| -a [name]: | Filename format for data files. Must be a string corresponding to the format of sscanf(). The default is "data/w%05d.fits". |
|---|---|
| -c [star]: | Aperture center follows this star. Default is 0. When -M or -C option is used default is 1. |
| -d [sec]: | Delay between processing frames. Default is 0. |
| -f [name]: | Search string for flat field images. Default is "flat*.fits". The string should contain a "*", and must (therefore) be in double quotes. |
| -i [iter]: | Number of iterations for MAP mode. Defaults to 1. |
| -l [name]: | Name for log file. Default is rtp.log |
| -m [nsig]: | In sky level processing, exclude pixels that deviate more than [nsig] sigma from mean value. Default is 3.0. |
| -n [num]: | Start processing at frame number [num]. Default is 0. |
| -o [name]: | Name of the target object. Default is picked from the FITS headers. |
| -r [rad]: | Aperture radius in pixels. Default is the maximum that will fit in the window. |
| -s [size]: | Size of sky annulus in pixels from the edge of the window. Default is 4. |
| -t [size]: | Sky field to use for the sky subtraction. Default is 1 (first in list). |
| -x [size]: | Aperture x-position. Defaults to the centre (excluding the first three bad columns. |
| -y [size]: | Aperture y-position. Defaults to centre |
| -z [size]: | Number of sky fields. Defaults to 1. |
| -B: | Batch mode processing. Generate output file and terminate. |
|---|---|
| -C: | Compute and save centering parameters. |
| -D: | Debug mode on. Will generate files of aperture masks etc. |
| -M: | Moving apertures. |
| -O: | Individual offsets for all stars. |
| -P: | Polarimetry mode. Assumes that input targets are in polarimetric pairs, and generates output files with corresponding differences. |
| -R: | Compute differential photometry in scaled differences instead of ratio. |
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Last modified: Monday, 31-Apr-2001 12:08:31 ACT