Macros
#define	_BSD_SOURCE
	strcasecmp() feature macro for glibc <= 2.19

Functions
double	app_to_cirs_ra (double jd_tt, enum novas_accuracy accuracy, double ra)

double	cirs_to_app_ra (double jd_tt, enum novas_accuracy accuracy, double ra)

int	cirs_to_itrs (double jd_tt_high, double jd_tt_low, double ut1_to_tt, enum novas_accuracy accuracy, double xp, double yp, const double in, double out)

int	cirs_to_tod (double jd_tt, enum novas_accuracy accuracy, const double in, double out)

int	ecl2equ (double jd_tt, enum novas_equator_type coord_sys, enum novas_accuracy accuracy, double elon, double elat, double ra, double dec)

int	gal2equ (double glon, double glat, double ra, double dec)

double	get_ut1_to_tt (int leap_seconds, double dut1)

double	get_utc_to_tt (int leap_seconds)

double	grav_redshift (double M_kg, double r_m)

int	grav_undef (double jd_tdb, enum novas_accuracy accuracy, const double pos_app, const double pos_obs, double *out)

int	grav_undo_planets (const double pos_app, const double pos_obs, const novas_planet_bundle planets, double out)

int	hor_to_itrs (const on_surface location, double az, double za, double itrs)

int	itrs_to_cirs (double jd_tt_high, double jd_tt_low, double ut1_to_tt, enum novas_accuracy accuracy, double xp, double yp, const double in, double out)

int	itrs_to_hor (const on_surface location, const double itrs, double az, double za)

int	itrs_to_tod (double jd_tt_high, double jd_tt_low, double ut1_to_tt, enum novas_accuracy accuracy, double xp, double yp, const double in, double out)

int	j2000_to_gcrs (const double in, double out)

int	make_airborne_observer (const on_surface location, const double vel, observer *obs)

int	make_cat_object (const cat_entry star, object source)

int	make_ephem_object (const char name, long num, object body)

int	make_redshifted_object (const char name, double ra, double dec, double z, object source)

int	make_solar_system_observer (const double sc_pos, const double sc_vel, observer *obs)

enum novas_planet	novas_planet_for_name (const char *name)

double	novas_v2z (double vel)

double	novas_z_add (double z1, double z2)

double	novas_z_inv (double z)

int	place_cirs (double jd_tt, const object source, enum novas_accuracy accuracy, sky_pos pos)

int	place_gcrs (double jd_tt, const object source, enum novas_accuracy accuracy, sky_pos pos)

int	place_icrs (double jd_tt, const object source, enum novas_accuracy accuracy, sky_pos pos)

int	place_j2000 (double jd_tt, const object source, enum novas_accuracy accuracy, sky_pos pos)

int	place_mod (double jd_tt, const object source, enum novas_accuracy accuracy, sky_pos pos)

int	place_tod (double jd_tt, const object source, enum novas_accuracy accuracy, sky_pos pos)

double	redshift_vrad (double vrad, double z)

int	tod_to_cirs (double jd_tt, enum novas_accuracy accuracy, const double in, double out)

int	tod_to_itrs (double jd_tt_high, double jd_tt_low, double ut1_to_tt, enum novas_accuracy accuracy, double xp, double yp, const double in, double out)

double	unredshift_vrad (double vrad, double z)

Detailed Description

Date: Created on Aug 24, 2024

Author: Attila Kovacs

SuperNOVAS only functions, which are not integral to the functionality of novas.c, and thus can live in a separate, more manageably sized, module.

Function Documentation

◆ app_to_cirs_ra()

double app_to_cirs_ra	(	double	jd_tt,
		enum novas_accuracy	accuracy,
		double	ra
	)

Converts an apparent right ascension coordinate (measured from the true equinox of date) to a CIRS R.A., measured from the CIO.

Parameters

jd_tt	[day] Terrestrial Time (TT) based Julian date
accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
ra	[h] the apparent R.A. coordinate measured from the true equinox of date.

Returns: [h] The CIRS right ascension coordinate, measured from the CIO [0:24], or NAN if the accuracy is invalid, or if there wan an error from cio_ra().

See also: cirs_to_app_ra(); tod_to_cirs()

Since: 1.0.1

Author: Attila Kovacs

References cio_ra().

◆ cirs_to_app_ra()

double cirs_to_app_ra	(	double	jd_tt,
		enum novas_accuracy	accuracy,
		double	ra
	)

Converts a CIRS right ascension coordinate (measured from the CIO) to an apparent R.A. measured from the true equinox of date.

Parameters

jd_tt	[day] Terrestrial Time (TT) based Julian date
accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
ra	[h] The CIRS right ascension coordinate, measured from the CIO.

Returns: [h] the apparent R.A. coordinate measured from the true equinox of date [0:24], or NAN if the accuracy is invalid, or if there wan an error from cio_ra().

See also: app_to_cirs_ra(); cirs_to_tod()

Since: 1.0.1

Author: Attila Kovacs

References cio_ra().

