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-#include "erfa.h"
-
-double eraS06a(double date1, double date2)
-/*
-** - - - - - - - -
-** e r a S 0 6 a
-** - - - - - - - -
-**
-** The CIO locator s, positioning the Celestial Intermediate Origin on
-** the equator of the Celestial Intermediate Pole, using the IAU 2006
-** precession and IAU 2000A nutation models.
-**
-** Given:
-** date1,date2 double TT as a 2-part Julian Date (Note 1)
-**
-** Returned (function value):
-** double the CIO locator s in radians (Note 2)
-**
-** 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 CIO locator s is the difference between the right ascensions
-** of the same point in two systems. The two systems are the GCRS
-** and the CIP,CIO, and the point is the ascending node of the
-** CIP equator. The CIO locator s remains a small fraction of
-** 1 arcsecond throughout 1900-2100.
-**
-** 3) The series used to compute s is in fact for s+XY/2, where X and Y
-** are the x and y components of the CIP unit vector; this series is
-** more compact than a direct series for s would be. The present
-** function uses the full IAU 2000A nutation model when predicting
-** the CIP position.
-**
-** Called:
-** eraPnm06a classical NPB matrix, IAU 2006/2000A
-** eraBpn2xy extract CIP X,Y coordinates from NPB matrix
-** eraS06 the CIO locator s, given X,Y, IAU 2006
-**
-** References:
-**
-** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P.,
-** "Expressions for the Celestial Intermediate Pole and Celestial
-** Ephemeris Origin consistent with the IAU 2000A precession-
-** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
-**
-** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
-** intermediate origin" (CIO) by IAU 2006 Resolution 2.
-**
-** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
-**
-** McCarthy, D. D., Petit, G. (eds.), 2004, IERS Conventions (2003),
-** IERS Technical Note No. 32, BKG
-**
-** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** Derived, with permission, from the SOFA library. See notes at end of file.
-*/
-{
- double rnpb[3][3], x, y, s;
-
-
-/* Bias-precession-nutation-matrix, IAU 20006/2000A. */
- eraPnm06a(date1, date2, rnpb);
-
-/* Extract the CIP coordinates. */
- eraBpn2xy(rnpb, &x, &y);
-
-/* Compute the CIO locator s, given the CIP coordinates. */
- s = eraS06(date1, date2, x, y);
-
- return s;
-
-}
-/*----------------------------------------------------------------------
-**
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** All rights reserved.
-**
-** This library is derived, with permission, from the International
-** Astronomical Union's "Standards of Fundamental Astronomy" library,
-** available from http://www.iausofa.org.
-**
-** The ERFA version is intended to retain identical functionality to
-** the SOFA library, but made distinct through different function and
-** file names, as set out in the SOFA license conditions. The SOFA
-** original has a role as a reference standard for the IAU and IERS,
-** and consequently redistribution is permitted only in its unaltered
-** state. The ERFA version is not subject to this restriction and
-** therefore can be included in distributions which do not support the
-** concept of "read only" software.
-**
-** Although the intent is to replicate the SOFA API (other than
-** replacement of prefix names) and results (with the exception of
-** bugs; any that are discovered will be fixed), SOFA is not
-** responsible for any errors found in this version of the library.
-**
-** If you wish to acknowledge the SOFA heritage, please acknowledge
-** that you are using a library derived from SOFA, rather than SOFA
-** itself.
-**
-**
-** TERMS AND CONDITIONS
-**
-** Redistribution and use in source and binary forms, with or without
-** modification, are permitted provided that the following conditions
-** are met:
-**
-** 1 Redistributions of source code must retain the above copyright
-** notice, this list of conditions and the following disclaimer.
-**
-** 2 Redistributions in binary form must reproduce the above copyright
-** notice, this list of conditions and the following disclaimer in
-** the documentation and/or other materials provided with the
-** distribution.
-**
-** 3 Neither the name of the Standards Of Fundamental Astronomy Board,
-** the International Astronomical Union nor the names of its
-** contributors may be used to endorse or promote products derived
-** from this software without specific prior written permission.
-**
-** THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
-** "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
-** LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
-** FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL THE
-** COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
-** INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
-** BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
-** LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
-** CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
-** LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
-** ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
-** POSSIBILITY OF SUCH DAMAGE.
-**
-*/