Stellar Object Detection Using the Wavelet Transform
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F11%3A00185994" target="_blank" >RIV/68407700:21230/11:00185994 - isvavai.cz</a>
Result on the web
<a href="http://ctn.cvut.cz/ap/download.php?id=646" target="_blank" >http://ctn.cvut.cz/ap/download.php?id=646</a>
DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Stellar Object Detection Using the Wavelet Transform
Original language description
Several algorithms are used nowadays for detecting stellar objects in astronomical images, for example in the DAOPHOT program package and in SExtractor (Software for source extraction). Our team has become acquainted with the wavelet transform and its good localization properties. After studying the manual for DAOPHOT and SExtractor, and becoming familiar with the a trous algorithm used for calculating the wavelet transform, we set ourselves the task to implement an ` algorithm for star detection on thebasis of the wavelet transform. We focused on detecting stellar objects in complex fields, such as globular clusters and galaxies. This paper describes a stellar object detection algorithm with the help of the wavelet transform, and presents our results.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
JA - Electronics and optoelectronics
OECD FORD branch
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Result continuities
Project
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Continuities
S - Specificky vyzkum na vysokych skolach
Others
Publication year
2011
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Acta Polytechnica
ISSN
1210-2709
e-ISSN
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Volume of the periodical
51
Issue of the periodical within the volume
6
Country of publishing house
CZ - CZECH REPUBLIC
Number of pages
4
Pages from-to
9-12
UT code for WoS article
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EID of the result in the Scopus database
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