dynamic Vacuum Calibration 期刊论文
Journal of Shanghai Jiaotong University (Science), 2021, 卷号: 26, 期号: 2, 页码: 193-200
作者:  Cheng, Yongjun;  Chen, Shuping;  Wang, Chenghong;  Xi, Zhenhua;  Sun, Wenjun
收藏  |  浏览/下载：13/0  |  提交时间：2021/06/03
He-shell flashes on the surface of oxygen-neon white dwarfs 期刊论文
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2021, 卷号: 21, 期号: 2, 页码: 9
作者:  Guo YL(郭云浪);  Liu DD(刘栋栋);  Wu, Chengyuan;  Wang B(王博)
收藏  |  浏览/下载：71/0  |  提交时间：2021/04/19
Detection of two bright radio bursts from magnetar SGR 1935 + 2154 期刊论文
Nature Astronomy, 2021, 卷号: 5, 页码: 414
作者:  Kirsten, F.;  Snelders, M. P.;  Jenkins, M.;  Nimmo, K.;  van den Eijnden, J.
收藏  |  浏览/下载：42/0  |  提交时间：2021/11/18
Astrophysics - High Energy Astrophysical Phenomena  Abstract: Fast radio bursts are millisecond-duration, bright radio signals (fluence 0.1-100 Jy ms) emitted from extragalactic sources of unknown physical origin. The recent CHIME/FRB and STARE2 detection of an extremely bright (fluence ~MJy ms) radio burst from the Galactic magnetar SGR 1935+2154 supports the hypothesis that (at least some) fast radio bursts are emitted by magnetars at cosmological distances. In follow-up observations totalling 522.7 h on source, we detect two bright radio bursts with fluences of 112 ± 22 Jy ms and 24 ± 5 Jy ms, respectively. Both bursts appear to be affected by interstellar scattering and we measure significant linear and circular polarization for the fainter burst. The bursts are separated in time by ~1.4 s, suggesting a non-Poissonian, clustered emission processsimilar to those seen in some repeating fast radio bursts. Together with the burst reported by CHIME/FRB and STARE2, as well as a much fainter burst seen by FAST (fluence 60 mJy ms), our observations demonstrate that SGR 1935+2154 can produce bursts with apparent energies spanning roughly seven orders of magnitude, and that the burst rate is comparable across this range. This raises the question of whether these four bursts arise from similar physical processes, and whether the fast radio burst population distribution extends to very low energies (~1030 erg, isotropic equivalent).  

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