INTEGRAL
Source Results page
As an example of the use of INTEGRAL Source Results page, produce the
lightcurves a Seyfert galaxy Mrk 3 in 20-40 and 40-80 keV energy bands.
Find the average spectrum of the source by summing up the spectra from
different revolutions. Fit it to a cutoff powerlaw model and see if
INTEGRAL detects the high-energy cut-off in the source spectrum. Find
the 20-100 keV flux of the source.
Determine the significance of source detection in 20-100 keV energy
interval.