◆ cirs_to_itrs()

int cirs_to_itrs	(	double	jd_tt_high,
		double	jd_tt_low,
		double	ut1_to_tt,
		enum novas_accuracy	accuracy,
		double	xp,
		double	yp,
		const double *	in,
		double *	out
	)

Rotates a position vector from the dynamical CIRS frame of date to the Earth-fixed ITRS frame (IAU 2000 standard method).

If both 'xp' and 'yp' are set to 0 no polar motion is included in the transformation.

If extreme (sub-microarcsecond) accuracy is not required, you can use UT1-based Julian date instead of the TT-based Julian date and set the 'ut1_to_tt' argument to 0.0. and you can use UTC-based Julian date the same way.for arcsec-level precision also.

REFERENCES:

Kaplan, G. H. et. al. (1989). Astron. Journ. 97, 1197-1210.
Kaplan, G. H. (2003), 'Another Look at Non-Rotating Origins', Proceedings of IAU XXV Joint Discussion 16.

Parameters

	jd_tt_high	[day] High-order part of Terrestrial Time (TT) based Julian date.
	jd_tt_low	[day] Low-order part of Terrestrial Time (TT) based Julian date.
	ut1_to_tt	[s] TT - UT1 Time difference in seconds
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
	xp	[arcsec] Conventionally-defined X coordinate of celestial intermediate pole with respect to ITRS pole, in arcseconds.
	yp	[arcsec] Conventionally-defined Y coordinate of celestial intermediate pole with respect to ITRS pole, in arcseconds.
	in	Position vector, geocentric equatorial rectangular coordinates, referred to CIRS axes (celestial system).
[out]	out	Position vector, geocentric equatorial rectangular coordinates, referred to ITRS axes (terrestrial system).

Returns: 0 if successful, -1 if either of the vector arguments is NULL, 1 if 'accuracy' is invalid, 2 if 'method' is invalid 10–20, 3 if the method and option are mutually incompatible, or else 10 + the error from cio_location(), or 20 + error from cio_basis().

See also: tod_to_itrs(); itrs_to_cirs(); gcrs_to_cirs(); cirs_to_gcrs(); cirs_to_tod()

Since: 1.0

Author: Attila Kovacs

References cel2ter(), EROT_ERA, and NOVAS_DYNAMICAL_CLASS.

◆ cirs_to_tod()

int cirs_to_tod	(	double	jd_tt,
		enum novas_accuracy	accuracy,
		const double *	in,
		double *	out
	)

Transforms a rectangular equatorial (x, y, z) vector from the Celestial Intermediate Reference System (CIRS) at the given epoch to the True of Date (TOD) reference system.

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date that defines the output epoch. Typically it does not require much precision, and Julian dates in other time measures will be unlikely to affect the result
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
	in	CIRS Input (x, y, z) position or velocity vector
[out]	out	Output position or velocity 3-vector in the True of Date (TOD) frame. It can be the same vector as the input.

Returns: 0 if successful, or -1 if either of the vector arguments is NULL or the accuracy is invalid, or 10 + the error from cio_location(), or else 20 + the error from cio_basis().

See also: tod_to_cirs(); cirs_to_app_ra(); cirs_to_gcrs(); cirs_to_itrs()

Since: 1.1

Author: Attila Kovacs

References cio_ra(), and spin().

◆ ecl2equ()

int ecl2equ	(	double	jd_tt,
		enum novas_equator_type	coord_sys,
		enum novas_accuracy	accuracy,
		double	elon,
		double	elat,
		double *	ra,
		double *	dec
	)

Convert ecliptic longitude and latitude to right ascension and declination. To convert GCRS ecliptic coordinates (mean ecliptic and equinox of J2000.0), set 'coord_sys' to NOVAS_GCRS_EQUATOR(2); in this case the value of 'jd_tt' can be set to anything, since J2000.0 is assumed. Otherwise, all input coordinates are dynamical at'jd_tt'.

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date. (Unused if 'coord_sys' is NOVAS_GCRS_EQUATOR[2])
	coord_sys	The astrometric reference system of the coordinates. If 'coord_sys' is NOVAS_GCRS_EQUATOR(2), the input GCRS coordinates are converted to J2000 ecliptic coordinates.
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
	elon	[deg] Ecliptic longitude in degrees, referred to specified ecliptic and equinox of date.
	elat	[deg] Ecliptic latitude in degrees, referred to specified ecliptic and equinox of date.
[out]	ra	[h] Right ascension in hours, referred to specified equator and equinox of date.
[out]	dec	[deg] Declination in degrees, referred to specified equator and equinox of date.

Returns: 0 if successful, or else 1 if the value of 'coord_sys' is invalid.

See also: ecl2equ_vec(); equ2ecl()

Since: 1.0

Author: Attila Kovacs

References ecl2equ_vec().

◆ gal2equ()

int gal2equ	(	double	glon,
		double	glat,
		double *	ra,
		double *	dec
	)

Converts galactic longitude and latitude to ICRS right ascension and declination.

