中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
机构
力学研究所 [1]
长春光学精密机械与物... [1]
上海神经科学研究所 [1]
高能物理研究所 [1]
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OAI收割 [4]
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会议论文 [2]
期刊论文 [2]
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2020 [1]
2015 [1]
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Introducing a special collection of papers in the Journal of High Energy Astrophysics on the Early Results of China's 1st X-ray Astronomy Satellite: Insight-HXMT
期刊论文
OAI收割
Journal of High Energy Astrophysics, 2020, 卷号: 27, 页码: 51-52
作者:
HXMT
  |  
收藏
  |  
浏览/下载:51/0
  |  
提交时间:2022/02/08
Astrophysics - High Energy Astrophysical Phenomena
Abstract: Insight-HXMT is the first Chinese X-ray astronomical mission, launched successfully on June 15, 2017, from China's Jiuquan Satellite Launch Center. Insight-HXMT was designed to have a broad energy coverage in X-rays, from 1-250 keV, with excellent timing and adequate energy resolution at soft X-rays, and the largest effective area at hard X-rays. This allows, in particular, to observe bright sources like X-ray binaries (XRBs) in their bright/outburst states with high cadence and high statistics at hard and soft X-rays at once. It was then expected that the Insight-HXMT mission will bring us new insights regarding the characteristics of several source classes. Examples include characterizing High-Mass X-ray Binaries (HMXBs) and the outburst evolution of Low-Mass X-ray Binaries (LMXBs). For instance, in HMXB systems, the region around their Alfven radius that is responsible to determine whether accretion or propeller occurs, or the region around the NS magnetic pole where the intense X-rays are supposed to be produced are specially appealing targets of study. For the LMXBs, the evolution the outburst and the properties of the compact objects themselves are obvious priority targets for Insight-HXMT. Due to the broad coverage in energy, Insight-HXMT is specially well suited to study the influence of thermonuclear (type-I) X-ray bursts upon the surrounding environment.
Mirror-Induced Self-Directed Behaviors in Rhesus Monkeys after Visual-Somatosensory Training
期刊论文
OAI收割
CURRENT BIOLOGY, 2015, 卷号: 25, 期号: 2, 页码: 212-217
作者:
Chang, Liangtang
;
Fang, Qin
;
Zhang, Shikun
;
Poo, Mu-ming
;
Gong, Neng
收藏
  |  
浏览/下载:41/0
  |  
提交时间:2015/04/22
CEBUS-APELLA
RECOGNIZE THEMSELVES
MACACA-FASCICULARIS
IMAGE STIMULATION
PAN-TROGLODYTES
VIDEO IMAGES
CHIMPANZEES
RESPONSES
Influence of post-annealing ambient on the superconducting properties and microstructure of YBa_2Cu_3O_7-δ films
会议论文
OAI收割
The 29th International Symposium on Rarefied Gas Dynamics, 中国陕西西安, 2014-07-13
作者:
Wang LH(王连红)
;
Liu C(刘崇)
;
Fan J(樊菁)
收藏
  |  
浏览/下载:30/0
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提交时间:2015/09/10
annealing
films
YBCO
amorphous
ambient
themselves
evaporation
fabricate
annealed
hence
The study of optical property for CdS nanocrystalline prepared by precipitation method (EI CONFERENCE)
会议论文
OAI收割
ICO20: Materials and Nanostructures, August 21, 2005 - August 26, 2005, Changchun, China
作者:
Zhang S.
;
Li W.
;
Li W.
收藏
  |  
浏览/下载:20/0
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提交时间:2013/03/25
CdS nanocrystalline were prepared by precipitation from a mixture of aqueous solutions of cadmium salts and sulfur salts without adding any surface-termination agent. Their crystal structures and particle sizes were determined by X-ray diffraction (XRD). The CdS nanocrystalline precipitated from different precursors exhibited three cases: cubic phase
hexagonal phase and a mixture of cubic and hexagonal phases. The photoluminescence (PL) of cadmium salt precursors and CdS nanocrystalline is also analyzed. Similar spectral band structure of cadmium salt precursors and CdS nanocrystalline is found. The spectral intensity of the CdS-Cd rich and CdS-S rich nanocrystalline shows that the precursors themselves have important effect on the PL of CdS nanocrystalline.