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	<title>Comments for Collider Blog</title>
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	<description>Commentary on Research at the Tevatron and the LHC</description>
	<lastBuildDate>Mon, 21 Sep 2009 11:18:48 +0000</lastBuildDate>
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		<title>Comment on Dark Matter is a Quantum Liquid by Astronomy Sri Lanka</title>
		<link>http://muon.wordpress.com/2008/12/27/dark-matter-is-a-quantum-liquid/#comment-4921</link>
		<dc:creator>Astronomy Sri Lanka</dc:creator>
		<pubDate>Mon, 21 Sep 2009 11:18:48 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=82#comment-4921</guid>
		<description>I prefer more talk going on the dark matter..Will welcome more films like &quot;Angels &amp; Demons &quot; to get more talk going on..

&lt;a href=&quot;http://www.iya2009sl.blogspot.com/&quot; rel=&quot;nofollow&quot;&gt; IYA 2009 Sri Lanka &lt;/a&gt;</description>
		<content:encoded><![CDATA[<p>I prefer more talk going on the dark matter..Will welcome more films like &#8220;Angels &amp; Demons &#8221; to get more talk going on..</p>
<p><a href="http://www.iya2009sl.blogspot.com/" rel="nofollow"> IYA 2009 Sri Lanka </a></p>
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		<title>Comment on Judging experiments by a priori theoretical expectations by Eclipse 2010</title>
		<link>http://muon.wordpress.com/2007/12/29/judging-experiments-by-a-priori-theoretical-expectations/#comment-4920</link>
		<dc:creator>Eclipse 2010</dc:creator>
		<pubDate>Mon, 21 Sep 2009 11:02:18 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/2007/12/29/judging-experiments-by-a-priori-theoretical-expectations/#comment-4920</guid>
		<description>It&#039;s great that you have a great history for this blog since 2006</description>
		<content:encoded><![CDATA[<p>It&#8217;s great that you have a great history for this blog since 2006</p>
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		<title>Comment on International Year of Astronomy: IYA2009 by Keith - Astronomy</title>
		<link>http://muon.wordpress.com/2009/01/05/international-year-of-astronomy-iya2009/#comment-4918</link>
		<dc:creator>Keith - Astronomy</dc:creator>
		<pubDate>Sun, 23 Aug 2009 09:21:32 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=202#comment-4918</guid>
		<description>I have been soooo annoyed this year with so much cloud cover in the UK, and due to global warming it is only going to get worse. Most clear nights are now in the winter. Good viewing, but flippin freezing.

I spend around 2 months of the year in Las Vegas, so always pack my small scope, great viewing out there if you drive 9,000ft up Mt Charleston.</description>
		<content:encoded><![CDATA[<p>I have been soooo annoyed this year with so much cloud cover in the UK, and due to global warming it is only going to get worse. Most clear nights are now in the winter. Good viewing, but flippin freezing.</p>
<p>I spend around 2 months of the year in Las Vegas, so always pack my small scope, great viewing out there if you drive 9,000ft up Mt Charleston.</p>
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		<title>Comment on Light Neutralinos and Charginos are Expected! by Guest</title>
		<link>http://muon.wordpress.com/2009/03/29/light-neutralinos-and-charginos-are-expected/#comment-4917</link>
		<dc:creator>Guest</dc:creator>
		<pubDate>Tue, 28 Jul 2009 03:44:28 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=279#comment-4917</guid>
		<description>&quot;The bad news is that the mass difference typically is small – less than 10 GeV in 80% of the cases generated by the scan.&quot;

This is very good new for the G2-MSSM where the LSP is Wino (if one turns off flavor violating effects) and is almost degenerate (\delta m~100-200 MeV) with the lightest chargino. In this case the relic density (which comes out pretty close to the observed value) is generated non-thermally via moduli decays.</description>
		<content:encoded><![CDATA[<p>&#8220;The bad news is that the mass difference typically is small – less than 10 GeV in 80% of the cases generated by the scan.&#8221;</p>
<p>This is very good new for the G2-MSSM where the LSP is Wino (if one turns off flavor violating effects) and is almost degenerate (\delta m~100-200 MeV) with the lightest chargino. In this case the relic density (which comes out pretty close to the observed value) is generated non-thermally via moduli decays.</p>
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		<title>Comment on Light Neutralinos and Charginos are Expected! by Michael Schmitt</title>
		<link>http://muon.wordpress.com/2009/03/29/light-neutralinos-and-charginos-are-expected/#comment-4903</link>
		<dc:creator>Michael Schmitt</dc:creator>
		<pubDate>Thu, 09 Apr 2009 07:30:14 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=279#comment-4903</guid>
		<description>Wonderful news. I look forward to talking to him there. :)</description>
		<content:encoded><![CDATA[<p>Wonderful news. I look forward to talking to him there. <img src='http://s.wordpress.com/wp-includes/images/smilies/icon_smile.gif' alt=':)' class='wp-smiley' /> </p>
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		<title>Comment on Light Neutralinos and Charginos are Expected! by Tim Tait</title>
		<link>http://muon.wordpress.com/2009/03/29/light-neutralinos-and-charginos-are-expected/#comment-4902</link>
		<dc:creator>Tim Tait</dc:creator>
		<pubDate>Wed, 08 Apr 2009 23:33:55 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=279#comment-4902</guid>
		<description>Another interesting note:  Jamie Gainer will be joining us at Northwestern next year as a postdoc!</description>
		<content:encoded><![CDATA[<p>Another interesting note:  Jamie Gainer will be joining us at Northwestern next year as a postdoc!</p>
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		<title>Comment on 100 Hours of Astronomy &#8211; Historic Telescope at Northwestern by dorigo</title>
		<link>http://muon.wordpress.com/2009/04/02/100-hours-of-astronomy-historic-telescope-at-northwestern/#comment-4894</link>
		<dc:creator>dorigo</dc:creator>
		<pubDate>Fri, 03 Apr 2009 20:40:15 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=294#comment-4894</guid>
		<description>True. The larger the telescope, the smaller S/N signals can be seen, because more S and more N are gathered. So the larger scope is like a higher luminosity measurement... But believe me, making amateur astronomers understand that a larger scope does not increase contrast (S/N) is tough!

