Spectra extracted from local region (8° < |b|) for each model along with the respective isotropic background (brown, long-dash-dotted) and the detected sources (orange, dotted). The models are split into the three basic emis- sion components: π⁰-decay (red, long-dashed), IC (green, dashed), and bremsstrahlung (cyan, dash-dotted). All components have been scaled with parameters found from the gamma-ray fits. Also shown is the total DGE (blue, long-dash-dashed) and total emission including resolved sources and isotropic background (magenta, solid). The Fermi-LAT data are shown as points and the error bars represent the statistical errors only that are in many cases smaller than the point size. The gray region represents the systematic error in the Fermi-LAT effective area. The inset skymap in the top right corner shows the Fermi-LAT counts in the region plotted. Bottom panel shows the fractional residual (data-model)/data.

Spectra for model ^SL^Z10^R20^T∞^C2.

Spectra for model ^SL^Z10^R20^T∞^C5.

Spectra for model ^SL^Z10^R20^T150^C2.

Spectra for model ^SL^Z10^R20^T150^C5.

Spectra for model ^SL^Z10^R30^T∞^C2.

Spectra for model ^SL^Z10^R30^T∞^C5.

Spectra for model ^SL^Z10^R30^T150^C2.

Spectra for model ^SL^Z10^R30^T150^C5.

Spectra for model ^SL^Z4^R20^T∞^C2.

Spectra for model ^SL^Z4^R20^T∞^C5.

Spectra for model ^SL^Z4^R20^T150^C2.

Spectra for model ^SL^Z4^R20^T150^C5.

Spectra for model ^SL^Z4^R30^T∞^C2.

Spectra for model ^SL^Z4^R30^T∞^C5.

Spectra for model ^SL^Z4^R30^T150^C2.

Spectra for model ^SL^Z4^R30^T150^C5.

Spectra for model ^SL^Z6^R20^T∞^C2.

Spectra for model ^SL^Z6^R20^T∞^C5.

Spectra for model ^SL^Z6^R20^T150^C2.

Spectra for model ^SL^Z6^R20^T150^C5.

Spectra for model ^SL^Z6^R30^T∞^C2.

Spectra for model ^SL^Z6^R30^T∞^C5.

Spectra for model ^SL^Z6^R30^T150^C2.

Spectra for model ^SL^Z6^R30^T150^C5.

Spectra for model ^SL^Z8^R20^T∞^C2.

Spectra for model ^SL^Z8^R20^T∞^C5.

Spectra for model ^SL^Z8^R20^T150^C2.

Spectra for model ^SL^Z8^R20^T150^C5.

Spectra for model ^SL^Z8^R30^T∞^C2.

Spectra for model ^SL^Z8^R30^T∞^C5.

Spectra for model ^SL^Z8^R30^T150^C2.

Spectra for model ^SL^Z8^R30^T150^C5.

Spectra for model ^SO^Z10^R20^T∞^C2.

Spectra for model ^SO^Z10^R20^T∞^C5.

Spectra for model ^SO^Z10^R20^T150^C2.

Spectra for model ^SO^Z10^R20^T150^C5.

Spectra for model ^SO^Z10^R30^T∞^C2.

Spectra for model ^SO^Z10^R30^T∞^C5.

Spectra for model ^SO^Z10^R30^T150^C2.

Spectra for model ^SO^Z10^R30^T150^C5.

Spectra for model ^SO^Z4^R20^T∞^C2.

Spectra for model ^SO^Z4^R20^T∞^C5.

Spectra for model ^SO^Z4^R20^T150^C2.

Spectra for model ^SO^Z4^R20^T150^C5.

Spectra for model ^SO^Z4^R30^T∞^C2.

Spectra for model ^SO^Z4^R30^T∞^C5.

Spectra for model ^SO^Z4^R30^T150^C2.

Spectra for model ^SO^Z4^R30^T150^C5.

Spectra for model ^SO^Z6^R20^T∞^C2.

Spectra for model ^SO^Z6^R20^T∞^C5.

