One way to get an
spectrum is to use a hole in the specimen
to measure the incident flux in each image. Sometimes this
is not possible or desirable; in this case, one may wish to use
an incident flux spectrum that was measured in some other way.
The spectrum should be saved in a simple ASCII format
of (eV,flux in kHz) stored line-by-line, such as an Excel
comma space value .csv file, or a .xas file
(comment lines that start with
text or things like ``!'', ``#'', etc. will be ignored).
You should make sure that this file was recorded under similar
conditions, like the same slit settings, ring current, and so on.
You can of course adjust for this when you create the
file.
You can manipulate these comma, space, value .csv
files with Excel, or the read_csv.pro and
write_csv.pro routines in the X1 IDL library located
here.