Return a list of supported sky coordinate systems IRA_ISCS
By default, Equatorial and Ecliptic coordinates are referred to the mean equinox of Besselian epoch
1950.0. The calling application can override this default by appending a string known as an "
equinox
specifier"
to the end of the SCS name (in fact all IRA routines will accept any unambiguous
abbreviation of the SCS name). An equinox specifier consists of a year with upto 4 decimal places,
preceded with the letter B or J to indicate a Besselian or Julian epoch, and enclosed in parentheses. The
named coordinate system is then referred to the mean equinox of the epoch given in the equinox
specifier. The following are examples of legal SCS values; EQUATORIAL(B1950), EQUAT(J2000),
ECLIP, ECLIP(1983.2534), etc. If the date is not preceded with either B or J (as in the last example), a
Besselian epoch is assumed if the date is less than 1984.0, and a Julian epoch is assumed
otherwise.
The currently supported sky coordinate systems are:
EQUATORIAL
The longitude axis is Right Ascension, the latitude axis is Declination. Other legal names can be made by appending an equinox specifier (eg EQUATORIAL(B1983.5) ). If no equinox specifier is added, the coordinates are referred to the mean equinox of Besselian epoch 1950.0. If the equinox is described by a Besselian epoch, the old FK4 Bessel-Newcomb system is used. If a Julian epoch is used, the new IAU 1976, FK5, Fricke system is used.
GALACTIC
The longitude axis is galactic longitude and the latitude axis is galactic latitude, given in the IAU 1958 galactic coordinate system.
ECLIPTIC
The longitude axis is ecliptic longitude and the latitude axis is ecliptic latitude. Other legal names can be made by appending an equinox specifier (eg ECLIPTIC(B1983.5) ). If no equinox specifier is added, the coordinates are referred to the mean equinox of Besselian epoch 1950.0.
AZEL
The longitude axis is horizon azimuth and the latitude axis is horizon elevation.
All sky coordinate values supplied to, or returned from any IRA routine, are given in units of radians.