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Comparison of Several Algorithms for Celestial object Classification

Identifieur interne : 000124 ( PascalFrancis/Corpus ); précédent : 000123; suivant : 000125

Comparison of Several Algorithms for Celestial object Classification

Auteurs : NANBO PENG ; YANXIA ZHANG ; YONGHENG ZHAO

Source :

RBID : Pascal:11-0004539

Descripteurs français

English descriptors

Abstract

We present a comparative study of implementation of supervised classification algorithms on classification of celestial objects. Three different algorithms including Linear Discriminant Analysis (LDA), K-Dimensional Tree (KD-tree), Support Vector Machines (SVMs) are used for classification of pointed sources from the Sloan Digital Sky Survey (SDSS) Data Release Seven. All of them have been applied and tested on the SDSS photometric data which are filtered by stringent conditions to make them play the best performance. Each of six performance metrics of SVMs can achieve very high performance (99.00%). The performances of KD-tree are also very good since six metrics are over 97.00%. Although five metrics are more than 90.00%, the performances of LDA are relatively poor because the accuracy of positive prediction only reaches 85.98%. Moreover, we discuss what input pattern is the best combination of different parameters for the effectiveness of these methods, respectively.

Notice en format standard (ISO 2709)

Pour connaître la documentation sur le format Inist Standard.

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A03   1    @0 Proc. SPIE Int. Soc. Opt. Eng.
A05       @2 7740
A06       @3 p. 2
A08 01  1  ENG  @1 Comparison of Several Algorithms for Celestial object Classification
A09 01  1  ENG  @1 Software and cyberinfrastructure for astronomy : 27-30 June 2010, San Diego, California, United States
A11 01  1    @1 NANBO PENG
A11 02  1    @1 YANXIA ZHANG
A11 03  1    @1 YONGHENG ZHAO
A12 01  1    @1 RADZIWILL (Nicole M.) @9 ed.
A12 02  1    @1 BRIDGER (Alan) @9 ed.
A14 01      @1 Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences @2 Beijing 100012 @3 CHN @Z 1 aut. @Z 2 aut. @Z 3 aut.
A18 01  1    @1 SPIE @3 USA @9 org-cong.
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A43 01      @1 INIST @2 21760 @5 354000174702880860
A44       @0 0000 @1 © 2011 INIST-CNRS. All rights reserved.
A45       @0 22 ref.
A47 01  1    @0 11-0004539
A60       @1 P @2 C
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A66 01      @0 USA
C01 01    ENG  @0 We present a comparative study of implementation of supervised classification algorithms on classification of celestial objects. Three different algorithms including Linear Discriminant Analysis (LDA), K-Dimensional Tree (KD-tree), Support Vector Machines (SVMs) are used for classification of pointed sources from the Sloan Digital Sky Survey (SDSS) Data Release Seven. All of them have been applied and tested on the SDSS photometric data which are filtered by stringent conditions to make them play the best performance. Each of six performance metrics of SVMs can achieve very high performance (99.00%). The performances of KD-tree are also very good since six metrics are over 97.00%. Although five metrics are more than 90.00%, the performances of LDA are relatively poor because the accuracy of positive prediction only reaches 85.98%. Moreover, we discuss what input pattern is the best combination of different parameters for the effectiveness of these methods, respectively.
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C03 01  X  SPA  @0 Análisis discriminante @5 06
C03 02  X  FRE  @0 Haute performance @5 07
C03 02  X  ENG  @0 High performance @5 07
C03 02  X  SPA  @0 Alto rendimiento @5 07
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C03 03  X  ENG  @0 Supervised classification @5 18
C03 03  X  SPA  @0 Clasificación supervisada @5 18
C03 04  X  FRE  @0 Source ponctuelle @5 19
C03 04  X  ENG  @0 Point source @5 19
C03 04  X  SPA  @0 Fuente puntual @5 19
C03 05  X  FRE  @0 Ciel @5 20
C03 05  X  ENG  @0 Sky @5 20
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C03 07  X  FRE  @0 Métrique @5 22
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C03 09  X  ENG  @0 Statistical analysis @5 24
C03 09  X  SPA  @0 Análisis estadístico @5 24
C03 10  X  FRE  @0 Classification à vaste marge @5 25
C03 10  X  ENG  @0 Vector support machine @5 25
C03 10  X  SPA  @0 Máquina ejemplo soporte @5 25
N21       @1 003
N44 01      @1 OTO
N82       @1 OTO
pR  
A30 01  1  ENG  @1 Software and cyberinfrastructure for astronomy @3 San Diego CA USA @4 2010

