Point Spread Functions in Identification of Astronomical Objects from Poisson Noised Image
Abstract
This article deals with modeling of astronomical objects, which is one of the most fundamental topics in astronomical science. Introduction part is focused on problem description and used methods. Point Spread Function Modeling part deals with description of basic models used in astronomical photometry and further on introduction of more sophisticated models such as combinations of interference, turbulence, focusing, etc. This paper also contains a~way of objective function definition based on the knowledge of Poisson distributed noise, which is included in astronomical data. The proposed methods are further applied to real astronomical data.
Persistent identifier
http://hdl.handle.net/11012/57924Document type
Peer reviewedDocument version
Final PDFSource
Radioengineering. 2016 vol. 25, č. 1, s. 169-176. ISSN 1210-2512http://www.radioeng.cz/fulltexts/2016/16_01_0040_0045.pdf
Collections
- 2016/1 [28]