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<title>My RSS Feed</title><link>http://home.physics.ucla.edu/~arisaka/home/index.html</link><description>Hot News&#x21;</description><dc:language>en</dc:language><dc:creator>user@domain.com</dc:creator><dc:rights>Copyright 2010 Katsushi Arisaka</dc:rights><dc:date>2012-12-28T11:06:32-08:00</dc:date><admin:generatorAgent rdf:resource="http://www.realmacsoftware.com/" />
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<lastBuildDate>Sat, 10 Jul 2010 12:20:55 -0700</lastBuildDate><item><title>XMASS anounced their solar axion limit</title><dc:creator>user@domain.com</dc:creator><category>Dark Matter</category><dc:date>2012-12-28T11:06:32-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/979f51f2d01e3d745ca67205e4a08843-15.html#unique-entry-id-15</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/979f51f2d01e3d745ca67205e4a08843-15.html#unique-entry-id-15</guid><content:encoded><![CDATA[<span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">XMASS dark matter experiment in Japan announced their solar axion limit, using 6.7 days, total of 5.6 ton-days.<br /></span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">Their limit below 1 keV axion mass is g_Ae < 5.4 &times; 10&minus;11 (90% C.L.). <br /></span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; "><a href="http://arxiv.org/abs/1212.6153" rel="self">http://arxiv.org/abs/1212.6153</a></span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">  (The final plot is given below.)<br /></span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">Their paper can be compared to the predicted sensitivity given by Arisaka Lab's analysis:<br /></span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; "><a href="http://arxiv.org/abs/1209.3810" rel="self">http://arxiv.org/abs/1209.3810</a></span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; "><br /></span><p style="text-align:center;"><img class="imageStyle" alt="XMASS axion" src="http://home.physics.ucla.edu/~arisaka/home/News/files/xmass-axion.png" width="554" height="531" /><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; "><a href="http://arxiv.org/abs/1209.3810" rel="self"><br /></a></span></p>]]></content:encoded></item><item><title>How do environments talk to genes?</title><dc:creator>user@domain.com</dc:creator><category>Neuroscience</category><dc:date>2012-12-21T17:52:00-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/4d6f69465724bb1832382b4921796f8a-14.html#unique-entry-id-14</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/4d6f69465724bb1832382b4921796f8a-14.html#unique-entry-id-14</guid><content:encoded><![CDATA[<span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">In </span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; "><a href="http://www.nature.com/neuro/journal/v16/n1/full/nn.3286.html" rel="self">Nature Neuroscience January 2013 issue</a></span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">, Moshe Szyf explains the environmental interaction onto genes.<br />A report elucidates the widely recognized, but poorly understood, concept of gene-environment interaction, finding a molecular mechanism in the case of post-traumatic stress disorder: demethylation of a glucocorticoid response element in the stress response regulator FKBP5 that depends on both the risk allele and childhood trauma.<br /></span><p style="text-align:center;"><img class="imageStyle" alt="Pasted Graphic 4" src="http://home.physics.ucla.edu/~arisaka/home/News/files/pasted-graphic-4.jpg" width="678" height="408" /></p>]]></content:encoded></item><item><title>Nine-Year WMAP results announced</title><dc:creator>user@domain.com</dc:creator><category>Cosmology</category><dc:date>2012-12-21T20:27:00-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/6124fdef76db302a442c9e0a561d4dd1-13.html#unique-entry-id-13</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/6124fdef76db302a442c9e0a561d4dd1-13.html#unique-entry-id-13</guid><content:encoded><![CDATA[<table border="0.000000" cellpadding="8.000000" cellspacing="0.500000"><tr height="0"><td valign="middle" width="634"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">The model fit implies that the age of the universe is 13.772+/-0.059 Gyr, and the fit Hubble constant is H0 = 69.32+/-0.80 km/s/Mpc. Inflation is also supported: the fluctuations are adiabatic, with Gaussian random phases; the detection of a deviation of the scalar spectral index from unity reported earlier by WMAP now has high statistical significance (n_s = 0.9608+/-0.0080); and the universe is close to flat/Euclidean, Omega_k = -0.0027 (+0.0039/-0.0038). Overall, the WMAP mission