Speaker
Dr
Viviana Niro
(IFT UAM/CSIS and UAM)
Description
In this talk, I'll show how updated information from gamma-rays experiments constrain the spectrum of the galactic sources previously detected by the Milagro collaboration.
I'll show the number of through-going muons expected from these sources at the IceCube detector and I'll discuss the statistical significance of each source as a function of the detector running time.
Moreover, I'll show also the constrains that could be set on the cut-off
energy and spectral index of the Milagro sources.
Primary author
Dr
Viviana Niro
(IFT UAM/CSIS and UAM)