REFERENCES:

Hipparcos and Tycho Catalogues, Vol. 1, Section 1.5.3.

Parameters

	glon	[deg] Galactic longitude in degrees.
	glat	[deg] Galactic latitude in degrees.
[out]	ra	[h] ICRS right ascension in hours.
[out]	dec	[deg] ICRS declination in degrees.

Returns: 0 if successful, or -1 if either of the output pointer arguments are NULL.

See also: equ2gal()

Since: 1.0

Author: Attila Kovacs

◆ get_ut1_to_tt()

double get_ut1_to_tt	(	int	leap_seconds,
		double	dut1
	)

Returns the TT - UT1 time difference given the leap seconds and the actual UT1 - UTC time difference as measured and published by IERS.

NOTES:

The current UT1 - UTC time difference, and polar offsets, historical data and near-term projections are published in the <a href="https://www.iers.org/IERS/EN/Publications/Bulletins/bulletins.html>IERS Bulletins

Parameters

leap_seconds	[s] Leap seconds at the time of observations
dut1	[s] UT1 - UTC time difference [-0.5:0.5]

Returns: [s] The TT - UT1 time difference that is suitable for used with all calls in this library that require a ut1_to_tt argument.

See also: get_utc_to_tt(); place(); cel_pole()

Since: 1.0

Author: Attila Kovacs

References get_utc_to_tt().

◆ get_utc_to_tt()

double get_utc_to_tt ( int leap_seconds )

Returns the difference between Terrestrial Time (TT) and Universal Coordinated Time (UTC)

Parameters

leap_seconds [s] The current leap seconds (see IERS Bulletins)

Returns: [s] The TT - UTC time difference

See also: get_ut1_to_tt(); julian_date()

Since: 1.0

Author: Attila Kovacs

References NOVAS_TAI_TO_TT.

◆ grav_redshift()

double grav_redshift	(	double	M_kg,
		double	r_m
	)

Returns the gravitational redshift (z) for light emitted near a massive spherical body at some distance from its center, and observed at some very large (infinite) distance away.

Parameters

M_kg	[kg] Mass of gravitating body that is contained inside the emitting radius.
r_m	[m] Radius at which light is emitted.

Returns: The gravitational redshift (z) for an observer at very large (infinite) distance from the gravitating body.

See also: redshift_vrad(); unredshift_vrad(); novas_z_add()

Since: 1.2

Author: Attila Kovacs

References C.

◆ grav_undef()

int grav_undef	(	double	jd_tdb,
		enum novas_accuracy	accuracy,
		const double *	pos_app,
		const double *	pos_obs,
		double *	out
	)

Computes the gravitationally undeflected position of an observed source position due to the major gravitating bodies in the solar system. This function valid for an observed body within the solar system as well as for a star.

If 'accuracy' is set to zero (full accuracy), three bodies (Sun, Jupiter, and Saturn) are used in the calculation. If the reduced-accuracy option is set, only the Sun is used in the calculation. In both cases, if the observer is not at the geocenter, the deflection due to the Earth is included.

The number of bodies used at full and reduced accuracy can be set by making a change to the code in this function as indicated in the comments.

REFERENCES:

Klioner, S. (2003), Astronomical Journal 125, 1580-1597, Section 6.

Parameters

	jd_tdb	[day] Barycentric Dynamical Time (TDB) based Julian date
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
	pos_app	[AU] Apparent position 3-vector of observed object, with respect to origin at observer (or the geocenter), referred to ICRS axes, components in AU.
	pos_obs	[AU] Position 3-vector of observer (or the geocenter), with respect to origin at solar system barycenter, referred to ICRS axes, components in AU.
[out]	out	[AU] Nominal position vector of observed object, with respect to origin at observer (or the geocenter), referred to ICRS axes, without gravitational deflection, components in AU. It can be the same vector as the input, but not the same as pos_obs.

Returns: 0 if successful, -1 if any of the pointer arguments is NULL (errno = EINVAL) or if the result did not converge (errno = ECANCELED), or else an error from obs_planets().

See also: grav_def(); novas_app_to_geom(); set_planet_provider(); set_planet_provider_hp(); grav_bodies_full_accuracy; grav_bodies_reduced_accuracy

Since: 1.1

Author: Attila Kovacs

References grav_bodies_full_accuracy, grav_bodies_reduced_accuracy, grav_undo_planets(), NOVAS_FULL_ACCURACY, and obs_planets().

◆ grav_undo_planets()

int grav_undo_planets	(	const double *	pos_app,
		const double *	pos_obs,
		const novas_planet_bundle *	planets,
		double *	out
	)

Computes the gravitationally undeflected position of an observed source position due to the specified Solar-system bodies.

REFERENCES:

Klioner, S. (2003), Astronomical Journal 125, 1580-1597, Section 6.