has resulted in a reduction of the cosmological parameter volume by a factor of 68,000 for the standard six-parameter LCDM model, based on CMB data alone. <br /></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://arxiv.org/abs/1212.5225" rel="self">http://arxiv.org/abs/1212.5225</a></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://arxiv.org/abs/1212.5226" rel="self">http://arxiv.org/abs/1212.5226</a></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span></td></tr></table><p style="text-align:center;"><img class="imageStyle" alt="WMAP 9years" src="http://home.physics.ucla.edu/~arisaka/home/News/files/wmap-9years.png" width="670" height="535" /><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; "><br /></span><img class="imageStyle" alt="WMAP Omega" src="http://home.physics.ucla.edu/~arisaka/home/News/files/wmap-omega.png" width="660" height="482" /><span style="font:15px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; "><br /></span></p>]]></content:encoded></item><item><title>Adrian Cheng&#x2c; Named to Forbes&#x2019; 30 Under 30 as a Rising Star in Science</title><dc:creator>user@domain.com</dc:creator><category>Arisaka Group</category><dc:date>2012-12-17T07:55:00-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/3e12c3d448ccb365b169a6c7304eee17-12.html#unique-entry-id-12</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/3e12c3d448ccb365b169a6c7304eee17-12.html#unique-entry-id-12</guid><content:encoded><![CDATA[A formal grad student of Arisaka Lab, Adrian Cheng, was named to "Forbes&rsquo; 30 Under 30 as a Rising Star in Science"<br />This is based on our development of high-speed two-photon microscopes while he was at UCLA.<br /><ul class="disc"><li><a href="http://www.forbes.com/special-report/2012/30-under-30/30-under-30_science.html" rel="self">The announcement by Forbes.</a></li><li><a href="http://www.alleninstitute.org/Media/documents/press_releases/2012_1217_PressRelease_ForbesAdrianCheng.html" rel="self">News by Allen Institute</a></li><li><a href="http://www.reuters.com/article/2012/12/17/idUS179266+17-Dec-2012+BW20121217" rel="self">News by Leuters</a></li></ul>The old news at UCLA in 2011 can found at <a href="http://www.dailybruin.com/index.php/article/2011/01/new_laser_microscope_technology_allows_scientists_to_see_neuron_activity_of_the_entire_brain" rel="self">Daily Bruin on Jan 18, 2011</a>.<br />Our original paper was published at<br /><ul class="disc"><li>Simultaneous two-photon calcium imaging at different depths with spatiotemporal multiplexing.</li><li>Cheng A, Gon&ccedil;alves JT, Golshani P, Arisaka K, Portera-Cailliau C.</li><li><a href="http://www.ncbi.nlm.nih.gov/pubmed/21217749" rel="self">Nat Methods. 2011 Feb;8(2):139-42. Epub 2011 Jan 9</a>.</li></ul><p style="text-align:center;"><img class="imageStyle" alt="Pasted Graphic 2" src="http://home.physics.ucla.edu/~arisaka/home/News/files/pasted-graphic-2.jpg" width="150" height="150" /></p>]]></content:encoded></item><item><title>6th Symposium on Large TPCs at Paris on Dec 17-19&#x2c; 2012</title><dc:creator>user@domain.com</dc:creator><category>Dark Matter</category><dc:date>2012-12-20T06:33:34-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/f90be93e550335d7ba9eb83f91ff2530-11.html#unique-entry-id-11</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/f90be93e550335d7ba9eb83f91ff2530-11.html#unique-entry-id-11</guid><content:encoded><![CDATA[SIXTH SYMPOSIUM ON LARGE TPCs FOR LOW ENERGY RARE EVENT DETECTION<br />at PARIS 13&egrave;me, France<br />on December 17-19, 2012<br /><a href="http://www-tpc-paris.cea.fr" rel="self">http://www-tpc-paris.cea.fr</a><br />Presentations are posted under "Slides".<br /><br /><p style="text-align:center;"><img class="imageStyle" alt="Pasted Graphic 1" src="http://home.physics.ucla.edu/~arisaka/home/News/files/pasted-graphic-1.jpg" width="336" height="350" /></p>]]></content:encoded></item><item><title>Astronomers detect nearest Earth-like neighbour</title><dc:creator>user@domain.com</dc:creator><category>Origin</category><dc:date>2012-12-19T03:59:01-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/ddf4aef4e179933a68afc996ca394733-10.html#unique-entry-id-10</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/ddf4aef4e179933a68afc996ca394733-10.html#unique-entry-id-10</guid><content:encoded><![CDATA[Scientists have been surprised by the unexpected discovery of a nearby solar system using a new experimental technique.<br />The system of five planets ranging in size from two to six times the Earth's mass orbiting the Sun-like star Tau Ceti, just 12 light years away.