XMM-Newton Science Analysis System
sp_partial (esas-0.9.28) [xmmsas_20131209_1901-13.5.0]
This task uses information from the spectral fit of a limited region
of the detector and from the full field-of-view to scale the fitted SP
normalization of the limited region to be appropriate for the full FOV.
This is useful for the case where bright diffuse emission in part of the FOV
may be affecting the SP spectral fit, many clusters of galaxies for example.
XMM-Newton SOC/SSC -- 2013-12-09