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		<id>https://www.scipedia.com/wd/index.php?action=history&amp;feed=atom&amp;title=Alonso-Floriano_et_al_2016a</id>
		<title>Alonso-Floriano et al 2016a - Revision history</title>
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		<updated>2026-05-12T00:23:47Z</updated>
		<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://www.scipedia.com/wd/index.php?title=Alonso-Floriano_et_al_2016a&amp;diff=198831&amp;oldid=prev</id>
		<title>Scipediacontent: Scipediacontent moved page Draft Content 357587112 to Alonso-Floriano et al 2016a</title>
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				<updated>2021-02-01T22:24:46Z</updated>
		
		<summary type="html">&lt;p&gt;Scipediacontent moved page &lt;a href=&quot;/public/Draft_Content_357587112&quot; class=&quot;mw-redirect&quot; title=&quot;Draft Content 357587112&quot;&gt;Draft Content 357587112&lt;/a&gt; to &lt;a href=&quot;/public/Alonso-Floriano_et_al_2016a&quot; title=&quot;Alonso-Floriano et al 2016a&quot;&gt;Alonso-Floriano et al 2016a&lt;/a&gt;&lt;/p&gt;
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				&lt;td colspan='1' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan='1' style=&quot;background-color: white; color:black; text-align: center;&quot;&gt;Revision as of 22:24, 1 February 2021&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan='2' style='text-align: center;' lang='en'&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
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		<author><name>Scipediacontent</name></author>	</entry>

	<entry>
		<id>https://www.scipedia.com/wd/index.php?title=Alonso-Floriano_et_al_2016a&amp;diff=198830&amp;oldid=prev</id>
		<title>Scipediacontent: Created page with &quot; == Abstract ==  CARMENES, the new Calar Alto spectrograph especially built for radial-velocity surveys of exoearths around M dwarfs, is a very complicated system. For reachin...&quot;</title>
		<link rel="alternate" type="text/html" href="https://www.scipedia.com/wd/index.php?title=Alonso-Floriano_et_al_2016a&amp;diff=198830&amp;oldid=prev"/>
				<updated>2021-02-01T22:24:41Z</updated>
		
		<summary type="html">&lt;p&gt;Created page with &amp;quot; == Abstract ==  CARMENES, the new Calar Alto spectrograph especially built for radial-velocity surveys of exoearths around M dwarfs, is a very complicated system. For reachin...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&lt;br /&gt;
== Abstract ==&lt;br /&gt;
&lt;br /&gt;
CARMENES, the new Calar Alto spectrograph especially built for radial-velocity surveys of exoearths around M dwarfs, is a very complicated system. For reaching the goal of 1 m/s radial-velocity accuracy, it is appropriate not only to monitor stars with the best observing procedure, but to monitor also the parameters of the CARMENES subsystems and safely store all the engineer and science data. Here we describe the CARMENES data flow from the different subsystems, through the instrument control system and pipeline, to the virtual-observatory data server and astronomers.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Original document ==&lt;br /&gt;
&lt;br /&gt;
The different versions of the original document can be found in:&lt;br /&gt;
&lt;br /&gt;
* [http://dx.doi.org/10.1117/12.2233574 http://dx.doi.org/10.1117/12.2233574]&lt;br /&gt;
&lt;br /&gt;
* [https://eprints.ucm.es/55714 https://eprints.ucm.es/55714]&lt;br /&gt;
&lt;br /&gt;
* [https://eprints.ucm.es/55714/1/cortescontreras04libre.pdf https://eprints.ucm.es/55714/1/cortescontreras04libre.pdf]&lt;br /&gt;
&lt;br /&gt;
* [http://ui.adsabs.harvard.edu/abs/2016SPIE.9910E..0EC/abstract http://ui.adsabs.harvard.edu/abs/2016SPIE.9910E..0EC/abstract],&lt;br /&gt;
: [https://www.spiedigitallibrary.org/conference-proceedings-of-spie/9910/1/CARMENES-data-flow/10.1117/12.2233574.full https://www.spiedigitallibrary.org/conference-proceedings-of-spie/9910/1/CARMENES-data-flow/10.1117/12.2233574.full],&lt;br /&gt;
: [https://academic.microsoft.com/#/detail/2470417756 https://academic.microsoft.com/#/detail/2470417756]&lt;/div&gt;</summary>
		<author><name>Scipediacontent</name></author>	</entry>

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