<br /><a href="http://www.abc.net.au/science/articles/2012/12/19/3657825.htm" rel="self">ABC News</a><br /><a href="http://arxiv.org/abs/1212.4058" rel="self">http://arxiv.org/abs/1212.4058</a><br /><br /><p style="text-align:center;"><img class="imageStyle" alt="Gliese-667c" src="http://home.physics.ucla.edu/~arisaka/home/News/files/gliese-667c.jpg" width="567" height="413" /></p>]]></content:encoded></item><item><title>&#x27;Obamadon&#x27; was wiped out by the asteroid</title><dc:creator>user@domain.com</dc:creator><category>Origin</category><dc:date>2012-12-11T00:40:15-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/2ea9bbbe152170f6aa7b8474f711c591-9.html#unique-entry-id-9</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/2ea9bbbe152170f6aa7b8474f711c591-9.html#unique-entry-id-9</guid><content:encoded><![CDATA[<span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://news.yale.edu/2012/12/10/asteroid-killed-dinosaurs-also-wiped-out-obamadon" rel="self">Asteroid that killed the dinosaurs also wiped out the &lsquo;Obamadon&rsquo;,</a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br />The asteroid collision widely thought to have killed the dinosaurs also led to extreme devastation among snake and lizard species, according to new research &mdash; including the extinction of a newly identified lizard Yale and Harvard scientists have named Obamadon gracilis.  The published paper can be fund </span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://www.pnas.org/content/early/2012/12/07/1211526110" rel="self">here</a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">.<br /></span><p style="text-align:center;"><img class="imageStyle" alt="lizard-interior" src="http://home.physics.ucla.edu/~arisaka/home/News/files/lizard-interior.jpg" width="510" height="398" /></p>]]></content:encoded></item><item><title>New South Pole Telescope shows Omaga = 1.006 +- 0.004</title><dc:creator>user@domain.com</dc:creator><category>Cosmology</category><dc:date>2012-10-26T09:00:00-07:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/b892cc78b9ea3c15fde4f5215b2f853b-8.html#unique-entry-id-8</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/b892cc78b9ea3c15fde4f5215b2f853b-8.html#unique-entry-id-8</guid><content:encoded><![CDATA[<span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">The </span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://pole.uchicago.edu" rel="self">South Pole Telescope</a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "> published the </span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://arxiv.org/abs/1210.7231" rel="self">new results</a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">.<br />Omega_K=-0.003+0.014-0.018. Using the SPT+WMAP7 data, the spectral index of scalar fluctuations tis ns=0.9623+/-0.0097 in the LCDM model, a 3.9sigma preference for a scale-dependent spectrum with ns<1. <br /><br /></span><p style="text-align:center;"><img class="imageStyle" alt="Pasted Graphic" src="http://home.physics.ucla.edu/~arisaka/home/News/files/pasted-graphic.jpg" width="908" height="406" /></p>]]></content:encoded></item><item><title>Neutralino excluded up to &#x7e;250 GeV</title><dc:creator>user@domain.com</dc:creator><category>CMS</category><dc:date>2012-11-16T10:00:00-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/c972f0fb3167bf738c1c3c47e574c137-7.html#unique-entry-id-7</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/c972f0fb3167bf738c1c3c47e574c137-7.html#unique-entry-id-7</guid><content:encoded><![CDATA[<span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">The neutralino is excluded up to ~250 GeV.<br />At the </span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://www.icepp.s.u-tokyo.ac.jp/hcp2012/" rel="self">Hadron Collider Physics Symposium 2012 </a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">hosted by Kyoto University, <br />the new </span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://cms.web.cern.ch/news/highlights-cms-results-presented-hcp" rel="self">CMS results</a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "> were reported.<br /><br /></span><p style="text-align:center;"><img class="imageStyle" alt="CMS Neutralino Limit" src="http://home.physics.ucla.edu/~arisaka/home/News/files/cms-neutralino-limit.png" width="631" height="487" /></p>]]></content:encoded></item><item><title>Higgs results updated with 7 sigma</title><dc:creator>user@domain.com</dc:creator><category>CMS</category><dc:date>2012-11-16T09:00:00-08:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/4dd1098d1db8c96dca1c85d015b5cbdc-6.html#unique-entry-id-6</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/4dd1098d1db8c96dca1c85d015b5cbdc-6.html#unique-entry-id-6</guid><content:encoded><![CDATA[<span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">Significance of Higgs particle has been up to 7 sigma now.