The GLS/radio projection in details
The AIPS memo 46 defines the global-sinusoidal projection (GLS)
in its section 2.3, which writes as
In this case, there is no rotation of the 2D plane compared to the
celestial system (e.g. ICRS).
are the celestial
coordinates, and
the coordinates of the
reference point. This can not be described in the CG02 formalism,
which makes this projection obsolete for writing in new FITS files.
Fortunately, the GLS projection at any declination and no rotation is
equivalent to a CG02 compliant Sanson-Flamsteed (SFL) projection at
zero declination (i.e. on the Equator)4. It is therefore possible to
recast a cube in GLS projection as a cube in SFL projection just by
patching the header and without any change on the data! The
demonstration and the exact translation to be performed are detailed
in the appendix section A.3. The Fig. 2
gives a visual representation of these transformations.
Figure:
Visual representation of the GLS-to-SFL
transformation. In all the plots, the grey region covers the
same area on sky. Top left: the grey region symbolizes
a
square degrees in the
2D AIPS-GLS
projected plane. Blue lines show the abscissa and ordinate
origins. There is no transformation possible to go to a native
sphere in the CG02 formalism. Top right: the reference
point is shifted to the Equator, i.e. by a
shift
(
in this example). The equations now match the
FITS-SFL formalism at
. Bottom left: the
area is SFL-unprojected to
spherical coordinates
on the 3D native sphere. The equator and zero reference meridian
are shown in green. The fiducial point
of
the SFL projection has coordinates
by
design. Bottom right: the whole sky orientation is kept
the same as before, but the coordinate system represented is now
the 3D celestial sphere. The equator and zero reference meridian
are shown in red.
is
in this example.
![\includegraphics[width=0.9\textwidth]{greg-projections-gls2sfl}](img26.svg) |