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Roman Krivonos
2024-11-01 11:40:05 +03:00
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@@ -14,10 +14,22 @@ Calibrates IBIS/ISGRI background model
Calibrates Crab detector count rate model.
### 01_crabmodel_plot_poly.py
Plot long-term Crab detector count rate approximated by cubic polynomial function (Fig. B7 in paper).
### 01_crabmodel_plot_sys.py
Plots the normalized distribution of the residuals between the IBIS/ISGRI Crab count rate and the corresponding polynomial fit (Fig. B8 in paper). The distribution is approximated with a Gaussian function.
### 02_grxe_resid.py
Calculates difference between detector count rate and that predicted by background model in mCrab units for `GAL` (Galaxy), `BKG` (Extragalactic), or `ALL` (all-sky) regions.
### 02_grxe_resid_plot.py
Plots normalized distribution of the relative residuals of the background model obtained in three energy bands for BKG region (Figs. A5 and A6 in paper).
### 02_grxe_map.py
Makes the map of the residuals in mCrab units (not covered in the paper).