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	<id>http://ovsa.njit.edu//wiki/index.php?action=history&amp;feed=atom&amp;title=2023_February</id>
	<title>2023 February - Revision history</title>
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	<updated>2026-04-17T18:01:02Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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		<id>http://ovsa.njit.edu//wiki/index.php?title=2023_February&amp;diff=7033&amp;oldid=prev</id>
		<title>Dgary: Created page with &quot;[http://www.ovsa.njit.edu/wiki/index.php/Expanded_Owens_Valley_Solar_Array#Observing_Log Back to Observing Log]  == February 20 == Observations resume with 8 antennas.  Ants 1, 2, 3, 4, 5, and 7 are more or less normal, while Ants 6 and 8 have much reduced sensitivity and hence are not calibrated above about 10 GHz.&quot;</title>
		<link rel="alternate" type="text/html" href="http://ovsa.njit.edu//wiki/index.php?title=2023_February&amp;diff=7033&amp;oldid=prev"/>
		<updated>2023-05-28T15:29:09Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;[http://www.ovsa.njit.edu/wiki/index.php/Expanded_Owens_Valley_Solar_Array#Observing_Log Back to Observing Log]  == February 20 == Observations resume with 8 antennas.  Ants 1, 2, 3, 4, 5, and 7 are more or less normal, while Ants 6 and 8 have much reduced sensitivity and hence are not calibrated above about 10 GHz.&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;[http://www.ovsa.njit.edu/wiki/index.php/Expanded_Owens_Valley_Solar_Array#Observing_Log Back to Observing Log]&lt;br /&gt;
&lt;br /&gt;
== February 20 ==&lt;br /&gt;
Observations resume with 8 antennas.  Ants 1, 2, 3, 4, 5, and 7 are more or less normal, while Ants 6 and 8 have much reduced sensitivity and hence are not calibrated above about 10 GHz.&lt;/div&gt;</summary>
		<author><name>Dgary</name></author>
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