X_CO Radial Profile

Radial dependence of the determined X_CO values. We do not show the values in the outer Galaxy as they are strongly biased.

Radial dependence of X_CO values for models ^SL^Z10^R20^T150^C2 (black X), ^SL^Z10^R20^T150^C5 (blue squares), ^SL^Z10^R20^T∞^C2 (red circles), and ^SL^Z10^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SL^Z10^R30^T150^C2 (black X), ^SL^Z10^R30^T150^C5 (blue squares), ^SL^Z10^R30^T∞^C2 (red circles), and ^SL^Z10^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SL^Z4^R20^T150^C2 (black X), ^SL^Z4^R20^T150^C5 (blue squares), ^SL^Z4^R20^T∞^C2 (red circles), and ^SL^Z4^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SL^Z4^R30^T150^C2 (black X), ^SL^Z4^R30^T150^C5 (blue squares), ^SL^Z4^R30^T∞^C2 (red circles), and ^SL^Z4^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SL^Z6^R20^T150^C2 (black X), ^SL^Z6^R20^T150^C5 (blue squares), ^SL^Z6^R20^T∞^C2 (red circles), and ^SL^Z6^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SL^Z6^R30^T150^C2 (black X), ^SL^Z6^R30^T150^C5 (blue squares), ^SL^Z6^R30^T∞^C2 (red circles), and ^SL^Z6^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SL^Z8^R20^T150^C2 (black X), ^SL^Z8^R20^T150^C5 (blue squares), ^SL^Z8^R20^T∞^C2 (red circles), and ^SL^Z8^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SL^Z8^R30^T150^C2 (black X), ^SL^Z8^R30^T150^C5 (blue squares), ^SL^Z8^R30^T∞^C2 (red circles), and ^SL^Z8^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SO^Z10^R20^T150^C2 (black X), ^SO^Z10^R20^T150^C5 (blue squares), ^SO^Z10^R20^T∞^C2 (red circles), and ^SO^Z10^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SO^Z10^R30^T150^C2 (black X), ^SO^Z10^R30^T150^C5 (blue squares), ^SO^Z10^R30^T∞^C2 (red circles), and ^SO^Z10^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SO^Z4^R20^T150^C2 (black X), ^SO^Z4^R20^T150^C5 (blue squares), ^SO^Z4^R20^T∞^C2 (red circles), and ^SO^Z4^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SO^Z4^R30^T150^C2 (black X), ^SO^Z4^R30^T150^C5 (blue squares), ^SO^Z4^R30^T∞^C2 (red circles), and ^SO^Z4^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SO^Z6^R20^T150^C2 (black X), ^SO^Z6^R20^T150^C5 (blue squares), ^SO^Z6^R20^T∞^C2 (red circles), and ^SO^Z6^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SO^Z6^R30^T150^C2 (black X), ^SO^Z6^R30^T150^C5 (blue squares), ^SO^Z6^R30^T∞^C2 (red circles), and ^SO^Z6^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SO^Z8^R20^T150^C2 (black X), ^SO^Z8^R20^T150^C5 (blue squares), ^SO^Z8^R20^T∞^C2 (red circles), and ^SO^Z8^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SO^Z8^R30^T150^C2 (black X), ^SO^Z8^R30^T150^C5 (blue squares), ^SO^Z8^R30^T∞^C2 (red circles), and ^SO^Z8^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SS^Z10^R20^T150^C2 (black X), ^SS^Z10^R20^T150^C5 (blue squares), ^SS^Z10^R20^T∞^C2 (red circles), and ^SS^Z10^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SS^Z10^R30^T150^C2 (black X), ^SS^Z10^R30^T150^C5 (blue squares), ^SS^Z10^R30^T∞^C2 (red circles), and ^SS^Z10^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SS^Z4^R20^T150^C2 (black X), ^SS^Z4^R20^T150^C5 (blue squares), ^SS^Z4^R20^T∞^C2 (red circles), and ^SS^Z4^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SS^Z4^R30^T150^C2 (black X), ^SS^Z4^R30^T150^C5 (blue squares), ^SS^Z4^R30^T∞^C2 (red circles), and ^SS^Z4^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SS^Z6^R20^T150^C2 (black X), ^SS^Z6^R20^T150^C5 (blue squares), ^SS^Z6^R20^T∞^C2 (red circles), and ^SS^Z6^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SS^Z6^R30^T150^C2 (black X), ^SS^Z6^R30^T150^C5 (blue squares), ^SS^Z6^R30^T∞^C2 (red circles), and ^SS^Z6^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SS^Z8^R20^T150^C2 (black X), ^SS^Z8^R20^T150^C5 (blue squares), ^SS^Z8^R20^T∞^C2 (red circles), and ^SS^Z8^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SS^Z8^R30^T150^C2 (black X), ^SS^Z8^R30^T150^C5 (blue squares), ^SS^Z8^R30^T∞^C2 (red circles), and ^SS^Z8^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SY^Z10^R20^T150^C2 (black X), ^SY^Z10^R20^T150^C5 (blue squares), ^SY^Z10^R20^T∞^C2 (red circles), and ^SY^Z10^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SY^Z10^R30^T150^C2 (black X), ^SY^Z10^R30^T150^C5 (blue squares), ^SY^Z10^R30^T∞^C2 (red circles), and ^SY^Z10^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SY^Z4^R20^T150^C2 (black X), ^SY^Z4^R20^T150^C5 (blue squares), ^SY^Z4^R20^T∞^C2 (red circles), and ^SY^Z4^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SY^Z4^R30^T150^C2 (black X), ^SY^Z4^R30^T150^C5 (blue squares), ^SY^Z4^R30^T∞^C2 (red circles), and ^SY^Z4^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SY^Z6^R20^T150^C2 (black X), ^SY^Z6^R20^T150^C5 (blue squares), ^SY^Z6^R20^T∞^C2 (red circles), and ^SY^Z6^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SY^Z6^R30^T150^C2 (black X), ^SY^Z6^R30^T150^C5 (blue squares), ^SY^Z6^R30^T∞^C2 (red circles), and ^SY^Z6^R30^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SY^Z8^R20^T150^C2 (black X), ^SY^Z8^R20^T150^C5 (blue squares), ^SY^Z8^R20^T∞^C2 (red circles), and ^SY^Z8^R20^T∞^C5 (green triangles).

Radial dependence of X_CO values for models ^SY^Z8^R30^T150^C2 (black X), ^SY^Z8^R30^T150^C5 (blue squares), ^SY^Z8^R30^T∞^C2 (red circles), and ^SY^Z8^R30^T∞^C5 (green triangles).

• 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