Parameters

	pos_app	[AU] Apparent position 3-vector of observed object, with respect to origin at observer (or the geocenter), referred to ICRS axes, components in AU.
	pos_obs	[AU] Position 3-vector of observer (or the geocenter), with respect to origin at solar system barycenter, referred to ICRS axes, components in AU.
	planets	Apparent planet data containing positions and velocities for the major gravitating bodies in the solar-system.
[out]	out	[AU] Nominal position vector of observed object, with respect to origin at observer (or the geocenter), referred to ICRS axes, without gravitational deflection, components in AU. It can be the same vector as the input, but not the same as pos_obs.

Returns: 0 if successful, -1 if any of the pointer arguments is NULL.

See also: obs_planets(); grav_planets(); novas_app_to_geom()

Since: 1.1

Author: Attila Kovacs

References grav_planets(), and novas_inv_max_iter.

◆ hor_to_itrs()

int hor_to_itrs	(	const on_surface *	location,
		double	az,
		double	za,
		double *	itrs
	)

Converts astrometric (unrefracted) azimuth and zenith angles at the specified observer location to a unit position vector in the Earth-fixed ITRS frame.

Parameters

	location	Observer location on Earth
	az	[deg] astrometric azimuth angle at observer location [0:360]. It may be NULL if not required.
	za	[deg] astrometric zenith angle at observer location [0:180]. It may be NULL if not required.
[out]	itrs	Unit 3-vector direction in Earth-fixed ITRS frame

Returns: 0 if successful, or else -1 if the location or the input vector is NULL.

See also: itrs_to_hor(); itrs_to_cirs(); itrs_to_tod(); refract()

Since: 1.0

Author: Attila Kovacs

References on_surface::latitude, and on_surface::longitude.

◆ itrs_to_cirs()

int itrs_to_cirs	(	double	jd_tt_high,
		double	jd_tt_low,
		double	ut1_to_tt,
		enum novas_accuracy	accuracy,
		double	xp,
		double	yp,
		const double *	in,
		double *	out
	)

Rotates a position vector from the Earth-fixed ITRS frame to the dynamical CIRS frame of date (IAU 2000 standard method).

If both 'xp' and 'yp' are set to 0 no polar motion is included in the transformation.

If extreme (sub-microarcsecond) accuracy is not required, you can use UT1-based Julian date instead of the TT-based Julian date and set the 'ut1_to_tt' argument to 0.0. and you can use UTC-based Julian date the same way.for arcsec-level precision also.

REFERENCES:

Kaplan, G. H. et. al. (1989). Astron. Journ. 97, 1197-1210.
Kaplan, G. H. (2003), 'Another Look at Non-Rotating Origins', Proceedings of IAU XXV Joint Discussion 16.

Parameters

	jd_tt_high	[day] High-order part of Terrestrial Time (TT) based Julian date.
	jd_tt_low	[day] Low-order part of Terrestrial Time (TT) based Julian date.
	ut1_to_tt	[s] TT - UT1 Time difference in seconds
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
	xp	[arcsec] Conventionally-defined X coordinate of celestial intermediate pole with respect to ITRS pole, in arcseconds.
	yp	[arcsec] Conventionally-defined Y coordinate of celestial intermediate pole with respect to ITRS pole, in arcseconds.
	in	Position vector, geocentric equatorial rectangular coordinates, referred to ITRS axes (terrestrial system)
[out]	out	Position vector, geocentric equatorial rectangular coordinates, referred to CIRS axes (celestial system).

Returns: 0 if successful, -1 if either of the vector arguments is NULL, 1 if 'accuracy' is invalid, or else 10 + the error from cio_location(), or 20 + error from cio_basis().

See also: itrs_to_tod(); cirs_to_itrs(); cirs_to_gcrs()

Since: 1.0

Author: Attila Kovacs

References EROT_ERA, NOVAS_DYNAMICAL_CLASS, and ter2cel().

◆ itrs_to_hor()

int itrs_to_hor	(	const on_surface *	location,
		const double *	itrs,
		double *	az,
		double *	za
	)

Converts a position vector in the Earth-fixed ITRS frame to astrometric (unrefracted) azimuth and zenith angles at the specified observer location.

Parameters

	location	Observer location on Earth
	itrs	3-vector position in Earth-fixed ITRS frame
[out]	az	[deg] astrometric azimuth angle at observer location [0:360]. It may be NULL if not required.
[out]	za	[deg] astrometric zenith angle at observer location [0:180]. It may be NULL if not required.

Returns: 0 if successful, or else -1 if the location or the input vector is NULL.

See also: hor_to_itrs(); cirs_to_itrs(); tod_to_itrs(); refract_astro()

Since: 1.0

Author: Attila Kovacs

References on_surface::latitude, and on_surface::longitude.

◆ itrs_to_tod()

int itrs_to_tod	(	double	jd_tt_high,
		double	jd_tt_low,
		double	ut1_to_tt,
		enum novas_accuracy	accuracy,
		double	xp,
		double	yp,
		const double *	in,
		double *	out
	)

Rotates a position vector from the Earth-fixed ITRS frame to the dynamical True of Date (TOD) frame of date (pre IAU 2000 method).

If both 'xp' and 'yp' are set to 0 no polar motion is included in the transformation.

