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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /noao/onedspec/doc/specshift.hlp | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'noao/onedspec/doc/specshift.hlp')
-rw-r--r-- | noao/onedspec/doc/specshift.hlp | 67 |
1 files changed, 67 insertions, 0 deletions
diff --git a/noao/onedspec/doc/specshift.hlp b/noao/onedspec/doc/specshift.hlp new file mode 100644 index 00000000..c72ebd0a --- /dev/null +++ b/noao/onedspec/doc/specshift.hlp @@ -0,0 +1,67 @@ +.help specshift Oct92 noao.onedspec +.ih +NAME +specshift -- Shift dispersion coordinate systems +.ih +USAGE +specshift spectra shift +.ih +PARAMETERS +.ls spectra +List of spectra to be modified. +.le +.ls shift +Dispersion coordinate shift to be added to the current dispersion coordinate +system. +.le +.ls apertures = "" +List of apertures to be modified. The null list +selects all apertures. A list consists of comma separated +numbers and ranges of numbers. A range is specified by a hyphen. An +optional step size may be given by using the 'x' followed by a number. +See \fBxtools.ranges\fR for more information. This parameter is ignored +for N-dimensional spatial spectra such as long slit and Fabry-Perot. +.le +.ls verbose = no +Print a record of each aperture modified? +.le +.ih +DESCRIPTION +This task applies a shift to the dispersion coordinate system of selected +spectra. The image data is not modified as with \fBimshift\fR but rather +the coordinate system is shifted relative to the data. The spectra to be +modified are selected by specifying a list of images and apertures. If no +aperture list is specified then all apertures in the images are modified. +For N-dimensional spatial spectra such as long slit and Fabry-Perot the +aperture list is ignored. + +The specified shift is added to the existing world coordinates. For linear +coordinate systems this has the effect of modifying CRVAL1, for linear +"multispec" coordinate systems this modifies the dispersion coordinate of +the first physical pixel, and for nonlinear "multispec" coordinate systems +this modifies the shift coefficient(s). + +It is also possible to shift the linearized coordinate systems (but not the +nonlinear coordinate systems) with \fBsapertures\fR or possibly with +\fBwcsedit\fR or \fBhedit\fR if the coordinate system is stored with a +global linear system. + +The \fIverbose\fR parameter lists the images, the apertures, the shift, and +the old and new values for the first physical pixel are printed. +.ih +EXAMPLES +1. To add 1.23 Angstroms to the coordinates of all apertures in the +image "ngc456.ms": + +.nf + cl> specshift ngc456.ms 1.23 +.fi +.ih +REVISIONS +.ls SPECSHIFT V2.10.3 +First version. +.le +.ih +SEE ALSO +sapertures, dopcor, imcoords.wcsreset, hedit, ranges, onedspec.package +.endhelp |