Investigating Gamma-Ray Lines from Dark Matter with Future Observatories
  We study the prospects for studying line features in gamma-ray spectra with
upcoming gamma-ray experiments, such as HESS-II, the Cherenkov Telescope Array
(CTA), and the GAMMA-400 satellite. As an example we use the narrow feature at
130 GeV seen in public data from the Fermi-LAT satellite. We found that all
three experiments should be able to confidently confirm or rule out the
presence of this 130 GeV feature. If it is real, it should be confirmed with a
confidence level higher than 5 sigma. Assuming it to be a spectral signature of
dark matter origin, GAMMA-400, thanks to a projected energy resolution of about
1.5% at 100 GeV, should also be able to resolve both the \gamma\gamma-line and
a corresponding Z\gamma- or H\gamma-feature, if the corresponding branching
ratio is comparable to that into two photons. It will also allow to distinguish
between a gamma-ray line and the similar feature resulting from internal
bremsstrahlung photons.
