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 ZHAOSource :
-
Proceedings of SPIE, the International Society for Optical Engineering [ 0277-786X ] ; 2010.
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.
pA |
A01 | 01 | 1 | | @0 0277-786X |
---|
A02 | 01 | | | @0 PSISDG |
---|
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. |
---|
A18 | 02 | 1 | | @1 American Astronomical Society @3 USA @9 org-cong. |
---|
A20 | | | | @2 77402M.1-77402M.10 |
---|
A21 | | | | @1 2010 |
---|
A23 | 01 | | | @0 ENG |
---|
A25 | 01 | | | @1 SPIE @2 Bellingham, Wash. |
---|
A26 | 01 | | | @0 978-0-8194-8230-3 |
---|
A26 | 02 | | | @0 0-8194-8230-7 |
---|
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 |
---|
A61 | | | | @0 A |
---|
A64 | 01 | 1 | | @0 Proceedings of SPIE, the International Society for Optical Engineering |
---|
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. |
---|
C02 | 01 | X | | @0 001D02B07B |
---|
C02 | 02 | X | | @0 001D02A06 |
---|
C03 | 01 | X | FRE | @0 Analyse discriminante @5 06 |
---|
C03 | 01 | X | ENG | @0 Discriminant analysis @5 06 |
---|
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 |
---|
C03 | 03 | X | FRE | @0 Classification supervisée @5 18 |
---|
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 |
---|
C03 | 05 | X | SPA | @0 Cielo @5 20 |
---|
C03 | 06 | X | FRE | @0 Photométrie @5 21 |
---|
C03 | 06 | X | ENG | @0 Photometry @5 21 |
---|
C03 | 06 | X | SPA | @0 Fotometría @5 21 |
---|
C03 | 07 | X | FRE | @0 Métrique @5 22 |
---|
C03 | 07 | X | ENG | @0 Metric @5 22 |
---|
C03 | 07 | X | SPA | @0 Métrico @5 22 |
---|
C03 | 08 | X | FRE | @0 Théorie graphe @5 23 |
---|
C03 | 08 | X | ENG | @0 Graph theory @5 23 |
---|
C03 | 08 | X | SPA | @0 Teoría grafo @5 23 |
---|
C03 | 09 | X | FRE | @0 Analyse statistique @5 24 |
---|
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
<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Comparison of Several Algorithms for Celestial object Classification</title>
<author><name sortKey="Nanbo Peng" sort="Nanbo Peng" uniqKey="Nanbo Peng" last="Nanbo Peng">NANBO PENG</name>
<affiliation><inist:fA14 i1="01"><s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>Beijing 100012</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
<author><name sortKey="Yanxia Zhang" sort="Yanxia Zhang" uniqKey="Yanxia Zhang" last="Yanxia Zhang">YANXIA ZHANG</name>
<affiliation><inist:fA14 i1="01"><s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>Beijing 100012</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
<author><name sortKey="Yongheng Zhao" sort="Yongheng Zhao" uniqKey="Yongheng Zhao" last="Yongheng Zhao">YONGHENG ZHAO</name>
<affiliation><inist:fA14 i1="01"><s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>Beijing 100012</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
</titleStmt>
<publicationStmt><idno type="wicri:source">INIST</idno>
<idno type="inist">11-0004539</idno>
<date when="2010">2010</date>
<idno type="stanalyst">PASCAL 11-0004539 INIST</idno>
<idno type="RBID">Pascal:11-0004539</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000124</idno>
</publicationStmt>
<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Comparison of Several Algorithms for Celestial object Classification</title>
<author><name sortKey="Nanbo Peng" sort="Nanbo Peng" uniqKey="Nanbo Peng" last="Nanbo Peng">NANBO PENG</name>
<affiliation><inist:fA14 i1="01"><s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>Beijing 100012</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
<author><name sortKey="Yanxia Zhang" sort="Yanxia Zhang" uniqKey="Yanxia Zhang" last="Yanxia Zhang">YANXIA ZHANG</name>