Cheers,
T</description>
		<content:encoded><![CDATA[<p>True. The larger the telescope, the smaller S/N signals can be seen, because more S and more N are gathered. So the larger scope is like a higher luminosity measurement&#8230; But believe me, making amateur astronomers understand that a larger scope does not increase contrast (S/N) is tough!</p>
<p>Cheers,<br />
T</p>
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		<title>Comment on 100 Hours of Astronomy &#8211; Historic Telescope at Northwestern by Michael Schmitt</title>
		<link>http://muon.wordpress.com/2009/04/02/100-hours-of-astronomy-historic-telescope-at-northwestern/#comment-4893</link>
		<dc:creator>Michael Schmitt</dc:creator>
		<pubDate>Fri, 03 Apr 2009 10:31:17 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=294#comment-4893</guid>
		<description>Thanks, Tommaso!  I&#039;ll pass along your suggestions to my astronomer colleagues.  Unfortunately I won&#039;t be able to view anything through the telescope at Northwestern since I am at CERN right now, for most of the rest of this year.

Interesting that &quot;contrast&quot; is crucial for viewing galaxies and other far-away objects.  This seems closely tied to a combination of S/B and resolution.  It would be amusing to describe a narrow Higgs peak on top of a small background as an image with &quot;high contrast&quot;! ;)</description>
		<content:encoded><![CDATA[<p>Thanks, Tommaso!  I&#8217;ll pass along your suggestions to my astronomer colleagues.  Unfortunately I won&#8217;t be able to view anything through the telescope at Northwestern since I am at CERN right now, for most of the rest of this year.</p>
<p>Interesting that &#8220;contrast&#8221; is crucial for viewing galaxies and other far-away objects.  This seems closely tied to a combination of S/B and resolution.  It would be amusing to describe a narrow Higgs peak on top of a small background as an image with &#8220;high contrast&#8221;! <img src='http://s.wordpress.com/wp-includes/images/smilies/icon_wink.gif' alt=';)' class='wp-smiley' /> </p>
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		<title>Comment on 100 Hours of Astronomy &#8211; Historic Telescope at Northwestern by dorigo</title>
		<link>http://muon.wordpress.com/2009/04/02/100-hours-of-astronomy-historic-telescope-at-northwestern/#comment-4892</link>
		<dc:creator>dorigo</dc:creator>
		<pubDate>Thu, 02 Apr 2009 22:28:25 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=294#comment-4892</guid>
		<description>Hi Michael,

good luck with the event! I know that most of these session are organized when there is some moon to see -this makes it easier to have success even if there are a few clouds around, since the moon is always a beautiful target. As for Saturn, it is guaranteed to awe beginners, although unfortunately this year the rings are almost at zero tilt, so one barely sees them, with a diminished return. But there should be other good targets, like M35, M44, and M13 - open and globular clusters which make quite a show even in nghts of close to full moon.

As for me, what really triggers me are galaxies in which I can see structure. For this one needs dark skies, so it is almost regularly off limits for reasonable gatherings (i.e. ones that do not aim at deserted places where nobody comes!). In fact, galaxies are faint, and it does not matter how large a telescope is, since what matters is contrast, and contrast requires dark skies.

Cheers,
T.</description>
		<content:encoded><![CDATA[<p>Hi Michael,</p>
<p>good luck with the event! I know that most of these session are organized when there is some moon to see -this makes it easier to have success even if there are a few clouds around, since the moon is always a beautiful target. As for Saturn, it is guaranteed to awe beginners, although unfortunately this year the rings are almost at zero tilt, so one barely sees them, with a diminished return. But there should be other good targets, like M35, M44, and M13 &#8211; open and globular clusters which make quite a show even in nghts of close to full moon.</p>
<p>As for me, what really triggers me are galaxies in which I can see structure. For this one needs dark skies, so it is almost regularly off limits for reasonable gatherings (i.e. ones that do not aim at deserted places where nobody comes!). In fact, galaxies are faint, and it does not matter how large a telescope is, since what matters is contrast, and contrast requires dark skies.</p>
<p>Cheers,<br />
T.</p>
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		<title>Comment on International Year of Astronomy: IYA2009 by 100 Hours of Astronomy - Historic Telescope at Northwestern &#171; Collider Blog</title>
		<link>http://muon.wordpress.com/2009/01/05/international-year-of-astronomy-iya2009/#comment-4891</link>
		<dc:creator>100 Hours of Astronomy - Historic Telescope at Northwestern &#171; Collider Blog</dc:creator>
		<pubDate>Thu, 02 Apr 2009 11:53:51 +0000</pubDate>
		<guid isPermaLink="false">http://muon.wordpress.com/?p=202#comment-4891</guid>
		<description>[...] this year I made a brief post drawing attention to the International Year of Astronomy, i.e., this year. Risa Wechsler at Cosmic [...]</description>
		<content:encoded><![CDATA[<p>[...] this year I made a brief post drawing attention to the International Year of Astronomy, i.e., this year. Risa Wechsler at Cosmic [...]</p>
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