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diff --git a/ast/erfa/pfw06.c b/ast/erfa/pfw06.c
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-#include "erfa.h"
-
-void eraPfw06(double date1, double date2,
- double *gamb, double *phib, double *psib, double *epsa)
-/*
-** - - - - - - - - -
-** e r a P f w 0 6
-** - - - - - - - - -
-**
-** Precession angles, IAU 2006 (Fukushima-Williams 4-angle formulation).
-**
-** Given:
-** date1,date2 double TT as a 2-part Julian Date (Note 1)
-**
-** Returned:
-** gamb double F-W angle gamma_bar (radians)
-** phib double F-W angle phi_bar (radians)
-** psib double F-W angle psi_bar (radians)
-** epsa double F-W angle epsilon_A (radians)
-**
-** 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) Naming the following points:
-**
-** e = J2000.0 ecliptic pole,
-** p = GCRS pole,
-** E = mean ecliptic pole of date,
-** and P = mean pole of date,
-**
-** the four Fukushima-Williams angles are as follows:
-**
-** gamb = gamma_bar = epE
-** phib = phi_bar = pE
-** psib = psi_bar = pEP
-** epsa = epsilon_A = EP
-**
-** 3) The matrix representing the combined effects of frame bias and
-** precession is:
-**
-** PxB = R_1(-epsa).R_3(-psib).R_1(phib).R_3(gamb)
-**
-** 4) The matrix representing the combined effects of frame bias,
-** precession and nutation is simply:
-**
-** NxPxB = R_1(-epsa-dE).R_3(-psib-dP).R_1(phib).R_3(gamb)
-**
-** where dP and dE are the nutation components with respect to the
-** ecliptic of date.
-**
-** Reference:
-**
-** Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351
-**
-** Called:
-** eraObl06 mean obliquity, IAU 2006
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** Derived, with permission, from the SOFA library. See notes at end of file.
-*/
-{
- double t;
-
-
-/* Interval between fundamental date J2000.0 and given date (JC). */
- t = ((date1 - ERFA_DJ00) + date2) / ERFA_DJC;
-
-/* P03 bias+precession angles. */
- *gamb = ( -0.052928 +
- ( 10.556378 +
- ( 0.4932044 +
- ( -0.00031238 +
- ( -0.000002788 +
- ( 0.0000000260 )
- * t) * t) * t) * t) * t) * ERFA_DAS2R;
- *phib = ( 84381.412819 +
- ( -46.811016 +
- ( 0.0511268 +
- ( 0.00053289 +
- ( -0.000000440 +
- ( -0.0000000176 )
- * t) * t) * t) * t) * t) * ERFA_DAS2R;
- *psib = ( -0.041775 +
- ( 5038.481484 +
- ( 1.5584175 +
- ( -0.00018522 +
- ( -0.000026452 +
- ( -0.0000000148 )
- * t) * t) * t) * t) * t) * ERFA_DAS2R;
- *epsa = eraObl06(date1, date2);
-
- return;
-
-}
-/*----------------------------------------------------------------------
-**
-**
-** 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.
-**
-*/