From a5b18b816b64efef905359fcf2a61a82c9e0379d Mon Sep 17 00:00:00 2001 From: Attila Kovacs Date: Fri, 10 Jan 2025 14:48:47 +0100 Subject: [PATCH] API docs tweaks and site update --- src/frames.c | 5 ++++- 1 file changed, 4 insertions(+), 1 deletion(-) diff --git a/src/frames.c b/src/frames.c index 1956555b..bdd62424 100644 --- a/src/frames.c +++ b/src/frames.c @@ -587,7 +587,9 @@ int novas_geom_posvel(const object *source, const novas_frame *frame, enum novas *
  • If `sys` is `NOVAS_TOD` (true equator and equinox of date), the less precise old (pre IAU * 2006) method is used, with the Lieske et al. 1977 nutation model, matching the behavior of the * original NOVAS C place() for that system. To obtain more precise TOD coordinates, set `sys` to - * `NOVAS_CIRS` here, and follow with cirs_to_tod() after.
    • + * `NOVAS_CIRS` here, and follow with cirs_to_tod() / cirs_to_app_ra() on the `out->r_hat` / + * `out->ra` respectively after (or you can use just convert one of the quantities, and use + * radec2vector() or vector2radec() to get the other even faster). * * * @param object Pointer to a celestial object data structure that is observed @@ -604,6 +606,7 @@ int novas_geom_posvel(const object *source, const novas_frame *frame, enum novas * @sa novas_app_to_hor() * @sa place() * @sa cirs_to_tod() + * @sa cirs_to_app_ra() * * @since 1.1 * @author Attila Kovacs