「トップページ」の編集履歴（バックアップ）一覧はこちら
「トップページ」(2014/07/18 (金) 16:30:21) の最新版変更点
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<h3>Papers</h3>
<p><span style="font-size:16px;"><span style="color:#0000FF;">○inhomogenious
X-ray heating</span></span></p>
<p><a href="http://arxiv.org/abs/1406.4157" style="font-size:13px;line-height:1.6em;">21 cm signal from cosmic dawn: Imprints of
spin temperature and fluctuations and peculiar velocities</a><span style="font-size:13px;line-height:1.6em;">(Raghunath Ghara,T. Roy Choudhury and Kanan
K. Datta)</span></p>
<p><a href="http://arxiv.org/abs/astro-ph/0607234">21 cm fluctuations from
inhomogeneous X-ray heating before reionization(Pritchard, Loeb)</a></p>
<p> </p>
<p><span style="font-size:16px;"><span style="color:#0000FF;">○1-point
statistics</span></span></p>
<p><a href="http://arxiv.org/abs/1312.1342"><span style="font-size:14px;line-height:1.2em;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;">
Distinguishing models of reionization using future radio observations of 21-cm
1-point statistics(</span></a><a href="http://arxiv.org/find/astro-ph/1/au:+Watkinson_C/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Catherine
A.Watkinson</a><a href="http://arxiv.org/abs/1312.1342"><span style="font-size:14px;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;">, </span></a><a href="http://arxiv.org/find/astro-ph/1/au:+Pritchard_J/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Jonathan
R. Pritchard</a><a href="http://arxiv.org/abs/1312.1342">)</a></p>
<p><a href="http://arxiv.org/abs/arXiv:0705.3246" style="font-size:14px;line-height:1.2em;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;">
The Difference PDF of 21-cm Fluctuations: A Powerful Statistical Tool for
Probing Cosmic Reionization</a> <u>(</u><a href="http://arxiv.org/find/astro-ph/1/au:+Barkana_R/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Rennan
Barkana</a><a href="http://arxiv.org/abs/arXiv:0705.3246" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;"> (Tel
Aviv University), </a><a href="http://arxiv.org/find/astro-ph/1/au:+Loeb_A/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Abraham
Loeb</a><a href="http://arxiv.org/abs/arXiv:0705.3246" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;"> (Harvard
University)</a></p>
<p><a href="http://arxiv.org/abs/0809.2428"><span style="font-size:14px;line-height:1.2em;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;">
Detection and extraction of signals from the epoch of reionization using higher
order one-point statistics(</span></a><a href="http://arxiv.org/find/astro-ph/1/au:+Harker_G/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Geraint
J. A. Harker</a><a href="http://arxiv.org/abs/0809.2428"><span style="font-size:14px;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;"> (1), </span></a><a href="http://arxiv.org/find/astro-ph/1/au:+Zaroubi_S/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Saleem
Zaroubi</a><a href="http://arxiv.org/abs/0809.2428"><span style="font-size:14px;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;"> (1))</span></a></p>
<p> </p>
<p>Yokoyama</p>
<p>http://arxiv.org/abs/0708.2424 (<a href="http://arxiv.org/abs/0708.2424">High-z 21cm fluctuations due to the
fluctuation of spin temperature</a>)</p>
<p>http://arxiv.org/abs/astro-ph/0610054 (<a href="http://arxiv.org/abs/astro-ph/0610054">Higher order contribution to relatively
low-z 21cm power spectrum</a>)</p>
<p>http://arxiv.org/abs/arXiv:0802.1710 (<a href="http://arxiv.org/abs/arXiv:0802.1710">Fitting formula for relatively low-z
21cm power spectrum</a>)</p>
<h3>Papers</h3>
<p><span style="color:#FF0000;"><span style="font-size:16px;">○inhomogenious
X-ray heating</span></span></p>
<p><a href="http://arxiv.org/abs/1406.4157" style="font-size:13px;line-height:1.6em;">21 cm signal from cosmic dawn: Imprints of
spin temperature and fluctuations and peculiar velocities</a><span style="font-size:13px;line-height:1.6em;">(Raghunath Ghara,T. Roy Choudhury and Kanan
K. Datta)</span></p>
<p><a href="http://arxiv.org/abs/astro-ph/0607234">21 cm fluctuations from
inhomogeneous X-ray heating before reionization(Pritchard, Loeb)</a></p>
<p> </p>
<p><span style="color:#FF0000;"><span style="font-size:16px;">○1-point
statistics</span></span></p>
<p><a href="http://arxiv.org/abs/1312.1342"><span style="font-size:14px;line-height:1.2em;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;">
Distinguishing models of reionization using future radio observations of 21-cm
1-point statistics(</span></a><a href="http://arxiv.org/find/astro-ph/1/au:+Watkinson_C/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Catherine
A.Watkinson</a><a href="http://arxiv.org/abs/1312.1342"><span style="font-size:14px;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;">, </span></a><a href="http://arxiv.org/find/astro-ph/1/au:+Pritchard_J/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Jonathan
R. Pritchard</a><a href="http://arxiv.org/abs/1312.1342">)</a></p>
<p><a href="http://arxiv.org/abs/arXiv:0705.3246" style="font-size:14px;line-height:1.2em;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;">
The Difference PDF of 21-cm Fluctuations: A Powerful Statistical Tool for
Probing Cosmic Reionization</a> <u>(</u><a href="http://arxiv.org/find/astro-ph/1/au:+Barkana_R/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Rennan
Barkana</a><a href="http://arxiv.org/abs/arXiv:0705.3246" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;"> (Tel
Aviv University), </a><a href="http://arxiv.org/find/astro-ph/1/au:+Loeb_A/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Abraham
Loeb</a><a href="http://arxiv.org/abs/arXiv:0705.3246" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;"> (Harvard
University)</a></p>
<p><a href="http://arxiv.org/abs/0809.2428"><span style="font-size:14px;line-height:1.2em;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;">
Detection and extraction of signals from the epoch of reionization using higher
order one-point statistics(</span></a><a href="http://arxiv.org/find/astro-ph/1/au:+Harker_G/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Geraint
J. A. Harker</a><a href="http://arxiv.org/abs/0809.2428"><span style="font-size:14px;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;"> (1), </span></a><a href="http://arxiv.org/find/astro-ph/1/au:+Zaroubi_S/0/1/0/all/0/1" style="font-size:14px;font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;text-decoration:none;">Saleem
Zaroubi</a><a href="http://arxiv.org/abs/0809.2428"><span style="font-size:14px;color:rgb(0,0,0);font-family:'Lucida Grande', helvetica, arial, verdana, sans-serif;line-height:24px;"> (1))</span></a></p>
<p> </p>
<p>Yokoyama</p>
<p>http://arxiv.org/abs/0708.2424 (<a href="http://arxiv.org/abs/0708.2424">High-z 21cm fluctuations due to the
fluctuation of spin temperature</a>)</p>
<p>http://arxiv.org/abs/astro-ph/0610054 (<a href="http://arxiv.org/abs/astro-ph/0610054">Higher order contribution to relatively
low-z 21cm power spectrum</a>)</p>
<p>http://arxiv.org/abs/arXiv:0802.1710 (<a href="http://arxiv.org/abs/arXiv:0802.1710">Fitting formula for relatively low-z
21cm power spectrum</a>)</p>
