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use crateltecm;
use crate;
/// Transformation from ecliptic coordinates (mean equinox and ecliptic
/// of date) to ICRS RA,Dec, using a long-term precession model.
///
/// Status: support function.
///
/// Given:
/// epj f64 Julian epoch (TT)
/// dl,db f64 ecliptic longitude and latitude (radians)
///
/// Returned:
/// dr,dd f64 ICRS right ascension and declination (radians)
///
/// Notes:
///
/// 1) No assumptions are made about whether the coordinates represent
/// starlight and embody astrometric effects such as parallax or
/// aberration.
///
/// 2) The transformation is approximately that from ecliptic longitude
/// and latitude (mean equinox and ecliptic of date) to mean J2000.0
/// right ascension and declination, 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
/// is used. It 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:
/// s2c spherical coordinates to unit vector
/// ltecm ICRS to ecliptic rotation matrix, long-term
/// trxp product of transpose of r-matrix and p-vector
/// c2s unit vector to spherical coordinates
/// anp normalize angle into range 0 to 2pi
/// anpm normalize angle into range +/- pi