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-#include "erfa.h"
-
-void eraLtecm(double epj, double rm[3][3])
-/*
-** - - - - - - - - -
-** e r a L t e c m
-** - - - - - - - - -
-**
-** ICRS equatorial to ecliptic rotation matrix, long-term.
-**
-** Given:
-** epj double Julian epoch (TT)
-**
-** Returned:
-** rm double[3][3] ICRS to ecliptic rotation matrix
-**
-** Notes:
-**
-** 1) The matrix is in the sense
-**
-** E_ep = rm x P_ICRS,
-**
-** where P_ICRS is a vector with respect to ICRS right ascension
-** and declination axes and E_ep is the same vector with respect to
-** the (inertial) ecliptic and equinox of epoch epj.
-**
-** 2) P_ICRS is a free vector, merely a direction, typically of unit
-** magnitude, and not bound to any particular spatial origin, such
-** as the Earth, Sun or SSB. No assumptions are made about whether
-** it represents starlight and embodies astrometric effects such as
-** parallax or aberration. The transformation is approximately that
-** between mean J2000.0 right ascension and declination and ecliptic
-** longitude and latitude, with only frame bias (always less than
-** 25 mas) to disturb this classical picture.
-**
-** 3) 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.
-**
-** Called:
-** eraLtpequ equator pole, long term
-** eraLtpecl ecliptic pole, long term
-** eraPxp vector product
-** eraPn normalize vector
-**
-** 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.
-*/
-{
-/* Frame bias (IERS Conventions 2010, Eqs. 5.21 and 5.33) */
- const double dx = -0.016617 * ERFA_DAS2R,
- de = -0.0068192 * ERFA_DAS2R,
- dr = -0.0146 * ERFA_DAS2R;
-
- double p[3], z[3], w[3], s, x[3], y[3];
-
-
-/* Equator pole. */
- eraLtpequ(epj, p);
-
-/* Ecliptic pole (bottom row of equatorial to ecliptic matrix). */
- eraLtpecl(epj, z);
-
-/* Equinox (top row of matrix). */
- eraPxp(p, z, w);
- eraPn(w, &s, x);
-
-/* Middle row of matrix. */
- eraPxp(z, x, y);
-
-/* Combine with frame bias. */
- rm[0][0] = x[0] - x[1]*dr + x[2]*dx;
- rm[0][1] = x[0]*dr + x[1] + x[2]*de;
- rm[0][2] = - x[0]*dx - x[1]*de + x[2];
- rm[1][0] = y[0] - y[1]*dr + y[2]*dx;
- rm[1][1] = y[0]*dr + y[1] + y[2]*de;
- rm[1][2] = - y[0]*dx - y[1]*de + y[2];
- rm[2][0] = z[0] - z[1]*dr + z[2]*dx;
- rm[2][1] = z[0]*dr + z[1] + z[2]*de;
- rm[2][2] = - z[0]*dx - z[1]*de + z[2];
-
-}
-/*----------------------------------------------------------------------
-**
-**
-** 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.
-**
-*/