Generate the matrix of precession between two epochs,
using the old, pre IAU 1976, Bessel-Newcomb model, in
Andoyer's formulation.
CALL:
CALL sla_PREBN (BEP0, BEP1, RMATP)
GIVEN:
BEP0
D
beginning Besselian epoch
BEP1
D
ending Besselian epoch
RETURNED:
RMATP
D(3,3)
precession matrix
NOTE:
The matrix is in the sense:
v1 = Mv0
where v1 is the star vector relative to the
mean equator and equinox of epoch BEP1, M is the
matrix RMATP and
v0 is the star vector relative to the
mean equator and equinox of epoch BEP0.