Spectra for model ^SO^Z6^R20^T150^C2.

Spectra for model ^SO^Z6^R20^T150^C5.

Spectra for model ^SO^Z6^R30^T∞^C2.

Spectra for model ^SO^Z6^R30^T∞^C5.

Spectra for model ^SO^Z6^R30^T150^C2.

Spectra for model ^SO^Z6^R30^T150^C5.

Spectra for model ^SO^Z8^R20^T∞^C2.

Spectra for model ^SO^Z8^R20^T∞^C5.

Spectra for model ^SO^Z8^R20^T150^C2.

Spectra for model ^SO^Z8^R20^T150^C5.

Spectra for model ^SO^Z8^R30^T∞^C2.

Spectra for model ^SO^Z8^R30^T∞^C5.

Spectra for model ^SO^Z8^R30^T150^C2.

Spectra for model ^SO^Z8^R30^T150^C5.

Spectra for model ^SS^Z10^R20^T∞^C2.

Spectra for model ^SS^Z10^R20^T∞^C5.

Spectra for model ^SS^Z10^R20^T150^C2.

Spectra for model ^SS^Z10^R20^T150^C5.

Spectra for model ^SS^Z10^R30^T∞^C2.

Spectra for model ^SS^Z10^R30^T∞^C5.

Spectra for model ^SS^Z10^R30^T150^C2.

Spectra for model ^SS^Z10^R30^T150^C5.

Spectra for model ^SS^Z4^R20^T∞^C2.

Spectra for model ^SS^Z4^R20^T∞^C5.

Spectra for model ^SS^Z4^R20^T150^C2.

Spectra for model ^SS^Z4^R20^T150^C5.

Spectra for model ^SS^Z4^R30^T∞^C2.

Spectra for model ^SS^Z4^R30^T∞^C5.

Spectra for model ^SS^Z4^R30^T150^C2.

Spectra for model ^SS^Z4^R30^T150^C5.

Spectra for model ^SS^Z6^R20^T∞^C2.

Spectra for model ^SS^Z6^R20^T∞^C5.

Spectra for model ^SS^Z6^R20^T150^C2.

Spectra for model ^SS^Z6^R20^T150^C5.

Spectra for model ^SS^Z6^R30^T∞^C2.

Spectra for model ^SS^Z6^R30^T∞^C5.

Spectra for model ^SS^Z6^R30^T150^C2.

Spectra for model ^SS^Z6^R30^T150^C5.

Spectra for model ^SS^Z8^R20^T∞^C2.

Spectra for model ^SS^Z8^R20^T∞^C5.

Spectra for model ^SS^Z8^R20^T150^C2.

Spectra for model ^SS^Z8^R20^T150^C5.

Spectra for model ^SS^Z8^R30^T∞^C2.

Spectra for model ^SS^Z8^R30^T∞^C5.

Spectra for model ^SS^Z8^R30^T150^C2.

Spectra for model ^SS^Z8^R30^T150^C5.

Spectra for model ^SY^Z10^R20^T∞^C2.

Spectra for model ^SY^Z10^R20^T∞^C5.

Spectra for model ^SY^Z10^R20^T150^C2.

Spectra for model ^SY^Z10^R20^T150^C5.

Spectra for model ^SY^Z10^R30^T∞^C2.

Spectra for model ^SY^Z10^R30^T∞^C5.

Spectra for model ^SY^Z10^R30^T150^C2.

Spectra for model ^SY^Z10^R30^T150^C5.

Spectra for model ^SY^Z4^R20^T∞^C2.

Spectra for model ^SY^Z4^R20^T∞^C5.

Spectra for model ^SY^Z4^R20^T150^C2.

Spectra for model ^SY^Z4^R20^T150^C5.

Spectra for model ^SY^Z4^R30^T∞^C2.

Spectra for model ^SY^Z4^R30^T∞^C5.

Spectra for model ^SY^Z4^R30^T150^C2.

Spectra for model ^SY^Z4^R30^T150^C5.

Spectra for model ^SY^Z6^R20^T∞^C2.

Spectra for model ^SY^Z6^R20^T∞^C5.

Spectra for model ^SY^Z6^R20^T150^C2.

Spectra for model ^SY^Z6^R20^T150^C5.

Spectra for model ^SY^Z6^R30^T∞^C2.

Spectra for model ^SY^Z6^R30^T∞^C5.

Spectra for model ^SY^Z6^R30^T150^C2.

Spectra for model ^SY^Z6^R30^T150^C5.

Spectra for model ^SY^Z8^R20^T∞^C2.

Spectra for model ^SY^Z8^R20^T∞^C5.

Spectra for model ^SY^Z8^R20^T150^C2.

Spectra for model ^SY^Z8^R20^T150^C5.

Spectra for model ^SY^Z8^R30^T∞^C2.

Spectra for model ^SY^Z8^R30^T∞^C5.

Spectra for model ^SY^Z8^R30^T150^C2.

Spectra for model ^SY^Z8^R30^T150^C5.

• CR spectra <download all>
  • Protons (H)
  • Helium (He)
  • Carbon (C)
  • Oxygen (O)
  • Boron over Carbon ratio (B/C)
  • Beryllium 10 over 9 ratio (¹⁰Be/⁹Be)
  • Electrons (e^-)
  • Electrons and Positrons (e^- + e⁺)
• GR spectra <download all>
  • Local region (8° < |b|)
  • Intermediate latitudes (10° < |b| < 20°)
  • North polar cap (60° < b)
  • South polar cap (-60° > b)
  • Outer Galaxy (|b| < 8° and 80° < l < 280°)
  • Inner Galaxy (|b| < 8° and -80° < l < 80°)
• GR profiles <download all>
  • Outer Galaxy latitude profile for 200 MeV – 1600 MeV (90° < l < 270°)
  • Outer Galaxy latitude profile for 1.6 GeV – 13 GeV (90° < l < 270°)
  • Outer Galaxy latitude profile for 13 GeV – 100 GeV (90° < l < 270°)
  • Latitude profile at intermediate longitudes for 200 MeV – 1600 MeV (30° < |l| < 90°)
  • Latitude profile at intermediate longitudes for 1.6 GeV – 13 GeV (30° < |l| < 90°)
  • Latitude profile at intermediate longitudes for 13 GeV – 100 GeV (30° < |l| < 90°)
  • Inner Galaxy latitude profile for 200 MeV – 1600 MeV (-30° < l < 30°)
  • Inner Galaxy latitude profile for 1.6 GeV – 13 GeV (-30° < l < 30°)
  • Inner Galaxy latitude profile for 13 GeV – 100 GeV (-30° < l < 30°)
  • Galactic plane longitude profile for 200 MeV – 1600 MeV (|b| < 5°)
  • Galactic plane longitude profile for 1.6 GeV – 13 GeV (|b| < 5°)
  • Galactic plane longitude profile for 13 GeV – 100 GeV (|b| < 5°)
  • Longitude profile at north intermediate latitudes for 200 MeV – 1600 MeV (10° < b < 20°)
  • Longitude profile at north intermediate latitudes for 1.6 GeV – 13 GeV (10° < b < 20°)
