<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>1405-5546</journal-id>
<journal-title><![CDATA[Computación y Sistemas]]></journal-title>
<abbrev-journal-title><![CDATA[Comp. y Sist.]]></abbrev-journal-title>
<issn>1405-5546</issn>
<publisher>
<publisher-name><![CDATA[Instituto Politécnico Nacional, Centro de Investigación en Computación]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S1405-55462004000300003</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[Feature Selection using Typical Testors applied to Estimation of Stellar Parameters]]></article-title>
<article-title xml:lang="es"><![CDATA[Selección de Características usando Testores Típicos aplicada a la Estimación de Parámetros Estelares]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Santos]]></surname>
<given-names><![CDATA[José Á]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Carrasco]]></surname>
<given-names><![CDATA[Ariel]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Martínez]]></surname>
<given-names><![CDATA[José F]]></given-names>
</name>
<xref ref-type="aff" rid="A01"/>
</contrib>
</contrib-group>
<aff id="A01">
<institution><![CDATA[,Instituto Nacional de Astrofísica Óptica y Electrónica (INAOE)  ]]></institution>
<addr-line><![CDATA[ ]]></addr-line>
<country>México</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>09</month>
<year>2004</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>09</month>
<year>2004</year>
</pub-date>
<volume>8</volume>
<numero>1</numero>
<fpage>15</fpage>
<lpage>23</lpage>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S1405-55462004000300003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S1405-55462004000300003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S1405-55462004000300003&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[In this paper a comparative analysis of feature selection using typical testors applied on astronomical data, is presented. The comparison is based on the classification efficiency using typical testors as feature selection method against the classification efficiency using Ramirez (2001) method, which uses genetic algorithms. The well-known K-nearest neighbors rule (KNN) was used as classifier. The feature selection based on typical testors was modified to be applied on a prediction problem of a real valued function. The feature selection obtained with typical testors reduces the amount of features in approximately 50% and the classification error index is better than both using the original data and Ramirez's method.]]></p></abstract>
<abstract abstract-type="short" xml:lang="es"><p><![CDATA[En este artículo se presenta un análisis comparativo de la selección de características usando testores típicos aplicada a la estimación de parámetros estelares. La comparación está basada en la eficiencia de clasificación al usar testores típicos como método de selección de variables contra la eficiencia de clasificación al usar el método de Ramírez (2001), el cual usa algoritmos genéticos. Como clasificador se usó la regla de K-vecinos más cercanos (KNN). Se propuso una modificación al concepto de testor típico para poder aplicarlo en problemas de predicción de una función con imagen en los números reales. En los experimentos, la selección de variables con testores típicos redujo la cantidad de características aproximadamente en un 50%. El error de clasificación usando nuestro método fue menor que usando todas las características o el método de Ramírez.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Feature Selection]]></kwd>
<kwd lng="en"><![CDATA[Typical Testors]]></kwd>
<kwd lng="en"><![CDATA[Logical Combinatorial Pattern Recognition]]></kwd>
<kwd lng="en"><![CDATA[Prediction of Stellar Parameters]]></kwd>
<kwd lng="es"><![CDATA[Selección de características]]></kwd>
<kwd lng="es"><![CDATA[Testores típicos]]></kwd>
<kwd lng="es"><![CDATA[Reconocimiento lógico combinatorio de patrones]]></kwd>
<kwd lng="es"><![CDATA[Predicción de parámetros estelares]]></kwd>
</kwd-group>
</article-meta>
