Pattern Aware Cache Management for Efficient Subset Retrieving of Astronomical Image Data

2016 ◽  
Author(s):  
Jie Wang ◽  
Ce Yu ◽  
Zhi Hong ◽  
Jian Xiao ◽  
Chen Li ◽  
...  
Keyword(s):  
Image Data ◽  
Cache Management ◽  
Astronomical Image

Astronomical Image Data Analysis in the Cloud

2015 ◽  
Author(s):  
Francisco Javier de la Mora Garcia ◽  
Teruhisa Hochin ◽  
Hiroki Nomiya
Keyword(s):  
Data Analysis ◽  
Image Data ◽  
Astronomical Image

Space variant point spread function modeling for astronomical image data processing

2007 ◽  
Author(s):  
Martin Řeřábek ◽  
Petr Páta ◽  
Karel Fliegel ◽  
Jan Švihlik ◽  
Pavel Koten
Keyword(s):  
Data Processing ◽  
Point Spread Function ◽  
Image Data ◽  
Astronomical Image ◽  
Point Spread ◽  
Spread Function ◽  
Space Variant

Processing of the astronomical image data obtained from UWFC optical systems

2008 ◽  
Author(s):  
Martin Řeřábek ◽  
Petr Páta ◽  
Pavel Koten
Keyword(s):  
Image Data ◽  
Optical Systems ◽  
Astronomical Image

scholarly journals Advanced Processing of Images Obtained from Wide-field Astronomical Optical Systems

10.14311/1334 ◽  
2011 ◽  
Vol 51 (1) ◽  
Author(s):  
M. Řeřábek ◽  
P. Páta
Keyword(s):  
Image Data ◽  
Optical Systems ◽  
General View ◽  
Wide Field ◽  
Optical Aberrations ◽  
Transfer Characteristics ◽  
Astronomical Image ◽  
Wide Range ◽  
Spread Function ◽  
Space Variant

The principal aim of this paper is to present a general view of the special optical systems used for acquiring astronomical image data, commonly referred to as WFC or UWFC (Ultra Wide Field Camera), and of their transfer characteristics. UWFC image data analysis is very difficult in general, not only because the systems have so-called space variant (SV) properties. Images obtained from UWFC systems are usually incorrectly presented due to a wide range of optical aberrations and distortions. The influence of the optical aberrations increases towards the margins of the field of view. These aberrations distort the point spread function of the optical system and rapidly cut the accuracy of the measurements. This paper deals with simulation and modelling of the UWFC optical systems used in astronomy and their transfer characteristics.

scholarly journals Comparison of Outlier Detection Methods on Astronomical Image Data

2021 ◽  
pp. 197-223
Author(s):  
Lars Doorenbos ◽  
Stefano Cavuoti ◽  
Massimo Brescia ◽  
Antonio D’Isanto ◽  
Giuseppe Longo
Keyword(s):  
Outlier Detection ◽  
Image Data ◽  
Detection Methods ◽  
Astronomical Image
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