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<title>ephem.git, branch master</title>
<subtitle>Astronomical ephemerides (unfinished)</subtitle>
<id>http://git.madore.org/cgit/ephem.git/atom?h=master</id>
<link rel='self' href='http://git.madore.org/cgit/ephem.git/atom?h=master'/>
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<updated>2012-04-19T22:59:31+00:00</updated>
<entry>
<title>Yet another test/exploratory class.</title>
<updated>2012-04-19T22:59:31+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-19T22:59:31+00:00</published>
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<id>urn:sha1:a2155ba8c57c9d414a184d192a5a7c46903391d3</id>
<content type='text'>
</content>
</entry>
<entry>
<title>Re-add (rewritten) functions to compute Smart97 functions.</title>
<updated>2012-04-19T17:57:53+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-19T17:57:53+00:00</published>
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<id>urn:sha1:f096845cb0b4087691c6d003574013f3bae82aed</id>
<content type='text'>
(This is intended as a test, not to be actually used.)
</content>
</entry>
<entry>
<title>Add a computation of zonal tide effects on UT1 (from IERS conventions).</title>
<updated>2012-04-18T17:57:07+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-18T17:57:07+00:00</published>
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<id>urn:sha1:aef12693c2ec946c5c88070f6707480df7eb26ec</id>
<content type='text'>
Plus a Test2 class which tests this on the TAI-UTC difference.
</content>
</entry>
<entry>
<title>Handle UTC between 1961 and 1972 ("rubber seconds").</title>
<updated>2012-04-18T17:56:43+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-18T17:56:43+00:00</published>
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<id>urn:sha1:223ae5a5e66fc6808bdb345caa7bfe567bb23024</id>
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</content>
</entry>
<entry>
<title>Slight improvement to test proram.</title>
<updated>2012-04-17T22:20:17+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-17T22:20:17+00:00</published>
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<id>urn:sha1:8be15afc02e4e82b30a4e8457098547ac4c062d2</id>
<content type='text'>
</content>
</entry>
<entry>
<title>Test: Compute final solar coordinates.</title>
<updated>2012-04-17T19:36:19+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-17T19:36:19+00:00</published>
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<id>urn:sha1:13a0fa9046fb85626ccd49f46fe4dec9f5e32e46</id>
<content type='text'>
</content>
</entry>
<entry>
<title>Various small fixes + add a simple test (computing solar coordinates).</title>
<updated>2012-04-17T19:09:36+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-17T19:09:36+00:00</published>
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<id>urn:sha1:12ab2221611336f6d209d643574fdc2d2b1fac16</id>
<content type='text'>
</content>
</entry>
<entry>
<title>Use J2000 ecliptic (rather than equatorial) coordinates as starting point for precession.</title>
<updated>2012-04-17T17:15:56+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-17T17:15:56+00:00</published>
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<id>urn:sha1:5f00eb3230d89f98d93c6e5bc8ecfa72e4e89b07</id>
<content type='text'>
We will assume that these are the coordinates returned by VSOP87.
</content>
</entry>
<entry>
<title>Use quaternions instead of 3*3 matrices to represent rotations.</title>
<updated>2012-04-03T15:11:35+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-04-03T15:11:35+00:00</published>
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<id>urn:sha1:b5dd88803374c586e165c77ac1dbf96c0d0f6ee7</id>
<content type='text'>
</content>
</entry>
<entry>
<title>Equation of the origins/equinoxes.</title>
<updated>2012-03-27T17:48:07+00:00</updated>
<author>
<name>David A. Madore</name>
<email>david+git@madore.org</email>
</author>
<published>2012-03-27T17:23:09+00:00</published>
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<id>urn:sha1:b0cb2767577a654db082f5ae9bbd69ffde725d2e</id>
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