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+#include "erfa.h"
+
+double eraGst00b(double uta, double utb)
+/*
+** - - - - - - - - - -
+** e r a G s t 0 0 b
+** - - - - - - - - - -
+**
+** Greenwich apparent sidereal time (consistent with IAU 2000
+** resolutions but using the truncated nutation model IAU 2000B).
+**
+** Given:
+** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
+**
+** Returned (function value):
+** double Greenwich apparent sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 date uta+utb is a Julian Date, apportioned in any
+** convenient way between the argument pair. For example,
+** JD=2450123.7 could be expressed in any of these ways, among
+** others:
+**
+** uta utb
+**
+** 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 and MJD methods are good compromises
+** between resolution and convenience. For UT, the date & time
+** method is best matched to the algorithm that is used by the Earth
+** Rotation Angle function, called internally: maximum precision is
+** delivered when the uta argument is for 0hrs UT1 on the day in
+** question and the utb argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) The result is compatible with the IAU 2000 resolutions, except
+** that accuracy has been compromised for the sake of speed and
+** convenience in two respects:
+**
+** . UT is used instead of TDB (or TT) to compute the precession
+** component of GMST and the equation of the equinoxes. This
+** results in errors of order 0.1 mas at present.
+**
+** . The IAU 2000B abridged nutation model (McCarthy & Luzum, 2001)
+** is used, introducing errors of up to 1 mas.
+**
+** 3) This GAST is compatible with the IAU 2000 resolutions and must be
+** used only in conjunction with other IAU 2000 compatible
+** components such as precession-nutation.
+**
+** 4) The result is returned in the range 0 to 2pi.
+**
+** 5) The algorithm is from Capitaine et al. (2003) and IERS
+** Conventions 2003.
+**
+** Called:
+** eraGmst00 Greenwich mean sidereal time, IAU 2000
+** eraEe00b equation of the equinoxes, IAU 2000B
+** eraAnp normalize angle into range 0 to 2pi
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
+** implement the IAU 2000 definition of UT1", Astronomy &
+** Astrophysics, 406, 1135-1149 (2003)
+**
+** McCarthy, D.D. & Luzum, B.J., "An abridged model of the
+** precession-nutation of the celestial pole", Celestial Mechanics &
+** Dynamical Astronomy, 85, 37-49 (2003)
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Copyright (C) 2013-2016, NumFOCUS Foundation.
+** Derived, with permission, from the SOFA library. See notes at end of file.
+*/
+{
+ double gmst00, ee00b, gst;
+
+
+ gmst00 = eraGmst00(uta, utb, uta, utb);
+ ee00b = eraEe00b(uta, utb);
+ gst = eraAnp(gmst00 + ee00b);
+
+ return gst;
+
+}
+/*----------------------------------------------------------------------
+**
+**
+** 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.
+**
+*/