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	<title>Comments on: Disentangling Gaussians</title>
	<atom:link href="http://bit-player.org/2010/disentangling-gaussians/feed" rel="self" type="application/rss+xml" />
	<link>http://bit-player.org/2010/disentangling-gaussians</link>
	<description>An amateur's outlook on computation and mathematics.</description>
	<pubDate>Thu, 17 May 2012 10:09:29 +0000</pubDate>
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		<title>By: Peter Rowlett</title>
		<link>http://bit-player.org/2010/disentangling-gaussians#comment-2994</link>
		<dc:creator>Peter Rowlett</dc:creator>
		<pubDate>Fri, 02 Jul 2010 10:19:02 +0000</pubDate>
		<guid isPermaLink="false">http://bit-player.org/?p=695#comment-2994</guid>
		<description>I included a link to this post in &lt;a href="http://travelsinamathematicalworld.blogspot.com/2010/07/carnival-of-mathematics-67.html" rel="nofollow"&gt;Carnival of Mathematics #67&lt;/a&gt;.</description>
		<content:encoded><![CDATA[<p>I included a link to this post in <a href="http://travelsinamathematicalworld.blogspot.com/2010/07/carnival-of-mathematics-67.html" rel="nofollow">Carnival of Mathematics #67</a>.</p>
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		<title>By: Elwood Downey</title>
		<link>http://bit-player.org/2010/disentangling-gaussians#comment-2946</link>
		<dc:creator>Elwood Downey</dc:creator>
		<pubDate>Fri, 11 Jun 2010 04:15:17 +0000</pubDate>
		<guid isPermaLink="false">http://bit-player.org/?p=695#comment-2946</guid>
		<description>Sounds applicable to performing photometry on images containing rich star fields where individual stars overlap. The usual technique uses deconvolution but assumes each star adheres to the same known Gaussian PSF (point spread function). More recent work (Magain, et al, 2007) solves simultaneously for the individual Gaussians and the PSF but still assumes the PSF is the same for all stars which becomes less likely as the image grows larger in size.</description>
		<content:encoded><![CDATA[<p>Sounds applicable to performing photometry on images containing rich star fields where individual stars overlap. The usual technique uses deconvolution but assumes each star adheres to the same known Gaussian PSF (point spread function). More recent work (Magain, et al, 2007) solves simultaneously for the individual Gaussians and the PSF but still assumes the PSF is the same for all stars which becomes less likely as the image grows larger in size.</p>
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