<br />The </span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://www.icepp.s.u-tokyo.ac.jp/hcp2012/" rel="self">Hadron Collider Physics Symposium 2012 </a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">hosted by Kyoto University, <br />The new </span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://cms.web.cern.ch/news/highlights-cms-results-presented-hcp" rel="self">CMS results</a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "> were reported.<br /><br /></span><p style="text-align:center;"><img class="imageStyle" alt="CMS Higgs 7sigma" src="http://home.physics.ucla.edu/~arisaka/home/News/files/cms-higgs-7sigma.png" width="567" height="544" /></p>]]></content:encoded></item><item><title>Higgs Particle has been discovered by LHC&#x21;  </title><dc:creator>user@domain.com</dc:creator><category>CMS</category><category>Arisaka Group</category><dc:date>2012-07-05T07:00:00-07:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/5ec833d397f7bfb065ec2af2bb3f593d-5.html#unique-entry-id-5</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/5ec833d397f7bfb065ec2af2bb3f593d-5.html#unique-entry-id-5</guid><content:encoded><![CDATA[<span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">Finally the Higgs Particle has been discovered by LHC!  <br />Here is the Higgs -> two gamma decay, observed by CMS.   <br />The paper is available </span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://arxiv.org/abs/1207.7235" rel="self">here</a></span><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">.</span><span style="font-size:14px; "><br /></span><p style="text-align:center;"><img class="imageStyle" alt="Higgs CMS" src="http://home.physics.ucla.edu/~arisaka/home/News/files/higgs-cms.png" width="591" height="570" /></p>]]></content:encoded></item><item><title>Axion search by Liquid Xenon</title><dc:creator>user@domain.com</dc:creator><category>Dark Matter</category><category>Arisaka Group</category><dc:date>2012-09-17T09:00:00-07:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/fa622465ddd4d61fe023a5261b750cbb-3.html#unique-entry-id-3</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/fa622465ddd4d61fe023a5261b750cbb-3.html#unique-entry-id-3</guid><content:encoded><![CDATA[<table border="0.000000" cellpadding="8.000000" cellspacing="0.500000"><tr height="0"><td valign="middle" width="634"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">Arisaka's group has studied a possibility of searching for axion and axion-like particles by liquid Xenon detectors such as XENON100 and XENON1T.  <br /></span></td></tr></table><p style="text-align:center;"><img class="imageStyle" alt="gaelimits3" src="http://home.physics.ucla.edu/~arisaka/home/News/files/gaelimits3.png" width="764" height="490" /><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span><table border="0.000000" cellpadding="8.000000" cellspacing="0.500000"><tr height="0"></p><p style="text-align:left;"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br />The paper has been submitted to Astroparticle Physcis Journal, and available at<br /></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><a href="http://arxiv.org/abs/1209.3810" rel="self">http://arxiv.org/abs/1209.3810</a></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span></td></tr></table></p>]]></content:encoded></item><item><title>XENON100 announced the new results from 225 days data</title><dc:creator>user@domain.com</dc:creator><category>Dark Matter</category><category>Arisaka Group</category><dc:date>2012-07-25T09:00:00-07:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/1650c086c6bc301ac3af59644ba5e774-2.html#unique-entry-id-2</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/1650c086c6bc301ac3af59644ba5e774-2.html#unique-entry-id-2</guid><content:encoded><![CDATA[<table border="0.000000" cellpadding="8.000000" cellspacing="0.500000"><tr height="0"><td valign="middle" width="634"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">The XENON100 collaboration submitted a paper with the new results of a 225 days  to PRL, excluding previously unexplored parameter space and questioning the light WIMP interpretation of the DAMA and CoGeNT results. <br /></span></td></tr></table><p style="text-align:center;"><img class="imageStyle" alt="XENO100-225days" src="http://home.physics.ucla.edu/~arisaka/home/News/files/xeno100-225days.png" width="699" height="498" /><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span><table border="0.000000" cellpadding="8.000000" cellspacing="0.500000"><tr