python gen_trans.py filter_name filter.res [atm.res qe.res ....]
filter_name is the name which will identify that filter for all
subsequent
uses of BPZ, (e.g F814W_WFPC2)
filter.res is the filter response per lambda in \AA
atm.res, qe.res are the atmosphere transmission, the CCD QE and
any
other correction which modifies the total throughput of the
telescope
as a funcion of wavelenght. This files don't need to have the
same
resolution or wavelenght coverage as the filter response. If
their
units are not in \AA, the program queries the user for the conversion
factor. The original files containing this information are modified
to
include the new wavelenght units. A safety copy (e.g. qe.res.bak)
is saved just in case.