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use ;
/// For a given TT date, compute the X,Y coordinates of the Celestial
/// Intermediate Pole and the CIO locator s, using the IAU 2000B
/// precession-nutation model.
///
/// Given:
/// date1,date2 double TT as a 2-part Julian Date (Note 1)
///
/// Returned:
/// x,y double Celestial Intermediate Pole (Note 2)
/// s double the CIO locator s (Note 3)
///
/// # Notes:
///
/// 1) The TT date date1+date2 is a Julian Date, apportioned in any
/// convenient way between the two arguments. For example,
/// JD(TT)=2450123.7 could be expressed in any of these ways,
/// among others:
///
/// | date1 | date2 | |
/// |-------------|--------------|----------------------|
/// |2450123.7 | 0.0 | (JD method) |
/// |2451545.0 | -1421.3 | (J2000 method) |
/// |2400000.5 | 50123.2 | (MJD method) |
/// |2450123.5 | 0.2 | (date & time method) |
///
/// The JD method is the most natural and convenient to use in
/// cases where the loss of several decimal digits of resolution
/// is acceptable. The J2000 method is best matched to the way
/// the argument is handled internally and will deliver the
/// optimum resolution. The MJD method and the date & time methods
/// are both good compromises between resolution and convenience.
///
/// 2) The Celestial Intermediate Pole coordinates are the x,y
/// components of the unit vector in the Geocentric Celestial
/// Reference System.
///
/// 3) The CIO locator s (in radians) positions the Celestial
/// Intermediate Origin on the equator of the CIP.
///
/// 4) The present function is faster, but slightly less accurate (about
/// 1 mas in X,Y), than the eraXys00a function.
///
/// # Called:
/// eraPnm00b classical NPB matrix, IAU 2000B
/// eraBpn2xy extract CIP X,Y coordinates from NPB matrix
/// eraS00 the CIO locator s, given X,Y, IAU 2000A
///
/// # Reference:
///
/// McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
/// IERS Technical Note No. 32, BKG (2004)
///
/// This revision: 2021 May 11