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Roman Krivonos 2024-11-01 14:59:43 +03:00
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scripts/README.md
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@ -6,11 +6,11 @@ The script number indicates the sequence of execution. The results are placed in
The corresponding shell scripts run Python code with different parameters.
### 01_bgdmodel.py
### 01_bgdmodel.py/01_bgdmodel.sh
Calibrates IBIS/ISGRI background model
### 01_crabmodel.py
### 01_crabmodel.py/01_crabmodel.sh
Calibrates Crab detector count rate model.
@ -22,7 +22,7 @@ Plot long-term Crab detector count rate approximated by cubic polynomial functio
Plots the normalized distribution of the residuals between the IBIS/ISGRI Crab count rate and the corresponding polynomial fit (Fig. B8 in the paper). The distribution is approximated with a Gaussian function.
### 02_grxe_resid.py
### 02_grxe_resid.py/02_grxe_resid.sh
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.
@ -30,11 +30,11 @@ Calculates difference between detector count rate and that predicted by backgrou
Plots normalized distribution of the relative residuals of the background model obtained in three energy bands for BKG region (Figs. A5 and A6 in the paper).
### 02_grxe_map.py
### 02_grxe_map.py/03_grxe_map.sh
Makes the map of the residuals in mCrab units (not shown in the paper).
### 03_grxe_flux.py
### 03_grxe_flux.py/03_grxe_flux.sh
Estimates flux in regions defined in config.py, and places result in products/Flux, e.g.: