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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/imred/generic/doc/darksub.hlp | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
Initial commit
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-rw-r--r-- | noao/imred/generic/doc/darksub.hlp | 60 |
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diff --git a/noao/imred/generic/doc/darksub.hlp b/noao/imred/generic/doc/darksub.hlp new file mode 100644 index 00000000..c6349e03 --- /dev/null +++ b/noao/imred/generic/doc/darksub.hlp @@ -0,0 +1,60 @@ +.help darksub Apr86 noao.imred.generic +.ih +NAME +darksub -- Scale and subtract a dark count image +.ih +USAGE +darksub input output darkimage +.ih +PARAMETERS +.ls input +List of input images from which to subtract the dark count image. +.le +.ls output +List of output dark count subtracted images. The output images may +be the same as the input images. The input and output image lists should +contain the same number of images. +.le +.ls darkimage +Dark count image to be scaled and subtracted from the input images. +.le +.ls exposure = "" +Header parameter name from which to obtain the exposure times. +.le +.ls pixtype = "1" +The pixel datatype of the dark subtracted images. The default ("1") +is the pixel datatype of the original image. The other choices are +"short", "integer", "long", "real", and "double". +.le +.ls verbose = yes +Print log of operations performed. +.le +.ih +DESCRIPTION +The dark count image is scaled by the ratio of the input image exposure to the +dark count image exposure and subtracted from each of the input images. +The exposures are obtained from the image headers under the specified +name. The output images may have the same names as the input images. +A temporary image is used for the scaled dark count image and the original +image is not modified. The pixel datatype of the output images is +specified by the parameter \fIpixtype\fR. The default ("1") uses the +datatype of the input image. A log of the operations performed may be +printed on the standard output when the verbose options is specified. + +Note that this task can be used to subtract any type of image from a set +of images in which the subtracted image must be scaled to a given exposure. +.ih +EXAMPLES +To subtract the dark count image 'dark' from obs1, obs2, and obs3: + +.nf + cl> darksub obs1,obs2 obs1,obs2 dark exp="exposure" + Tue 18:50:56 08-Apr-86 + obs1 = obs1 - 5.0049997336067 * dark + Tue 18:51:05 08-Apr-86 + obs2 = obs2 - 5.009999733075 * dark +.fi +.ih +SEE ALSO +imarith +.endhelp |