Warp - warp (transform) input dataset
astwarp [OPTION...] ASTRdata
Warp is part of GNU Astronomy Utilities 0.19. Warp will resample
the pixel grid of an input image. By default (if no special linear warping
is requested), it will align the image to the WCS coordinates in anyand
remove any possible distortion. Linear warping (like '--rotate' or
'--scale') should be explicitly requested with the options under the
"Linear warps" group below.
For more information, please run any of the following commands. In
particular the second contains a very comprehensive explanation of Warp's
invocation: expected input(s), output(s), and a full description of all the
options.
- All options and their
values:
- $ astwarp -P
- Inputs/Outputs
and options:
- $ info astwarp
- Full section in
manual/book:
- $ info Warp
- Full Gnuastro
manual/book:
- $ info gnuastro
If you couldn't find your answer in the manual, you can get direct
help from experienced Gnuastro users and developers. For more information,
please run:
- $ info help-gnuastro
Warp options:
- Input:
- --hendwcs=INT
- Header keyword number to end reading WCS.
- --hstartwcs=INT
- Header keyword number to start reading WCS.
- -h,
--hdu=STR/INT
- Extension name or number of input data.
- Output:
- -C,
--coveredfrac=FLT
- Acceptable fraction of output pixel covered.
- -D,
--dontdelete
- Don't delete output if it exists.
- -k, --keepwcs
- Do not apply warp to input's WCS
- -K,
--keepinputdir
- Keep input directory for automatic output.
- -o,
--output=STR
- Output file name.
- -T,
--type=STR
- Type of output: e.g., int16, float32, etc...
- --wcslinearmatrix=STR
- WCS linear matrix of output ('pc' or 'cd').
- Align with WCS coordinates (correcting distortion, default mode)
- --checkmaxfrac
- Moire pattern: Max.frac. input pixels on output.
- --ctype=STR[,STR]
- FITS standard CTYPE value (e.g., 'RA---TAN').
- -c,
--center=FLT,FLT
- Center coordinate of the output image in RA,DEC.
- --edgesampling=INT
- Number of extra samplings in pixel sides.
- -G,
--gridfile=FITS
- File to use for output grid.
- -H,
--gridhdu=STR
- HDU/extension to use for output grid.
--widthinpix --width is in pixels, not in WCS
coordinates.
- -w,
--width=INT,INT
- Output image size in both dimensions.
- -x,
--cdelt=FLT[,FLT]
- Pixel scale of output (usually degrees/pixel).
- Linear warps (must be called explicitly on command-line)
- --centeroncorner
- Center of coordinates on first pixel corner.
- -e,
--shear=FLT[,FLT]
- Shear along the given axis(es).
- -f,
--flip=INT[,INT]
- Flip along the given axis(es).
- -m,
--matrix=STR
- Raw transformation matrix, highest priority.
- -p,
--project=FLT[,FLT]
- Project along the given axis(es).
- -r,
--rotate=FLT
- Rotate by the given angle in degrees.
- -s,
--scale=FLT[,FLT]
- Scale along the given axis(es).
- -t,
--translate=FLT[,FLT]
- Translate along the given axis(es).
- Operating modes:
- -?, --help
- give this help list
- --checkconfig
- List all config files and variables read.
- --cite
- BibTeX citation for this program.
- --config=STR
- Read configuration file STR immediately.
- --lastconfig
- Do not parse any more configuration files.
- --log
- Information about output(s) in a log file.
- --minmapsize=INT
- Min. bytes to avoid RAM automatically.
- -N,
--numthreads=INT
- Number of CPU threads to use.
- --onlyversion=STR
- Only run if the program version is STR.
- -P,
--printparams
- Print parameter values to be used and abort.
- --quietmmap
- Don't print mmap'd file's name and size.
- -q, --quiet
- Only report errors, remain quiet about steps.
- -S,
--setdirconf
- Set default values for this directory and abort.
- --usage
- give a short usage message
- -U,
--setusrconf
- Set default values for this user and abort.
- -V, --version
- print program version
Mandatory or optional arguments to long options are also mandatory
or optional for any corresponding short options.
GNU Astronomy Utilities home page:
http://www.gnu.org/software/gnuastro/
Report bugs to bug-gnuastro@gnu.org.
Copyright © 2015-2022 Free Software Foundation, Inc.
License GPLv3+: GNU General public license version 3 or later.
This is free software: you are free to change and redistribute it. There is NO
WARRANTY, to the extent permitted by law.
Written/developed by Mohammad Akhlaghi and Pedram
Ashofteh-Ardakani
The full documentation for Warp is maintained as a Texinfo
manual. If the info and Warp programs are properly installed
at your site, the command
- info Warp
should give you access to the complete manual.