Format Inist (serveur)

NO : PASCAL 11-0004539 INIST
ET : Comparison of Several Algorithms for Celestial object Classification
AU : NANBO PENG; YANXIA ZHANG; YONGHENG ZHAO; RADZIWILL (Nicole M.); BRIDGER (Alan)
AF : Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences/Beijing 100012/Chine (1 aut., 2 aut., 3 aut.)
DT : Publication en série; Congrès; Niveau analytique
SO : Proceedings of SPIE, the International Society for Optical Engineering; ISSN 0277-786X; Coden PSISDG; Etats-Unis; Da. 2010; Vol. 7740; No. p. 2; 77402M.1-77402M.10; Bibl. 22 ref.
LA : Anglais
EA : We present a comparative study of implementation of supervised classification algorithms on classification of celestial objects. Three different algorithms including Linear Discriminant Analysis (LDA), K-Dimensional Tree (KD-tree), Support Vector Machines (SVMs) are used for classification of pointed sources from the Sloan Digital Sky Survey (SDSS) Data Release Seven. All of them have been applied and tested on the SDSS photometric data which are filtered by stringent conditions to make them play the best performance. Each of six performance metrics of SVMs can achieve very high performance (99.00%). The performances of KD-tree are also very good since six metrics are over 97.00%. Although five metrics are more than 90.00%, the performances of LDA are relatively poor because the accuracy of positive prediction only reaches 85.98%. Moreover, we discuss what input pattern is the best combination of different parameters for the effectiveness of these methods, respectively.
CC : 001D02B07B; 001D02A06
FD : Analyse discriminante; Haute performance; Classification supervisée; Source ponctuelle; Ciel; Photométrie; Métrique; Théorie graphe; Analyse statistique; Classification à vaste marge
ED : Discriminant analysis; High performance; Supervised classification; Point source; Sky; Photometry; Metric; Graph theory; Statistical analysis; Vector support machine
SD : Análisis discriminante; Alto rendimiento; Clasificación supervisada; Fuente puntual; Cielo; Fotometría; Métrico; Teoría grafo; Análisis estadístico; Máquina ejemplo soporte
LO : INIST-21760.354000174702880860
ID : 11-0004539

Links to Exploration step

Pascal:11-0004539

Le document en format XML

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<DT>Publication en série; Congrès; Niveau analytique</DT>
<SO>Proceedings of SPIE, the International Society for Optical Engineering; ISSN 0277-786X; Coden PSISDG; Etats-Unis; Da. 2010; Vol. 7740; No. p. 2; 77402M.1-77402M.10; Bibl. 22 ref.</SO>
<LA>Anglais</LA>
<EA>We present a comparative study of implementation of supervised classification algorithms on classification of celestial objects. Three different algorithms including Linear Discriminant Analysis (LDA), K-Dimensional Tree (KD-tree), Support Vector Machines (SVMs) are used for classification of pointed sources from the Sloan Digital Sky Survey (SDSS) Data Release Seven. All of them have been applied and tested on the SDSS photometric data which are filtered by stringent conditions to make them play the best performance. Each of six performance metrics of SVMs can achieve very high performance (99.00%). The performances of KD-tree are also very good since six metrics are over 97.00%. Although five metrics are more than 90.00%, the performances of LDA are relatively poor because the accuracy of positive prediction only reaches 85.98%. Moreover, we discuss what input pattern is the best combination of different parameters for the effectiveness of these methods, respectively.</EA>
<CC>001D02B07B; 001D02A06</CC>
<FD>Analyse discriminante; Haute performance; Classification supervisée; Source ponctuelle; Ciel; Photométrie; Métrique; Théorie graphe; Analyse statistique; Classification à vaste marge</FD>
<ED>Discriminant analysis; High performance; Supervised classification; Point source; Sky; Photometry; Metric; Graph theory; Statistical analysis; Vector support machine</ED>
<SD>Análisis discriminante; Alto rendimiento; Clasificación supervisada; Fuente puntual; Cielo; Fotometría; Métrico; Teoría grafo; Análisis estadístico; Máquina ejemplo soporte</SD>
<LO>INIST-21760.354000174702880860</LO>
<ID>11-0004539</ID>
</server>
</inist>
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