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	<title>The AstroStat Slog &#187; Maxwell distribution</title>
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		<title>[ArXiv] 1st week, Dec. 2007</title>
		<link>http://groundtruth.info/AstroStat/slog/2007/arxiv-1st-week-dec-2007/</link>
		<comments>http://groundtruth.info/AstroStat/slog/2007/arxiv-1st-week-dec-2007/#comments</comments>
		<pubDate>Fri, 07 Dec 2007 19:15:04 +0000</pubDate>
		<dc:creator>hlee</dc:creator>
				<category><![CDATA[arXiv]]></category>
		<category><![CDATA[CMB]]></category>
		<category><![CDATA[cosmic shear]]></category>
		<category><![CDATA[cross-correlation]]></category>
		<category><![CDATA[Hubble constant]]></category>
		<category><![CDATA[Maxwell distribution]]></category>
		<category><![CDATA[Point Process]]></category>
		<category><![CDATA[PSF]]></category>
		<category><![CDATA[SZ]]></category>
		<category><![CDATA[wavelet]]></category>
		<category><![CDATA[X-Atlas]]></category>

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		<description><![CDATA[There&#8217;s only one day in the first week of December with no preprint appearance. Dubbing the week of Dec. 2nd as the first week is hoped to be accepted. 

[stat.ML:0711.4983]
 A Method for Compressing Parameters in Bayesian Models with Application to Logistic Sequence Prediction Models  L. Li and R. M. Neal
[astro-ph:0711.4886]
Requirements on PSF Calibration [...]]]></description>
			<content:encoded><![CDATA[<p>There&#8217;s only one day in the first week of December with no preprint appearance. Dubbing the week of Dec. 2nd as the first week is hoped to be accepted.<span id="more-197"></span> <!---more ---></p>
<ul>
<li><a href="http://arxiv.org/abs/0711.4983">[stat.ML:0711.4983]</a><br />
<strong> A Method for Compressing Parameters in Bayesian Models with Application to Logistic Sequence Prediction Models </strong> L. Li and R. M. Neal</li>
<li><a href="http://arxiv.org/abs/0711.4886">[astro-ph:0711.4886]</a><br />
<strong>Requirements on PSF Calibration for Dark Energy from Cosmic Shear </strong> S. Paulin-Henriksson et.al.</li>
<li><a href="http://arxiv.org/abs/0711.4895">[astro-ph:0711.4895]</a><br />
<strong> The impact of going beyond the Maxwell distribution in direct dark matter detection rates </strong> J. D.  Vergados, S. H. Hansen, and O. Host</li>
<li><a href="http://arxiv.org/abs/0712.0003">[astro-ph:0712.0003]</a><br />
<strong>The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites </strong> J. Chen</li>
<li><a href="http://arxiv.org/abs/0712.0283">[stat.ME:0712.0283]</a><br />
<strong> Wavelet methods in statistics: Some recent developments and their applications </strong> A. Antoniadis</li>
<li><a href="http://arxiv.org/abs/0712.0189">[stat.ML:0712.0189]</a><br />
<strong> Summarization and Classification of Non-Poisson Point Processes </strong> J. Picka and M. Deng</li>
<li><a href="http://arxiv.org/abs/0712.0588">[astro-ph:0712.0588]</a><br />
<strong> SZ and CMB reconstruction using Generalized Morphological Component  Analysis </strong> J. Bobin et. al.</li>
<li><a href="http://arxiv.org/abs/0712.0610">[astro-ph:0712.0610]</a><br />
<strong> X-Atlas: An Online Archive of Chandra&#8217;s Stellar High Energy Transmission Gratings Observations </strong> O. W. Westbrook et.al.</li>
<li><a href="http://arxiv.org/abs/0712.0618">[astro-ph:0712.0618]</a><br />
<strong>Precision of Hubble constant derived using black hole binary absolute  distances and statistical redshift information </strong> C. L. MacLeod and C. J. Hogan</li>
</ul>
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