If extreme (sub-microarcsecond) accuracy is not required, you can use UT1-based Julian date instead of the TT-based Julian date and set the 'ut1_to_tt' argument to 0.0. and you can use UTC-based Julian date the same way.for arcsec-level precision also.

REFERENCES:

Kaplan, G. H. et. al. (1989). Astron. Journ. 97, 1197-1210.
Kaplan, G. H. (2003), 'Another Look at Non-Rotating Origins', Proceedings of IAU XXV Joint Discussion 16.

Parameters

	jd_tt_high	[day] High-order part of Terrestrial Time (TT) based Julian date.
	jd_tt_low	[day] Low-order part of Terrestrial Time (TT) based Julian date.
	ut1_to_tt	[s] TT - UT1 Time difference in seconds
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
	xp	[arcsec] Conventionally-defined X coordinate of celestial intermediate pole with respect to ITRS pole, in arcseconds.
	yp	[arcsec] Conventionally-defined Y coordinate of celestial intermediate pole with respect to ITRS pole, in arcseconds.
	in	Position vector, geocentric equatorial rectangular coordinates, referred to ITRS axes (terrestrial system)
[out]	out	Position vector, geocentric equatorial rectangular coordinates, referred to True of Date (TOD) axes (celestial system)

Returns: 0 if successful, -1 if either of the vector arguments is NULL, 1 if 'accuracy' is invalid, or else 10 + the error from cio_location(), or 20 + error from cio_basis().

See also: itrs_to_cirs(); tod_to_itrs(); tod_to_j2000()

Since: 1.0

Author: Attila Kovacs

References EROT_GST, NOVAS_DYNAMICAL_CLASS, and ter2cel().

◆ j2000_to_gcrs()

int j2000_to_gcrs	(	const double *	in,
		double *	out
	)

Change J2000 coordinates to GCRS coordinates. Same as frame_tie() called with J2000_TO_ICRS

Parameters

	in	J2000 input 3-vector
[out]	out	GCRS output 3-vector

Returns: 0 if successful, or else an error from frame_tie()

See also: j2000_to_tod(); gcrs_to_j2000()

Since: 1.0

Author: Attila Kovacs

References frame_tie(), and J2000_TO_ICRS.

◆ make_airborne_observer()

int make_airborne_observer	(	const on_surface *	location,
		const double *	vel,
		observer *	obs
	)

Populates an 'observer' data structure for an observer moving relative to the surface of Earth, such as an airborne observer. Airborne observers have an earth fixed momentary location, defined by longitude, latitude, and altitude, the same was as for a stationary observer on Earth, but are moving relative to the surface, such as in an aircraft or balloon observatory.

Parameters

	location	Current longitude, latitude and altitude, and local weather (temperature and pressure)
	vel	[km/s] Surface velocity.
[out]	obs	Pointer to data structure to populate.

Returns: 0 if successful, or -1 if the output argument is NULL.

See also: make_observer_at geocenter(); make_observer_in_space(); make_observer_on_surface(); make_solar_system_observer(); novas_calc_geometric_position(); place()

Since: 1.1

Author: Attila Kovacs

References IN_SPACE_INIT, make_observer(), NOVAS_AIRBORNE_OBSERVER, and in_space::sc_vel.

◆ make_cat_object()

int make_cat_object	(	const cat_entry *	star,
		object *	source
	)

Populates and object data structure with the data for a catalog source.

Parameters

	star	Pointer to structure to populate with the catalog data for a celestial object located outside the solar system.
[out]	source	Pointer to the celestial object data structure to be populated.

Returns: 0 if successful, or -1 if 'cel_obj' is NULL or when type is NOVAS_CATALOG_OBJECT and 'star' is NULL, or else 1 if 'type' is invalid, 2 if 'number' is out of legal range or 5 if 'name' is too long.

See also: make_cat_entry(); make_planet(); make_ephem_object(); place()

Since: 1.1

Author: Attila Kovacs

References make_object(), NOVAS_CATALOG_OBJECT, cat_entry::starname, and cat_entry::starnumber.

◆ make_ephem_object()

int make_ephem_object	(	const char *	name,
		long	num,
		object *	body
	)

Sets a celestial object to be a Solar-system ephemeris body. Typically this would be used to define minor planets, asteroids, comets and planetary satellites.

Parameters

	name	Name of object. By default converted to upper-case, unless novas_case_sensitive() was called with a non-zero argument. Max. SIZE_OF_OBJ_NAME long, including termination. If the ephemeris provider uses names, then the name should match those of the ephemeris provider – otherwise it is not important.
	num	Solar-system body ID number (e.g. NAIF). The number should match the needs of the ephemeris provider used with NOVAS. (If the ephemeris provider is by name and not ID number, then the number here is not important).
[out]	body	Pointer to structure to populate.

Returns: 0 if successful, or else -1 if the 'planet' pointer is NULL or the name is too long.

