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After the background is found, autobk will write autobk.log,
containing a synopsis of the program inputs and outputs. An output data
file for the
found from the background removal will also be
written. There are several additional data files that can be written, each
of which contains different ways of representing data in the background
removal process. Many of these are of only diagnostic interest, but some
(especially those representing
and pre-edge subtracted
) are
quite convenient. Each optional output file has its own keyword to select
whether or not it is written. The naming conventions for the output files
will be discussed in the next section.
The most useful of the optional outputs is
, which will be written by
default (i.e. , unless you put bkgout = false in autobk.inp). This
will give the
at the same energy points as the input
data.
Outside the energy region used in the background removal (e.g. , in the
pre-edge region), this function will take the same values of the input
absorption data. The background can also be written to k -space
using bkgksp = true. The data itself can be written in
R -space (that is, after the Fourier transform with the same window
and k -weighting on
used for the background removal) using
datrsp = true. If a standard
is used in the background
removal, it can be written to k -space using theksp = true
and to R -space using thersp = true. This will contain the
standard after its amplitude has been altered in the fit.
All outputs in k -space will be written between
and
. Outputs in R -space will be written between 0 and
10.0Å. Since the Fourier Transform Window (which smoothes the data and
reduces ``ringing'' in
) used in background removal is typically
much sharper than for analysis, the R -space outputs from autobk
are not intended for general use, but only for diagnostic checks of the
background removal.