Account for EOP libration correction
Add the variations in pole coordinates corresponding to motions with periods less than two days in space that are not part of the IAU 2000 nutation model. In IERS Convention 2010, see equation 5.11, Table 5.1a (which is already present in the resources) for pole corrections and Table 5.1b for UT1 and LOD corrections. In the current implementation, only corrections due to ocean tide effects are taken into account.
Edited by Gaëtan Pierre