Given a set of dithering positions ('positions-cat.fits' in the example above), and an image
('image.fits' which can be from any part of the sky, only its distortion and orientation are important),
build the exposure map of the output stack after applying that dither (where each pixel contains the
number of exposures that were used in it). The field of the final stack can be set with the '--center'
and '--width' options.
astscript-pointing-simulateoptions:
Input:
-h, --hdu=STR/INT
HDU name or number of the positions catalog.
-i, --img=STR
Name of reference image.
-H, --imghdu=STR/INT
HDU name or number of the input image.
-r, --racol=STR/INT
Name/number of column containing RA.
-d, --deccol=STR/INT
Name/number of column containing Declination.
--mksrc=STR
Makefile (for developers when debugging).
Hooks:
--hook-warp-before='COMMAND' Before warping each exposure;
Input: ''. Output: ''.
--hook-warp-after='COMMAND' After warping each exposure;
Input: ''. Output: ''.
Output:
-o, --output=STR
Name of finally stacked image.
-C, --center=FLT,FLT
Center of output stack (in RA,Dec).
-w, --width=FLT,FLT
Width of output stack (in WCS).
--ctype=STR,STR
Projection of output (CTYPEi in WCS).
--widthinpix
Interpret '--width' values in pixels.
--stack-operator="STR" Arithmetic operator to use for stacking.
-t, --tmpdir=STR
Directory to keep temporary files.
-k, --keeptmp
Keep temporal/auxiliar files.
Operating mode:
-?, --help
Print this help.
-N, --numthreads=INT
Number of threads; maximum if not given.
--cite BibTeX citation for this program.
-q, --quiet
Don't print any extra information in stdout.
-V, --version
Print program version.
Mandatory or optional arguments to long options are also mandatory or optional for any corresponfing
short options.
GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/