See also: set_ephem_provider(); make_planet(); make_cat_entry(); place()

Since: 1.0

Author: Attila Kovacs

References make_object(), and NOVAS_EPHEM_OBJECT.

◆ make_redshifted_object()

int make_redshifted_object	(	const char *	name,
		double	ra,
		double	dec,
		double	z,
		object *	source
	)

Populates a celestial object data structure with the parameters for a redhifted catalog source, such as a distant quasar or galaxy. It is similar to make_cat_object() except that it takes a Doppler-shift (z) instead of radial velocity and it assumes no parallax and no proper motion (appropriately for a distant redshifted source). The catalog name is set to EXT to indicate an extragalactic source, and the catalog number defaults to 0. The user may change these default field values as appropriate afterwards, if necessary.

Parameters

	name	Object name (less than SIZE_OF_OBJ_NAME in length). It may be NULL.
	ra	[h] Right ascension of the object (hours).
	dec	[deg] Declination of the object (degrees).
	z	Redhift value (λ_obs / λ_rest - 1 = f_rest / f_obs - 1).
[out]	source	Pointer to structure to populate.

Returns: 0 if successful, or 5 if 'name' is too long, else -1 if the 'source' pointer is NULL.

See also: make_cat_object(); novas_v2z()

Since: 1.2

Author: Attila Kovacs

References make_cat_entry(), make_cat_object(), and novas_z2v().

◆ make_solar_system_observer()

int make_solar_system_observer	(	const double *	sc_pos,
		const double *	sc_vel,
		observer *	obs
	)

Populates an 'observer' data structure, for an observer situated on a near-Earth spacecraft, with the specified geocentric position and velocity vectors. Solar-system observers are similar to observers in Earth-orbit but their momentary position and velocity is defined relative to the Solar System Barycenter, instead of the geocenter.

Parameters

	sc_pos	[AU] Solar-system barycentric (x, y, z) position vector in ICRS.
	sc_vel	[AU/day] Solar-system barycentric (x, y, z) velocity vector in ICRS.
[out]	obs	Pointer to the data structure to populate

Returns: 0 if successful, or -1 if the output argument is NULL.

See also: make_observer_in_space(); make_observer_on_surface(); make_observer_at_geocenter(); make_airborne_observer(); novas_calc_geometric_position(); place()

Since: 1.1

Author: Attila Kovacs

References make_in_space(), make_observer(), and NOVAS_SOLAR_SYSTEM_OBSERVER.

◆ novas_planet_for_name()

enum novas_planet novas_planet_for_name ( const char * name )

Returns the NOVAS planet ID for a given name (case insensitive), or -1 if no match is found.

Parameters

name	The planet name, or that for the "Sun", "Moon" or "SSB" (case insensitive). The spelled out "Solar System Barycenter" is also recognized with either spaces, hyphens ('-') or underscores ('_') separating the case insensitive words.

Returns: The NOVAS major planet ID, or -1 (errno set to EINVAL) if the input name is NULL or if there is no match for the name provided.

Author: Attila Kovacs

Since: 1.2

See also: make_planet()

References NOVAS_PLANET_NAMES_INIT, NOVAS_PLANETS, and NOVAS_SSB.

◆ novas_v2z()

double novas_v2z ( double vel )

Converts a radial recession velocity to a redshift value (z = δf / f_rest). It is based on the relativistic formula:

 1 + z = sqrt((1 + β) / (1 - β))

where β = v / c.

Parameters

vel	[km/s] velocity (i.e. rate) of recession.

Returns: the corresponding redshift value (δλ / λ_rest), or NAN if the input velocity is invalid (i.e., it exceeds the speed of light).

See also: novas_z2v(); novas_z_add()

Author: Attila Kovacs

Since: 1.2

References C.

◆ novas_z_add()

double novas_z_add	(	double	z1,
		double	z2
	)

Compounds two redshift corrections, e.g. to apply (or undo) a series gravitational redshift corrections and/or corrections for a moving observer. It's effectively using (1 + z) = (1 + z1) * (1 + z2).

Parameters

z1	One of the redshift values
z2	The other redshift value

Returns: The compound redshift value, ot NAN if either input redshift is invalid (errno will be set to EINVAL).

See also: grav_redshift(); redshift_vrad(); unredshift_vrad()

Since: 1.2

Author: Attila Kovacs

◆ novas_z_inv()

double novas_z_inv ( double z )

Returns the inverse of a redshift value, that is the redshift for a body moving with the same velocity as the original but in the opposite direction.

Parameters

z	A redhift value

Returns: The redshift value for a body moving in the opposite direction with the same speed, or NAN if the input redshift is invalid.

See also: novas_z_add()

Since: 1.2

Author: Attila Kovacs

◆ place_cirs()

int place_cirs	(	double	jd_tt,
		const object *	source,
		enum novas_accuracy	accuracy,
		sky_pos *	pos
	)

Computes the Celestial Intermediate Reference System (CIRS) dynamical position position of a source as 'seen' from the geocenter at the given time of observation. See place() for more information.

