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diff --git a/ast/erfa/ltpecl.c b/ast/erfa/ltpecl.c
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-#include "erfa.h"
-
-void eraLtpecl(double epj, double vec[3])
-/*
-** - - - - - - - - - -
-** e r a L t p e c l
-** - - - - - - - - - -
-**
-** Long-term precession of the ecliptic.
-**
-** Given:
-** epj double Julian epoch (TT)
-**
-** Returned:
-** vec double[3] ecliptic pole unit vector
-**
-** Notes:
-**
-** 1) The returned vector is with respect to the J2000.0 mean equator
-** and equinox.
-**
-** 2) The Vondrak et al. (2011, 2012) 400 millennia precession model
-** agrees with the IAU 2006 precession at J2000.0 and stays within
-** 100 microarcseconds during the 20th and 21st centuries. It is
-** accurate to a few arcseconds throughout the historical period,
-** worsening to a few tenths of a degree at the end of the
-** +/- 200,000 year time span.
-**
-** References:
-**
-** Vondrak, J., Capitaine, N. and Wallace, P., 2011, New precession
-** expressions, valid for long time intervals, Astron.Astrophys. 534,
-** A22
-**
-** Vondrak, J., Capitaine, N. and Wallace, P., 2012, New precession
-** expressions, valid for long time intervals (Corrigendum),
-** Astron.Astrophys. 541, C1
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** Derived, with permission, from the SOFA library. See notes at end of file.
-*/
-{
-/* Obliquity at J2000.0 (radians). */
- static const double eps0 = 84381.406 * ERFA_DAS2R;
-
-/* Polynomial coefficients */
- enum { NPOL = 4 };
- static const double pqpol[2][NPOL] = {
- { 5851.607687,
- -0.1189000,
- -0.00028913,
- 0.000000101},
- {-1600.886300,
- 1.1689818,
- -0.00000020,
- -0.000000437}
- };
-
-/* Periodic coefficients */
- static const double pqper[][5] = {
- { 708.15,-5486.751211,-684.661560, 667.666730,-5523.863691},
- {2309.00, -17.127623,2446.283880,-2354.886252, -549.747450},
- {1620.00, -617.517403, 399.671049, -428.152441, -310.998056},
- { 492.20, 413.442940,-356.652376, 376.202861, 421.535876},
- {1183.00, 78.614193,-186.387003, 184.778874, -36.776172},
- { 622.00, -180.732815,-316.800070, 335.321713, -145.278396},
- { 882.00, -87.676083, 198.296701, -185.138669, -34.744450},
- { 547.00, 46.140315, 101.135679, -120.972830, 22.885731}
- };
- static const int NPER = (int) ( sizeof pqper / 5 / sizeof (double) );
-
-/* Miscellaneous */
- int i;
- double t, p, q, w, a, s, c;
-
-
-/* Centuries since J2000. */
- t = ( epj - 2000.0 ) / 100.0;
-
-/* Initialize P_A and Q_A accumulators. */
- p = 0.0;
- q = 0.0;
-
-/* Periodic terms. */
- w = ERFA_D2PI*t;
- for ( i = 0; i < NPER; i++ ) {
- a = w/pqper[i][0];
- s = sin(a);
- c = cos(a);
- p += c*pqper[i][1] + s*pqper[i][3];
- q += c*pqper[i][2] + s*pqper[i][4];
- }
-
-/* Polynomial terms. */
- w = 1.0;
- for ( i = 0; i < NPOL; i++ ) {
- p += pqpol[0][i]*w;
- q += pqpol[1][i]*w;
- w *= t;
- }
-
-/* P_A and Q_A (radians). */
- p *= ERFA_DAS2R;
- q *= ERFA_DAS2R;
-
-/* Form the ecliptic pole vector. */
- w = 1.0 - p*p - q*q;
- w = w < 0.0 ? 0.0 : sqrt(w);
- s = sin(eps0);
- c = cos(eps0);
- vec[0] = p;
- vec[1] = - q*c - w*s;
- vec[2] = - q*s + w*c;
-
-}
-/*----------------------------------------------------------------------
-**
-**
-** 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.
-**
-*/