Calibration Access and Data Handbook
Previous: Generation from Ground Calibration
It is not expected to update these CCF files on the short term, neither
is there a dedicated calibration activity.
However on the longterm it will be possible to estimate the diffuse
background components (DGL and Zodiacal light).
Background levels of individual science observations can be stored as
function of galactic longitude and latitude (l,b), the helioecliptic
and filter passband.
The two background components can be disentangled in this