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date of observation.
	source	Catalog source or solar_system body.
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
[out]	pos	Structure to populate with the calculated CIRS position data

Returns: 0 if successful, or -1 if any of the input pointer arguments is NULL, or else an error from place().

See also: place_tod(); place_gcrs()

Since: 1.0

Author: Attila Kovacs

References NOVAS_CIRS, and place().

◆ place_gcrs()

int place_gcrs	(	double	jd_tt,
		const object *	source,
		enum novas_accuracy	accuracy,
		sky_pos *	pos
	)

Computes the Geocentric Celestial Reference System (GCRS) position of a source (as 'seen' from the geocenter) at the given time of observation. Unlike place_icrs(), this includes aberration for the moving frame of the geocenter as well as gravitational deflections calculated for a virtual observer located at the geocenter. See place() for more information.

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date of observation.
	source	Catalog source or solar_system body.
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
[out]	pos	Structure to populate with the calculated GCRS position data

Returns: 0 if successful, or -1 if any of the input pointer arguments is NULL, or else an error from place().

See also: place_icrs(); place_cirs(); place_tod(); virtual_star(); virtual_planet()

Since: 1.0

Author: Attila Kovacs

References NOVAS_GCRS, and place().

◆ place_icrs()

int place_icrs	(	double	jd_tt,
		const object *	source,
		enum novas_accuracy	accuracy,
		sky_pos *	pos
	)

Computes the International Celestial Reference System (ICRS) position of a source. (from the geocenter). Unlike place_gcrs(), this version does not include aberration or gravitational deflection corrections.

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date of observation.
	source	Catalog source or solar_system body.
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
[out]	pos	Structure to populate with the calculated geocentric ICRS position data (Unlike place_gcrs(), the calculated coordinates do not account for aberration or gravitational deflection).

Returns: 0 if successful, or -1 if any of the input pointer arguments is NULL, or else an error from place().

See also: place_gcrs(); place_cirs(); place_tod(); mean_star()

Since: 1.0

Author: Attila Kovacs

References NOVAS_ICRS, and place().

◆ place_j2000()

int place_j2000	(	double	jd_tt,
		const object *	source,
		enum novas_accuracy	accuracy,
		sky_pos *	pos
	)

Computes the J2000 dynamical position position of a source as 'seen' from the geocenter at the given time of observation. See place() for more information.

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date of observation.
	source	Catalog source or solar_system body.
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
[out]	pos	Structure to populate with the calculated CIRS position data

Returns: 0 if successful, or -1 if any of the input pointer arguments is NULL, or else an error from place().

See also: place_cirs(); place_gcrs(); app_star(); app_planet()

Since: 1.1

Author: Attila Kovacs

References NOVAS_J2000, and place().

◆ place_mod()

int place_mod	(	double	jd_tt,
		const object *	source,
		enum novas_accuracy	accuracy,
		sky_pos *	pos
	)

Computes the Mean of Date (MOD) dynamical position position of a source as 'seen' from the geocenter at the given time of observation. See place() for more information.

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date of observation.
	source	Catalog source or solar_system body.
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
[out]	pos	Structure to populate with the calculated CIRS position data

Returns: 0 if successful, or -1 if any of the input pointer arguments is NULL, or else an error from place().

See also: place_cirs(); place_gcrs(); app_star(); app_planet()

Since: 1.1

Author: Attila Kovacs

References NOVAS_MOD, and place().

◆ place_tod()

int place_tod	(	double	jd_tt,
		const object *	source,
		enum novas_accuracy	accuracy,
		sky_pos *	pos
	)

Computes the True of Date (TOD) dynamical position position of a source as 'seen' from the geocenter at the given time of observation. See place() for more information.

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date of observation.
	source	Catalog source or solar_system body.
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
[out]	pos	Structure to populate with the calculated CIRS position data

Returns: 0 if successful, or -1 if any of the input pointer arguments is NULL, or else an error from place().

See also: place_cirs(); place_gcrs(); app_star(); app_planet()

Since: 1.0

Author: Attila Kovacs

References NOVAS_TOD, and place().

◆ redshift_vrad()

double redshift_vrad	(	double	vrad,
		double	z
	)

Applies an incremental redshift correction to a radial velocity. For example, you may use this function to correct a radial velocity calculated by rad_vel() or rad_vel2() for a Solar-system body to account for the gravitational redshift for light originating at a specific distance away from the body. For the Sun, you may want to undo the redshift correction applied for the photosphere using unredshift_vrad() first.

Parameters

vrad	[km/s] Radial velocity
z	Redshift correction to apply

Returns: [km/s] The redshift corrected radial velocity or NAN if the redshift value is invalid (errno will be set to EINVAL).

See also: unredshift_vrad(); grav_redshift(); novas_z_add()

Since: 1.2

Author: Attila Kovacs

References novas_v2z(), and novas_z2v().

◆ tod_to_cirs()

int tod_to_cirs	(	double	jd_tt,
		enum novas_accuracy	accuracy,
		const double *	in,
		double *	out
	)

Transforms a rectangular equatorial (x, y, z) vector from the True of Date (TOD) reference system to the Celestial Intermediate Reference System (CIRS) at the given epoch to the .

