PAW (Physics Analysis
Workstation) is a CERN
application used to analyze and plot data. There is a full writeup
on PAW available from CERN (see the "PAW" link above), as well as a "help"
command in PAW, but you generally have to have an idea of the command
you're looking for before the official documentation is of much use.
Also, there is a very comprehensive
PAW home page at CERN which contains almost all of the information
found here, and much, much more.
The example kumac file given below will introduce you to some common
PAW commands.
Note: To run paw, you need to "setup cern", and execute "pawX11".
PAW commands are organized in a tree structure. For example
tgroup/sgroup/command {arguments}
means execute the command command in the subgroup sgroup
of the top group tgroup. If command is unique among all groups
and subgroups, it is not necessary to specify the group:
command {arguments}.
There are several means of organizing and manipulating data in PAW:
Every PAW command can be executed in a command file called a KUMAC. (Kuip
MACROS).
See this
example, which is also a very basic PAW tutorial.
An important macro is .pawlogon.kumac in your home directory,
which executes your favorite commands each time you start a PAW session.
Another useful macro is last.kumac, which is created by PAW, and
contains a record of the commands executed in each session.
Please read the MACRO section of the online PAW help and PAW documentation.
See the help for the option and the set commands for information on setting attributes such as the size and font of histogram titles, whether to use logarithmic or linear axes, etc. There is a very useful graphical display of these attributes in the PAW FAQ and the PAW documentation.
To make a hard copy, do the following:
fort/file lun {filename.ps} - open a file on logical
unit lun. (The logical unit is similar to a file descriptor, but
you choose it. It's a number from 1 to 99.) The filename doesn't
have to end in .ps, but it's a good idea since it will be a postscript
file.
meta lun - make the file you just opened as a postscript meta
file.
Make your plots.
close lun - close the meta file.
You are now ready to view the file with ghostview or send it to a
printer.