Move doc to SuperNOVAS.home repo

README.md

@@ -42,7 +42,7 @@ The primary goals of SuperNOVAS is to improve on the stock NOVAS C library by:
  - Fixing [outstanding issues](#fixed-issues)
  - Improving the ease of use by using `enum`s instead of integer constants, which also allows for some checking
    of use during compilations (such as using the incorrect `enum` type).
- - Improving [API documentation](https://smithsonian.github.io/supernovas.github.io/apidoc/html/) with 
+ - Improving [API documentation](https://smithsonian.github.io/SuperNOVAS.home/apidoc/html/) with 
    [Doxygen](https://www.doxygen.nl/) to provide browsable cross-referenced API docs. 
  - Streamlining calculations where possible
  - Adding `const` modifier to prototype arguments where appropriate
@@ -74,9 +74,9 @@ Outside contributions are very welcome. See how you can contribute
 
 Here are some links to SupeNOVAS related content online:
 
- - [API Documentation](https://smithsonian.github.io/supernovas.github.io/apidoc/html/)
+ - [API Documentation](https://smithsonian.github.io/SuperNOVAS.home/apidoc/html/)
  - [Project site](https://github.com/Smithsonian/SuperNOVAS/) on GitHUB. 
- - [SuperNOVAS page](https://smithsonian.github.io/supernovas.github.io) page on github.io. 
+ - [SuperNOVAS page](https://smithsonian.github.io/SuperNOVAS.home) page on github.io. 
  - [How to Contribute](https://github.com/Smithsonian/SuperNOVAS/CONTRIBUTING.md) guide
  - The [NOVAS](https://aa.usno.navy.mil/software/novas_info) home page at the US Naval Observatory.
  - The [NOVAS C](https://aa.usno.navy.mil/software/novasc_intro) library page. 
@@ -135,7 +135,7 @@ practical considerations before that level of accuracy is reached.
     small irregular variations in the orientation of the rotational axis and the rotation period, which are referred to 
     as the polar wobble. The [IERS Bulletins](https://www.iers.org/IERS/EN/Publications/Bulletins/bulletins.html) 
     provide up-to-date measurements, historical data and  and near-term projections for the polar offsets and the 
-    UT1-UTC time difference and leap-seconds. In SuperNOVAS you can use `cel_pole()` and `ut1_to_tt()` functions to 
+    UT1-UTC time difference and leap-seconds. In SuperNOVAS you can use `cel_pole()` and `get_ut1_to_tt()` functions to 
     apply / use the published values from these to improve the astrometic precision of calls such as `calc_pos()`, or 
     `topo_star()`. Without setting and using the polar offset parameters, positions for Earth-based observations will
     be accurate at the arcsecond level only.

include/novas.h

@@ -672,7 +672,7 @@ int radec2vector(double ra, double dec, double dist, double *vector);
 
 int starvectors(const cat_entry *star, double *pos, double *vel);
 
-double ut1_to_tt(int leap_seconds, double dut1);
+double get_ut12tt(int leap_seconds, double dut1);
 
 int tdb2tt(double tdb_jd, double *tt_jd, double *secdiff);
 

src/novas.c

@@ -356,7 +356,7 @@ int set_planet_calc_hp(novas_planet_calculator_hp f) {
  *
  * @sa calc_planet_pos()
  * @sa calc_star_pos()
- * @sa ut1_to_tt()
+ * @sa get_ut1_to_tt()
  *
  *
  * @author Attila Kovacs
@@ -445,7 +445,7 @@ int calc_frame_pos(const object *source, const astro_frame *frame, enum novas_ac
  *                  is invalid, or an error code <10 if from function place().
  *
  * @sa calc_frame_pos()
- * @sa ut1_to_tt()
+ * @sa get_ut1_to_tt()
  *
  * @author Attila Kovacs
  * @since 1.0
@@ -748,7 +748,7 @@ short astro_planet(double jd_tt, const object *ss_body, enum novas_accuracy accu
  * @sa topo_star()
  * @sa virtual_star()
  * @sa astro_planet()
- * @sa ut1_to_tt()
+ * @sa get_ut1_to_tt()
  */
 short topo_star(double jd_tt, double ut1_to_tt, const cat_entry *star, const on_surface *position, enum novas_accuracy accuracy,
         double *ra, double *dec) {
@@ -791,7 +791,7 @@ short topo_star(double jd_tt, double ut1_to_tt, const cat_entry *star, const on_
  * @sa topo_star()
  * @sa virtual_star()
  * @sa astro_planet()
- * @sa ut1_to_tt()
+ * @sa get_ut1_to_tt()
  */
 short local_star(double jd_tt, double ut1_to_tt, const cat_entry *star, const on_surface *position, enum novas_accuracy accuracy,
         double *ra, double *dec) {
@@ -833,7 +833,7 @@ short local_star(double jd_tt, double ut1_to_tt, const cat_entry *star, const on
  * @sa topo_planet()
  * @sa virtual_planet()
  * @sa astro_star()
- * @sa ut1_to_tt()
+ * @sa get_ut1_to_tt()
  */
 short topo_planet(double jd_tt, const object *ss_body, double ut1_to_tt, const on_surface *position, enum novas_accuracy accuracy,
         double *ra, double *dec, double *dis) {
@@ -875,7 +875,7 @@ short topo_planet(double jd_tt, const object *ss_body, double ut1_to_tt, const o
  * @sa topo_planet()
  * @sa virtual_planet()
  * @sa app_star()
- * @sa ut1_to_tt()
+ * @sa get_ut1_to_tt()
  */
 short local_planet(double jd_tt, const object *ss_body, double ut1_to_tt, const on_surface *position, enum novas_accuracy accuracy,
         double *ra, double *dec, double *dis) {
@@ -1023,7 +1023,7 @@ short mean_star(double jd_tt, double ra, double dec, enum novas_accuracy accurac
  *                      80--90 errro is 80 + error from cio_location(), 90--100 error is 90 + error from cio_basis().
  *
  * @sa cel_pole()
- * @sa ut1_to_tt()
+ * @sa get_ut1_to_tt()
  */
 short place(double jd_tt, const object *cel_object, const observer *location, double ut1_to_tt, enum novas_reference_system coord_sys,
         enum novas_accuracy accuracy, sky_pos *output) {
@@ -2390,7 +2390,7 @@ int e_tilt(double jd_tdb, enum novas_accuracy accuracy, double *mobl, double *to
  * @return          0 if successful, or else 1 if 'type' is invalid.
  *
  *
- * @sa ut1_to_tt()
+ * @sa get_ut1_to_tt()
  */
 short cel_pole(double tjd, enum novas_pole_offset_type type, double dpole1, double dpole2) {
   double dx, dy, t, mean_ob, sin_e, x, dz, dp1[3], dp2[3], dp3[3];
@@ -3902,14 +3902,14 @@ int starvectors(const cat_entry *star, double *pos, double *vel) {
  * @param leap_seconds  [s] Leap seconds at gthe time of observations
  * @param dut1          [s] UT1 - UTC time difference [-0.5:0.5]
  * @return              [s] The TT - UT1 time difference that is suitable for used with all
- *                      calls in this library that require a <code>ut12tt</code> argument.
+ *                      calls in this library that require a <code>ut1_to_tt</code> argument.
  *
  * @sa cel_pole()
  *
  * @since 1.0
  * @author Attila Kovacs
  */
-double ut1_to_tt(int leap_seconds, double dut1) {
+double get_ut1_to_tt(int leap_seconds, double dut1) {
   return NOVAS_TAI_TO_TT + leap_seconds + dut1;
 }