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	<title>Thesis Neminis &#187; Classification</title>
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	<link>http://thesis.neminis.org</link>
	<description>Diario di lavoro della tesi di Vincenzo Russo / Work-log of Vincenzo Russo’s Thesis</description>
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		<title>Knowledge Discovery portal</title>
		<link>http://thesis.neminis.org/2008/01/09/knowledge-discovery-portal/</link>
		<comments>http://thesis.neminis.org/2008/01/09/knowledge-discovery-portal/#comments</comments>
		<pubDate>Wed, 09 Jan 2008 13:27:55 +0000</pubDate>
		<dc:creator>vincenzo russo</dc:creator>
				<category><![CDATA[Classification]]></category>
		<category><![CDATA[Clustering]]></category>
		<category><![CDATA[Data Mining]]></category>
		<category><![CDATA[Dataset]]></category>
		<category><![CDATA[Software]]></category>
		<category><![CDATA[Text Mining]]></category>

		<guid isPermaLink="false">http://thesis.neminis.org/2008/01/09/knowledge-discovery-portal/</guid>
		<description><![CDATA[KDnuggets.com (KD stands for Knowledge Discovery) is the leading source of information on Data Mining, Web Mining, Knowledge Discovery, and Decision Support Topics, including News, Software, Solutions, Companies, Jobs, Courses, Meetings, Publications, and more. Go to KDnuggets.com]]></description>
			<content:encoded><![CDATA[<p>KDnuggets.com (KD stands for Knowledge Discovery) is the leading source of information on Data Mining, Web Mining, Knowledge Discovery, and Decision Support Topics, including News, Software, Solutions, Companies, Jobs, Courses, Meetings, Publications, and more.</p>
<p><a href="http://www.kdnuggets.com/index.html">Go to KDnuggets.com</a></p>
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		<title>[OT] Star galaxies separation via SVM/CVM classification &#8211; Part 2</title>
		<link>http://thesis.neminis.org/2007/11/04/ot-star-galaxies-separation-via-svmcvm-classification-part-2/</link>
		<comments>http://thesis.neminis.org/2007/11/04/ot-star-galaxies-separation-via-svmcvm-classification-part-2/#comments</comments>
		<pubDate>Sun, 04 Nov 2007 11:14:45 +0000</pubDate>
		<dc:creator>vincenzo russo</dc:creator>
				<category><![CDATA[Astrophysics]]></category>
		<category><![CDATA[Classification]]></category>
		<category><![CDATA[Off-Topic]]></category>
		<category><![CDATA[SVM]]></category>

		<guid isPermaLink="false">http://thesis.neminis.org/2007/11/04/ot-star-galaxies-separation-via-svmcvm-classification-part-2/</guid>
		<description><![CDATA[This is a modification of the experiments in this post. I rapidly built a new training set and this time I use only this training set for training the SVM/CVM. Than, I test the new trained classifier on all three &#8230; <a href="http://thesis.neminis.org/2007/11/04/ot-star-galaxies-separation-via-svmcvm-classification-part-2/">Continue reading <span class="meta-nav">&#8594;</span></a>]]></description>
			<content:encoded><![CDATA[<p>This is a modification of the experiments in <a href="http://thesis.neminis.org/2007/10/14/ot-star-galaxies-separation-via-svm-classification/">this post</a>.</p>
<p>I rapidly built a new training set and this time I use only this training set for training the SVM/CVM. Than, I test the  new trained classifier on all three dataset of the previous post.</p>
<p>The training set contain 500 points and has been built using stars and galaxies from another portion of sky.</p>
<p><strong>New accuracy results (SVM)</strong></p>
<p>Longo 01: 95,96 %<br />
Longo 02: 98,08 %<br />
Longo 03: 97,956 %</p>
<p><strong>New accuracy results (CVM)</strong></p>
<p>Longo 01: 96,31 %<br />
Longo 02: 97,67 %<br />
Longo 03: 97,138 %</p>
<p>Let us consider the Longo 02 tested with CVM. We have</p>
<p>Completeness for Stars: 98,4 %<br />
Contamination for Stars: 4,7 %</p>
<p>Completeness for Galaxies: 95,4 %<br />
Contamination for Galaxies: 1,5 %</p>
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		<title>[OT] Star galaxies separation via SVM/CVM classification</title>
		<link>http://thesis.neminis.org/2007/10/14/ot-star-galaxies-separation-via-svm-classification/</link>
		<comments>http://thesis.neminis.org/2007/10/14/ot-star-galaxies-separation-via-svm-classification/#comments</comments>
		<pubDate>Sun, 14 Oct 2007 16:44:47 +0000</pubDate>
		<dc:creator>vincenzo russo</dc:creator>
				<category><![CDATA[Astrophysics]]></category>
		<category><![CDATA[Classification]]></category>
		<category><![CDATA[Off-Topic]]></category>
		<category><![CDATA[SVM]]></category>

		<guid isPermaLink="false">http://thesis.neminis.org/2007/10/14/ot-star-galaxies-separation-via-svm-classification/</guid>
		<description><![CDATA[We have used some astrophysics star/galaxies datasets for our clustering problems, because they have heavily overlapping clusters. Here we present some results of an SVM classification performed on the same datasets. In fact, S/G separation is usually faced in a &#8230; <a href="http://thesis.neminis.org/2007/10/14/ot-star-galaxies-separation-via-svm-classification/">Continue reading <span class="meta-nav">&#8594;</span></a>]]></description>
			<content:encoded><![CDATA[<p>We have used some astrophysics star/galaxies datasets for our clustering problems, because they have heavily overlapping clusters.</p>
<p>Here we present some results of an SVM classification performed on the same datasets. In fact, S/G separation is usually faced in a supervised way.</p>
<p>We have used a simple nonlinear SVM/<a href="http://www.cse.ust.hk/~ivor/cvm.html">CVM</a> classifier with a linear kernel (K(x,y) = x&#8217; * y).</p>
<p>For each dataset, we have used 5% of it as training set. The rest is the test set.</p>
<p><strong>Datasets: </strong></p>
<p>Longo 01, 2500 items, 2000 stars, 500 galaxies<br />
Longo 02, 9816 items, 2935 stars, 6883 galaxies<br />
Longo 03, 10940 items, 2978 stars, 7964 galaxies</p>
<p><strong>Accuracy results: </strong></p>
<p>Longo 01: 95%<br />
Longo 02: 98,0746%<br />
Longo 03: 97,925%</p>
<p><strong>Accuracy results with <a href="http://www.cse.ust.hk/~ivor/cvm.html">CVM</a>: </strong></p>
<p>Longo 01: 94,98%<br />
Longo 02: 97,5%<br />
Longo 03: 95,2%</p>
<p>Probably, other kernels could lead to better results, but it is necessary to understand in which way tune the hyperparameters, such as the kernel width and the soft margin constant, etc.</p>
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