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author | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
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committer | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
commit | fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4 (patch) | |
tree | bdda434976bc09c864f2e4fa6f16ba1952b1e555 /noao/onedspec/doc/ndprep.hlp | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
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diff --git a/noao/onedspec/doc/ndprep.hlp b/noao/onedspec/doc/ndprep.hlp new file mode 100644 index 00000000..6f59ba4b --- /dev/null +++ b/noao/onedspec/doc/ndprep.hlp @@ -0,0 +1,115 @@ +.help ndprep Mar92 noao.onedspec +.ih +NAME +ndprep -- Make a neutral density filter calibration image +.ih +USAGE +ndprep filter_curve output +.ih +PARAMETERS +.ls filter_curve +Neutral density filter curve. The directory specified by the parameter +\fIdirectory\fR is prepended to this name so if a directory is specified +then it should not be given here. If '?' a list of filter curves +in the specified directory is typed. +.le +.ls output +Output neutral density filter image. +.le +.ls w0 +Starting wavelength for the output image in Angstroms. +.le +.ls dw +Wavelength increment for the output image in Angstroms. +.le +.ls nw +Number of wavelength points for the output image (i.e. the size of the +output image). +.le +.ls nspace = 0 +Number of spatial points for a two dimensional image. If the value is +zero then a one dimensional image is created. +.le +.ls logarithm = no +Use logarithmic wavelengths and intervals? If yes then the wavelengths +will have the same starting and ending points and number of pixels but +the wavelength intervals will be logarithmic. +.le +.ls flux = yes +Conserve flux when rebinning to logarithmic wavelength intervals? +.le +.ls dispaxis = 1 +Dispersion axis for two dimensional images. Dispersion along the lines +is 1 and dispersion along the columns is 2. +.le +.ls directory = "onedstds$ctio/" +Directory containing neutral density filter curves. This directory is +prepended to the specified fiter curve file (and so must end with '/' +or '$'). +.le +.ih +DESCRIPTION +A neutral density (ND) filter curve is converted to a calibration image +with the same size and wavelength range as the images to be calibrated. +A list of standard neutral density curves is typed if the filter +curve name is given as '?'. The ND curves are text files containing +wavelength and filter transmission pairs. Comments begin with '#'. +A plot of the ND curve can be obtained using \fBgraph\fR. + +The ND curve is first interpolated to a one dimensional image of +\fInw\fR wavelength points with starting wavelength \fIwO\fR and +wavelength increment \fIdw\fR using the task \fBsinterp\fR. The +wavelength parameters must be in the same units as the filter curves +(currently Angstroms) even if the final calibration image is to be in +logarithmic wavelength intervals. If logarithmic wavelength format +is specified the image is rebinned over the same wavelength range with +the same number of points using the task \fBdispcor\fR. The rebinning +may include flux conservation to account for the changing size of +pixels or simply interpolate. Note that flux conservation will +change the apparent shape of the ND curve. + +If the number of points across the dispersion, \fInspace\fR is zero then +the final calibration image is one dimensional. If it is greater than +zero the one dimensional ND image is expanded to the specified number +of spatial points with the dispersion axis specified by the parameter +\fIdispaxis\fR (1 = dispersion along the lines, 2 = dispersion along +the columns). +.ih +EXAMPLES +To get a list of standard ND filter curves: + + cl> ndprep ? + +To graph the ND filter curve: + + cl> graph onedstds$ctio/nd1m.100mag.dat + +Naturally, if a calibration image is made then the image plotting tasks +such as \fBgraph\fR, \fBimplot\fR, and \fBsplot\fR may also be used. + +To make a one dimensional ND calibration spectrum: + +.nf + cl> ndprep w0=4000 dw=1.2 nw=512 + Input ND filter curve: onedstds$ctio/nd1m.100mag.dat + Output calibration image: NDimage +.fi + +To make a two dimensional ND calibration spectrum in logarithmic wavelength: + +.nf + cl> ndprep w0=4000 dw=1.2 nw=512 nspace=200 log+ + Input ND filter curve: onedstds$ctio/nd4m.u000mag.dat + Output calibration image: NDimage +.fi +.ih +REVISIONS +.ls NDPREP V2.10 +This task was moved from the \fBproto\fR package. It was originally +written at CTIO for CTIO data. It's functionality is largely unchanged +though it has been updated for changes in the \fBonedspec\fR package. +.le +.ih +SEE ALSO +sinterp, dispcor +.endhelp |