中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页
机构
成果
学者
登录
注册
登陆
×
验证码:
换一张
忘记密码?
记住我
×
校外用户登录
CAS IR Grid
机构
高能物理研究所 [4]
国家天文台 [2]
金属研究所 [1]
地质与地球物理研究所 [1]
上海天文台 [1]
数学与系统科学研究院 [1]
更多
采集方式
OAI收割 [16]
内容类型
期刊论文 [16]
发表日期
2024 [2]
2023 [1]
2021 [1]
2020 [4]
2019 [3]
2016 [2]
更多
学科主题
Astronomy ... [1]
天文学 [1]
天文学::恒星与银河... [1]
天文学::恒星与银河... [1]
筛选
浏览/检索结果:
共16条,第1-10条
帮助
条数/页:
5
10
15
20
25
30
35
40
45
50
55
60
65
70
75
80
85
90
95
100
排序方式:
请选择
提交时间升序
提交时间降序
作者升序
作者降序
题名升序
题名降序
发表日期升序
发表日期降序
Self-adaptive LED spectrum-tunable light source with high output irradiance and uniformity
期刊论文
OAI收割
OPTICS COMMUNICATIONS, 2024, 卷号: 569
作者:
Li, Zhengang
;
Liu, Jiaxiang
;
Pan, Ying
;
Cheng, Zhen
;
Si, Ganshang
  |  
收藏
  |  
浏览/下载:25/0
  |  
提交时间:2024/11/22
Light emitting diode
Spectral fitting algorithm
Differential evolution
Half-integrating sphere
Light mixing system
Roughness Evolution of Granite Flat Fracture Surfaces during Sliding Processes
期刊论文
OAI收割
APPLIED SCIENCES-BASEL, 2024, 卷号: 14, 期号: 13, 页码: 19
作者:
Yang, Hengtao
;
Bai, Bing
;
Lin, Hang
  |  
收藏
  |  
浏览/下载:8/0
  |  
提交时间:2025/06/27
granite fracture surfaces
shear slip
roughness evolution
power spectral density (PSD)
Red fruits exhibit lower colour diversity than red flowers as perceived by birds
期刊论文
OAI收割
FUNCTIONAL ECOLOGY, 2023, 卷号: 37, 期号: 12, 页码: 3164-3176
作者:
  |  
收藏
  |  
浏览/下载:29/0
  |  
提交时间:2024/07/10
bird
colour vision
evolutionary history
flower
fruit
pollination
red
seed dispersal
INTERSPECIFIC POLLEN TRANSFER
HUMMINGBIRD POLLINATION
SPECTRAL SENSITIVITY
SEED SIZE
EVOLUTION
DISPERSAL
VISION
BEE
DIVERSIFICATION
CONVERGENCE
Spectral Method for Phase Retrieval: An Expectation Propagation Perspective
期刊论文
OAI收割
IEEE TRANSACTIONS ON INFORMATION THEORY, 2021, 卷号: 67, 期号: 2, 页码: 1332-1355
作者:
Ma, Junjie
;
Dudeja, Rishabh
;
Xu, Ji
  |  
收藏
  |  
浏览/下载:64/0
  |  
提交时间:2021/04/26
Phase measurement
Message passing
Tools
Signal processing algorithms
Prediction algorithms
Numerical models
Approximation algorithms
Phase retrieval
spectral method
coded diffraction pattern
expectation propagation (EP)
approximate message passing (AMP)
state evolution
orthogonal AMP
vector AMP
ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP). II. Survey Overview: A First Look at 1.3 mm Continuum Maps and Molecular Outflows
期刊论文
OAI收割
The Astrophysical Journal Supplement Series, 2020, 卷号: 251, 期号: 2, 页码: 35
作者:
Dutta, Somnath
;
Lee, Chin-Fei
;
Liu, Tie
;
Hirano, Naomi
;
Liu, Sheng-Yuan
  |  
收藏
  |  
浏览/下载:63/0
  |  
提交时间:2020/12/28
Star formation
Star forming regions
Early stellar evolution
Protostars
Low mass stars
Stellar jets
Stellar winds
Astrochemistry
Stellar abundances
Spectral energy distribution
Dense interstellar clouds
Interstellar medium
ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP). II. Survey Overview: A First Look at 1.3 mm Continuum Maps and Molecular Outflows
期刊论文
OAI收割
The Astrophysical Journal Supplement Series, 2020, 卷号: 251, 期号: 2
作者:
Dutta,Somnath
;
Lee,Chin-Fei
;
Liu,Tie
;
Hirano,Naomi
;
Liu,Sheng-Yuan
  |  
收藏
  |  
浏览/下载:44/0
  |  
提交时间:2021/12/06
Star formation
Star forming regions
Early stellar evolution
Protostars
Low mass stars
Stellar jets
Stellar winds
Astrochemistry
Stellar abundances
Spectral energy distribution
Dense interstellar clouds
Interstellar medium
Estimating Dust Attenuation from Galactic Spectra. I. Methodology and Tests
期刊论文
OAI收割
The Astrophysical Journal, 2020, 卷号: 896, 期号: 1
作者:
Li,Niu
;
Li,Cheng
;
Mo,Houjun
;
Hu,Jian
;
Zhou,Shuang
  |  
收藏
  |  
浏览/下载:37/0
  |  
提交时间:2021/12/06
Dust continuum emission
Interstellar medium
Galaxies
Interstellar dust extinction
Stellar populations
Extragalactic astronomy
Spectral energy distribution
Spectroscopy
Galaxy evolution
Galaxy processes
