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	<title>Comments on: Another HAT trick (plus XO-2b)</title>
	<atom:link href="http://oklo.org/2007/05/02/another-hat-trick/feed/" rel="self" type="application/rss+xml" />
	<link>http://oklo.org/2007/05/02/another-hat-trick/</link>
	<description>characterizing planetary systems</description>
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		<title>By: systemic - fit to be timed</title>
		<link>http://oklo.org/2007/05/02/another-hat-trick/comment-page-1/#comment-3300</link>
		<dc:creator>systemic - fit to be timed</dc:creator>
		<pubDate>Sat, 08 Sep 2007 19:51:49 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=208#comment-3300</guid>
		<description>[...] To see how it works, consider the recently discovered transiting planet XO-2. The published radial velocity data for this planet is already bundled with the console. On the AXA site, a total of five transits have already been archived for XO-2. Each of these transits has a measured Heliocentric Julian Date (HJD) for the time of transit midpoint, along with an associated uncertainty. I copied these data into a newly created &#8220;X0-2.tds&#8221; file in my console&#8217;s datafiles folder: [...]</description>
		<content:encoded><![CDATA[<p>[...] To see how it works, consider the recently discovered transiting planet XO-2. The published radial velocity data for this planet is already bundled with the console. On the AXA site, a total of five transits have already been archived for XO-2. Each of these transits has a measured Heliocentric Julian Date (HJD) for the time of transit midpoint, along with an associated uncertainty. I copied these data into a newly created &#8220;X0-2.tds&#8221; file in my console&#8217;s datafiles folder: [...]</p>
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		<title>By: greg</title>
		<link>http://oklo.org/2007/05/02/another-hat-trick/comment-page-1/#comment-2303</link>
		<dc:creator>greg</dc:creator>
		<pubDate>Fri, 04 May 2007 16:46:37 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=208#comment-2303</guid>
		<description>Hi Theo,

Thanks for the CoRoT link. We&#039;ll likely be seeing a lot more stuff from them in the very near future.

At the moment, the systemic console is designed only to handle radial velocity data. We have plans, however, to give it the capability to simultaneously fit RV and photometric data.

best,
Greg</description>
		<content:encoded><![CDATA[<p>Hi Theo,</p>
<p>Thanks for the CoRoT link. We&#8217;ll likely be seeing a lot more stuff from them in the very near future.</p>
<p>At the moment, the systemic console is designed only to handle radial velocity data. We have plans, however, to give it the capability to simultaneously fit RV and photometric data.</p>
<p>best,<br />
Greg</p>
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	<item>
		<title>By: TheoA</title>
		<link>http://oklo.org/2007/05/02/another-hat-trick/comment-page-1/#comment-2294</link>
		<dc:creator>TheoA</dc:creator>
		<pubDate>Thu, 03 May 2007 18:13:13 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=208#comment-2294</guid>
		<description>In keeping with the theme COROT has scored its first planet!

http://www.esa.int/esaCP/SEMCKNU681F_index_1.html#subhead1

The flux image shows some intriguing variations at ingress and egress. Rings, maybe a moon, or just an overactive imagination.

Is the systemic designed to deal with such a dense data set?</description>
		<content:encoded><![CDATA[<p>In keeping with the theme COROT has scored its first planet!</p>
<p><a href="http://www.esa.int/esaCP/SEMCKNU681F_index_1.html#subhead1" rel="nofollow">http://www.esa.int/esaCP/SEMCKNU681F_index_1.html#subhead1</a></p>
<p>The flux image shows some intriguing variations at ingress and egress. Rings, maybe a moon, or just an overactive imagination.</p>
<p>Is the systemic designed to deal with such a dense data set?</p>
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	<item>
		<title>By: Eric F Diaz</title>
		<link>http://oklo.org/2007/05/02/another-hat-trick/comment-page-1/#comment-2279</link>
		<dc:creator>Eric F Diaz</dc:creator>
		<pubDate>Wed, 02 May 2007 11:30:19 +0000</pubDate>
		<guid isPermaLink="false">http://oklo.org/?p=208#comment-2279</guid>
		<description>Hi Greg,

I noticed that you mentioned Spitzer is being used in the analysis of the weather pattern of this planet. I was wondering if SOFIA, the airborne IR telescope, would be of any use in a analysis such as this?</description>
		<content:encoded><![CDATA[<p>Hi Greg,</p>
<p>I noticed that you mentioned Spitzer is being used in the analysis of the weather pattern of this planet. I was wondering if SOFIA, the airborne IR telescope, would be of any use in a analysis such as this?</p>
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