</front><body><![CDATA[ <p align="center"><font face="verdana" size="4"><b>Feature Selection using Typical Testors applied to Estimation of Stellar Parameters</b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="3"><b><i>Selecci&oacute;n de Caracter&iacute;sticas usando Testores T&iacute;picos aplicada a la Estimaci&oacute;n de Par&aacute;metros Estelares</i></b></font></p>     <p align="center"><font face="verdana" size="2">&nbsp;</font></p>     <p align="center"><font face="verdana" size="2"><b>Jos&eacute; &Aacute;. Santos, Ariel Carrasco and Jos&eacute; F. Mart&iacute;nez</b></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><i><sup>1 </sup>Instituto Nacional de Astrof&iacute;sica &Oacute;ptica y Electr&oacute;nica (INAOE), M&eacute;xico <a href="mailto:angellisse@hotmail.com">angellisse@hotmail.com</a> ; <a href="mailto:ariel@inaoep.mx">ariel@inaoep.mx</a> ; <a href="mailto:fmartinez@inaoep.mx">fmartinez@inaoep.mx</a></i></font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2">Article received on august 18, 2003    <br> Accepted on august 05, 2004</font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Abstract</b></font></p>     <p align="justify"><font face="verdana" size="2">In this paper a comparative analysis of feature selection using typical testors applied on astronomical data, is presented. The comparison is based on the classification efficiency using typical testors as feature selection method against the classification efficiency using Ramirez (2001) method, which uses genetic algorithms. The well&#150;known K&#150;nearest neighbors rule (KNN) was used as classifier. The feature selection based on typical testors was modified to be applied on a prediction problem of a real valued function. The feature selection obtained with typical testors reduces the amount of features in approximately 50% and the classification error index is better than both using the original data and Ramirez's method. </font></p>     <p align="justify"><font face="verdana" size="2"><b>Keywords: </b>Feature Selection; Typical Testors; Logical Combinatorial Pattern Recognition; Prediction of Stellar Parameters.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Resumen</b></font></p>     <p align="justify"><font face="verdana" size="2">En este art&iacute;culo se presenta un an&aacute;lisis comparativo de la selecci&oacute;n de caracter&iacute;sticas usando testores t&iacute;picos aplicada a la estimaci&oacute;n de par&aacute;metros estelares. La comparaci&oacute;n est&aacute; basada en la eficiencia de clasificaci&oacute;n al usar testores t&iacute;picos como m&eacute;todo de selecci&oacute;n de variables contra la eficiencia de clasificaci&oacute;n al usar el m&eacute;todo de Ram&iacute;rez (2001), el cual usa algoritmos gen&eacute;ticos. Como clasificador se us&oacute; la regla de K&#150;vecinos m&aacute;s cercanos (KNN). Se propuso una modificaci&oacute;n al concepto de testor t&iacute;pico para poder aplicarlo en problemas de predicci&oacute;n de una funci&oacute;n con imagen en los n&uacute;meros reales. En los experimentos, la selecci&oacute;n de variables con testores t&iacute;picos redujo la cantidad de caracter&iacute;sticas aproximadamente en un 50%. El error de clasificaci&oacute;n usando nuestro m&eacute;todo fue menor que usando todas las caracter&iacute;sticas o el m&eacute;todo de Ram&iacute;rez.</font></p>     <p align="justify"><font face="verdana" size="2"><b>Palabras Clave: </b>Selecci&oacute;n de caracter&iacute;sticas, Testores t&iacute;picos, Reconocimiento l&oacute;gico combinatorio de patrones, Predicci&oacute;n de par&aacute;metros estelares.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><a href="/pdf/cys/v8n1/v8n1a3.pdf" target="_blank">DESCARGAR ART&Iacute;CULO EN FORMATO PDF</a></font></p>     ]]></body>
<body><![CDATA[<p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>Acknowledgement</b></font></p>     <p align="justify"><font face="verdana" size="2">This work was financially supported by CONACyT (Mexico) through projects J38707&#150;A and I38436&#150;A.</font></p>     <p align="justify"><font face="verdana" size="2">&nbsp;</font></p>     <p align="justify"><font face="verdana" size="2"><b>References</b></font></p>     <!-- ref --><p align="justify"><font face="verdana" size="2">1. <b>Alba Cabrera E., </b>"New extensions of testor concept for different types of similarity functions" Ph. D. Thesis, ICIMAF, Cuba, 1997. 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</ref-list>
</back>
</article>