Interstellar absorption
Sky surveys
An underlying clock in the extreme flip-flop state transitions of the black hole transient Swift J1658.2-4242
期刊论文
OAI收割
Astronomy and Astrophysics, 2020, 卷号: 641, 页码: A101
作者:
HXMT
  |  
收藏
  |  
浏览/下载:70/0
  |  
提交时间:2022/02/08
accretion
accretion disks
black hole physics
X-rays: binaries
time
Astrophysics - High Energy Astrophysical Phenomena
Abstract:
Aims: Flip-flops are top-hat-like X-ray flux variations, which have been observed in some transient accreting black hole binary systems, and feature simultaneous changes in the spectral hardness and the power density spectrum (PDS). They occur at a crucial time in the evolution of these systems, when the accretion disc emission starts to dominate over coronal emission. Flip-flops remain a poorly understood phenomenon, so we aim to thoroughly investigate them in a system featuring several such transitions.
Methods: Within the multitude of observations of
Swift J1658.2-4242
during its outburst in early 2018, we detected 15 flip-flops, enabling a detailed analysis of their individual properties and the differences between them. We present observations by XMM-Newton, NuSTAR, Astrosat, Swift, Insight-HXMT, INTEGRAL, and ATCA. We analysed their light curves, searched for periodicities, computed their PDSs, and fitted their X-ray spectra, to investigate the source behaviour during flip-flop transitions and how the interval featuring flip-flops differs from the rest of the outburst.
Results: The flip-flops of Swift J1658.2-4242 are of an extreme variety, exhibiting flux differences of up to 77% within 100 s, which is much larger than what has been seen previously. We observed radical changes in the PDS simultaneous with the sharp flux variations, featuring transitions between the quasi-periodic oscillation types C and A, which have never been observed before. Changes in the PDS are delayed, but more rapid than changes in the light curve. Flip-flops occur in two intervals within the outburst, separated by about two weeks in which these phenomena were not seen. Transitions between the two flip-flop states occurred at random integer multiples of a fundamental period of 2.761 ks in the first interval and 2.61 ks in the second. Spectral analysis reveals the high and low flux flip-flop states to be very similar, but distinct from intervals lacking flip-flops. A change of the inner temperature of the accretion disc is responsible for most of the flux difference in the flip-flops. We also highlight the importance of correcting for the influence of the dust scattering halo on the X-ray spectra.
Real-Time Evolution Dynamics of Double-Pulse Mode-Locking
期刊论文
OAI收割
IEEE JOURNAL OF SELECTED TOPICS IN QUANTUM ELECTRONICS, 2019, 卷号: 25, 期号: 4
作者:
Wang, Guomei
;
Chen, Guangwei
;
Li, Wenlei
;
Zeng, Chao
  |  
收藏
  |  
浏览/下载:148/0
  |  
提交时间:2019/07/19
Dispersive Fourier transform technique
spectral evolution dynamics
double-pulse mode-locking
Er-doped fiber laser
Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations
期刊论文
OAI收割
Journal of High Energy Astrophysics, 2019, 卷号: 23, 页码: 29-32
作者:
HXMT
  |  
收藏
  |  
浏览/下载:62/0
  |  
提交时间:2022/02/08
Stars: neutron star
Pulsars: binary(Her X-1)
X-rays: stars
Astrophysics - High Energy Astrophysical Phenomena
Abstract: The long-term evolution of the centroid energy of the CRSF in Her X-1 is still a mystery. We report a new measurement from a campaign between Insight-HXMT and NuSTAR performed in February 2018. Generally, the two satellites show well consistent results of timing and spectral properties. The joint spectral analysis confirms that the previously observed long decay phase has ended, and that the line energy instead keeps constant around 37.5 keV after flux correction.