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.

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.

PHOT [BRIEF]
Print out the stellar photometry results. BRIEF produces a short listing.

APER
Print out the aperture photometry results.

DIRECTORIES
Print the default directories.

IMAGES or SPECTRA
Print headers for images or spectra in the default directory. (Use PRINT DIRECTORIES to see which directory this is)

LINEID
Print wavelength v. pixel identifications obtained with the LINEID command.

STRINGS
Print all defines strings. See the command STRING to define strings.