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* Use J2000 ecliptic (rather than equatorial) coordinates as starting point ↵David A. Madore2012-04-172-2/+5
| | | | | | for precession. We will assume that these are the coordinates returned by VSOP87.
* Use quaternions instead of 3*3 matrices to represent rotations.David A. Madore2012-04-033-54/+46
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* Equation of the origins/equinoxes.David A. Madore2012-03-273-1/+45
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* Nutation.David A. Madore2012-03-274-3/+2493
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* Use generalized Poisson series for VSOP87.David A. Madore2012-03-272-2506/+2524
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* Implement more general Poisson series.David A. Madore2012-03-271-14/+77
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* Simple matrix library + formula for precession.David A. Madore2012-03-275-439/+111
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* Initial commit. This version doesn't do much but evaluate VSOP87/Smart97 ↵David A. Madore2012-03-276-0/+3196
series.