  • Longitude profile at north intermediate latitudes for 13 GeV – 100 GeV (10° < b < 20°)
  • Longitude profile at south intermediate latitudes for 200 MeV – 1600 MeV (-20° < b < -10°)
  • Longitude profile at south intermediate latitudes for 1.6 GeV – 13 GeV (-20° < b < -10°)
  • Longitude profile at south intermediate latitudes for 13 GeV – 100 GeV (-20° < b < -10°)
• GR residual maps <download all>
  • In units of standard deviation
  • Fractional, (data - model)/data
• Absolute difference between residual maps of different models <download all>
  • Compared to reference model
  • CR source distributions varied
  • Vertical halo size varied
  • Radial halo size varied
  • Spin temperature varied
  • E(B-V) magnitude cut varied
• The spectrum of the isotropic component <download all>
• Radial dependence of X_CO <download all>
• Source spectra for all 1FGL sources for all of the models. Shown on each page are for models for the combination of T_S values and E(B-V) magnitude cuts. <download all>
  • ^SS^Z4^R20
  • ^SS^Z4^R30
  • ^SS^Z6^R20
  • ^SS^Z6^R30
  • ^SS^Z8^R20
  • ^SS^Z8^R30
  • ^SS^Z10^R20
  • ^SS^Z10^R30
  • ^SL^Z4^R20
  • ^SL^Z4^R30
  • ^SL^Z6^R20
  • ^SL^Z6^R30
  • ^SL^Z8^R20
  • ^SL^Z8^R30
  • ^SL^Z10^R20
  • ^SL^Z10^R30
  • ^SY^Z4^R20
  • ^SY^Z4^R30
  • ^SY^Z6^R20
  • ^SY^Z6^R30
  • ^SY^Z8^R20
  • ^SY^Z8^R30
  • ^SY^Z10^R20
  • ^SY^Z10^R30
  • ^SO^Z4^R20
  • ^SO^Z4^R30
  • ^SO^Z6^R20
  • ^SO^Z6^R30
  • ^SO^Z8^R20
  • ^SO^Z8^R30
  • ^SO^Z10^R20
  • ^SO^Z10^R30
• GALDEF files for the runs <download all>
• Output files from the GALPROP runs
  • ^SS^Z4^R20^T150^C2
  • ^SS^Z4^R20^T150^C5
  • ^SS^Z4^R20^T∞^C2
  • ^SS^Z4^R20^T∞^C5
  • ^SS^Z4^R30^T150^C2
  • ^SS^Z4^R30^T150^C5
  • ^SS^Z4^R30^T∞^C2
  • ^SS^Z4^R30^T∞^C5
  • ^SS^Z6^R20^T150^C2
  • ^SS^Z6^R20^T150^C5
  • ^SS^Z6^R20^T∞^C2
  • ^SS^Z6^R20^T∞^C5
  • ^SS^Z6^R30^T150^C2
  • ^SS^Z6^R30^T150^C5
  • ^SS^Z6^R30^T∞^C2
  • ^SS^Z6^R30^T∞^C5
  • ^SS^Z8^R20^T150^C2
  • ^SS^Z8^R20^T150^C5
  • ^SS^Z8^R20^T∞^C2
  • ^SS^Z8^R20^T∞^C5
  • ^SS^Z8^R30^T150^C2
  • ^SS^Z8^R30^T150^C5
  • ^SS^Z8^R30^T∞^C2
  • ^SS^Z8^R30^T∞^C5
  • ^SS^Z10^R20^T150^C2
  • ^SS^Z10^R20^T150^C5
  • ^SS^Z10^R20^T∞^C2
  • ^SS^Z10^R20^T∞^C5
  • ^SS^Z10^R30^T150^C2