height="0"></p><p style="text-align:left;"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">The preprint can be found here: <br /><br /></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><a href="http://arxiv.org/abs/1207.5988" rel="self">http://arxiv.org/abs/1207.5988</a></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span></td></tr></table></p>]]></content:encoded></item><item><title>XENON100 announced the new results</title><dc:creator>user@domain.com</dc:creator><category>Dark Matter</category><category>Arisaka Group</category><dc:date>2010-05-03T12:21:00-07:00</dc:date><link>http://home.physics.ucla.edu/~arisaka/home/News/files/def8e41db56bd1cb54e50289cd41cbc2-0.html#unique-entry-id-0</link><guid isPermaLink="true">http://home.physics.ucla.edu/~arisaka/home/News/files/def8e41db56bd1cb54e50289cd41cbc2-0.html#unique-entry-id-0</guid><content:encoded><![CDATA[<table border="0.000000" cellpadding="8.000000" cellspacing="0.500000"><tr height="0"><td valign="middle" width="634"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">The XENON100 collaboration submitted a paper with the first results of a 11.2 days background analysis to PRL, excluding previously unexplored parameter space and questioning the light WIMP interpretation of the DAMA and CoGeNT results. <br /></span></td></tr></table><p style="text-align:center;"><img class="imageStyle" alt="" src="http://home.physics.ucla.edu/~arisaka/home/News/files/xe100_excl.gif" width="574" height="408" /><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span><table border="0.000000" cellpadding="8.000000" cellspacing="0.500000"><tr height="0"></p><p style="text-align:left;"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">The preprint can be found here: <br /><br /></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><a href="" rel="external">arXiv:1005.0380</a></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; ">.<br /><br />These results are also covered in the media:<br /></span></td></tr><tr height="0"><span style="font:14px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; "><br />
</span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><a href="http://www.nytimes.com/2010/05/04/science/space/04dark.html" rel="external">The New York Times</a></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><br /></u></span></td></tr><tr height="0"><span style="font:14px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">
</span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><a href="http://www.newscientist.com/article/dn18839" rel="external">New Scientist</a></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><br /></u></span></td></tr><tr height="0"><span style="font:14px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">
</span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><a href="http://blogs.nature.com/news/thegreatbeyond/2010/05/dark_matter_stays_dark.html" rel="external">Nature Blog</a></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><br /></u></span></td></tr><tr height="0"><span style="font:14px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">
</span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><a href="http://blogs.discovermagazine.com/cosmicvariance/2010/05/04/clearly-seeing-nothing/" rel="external">Discover Magazine Blog</a></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><br /></u></span></td></tr><tr height="0"><span style="font:14px &#39;Lucida Grande&#39;, LucidaGrande, Verdana, sans-serif; ">
</span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><a href="http://www.scientificamerican.com/article.cfm?id=xenon-100-dark-matter" rel="external">Scientific American</a></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><br /></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><br /></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; font-weight:bold; font-weight:bold; ">Wired - XENON100<br /></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><em>August 6, 2009:</em></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "> An </span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; color:#0000EE;"><u><a href="http://xenon.physics.rice.edu/pics/wired2009.pdf" rel="external">article</a></u></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "> about the hunt for Dark Matter and XENON100 appeared in the UK version of the </span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "><em>Wired</em></span></td></tr><tr height="0"><span style="font:14px Arial, Verdana, Helvetica, sans-serif; "> magazine.</span></td></tr></table></p>]]></content:encoded></item></channel>
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