PRINT: Print Data Files, Spectra, or Image Subsections
- Form: PRINT [data keywords] [output redirection]
-
- data keywords
- specify which information is printed
PRINT will print out a formatted listing of reduced data, spectra or image
subsections. The output from PRINT appears on your terminal; to send it to
a file use the '
filename' construct. PRINT recognizes the following
keywords:
- object [BOX=n]
- Print out the pixel values of object (in
the subsection specified by box 'n'). If the object is a
wavelength- calibrated spectrum, the wavelengths will be printed.
- PRINT 1 BOX=2
- PRINT $Q BOX=4
imagesec.dat
- BOXES
- Print out the sizes, centers, and origins of all boxes
defined.
- PROF [MEDIAN] [MAG] [SPIRAL]
- Print out the surface
photometry profile. If the MEDIAN keyword is specified, the median
surface brightnesses, rather than the mean, will be printed. If the
MAG keyword is specified, the surface brightnesses and total counts
will be output in magnitude units. If the SPIRAL keyword is given
(for SPIRAL galaxies), then some extra information, like the disk
scale length, disk/tot, etc. will be printed - if these values have
been computed using CORRECT.
- PRINT PROFILE
- PRINT PROFILE
prof.dat
- PHOT [BRIEF]
- Print out the stellar photometry results.
BRIEF produces a short listing.
- PRINT PHOT
- PRINT PHOT BRIEF
- PRINT PHOT
photlist.dat
- APER
- Print out the aperture photometry results.
- PRINT APER
- PRINT APER
aperlist.dat
- DIRECTORIES
- Print the default directories.
- PRINT DIRECTORIES
- PRINT DIRECTORIES
dirs.dat
- IMAGES or SPECTRA
- Print headers for images or spectra in the
default directory. (Use PRINT DIRECTORIES to see which directory
this is)
- PRINT IMAGES
- PRINT SPECTRA
imlist.dat
- LINEID
- Print wavelength v. pixel identifications obtained
with the LINEID command.
- PRINT LINEID
- PRINT LINEID
lines.dat
- STRINGS
- Print all defines strings. See the command STRING
to define strings.
- PRINT STRINGS
- PRINT STRINGS
string.txt