  • ^SS^Z10^R30^T150^C5
  • ^SS^Z10^R30^T∞^C2
  • ^SS^Z10^R30^T∞^C5
  • ^SL^Z4^R20^T150^C2
  • ^SL^Z4^R20^T150^C5
  • ^SL^Z4^R20^T∞^C2
  • ^SL^Z4^R20^T∞^C5
  • ^SL^Z4^R30^T150^C2
  • ^SL^Z4^R30^T150^C5
  • ^SL^Z4^R30^T∞^C2
  • ^SL^Z4^R30^T∞^C5
  • ^SL^Z6^R20^T150^C2
  • ^SL^Z6^R20^T150^C5
  • ^SL^Z6^R20^T∞^C2
  • ^SL^Z6^R20^T∞^C5
  • ^SL^Z6^R30^T150^C2
  • ^SL^Z6^R30^T150^C5
  • ^SL^Z6^R30^T∞^C2
  • ^SL^Z6^R30^T∞^C5
  • ^SL^Z8^R20^T150^C2
  • ^SL^Z8^R20^T150^C5
  • ^SL^Z8^R20^T∞^C2
  • ^SL^Z8^R20^T∞^C5
  • ^SL^Z8^R30^T150^C2
  • ^SL^Z8^R30^T150^C5
  • ^SL^Z8^R30^T∞^C2
  • ^SL^Z8^R30^T∞^C5
  • ^SL^Z10^R20^T150^C2
  • ^SL^Z10^R20^T150^C5
  • ^SL^Z10^R20^T∞^C2
  • ^SL^Z10^R20^T∞^C5
  • ^SL^Z10^R30^T150^C2
  • ^SL^Z10^R30^T150^C5
  • ^SL^Z10^R30^T∞^C2
  • ^SL^Z10^R30^T∞^C5
  • ^SY^Z4^R20^T150^C2
  • ^SY^Z4^R20^T150^C5
  • ^SY^Z4^R20^T∞^C2
  • ^SY^Z4^R20^T∞^C5
  • ^SY^Z4^R30^T150^C2
  • ^SY^Z4^R30^T150^C5
  • ^SY^Z4^R30^T∞^C2
  • ^SY^Z4^R30^T∞^C5
  • ^SY^Z6^R20^T150^C2
  • ^SY^Z6^R20^T150^C5
  • ^SY^Z6^R20^T∞^C2
  • ^SY^Z6^R20^T∞^C5
  • ^SY^Z6^R30^T150^C2
  • ^SY^Z6^R30^T150^C5
  • ^SY^Z6^R30^T∞^C2
  • ^SY^Z6^R30^T∞^C5
  • ^SY^Z8^R20^T150^C2
  • ^SY^Z8^R20^T150^C5
  • ^SY^Z8^R20^T∞^C2
  • ^SY^Z8^R20^T∞^C5
  • ^SY^Z8^R30^T150^C2
  • ^SY^Z8^R30^T150^C5
  • ^SY^Z8^R30^T∞^C2
  • ^SY^Z8^R30^T∞^C5
  • ^SY^Z10^R20^T150^C2
  • ^SY^Z10^R20^T150^C5
  • ^SY^Z10^R20^T∞^C2
  • ^SY^Z10^R20^T∞^C5
  • ^SY^Z10^R30^T150^C2
  • ^SY^Z10^R30^T150^C5
  • ^SY^Z10^R30^T∞^C2
  • ^SY^Z10^R30^T∞^C5
  • ^SO^Z4^R20^T150^C2
  • ^SO^Z4^R20^T150^C5
  • ^SO^Z4^R20^T∞^C2
  • ^SO^Z4^R20^T∞^C5
  • ^SO^Z4^R30^T150^C2
  • ^SO^Z4^R30^T150^C5
  • ^SO^Z4^R30^T∞^C2
  • ^SO^Z4^R30^T∞^C5
  • ^SO^Z6^R20^T150^C2
  • ^SO^Z6^R20^T150^C5
  • ^SO^Z6^R20^T∞^C2
  • ^SO^Z6^R20^T∞^C5
  • ^SO^Z6^R30^T150^C2
  • ^SO^Z6^R30^T150^C5
  • ^SO^Z6^R30^T∞^C2
  • ^SO^Z6^R30^T∞^C5
  • ^SO^Z8^R20^T150^C2
  • ^SO^Z8^R20^T150^C5
  • ^SO^Z8^R20^T∞^C2
  • ^SO^Z8^R20^T∞^C5
  • ^SO^Z8^R30^T150^C2
  • ^SO^Z8^R30^T150^C5
  • ^SO^Z8^R30^T∞^C2
  • ^SO^Z8^R30^T∞^C5
  • ^SO^Z10^R20^T150^C2
  • ^SO^Z10^R20^T150^C5
  • ^SO^Z10^R20^T∞^C2
  • ^SO^Z10^R20^T∞^C5
  • ^SO^Z10^R30^T150^C2
  • ^SO^Z10^R30^T150^C5
  • ^SO^Z10^R30^T∞^C2
  • ^SO^Z10^R30^T∞^C5