Parameters

	jd_tt	[day] Terrestrial Time (TT) based Julian date that defines the output epoch. Typically it does not require much precision, and Julian dates in other time measures will be unlikely to affect the result
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
	in	CIRS Input (x, y, z) position or velocity vector
[out]	out	Output position or velocity 3-vector in the True of Date (TOD) frame. It can be the same vector as the input.

Returns: 0 if successful, or -1 if either of the vector arguments is NULL or the accuracy is invalid, or 10 + the error from cio_location(), or else 20 + the error from cio_basis().

See also: cirs_to_tod(); app_to_cirs_ra(); tod_to_gcrs(); tod_to_j2000(); tod_to_itrs()

Since: 1.1

Author: Attila Kovacs

References cio_ra(), and spin().

◆ tod_to_itrs()

int tod_to_itrs	(	double	jd_tt_high,
		double	jd_tt_low,
		double	ut1_to_tt,
		enum novas_accuracy	accuracy,
		double	xp,
		double	yp,
		const double *	in,
		double *	out
	)

Rotates a position vector from the dynamical True of Date (TOD) frame of date the Earth-fixed ITRS frame (pre IAU 2000 method).

If both 'xp' and 'yp' are set to 0 no polar motion is included in the transformation.

If extreme (sub-microarcsecond) accuracy is not required, you can use UT1-based Julian date instead of the TT-based Julian date and set the 'ut1_to_tt' argument to 0.0. and you can use UTC-based Julian date the same way.for arcsec-level precision also.

REFERENCES:

Kaplan, G. H. et. al. (1989). Astron. Journ. 97, 1197-1210.
Kaplan, G. H. (2003), 'Another Look at Non-Rotating Origins', Proceedings of IAU XXV Joint Discussion 16.

Parameters

	jd_tt_high	[day] High-order part of Terrestrial Time (TT) based Julian date.
	jd_tt_low	[day] Low-order part of Terrestrial Time (TT) based Julian date.
	ut1_to_tt	[s] TT - UT1 Time difference in seconds.
	accuracy	NOVAS_FULL_ACCURACY (0) or NOVAS_REDUCED_ACCURACY (1)
	xp	[arcsec] Conventionally-defined X coordinate of celestial intermediate pole with respect to ITRS pole, in arcseconds.
	yp	[arcsec] Conventionally-defined Y coordinate of celestial intermediate pole with respect to ITRS pole, in arcseconds.
	in	Position vector, geocentric equatorial rectangular coordinates, referred to True of Date (TOD) axes (celestial system).
[out]	out	Position vector, geocentric equatorial rectangular coordinates, referred to ITRS axes (terrestrial system).

Returns: 0 if successful, -1 if either of the vector arguments is NULL, 1 if 'accuracy' is invalid, 2 if 'method' is invalid 10–20, 3 if the method and option are mutually incompatible, or else 10 + the error from cio_location(), or 20 + error from cio_basis().

See also: cirs_to_itrs(); itrs_to_tod(); j2000_to_tod(); tod_to_gcrs(); tod_to_j2000(); tod_to_cirs()

Since: 1.0

Author: Attila Kovacs

References cel2ter(), EROT_GST, and NOVAS_DYNAMICAL_CLASS.

◆ unredshift_vrad()

double unredshift_vrad	(	double	vrad,
		double	z
	)

Undoes an incremental redshift correction that was applied to radial velocity.

Parameters

vrad	[km/s] Radial velocity
z	Redshift correction to apply

Returns: [km/s] The radial velocity without the redshift correction or NAN if the redshift value is invalid. (errno will be set to EINVAL)

See also: redshift_vrad(); grav_redshift()

Since: 1.2

Author: Attila Kovacs

References novas_v2z(), and novas_z2v().

Macros

Functions

Detailed Description

Function Documentation

◆ app_to_cirs_ra()

◆ cirs_to_app_ra()

◆ cirs_to_itrs()

◆ cirs_to_tod()

◆ ecl2equ()

◆ gal2equ()

◆ get_ut1_to_tt()

◆ get_utc_to_tt()

◆ grav_redshift()

◆ grav_undef()

◆ grav_undo_planets()

◆ hor_to_itrs()

◆ itrs_to_cirs()

◆ itrs_to_hor()

◆ itrs_to_tod()

◆ j2000_to_gcrs()

◆ make_airborne_observer()

◆ make_cat_object()

◆ make_ephem_object()

◆ make_redshifted_object()

◆ make_solar_system_observer()

◆ novas_planet_for_name()

◆ novas_v2z()

◆ novas_z_add()

◆ novas_z_inv()

◆ place_cirs()

◆ place_gcrs()

◆ place_icrs()

◆ place_j2000()

◆ place_mod()

◆ place_tod()

◆ redshift_vrad()

◆ tod_to_cirs()

◆ tod_to_itrs()

◆ unredshift_vrad()