CCDPACK is available for use from the IRAF command line. If it is available on your system then you should initialise it in the usual way:
and all the commands that are available will be listed. You can also get help on the commands in the usual way. A useful document to consult is SUN/217.cl> ccdpack
The way that CCDPACK commands work from the CL is pretty much as is
described in the preceeding sections, except you'll need to write your
scripts in CL and you'll also be constrained to the choice of having
to use CCDSETUP to define the CCD characteristics and
package preferences, or not having its facilities at all (all the
information about the behaviour and order of parameters through-out
this document is also largely irrelevant). If you choose to use
CCDSETUP (the default position) then you must run it to
define the values of all the ``global'' parameters used by the other
CCDPACK commands. You can spot global parameters in other commands as
they all have a [G] indicator after their descriptions. You
will not be able to set the values of these parameters by using
eparam, but you can set their values on the command-line.
If this approach is too strange for you to accept then you can switch off this behaviour by issuing the command:
immediately after initialising CCDPACK. You can achieve this effect permanently by adding the command:cc> use_globals
to your login.cl. If you have already run another CCDPACK command before using use_globals then run the flpr command to make the change propagate. Once you have switched off the use of global variables then the CCDSETUP command becomes redundant and provides no useful functions (as do CCDSHOW and CCDCLEAR). Now when you run the other commands you can eparam all parameters.set CCDPACK_GLOBALS=no
One thing that you may find a problem for large sets of data is the loss of efficiency due to the conversion processes that CCDPACK uses to access non-NDF data. To get around this you can tell CCDPACK to output its results as NDFs by using the command:
and then not adding a file extension to any output names. You can now process these new data sets much more efficiently. To get your images back into IRAF format do use a file extension type of .imh for the last stage of the processing pipeline.cc> use_ndf
CCDPACK