We now demonstrate the viable models that can fit all the available **data** for charged cosmic rays including the new FERMI and HESS data. For our analysis we fit to the PAMELA e + /(e + +e − ) **data** and the e + +e − **data** from FERMI and HESS. We also include the preliminary un-normalized PAMELA e − spectrum available at [17], although it has a minor impact. We then describe the predictions and bounds for ICS as discussed in Section 3, and include bounds from several other observations previously studied in [11,38,37,12]. These include the bounds from the HESS photon measurements in the Galactic Center and Galactic Ridge and from up-going muons measured at SuperKamiokande.