<affiliation><inist:fA14 i1="01"><s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>Beijing 100012</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
<author><name sortKey="Yongheng Zhao" sort="Yongheng Zhao" uniqKey="Yongheng Zhao" last="Yongheng Zhao">YONGHENG ZHAO</name>
<affiliation><inist:fA14 i1="01"><s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>Beijing 100012</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</inist:fA14>
</affiliation>
</author>
</analytic>
<series><title level="j" type="main">Proceedings of SPIE, the International Society for Optical Engineering</title>
<title level="j" type="abbreviated">Proc. SPIE Int. Soc. Opt. Eng.</title>
<idno type="ISSN">0277-786X</idno>
<imprint><date when="2010">2010</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt><title level="j" type="main">Proceedings of SPIE, the International Society for Optical Engineering</title>
<title level="j" type="abbreviated">Proc. SPIE Int. Soc. Opt. Eng.</title>
<idno type="ISSN">0277-786X</idno>
</seriesStmt>
</fileDesc>
<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Discriminant analysis</term>
<term>Graph theory</term>
<term>High performance</term>
<term>Metric</term>
<term>Photometry</term>
<term>Point source</term>
<term>Sky</term>
<term>Statistical analysis</term>
<term>Supervised classification</term>
<term>Vector support machine</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Analyse discriminante</term>
<term>Haute performance</term>
<term>Classification supervisée</term>
<term>Source ponctuelle</term>
<term>Ciel</term>
<term>Photométrie</term>
<term>Métrique</term>
<term>Théorie graphe</term>
<term>Analyse statistique</term>
<term>Classification à vaste marge</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">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.</div>
</front>
</TEI>
<inist><standard h6="B"><pA><fA01 i1="01" i2="1"><s0>0277-786X</s0>
</fA01>
<fA02 i1="01"><s0>PSISDG</s0>
</fA02>
<fA03 i2="1"><s0>Proc. SPIE Int. Soc. Opt. Eng.</s0>
</fA03>
<fA05><s2>7740</s2>
</fA05>
<fA06><s3>p. 2</s3>
</fA06>
<fA08 i1="01" i2="1" l="ENG"><s1>Comparison of Several Algorithms for Celestial object Classification</s1>
</fA08>
<fA09 i1="01" i2="1" l="ENG"><s1>Software and cyberinfrastructure for astronomy : 27-30 June 2010, San Diego, California, United States</s1>
</fA09>
<fA11 i1="01" i2="1"><s1>NANBO PENG</s1>
</fA11>
<fA11 i1="02" i2="1"><s1>YANXIA ZHANG</s1>
</fA11>
<fA11 i1="03" i2="1"><s1>YONGHENG ZHAO</s1>
</fA11>
<fA12 i1="01" i2="1"><s1>RADZIWILL (Nicole M.)</s1>
<s9>ed.</s9>
</fA12>
<fA12 i1="02" i2="1"><s1>BRIDGER (Alan)</s1>
<s9>ed.</s9>
</fA12>
<fA14 i1="01"><s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>Beijing 100012</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
</fA14>
<fA18 i1="01" i2="1"><s1>SPIE</s1>
<s3>USA</s3>
<s9>org-cong.</s9>
</fA18>
<fA18 i1="02" i2="1"><s1>American Astronomical Society</s1>
<s3>USA</s3>
<s9>org-cong.</s9>
</fA18>
<fA20><s2>77402M.1-77402M.10</s2>
</fA20>
<fA21><s1>2010</s1>
</fA21>
<fA23 i1="01"><s0>ENG</s0>
</fA23>
<fA25 i1="01"><s1>SPIE</s1>
<s2>Bellingham, Wash.</s2>
</fA25>
<fA26 i1="01"><s0>978-0-8194-8230-3</s0>
</fA26>
<fA26 i1="02"><s0>0-8194-8230-7</s0>
</fA26>
<fA43 i1="01"><s1>INIST</s1>
<s2>21760</s2>
<s5>354000174702880860</s5>
</fA43>
<fA44><s0>0000</s0>
<s1>© 2011 INIST-CNRS. All rights reserved.</s1>
</fA44>
<fA45><s0>22 ref.</s0>
</fA45>
<fA47 i1="01" i2="1"><s0>11-0004539</s0>
</fA47>
<fA60><s1>P</s1>
<s2>C</s2>
</fA60>
<fA64 i1="01" i2="1"><s0>Proceedings of SPIE, the International Society for Optical Engineering</s0>
</fA64>
<fA66 i1="01"><s0>USA</s0>
</fA66>
