Member cel2ter (double jd_ut1_high, double jd_ut1_low, double ut1_to_tt, enum novas_earth_rotation_measure erot, enum novas_accuracy accuracy, enum novas_equatorial_class coordType, double xp, double yp, const double *in, double *out): This function can be confusing to use due to the input coordinate system being specified by a combination of two options. Use itrs_to_cirs() or itrs_to_tod() instead. You can then follow these with other conversions to GCRS (or whatever else) as appropriate.
Member cel_pole (double jd_tt, enum novas_pole_offset_type type, double dpole1, double dpole2): This old way of incorporating Earth orientation parameters into the true equator and equinox is now disfavored. Instead, the pole offsets should be used only to convert between the Terrestrial Intermediate Reference System (TIRS) / Pseudo Earth Fixed (PEF) and the International Terrestrial Reference System (ITRS) going forward, e.g. via novas_app_to_hor() / novas_hor_to_app() or else wobble().
Member cio_array (double jd_tdb, long n_pts, ra_of_cio *restrict cio): This function is no longer used within SuperNOVAS. It is still provided, however, in order to retain 100% API compatibility with NOVAS C.
Member cio_basis (double jd_tdb, double ra_cio, enum novas_cio_location_type loc_type, enum novas_accuracy accuracy, double *restrict x, double *restrict y, double *restrict z): This function is no longer used internally in the library, and users are recommended against using it themselves, since SuperNOVAS provides better ways to convert between GCRS and CIRS using frames or via gcrs_to_cirs() / cirs_to_gcrs() or novas_transform() functions.
Member cio_location (double jd_tdb, enum novas_accuracy accuracy, double *restrict ra_cio, short *restrict loc_type): This function is no longer used internally in the library. Given that the CIO is defined on the dynamical equator of date, it is not normally meaningful to provide an R.A. coordinate for it in GCRS. Instead, you might use cio_ra() to get the CIO location w.r.t. the equinox of date (on the same dynamical equator), or equivalently ira_equinox() to return the negated value of the same.
Member equ2hor (double jd_ut1, double ut1_to_tt, enum novas_accuracy accuracy, double xp, double yp, const on_surface *restrict location, double ra, double dec, enum novas_refraction_model ref_option, double *restrict zd, double *restrict az, double *restrict rar, double *restrict decr): You should use the frame-based novas_app_to_hor() instead, or else the more explicit (less ambiguous) tod_to_itrs() followed by itrs_to_hor(), and possibly following it with an atmospheric refraction correction if appropriate.
Member local_planet (double jd_tt, const object *restrict ss_body, double ut1_to_tt, const on_surface *restrict position, enum novas_accuracy accuracy, double *restrict ra, double *restrict dec, double *restrict dis): Using the frame-based novas_sky_pos() with NOVAS_ICRS or NOVARS_GCRS as the reference system is now preferred for the equivalent calculations.
Member local_star (double jd_tt, double ut1_to_tt, const cat_entry *restrict star, const on_surface *restrict position, enum novas_accuracy accuracy, double *restrict ra, double *restrict dec): Using the frame-based novas_sky_pos() with NOVAS_ICRS or NOVARS_GCRS as the reference system is now preferred for the equivalent calculations.
Member make_object (enum novas_object_type type, long number, const char *name, const cat_entry *star, object *source): More functionality and more readable, code results from using one of the specific alternatives: make_cat_object(), make_redshifted_object(), make_planet(), make_ephem_object(), or make_orbital_object().
Member make_observer (enum novas_observer_place where, const on_surface *loc_surface, const in_space *loc_space, observer *obs): It is recommended that you use one of the more specific ways of initializing the observer data structure, e.g. with make_itrf_observer(), make_gps_observer(), make_observer_at_site(), make_airborne_observer() make_solar_system_observer(), or make_observer_at_geocenter(). This function will be available for the foreseeable future also.
Member make_observer_on_surface (double latitude, double longitude, double height, double temperature, double pressure, observer *restrict obs): This old NOVAS C function has a few too many caveats. It is recommended that you use make_itrf_observer(), make_gps_observer(), or make_observer_at_site() instead (all of which set default mean annual weather parameters for approximate refraction correction), and optionally set actual weather data afterwards, based on the measurements available. This function will be available for the foreseeable future also.
Member make_on_surface (double latitude, double longitude, double height, double temperature, double pressure, on_surface *restrict loc): This old NOVAS C function has a few too many caveats. It is recommended that you use make_itrf_site() or make_gps_site() instead (both of which set default mean annual weather parameters for approximate refraction correction), and optionally set actual weather data afterwards, based on the measurements available. This function will be available for the foreseeable future also.
Member set_cio_locator_file (const char *restrict filename): SuperNOVAS no longer uses a NOVAS-type CIO locator file, or accesses one in any way. This function is now a dummy.
Member sidereal_time (double jd_ut1_high, double jd_ut1_low, double ut1_to_tt, enum novas_equinox_type gst_type, enum novas_earth_rotation_measure erot, enum novas_accuracy accuracy, double *restrict gst): Use novas_gmst() or novas_gast() instead to get the same results simpler.
Member ter2cel (double jd_ut1_high, double jd_ut1_low, double ut1_to_tt, enum novas_earth_rotation_measure erot, enum novas_accuracy accuracy, enum novas_equatorial_class coordType, double xp, double yp, const double *in, double *out): This function can be confusing to use due to the output coordinate system being specified by a combination of two options. Use itrs_to_cirs() or itrs_to_tod() instead. You can then follow these with other conversions to GCRS (or whatever else) as appropriate.
Member topo_planet (double jd_tt, const object *restrict ss_body, double ut1_to_tt, const on_surface *restrict position, enum novas_accuracy accuracy, double *restrict ra, double *restrict dec, double *restrict dis): Using the frame-based novas_sky_pos() with NOVAS_TOD as the reference system is now preferred for topocentric calculations.
Member topo_star (double jd_tt, double ut1_to_tt, const cat_entry *restrict star, const on_surface *restrict position, enum novas_accuracy accuracy, double *restrict ra, double *restrict dec): Using the frame-based novas_sky_pos() with NOVAS_TOD as the reference system is now preferred for topocentric calculations.