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
自动化研究所 [2]
长春光学精密机械与物... [1]
国家天文台 [1]
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OAI收割 [4]
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期刊论文 [3]
会议论文 [1]
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2019 [1]
2013 [1]
2012 [1]
2006 [1]
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A high-resolution self-consistent whole sky foreground model
期刊论文
OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2019, 卷号: 62, 期号: 8, 页码: 13
作者:
Huang, QiZhi
;
Wu, FengQuan
;
Chen, XueLei
  |  
收藏
  |  
浏览/下载:15/0
  |  
提交时间:2020/03/10
neutral hydrogen
21 cm line
foreground model
whole sky map
simulation
Object Detection via Structural Feature Selection and Shape Model
期刊论文
OAI收割
IEEE TRANSACTIONS ON IMAGE PROCESSING, 2013, 卷号: 22, 期号: 12, 页码: 4984-4995
作者:
Zhang, Huigang
;
Bai, Xiao
;
Zhou, Jun
;
Cheng, Jian
;
Zhao, Huijie
收藏
  |  
浏览/下载:33/0
  |  
提交时间:2015/08/12
Object detection
foreground feature selection
part-based shape model
Foreground Object Detection Using Top-Down Information Based on EM Framework
期刊论文
OAI收割
IEEE TRANSACTIONS ON IMAGE PROCESSING, 2012, 卷号: 21, 期号: 9, 页码: 4204-4217
作者:
Liu, Zhou
;
Huang, Kaiqi
;
Tan, Tieniu
收藏
  |  
浏览/下载:34/0
  |  
提交时间:2015/08/12
Background model
expectation maximization (EM) framework
foreground detection
Markov random fields (MRFs)
An improved two-dimensional entropy method for star trail tracing in deep sky (EI CONFERENCE)
会议论文
OAI收割
ICO20: Optical Information Processing, August 21, 2005 - August 26, 2005, Changchun, China
作者:
Wang Y.-J.
;
Yao Z.-J.
收藏
  |  
浏览/下载:32/0
  |  
提交时间:2013/03/25
The trace of star trail is an important component of deep sky detection. The stars are low contrast targets
and their self-rotation will make their brightness change in cycle. Above all
the trail trace is vulnerable to the block and disturbance of other stars. Traditional one-dimensional maximum entropy thresholding algorithm is vulnerable to the noise
and the calculation of two-dimensional entropy methods is too large and takes too much time. This paper proposes an improved two-dimensional entropy threshold algorithm. We use recursion iteration method to eliminate the redundancy calculation
and reduce the size of two-dimensional histogram based on the deep sky stars characteristic
such as low contrast
fuzziness and the centralized histogram. We also combine our algorithm with the space trail trace model to forecast the star trace. Experiments results show
when the star are blocked or they turn dark
the method still can well extrapolate the star trace. Our method improves the capability of trailing the ebb and small star
and increases the precision of tracing. It is also robust to the noise
so there is a good application foreground for the method.