Some of the objects below are provided as arrays of 2-tuples where the first element is the center of the bin time interval (in MET).
| ts: |
The likelihood Test Statistic. |
| flux: |
Average integrated photon flux or energy flux of photons with energies from 0.1 to 100 GeV. Units in photons/cm^2/s if photon flux is selected, MeV/cm^2/s if energy flux is selected. |
| flux_upper_limits: |
95% Photon flux upper limits, in photons/cm^2/s, or energy flux upper limits in MeV/cm^2/s. |
| flux_error: |
1-sigma symmetric gaussian equivalent statistical uncertainty in photons/cm^2/s if photon flux is selected, MeV/cm^2/s if energy flux is selected. |
| photon_index: |
Photon index if source spectral shape is power-law, alpha if it is logparabola. |
| photon_index_error: |
1-sigma symmetric gaussian equivalent photon index/alpha statistical uncertainty. |
| fit_tolerance: |
Relative fit tolerance. |
| fit_convergence: |
MINUIT return code. Anything other than '0' means that the analysis did not converge. Please read the caveats about non-convergent analyses. |
| dlogl: |
Delta log-likelihood between a fixed index and free index fit. The difference in degrees of freedom between these two hypothesis is of 1 for both power-law and logparabola spectral models (beta is fixed to the catalog value). |
| EG: |
Isotropic diffuse background Normalization. |
| GAL: |
Galactic diffuse background Prefactor. |
| bin_id: |
Time bin number. |