Serveur d'exploration Cyberinfrastructure

Attention, ce site est en cours de développement !
Attention, site généré par des moyens informatiques à partir de corpus bruts.
Les informations ne sont donc pas validées.

A Simple and Effective Algorithm for Quasar Candidate Selection

Identifieur interne : 000B65 ( Main/Exploration ); précédent : 000B64; suivant : 000B66

A Simple and Effective Algorithm for Quasar Candidate Selection

Auteurs : NANBO PENG [République populaire de Chine] ; YANXIA ZHANG [République populaire de Chine] ; TONG PEI [République populaire de Chine] ; YONGHENG ZHAO [République populaire de Chine]

Source :

RBID : Pascal:11-0070244

Descripteurs français

English descriptors

Abstract

K-Nearest Neighbor (kNN) algorithm is one of the simplest and most flexible and effective classification algorithms, which has been widely used in many fields. Using the multi-band samples extracted from large surveys of SDSS DR7 and UKIDSS DR3, we investigate the performance of kNN with different combinations of colors to select quasar candidates. The color histograms of quasars and stars is helpful to select the optimal input pattern for the classifier of kNN. The best input pattern is (u-g, g-r, r-i, i-z, z-Y,Y-J, J-H, H-K, Y-K, g-z). In our case, the performance of kNN is assessed by different performance metrics, which indicate kNN has rather high performance for discriminating quasars from stars. As a result, kNN is an applicable and effective method to select quasar candidates for large sky survey projects.


Affiliations:


Links toward previous steps (curation, corpus...)


Le document en format XML

<record>
<TEI>
<teiHeader>
<fileDesc>
<titleStmt>
<title xml:lang="en" level="a">A Simple and Effective Algorithm for Quasar Candidate Selection</title>
<author>
<name sortKey="Nanbo Peng" sort="Nanbo Peng" uniqKey="Nanbo Peng" last="Nanbo Peng">NANBO PENG</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>100012 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Yanxia Zhang" sort="Yanxia Zhang" uniqKey="Yanxia Zhang" last="Yanxia Zhang">YANXIA ZHANG</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>100012 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Tong Pei" sort="Tong Pei" uniqKey="Tong Pei" last="Tong Pei">TONG PEI</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>100012 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Yongheng Zhao" sort="Yongheng Zhao" uniqKey="Yongheng Zhao" last="Yongheng Zhao">YONGHENG ZHAO</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>100012 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</affiliation>
</author>
</titleStmt>
<publicationStmt>
<idno type="wicri:source">INIST</idno>
<idno type="inist">11-0070244</idno>
<date when="2010">2010</date>
<idno type="stanalyst">PASCAL 11-0070244 INIST</idno>
<idno type="RBID">Pascal:11-0070244</idno>
<idno type="wicri:Area/PascalFrancis/Corpus">000049</idno>
<idno type="wicri:Area/PascalFrancis/Curation">000196</idno>
<idno type="wicri:Area/PascalFrancis/Checkpoint">000172</idno>
<idno type="wicri:doubleKey">0277-786X:2010:Nanbo Peng:a:simple:and</idno>
<idno type="wicri:Area/Main/Merge">000B71</idno>
<idno type="wicri:Area/Main/Curation">000B65</idno>
<idno type="wicri:Area/Main/Exploration">000B65</idno>
</publicationStmt>
<sourceDesc>
<biblStruct>
<analytic>
<title xml:lang="en" level="a">A Simple and Effective Algorithm for Quasar Candidate Selection</title>
<author>
<name sortKey="Nanbo Peng" sort="Nanbo Peng" uniqKey="Nanbo Peng" last="Nanbo Peng">NANBO PENG</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>100012 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Yanxia Zhang" sort="Yanxia Zhang" uniqKey="Yanxia Zhang" last="Yanxia Zhang">YANXIA ZHANG</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>100012 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Tong Pei" sort="Tong Pei" uniqKey="Tong Pei" last="Tong Pei">TONG PEI</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>100012 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Yongheng Zhao" sort="Yongheng Zhao" uniqKey="Yongheng Zhao" last="Yongheng Zhao">YONGHENG ZHAO</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Key Laboratory of Optical Astronomy, National Astronomical Observatories; Chinese Academy of Sciences</s1>
<s2>100012 Beijing</s2>
<s3>CHN</s3>
<sZ>1 aut.</sZ>
<sZ>2 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>4 aut.</sZ>
</inist:fA14>
<country>République populaire de Chine</country>
<placeName>
<settlement type="city">Pékin</settlement>
</placeName>
</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>Classification</term>
<term>Color image</term>
<term>Cosmology</term>
<term>High performance</term>
<term>Histogram</term>
<term>Metrics</term>
<term>Nearest neighbour</term>
<term>Quasars</term>
<term>Stars</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Cosmologie</term>
<term>Plus proche voisin</term>
<term>Classification</term>
<term>Image couleur</term>
<term>Histogramme</term>
<term>Haute performance</term>
<term>Métrique</term>
<term>Quasar</term>
<term>Etoile</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr">
<term>Cosmologie</term>
<term>Classification</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">K-Nearest Neighbor (kNN) algorithm is one of the simplest and most flexible and effective classification algorithms, which has been widely used in many fields. Using the multi-band samples extracted from large surveys of SDSS DR7 and UKIDSS DR3, we investigate the performance of kNN with different combinations of colors to select quasar candidates. The color histograms of quasars and stars is helpful to select the optimal input pattern for the classifier of kNN. The best input pattern is (u-g, g-r, r-i, i-z, z-Y,Y-J, J-H, H-K, Y-K, g-z). In our case, the performance of kNN is assessed by different performance metrics, which indicate kNN has rather high performance for discriminating quasars from stars. As a result, kNN is an applicable and effective method to select quasar candidates for large sky survey projects.</div>
</front>
</TEI>
<affiliations>
<list>
<country>
<li>République populaire de Chine</li>
</country>
<settlement>
<li>Pékin</li>
</settlement>
</list>
<tree>
<country name="République populaire de Chine">
<noRegion>
<name sortKey="Nanbo Peng" sort="Nanbo Peng" uniqKey="Nanbo Peng" last="Nanbo Peng">NANBO PENG</name>
</noRegion>
<name sortKey="Tong Pei" sort="Tong Pei" uniqKey="Tong Pei" last="Tong Pei">TONG PEI</name>
<name sortKey="Yanxia Zhang" sort="Yanxia Zhang" uniqKey="Yanxia Zhang" last="Yanxia Zhang">YANXIA ZHANG</name>
<name sortKey="Yongheng Zhao" sort="Yongheng Zhao" uniqKey="Yongheng Zhao" last="Yongheng Zhao">YONGHENG ZHAO</name>
</country>
</tree>
</affiliations>
</record>

Pour manipuler ce document sous Unix (Dilib)

EXPLOR_STEP=$WICRI_ROOT/Ticri/CIDE/explor/CyberinfraV1/Data/Main/Exploration
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000B65 | SxmlIndent | more

Ou

HfdSelect -h $EXPLOR_AREA/Data/Main/Exploration/biblio.hfd -nk 000B65 | SxmlIndent | more

Pour mettre un lien sur cette page dans le réseau Wicri

{{Explor lien
   |wiki=    Ticri/CIDE
   |area=    CyberinfraV1
   |flux=    Main
   |étape=   Exploration
   |type=    RBID
   |clé=     Pascal:11-0070244
   |texte=   A Simple and Effective Algorithm for Quasar Candidate Selection
}}

Wicri

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