<fC01 i1="01" l="ENG"><s0>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.</s0>
</fC01>
<fC02 i1="01" i2="X"><s0>001D02B07B</s0>
</fC02>
<fC02 i1="02" i2="X"><s0>001D02A06</s0>
</fC02>
<fC03 i1="01" i2="X" l="FRE"><s0>Analyse discriminante</s0>
<s5>06</s5>
</fC03>
<fC03 i1="01" i2="X" l="ENG"><s0>Discriminant analysis</s0>
<s5>06</s5>
</fC03>
<fC03 i1="01" i2="X" l="SPA"><s0>Análisis discriminante</s0>
<s5>06</s5>
</fC03>
<fC03 i1="02" i2="X" l="FRE"><s0>Haute performance</s0>
<s5>07</s5>
</fC03>
<fC03 i1="02" i2="X" l="ENG"><s0>High performance</s0>
<s5>07</s5>
</fC03>
<fC03 i1="02" i2="X" l="SPA"><s0>Alto rendimiento</s0>
<s5>07</s5>
</fC03>
<fC03 i1="03" i2="X" l="FRE"><s0>Classification supervisée</s0>
<s5>18</s5>
</fC03>
<fC03 i1="03" i2="X" l="ENG"><s0>Supervised classification</s0>
<s5>18</s5>
</fC03>
<fC03 i1="03" i2="X" l="SPA"><s0>Clasificación supervisada</s0>
<s5>18</s5>
</fC03>
<fC03 i1="04" i2="X" l="FRE"><s0>Source ponctuelle</s0>
<s5>19</s5>
</fC03>
<fC03 i1="04" i2="X" l="ENG"><s0>Point source</s0>
<s5>19</s5>
</fC03>
<fC03 i1="04" i2="X" l="SPA"><s0>Fuente puntual</s0>
<s5>19</s5>
</fC03>
<fC03 i1="05" i2="X" l="FRE"><s0>Ciel</s0>
<s5>20</s5>
</fC03>
<fC03 i1="05" i2="X" l="ENG"><s0>Sky</s0>
<s5>20</s5>
</fC03>
<fC03 i1="05" i2="X" l="SPA"><s0>Cielo</s0>
<s5>20</s5>
</fC03>
<fC03 i1="06" i2="X" l="FRE"><s0>Photométrie</s0>
<s5>21</s5>
</fC03>
<fC03 i1="06" i2="X" l="ENG"><s0>Photometry</s0>
<s5>21</s5>
</fC03>
<fC03 i1="06" i2="X" l="SPA"><s0>Fotometría</s0>
<s5>21</s5>
</fC03>
<fC03 i1="07" i2="X" l="FRE"><s0>Métrique</s0>
<s5>22</s5>
</fC03>
<fC03 i1="07" i2="X" l="ENG"><s0>Metric</s0>
<s5>22</s5>
</fC03>
<fC03 i1="07" i2="X" l="SPA"><s0>Métrico</s0>
<s5>22</s5>
</fC03>
<fC03 i1="08" i2="X" l="FRE"><s0>Théorie graphe</s0>
<s5>23</s5>
</fC03>
<fC03 i1="08" i2="X" l="ENG"><s0>Graph theory</s0>
<s5>23</s5>
</fC03>
<fC03 i1="08" i2="X" l="SPA"><s0>Teoría grafo</s0>
<s5>23</s5>
</fC03>
<fC03 i1="09" i2="X" l="FRE"><s0>Analyse statistique</s0>
<s5>24</s5>
</fC03>
<fC03 i1="09" i2="X" l="ENG"><s0>Statistical analysis</s0>
<s5>24</s5>
</fC03>
<fC03 i1="09" i2="X" l="SPA"><s0>Análisis estadístico</s0>
<s5>24</s5>
</fC03>
<fC03 i1="10" i2="X" l="FRE"><s0>Classification à vaste marge</s0>
<s5>25</s5>
</fC03>
<fC03 i1="10" i2="X" l="ENG"><s0>Vector support machine</s0>
<s5>25</s5>
</fC03>
<fC03 i1="10" i2="X" l="SPA"><s0>Máquina ejemplo soporte</s0>
<s5>25</s5>
</fC03>
<fN21><s1>003</s1>
</fN21>
<fN44 i1="01"><s1>OTO</s1>
</fN44>
<fN82><s1>OTO</s1>
</fN82>
</pA>
<pR><fA30 i1="01" i2="1" l="ENG"><s1>Software and cyberinfrastructure for astronomy</s1>
<s3>San Diego CA USA</s3>
<s4>2010</s4>
</fA30>
</pR>
</standard>
<server><NO>PASCAL 11-0004539 INIST</NO>
<ET>Comparison of Several Algorithms for Celestial object Classification</ET>
<AU>NANBO PENG; YANXIA ZHANG; YONGHENG ZHAO; RADZIWILL (Nicole M.); BRIDGER (Alan)</AU>
<AF>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences/Beijing 100012/Chine (1 aut., 2 aut., 3 aut.)</AF>
<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>
</record>
Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Ticri/CIDE/explor/CyberinfraV1/Data/PascalFrancis/Corpus
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000124 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/PascalFrancis/Corpus/biblio.hfd -nk 000124 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Ticri/CIDE
|area= CyberinfraV1
|flux= PascalFrancis
|étape= Corpus
|type= RBID
|clé= Pascal:11-0004539
|texte= Comparison of Several Algorithms for Celestial object Classification
}}
| This area was generated with Dilib version V0.6.25. Data generation: Thu Oct 27 09:30:58 2016. Site generation: Sun Mar 10 23:08:40 2024 | |