generated from erosita/uds
49 lines
1.6 KiB
Markdown
49 lines
1.6 KiB
Markdown
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Don't forget to activate environment: `source <MY PATH>/venv/bin/activate`
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The script number indicates the sequence of execution. The results are placed in `ridge/products/`.
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The corresponding shell scripts run Python code with different parameters.
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### 01_bgdmodel.py
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Calibrates IBIS/ISGRI background model
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### 01_crabmodel.py
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Calibrates Crab detector count rate model.
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### 01_crabmodel_plot_poly.py
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Plot long-term Crab detector count rate approximated by cubic polynomial function (Fig. B7 in paper).
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### 01_crabmodel_plot_sys.py
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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.
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### 02_grxe_resid.py
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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.
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### 02_grxe_resid_plot.py
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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).
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### 02_grxe_map.py
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Makes the map of the residuals in mCrab units (not covered in the paper).
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### 03_grxe_spec.py
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Extract spectrum of selected sky region, e.g.:
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```./03_grxe_spec.py GC``` or ```./03_grxe_spec.py M81```
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If you do not specify the sky region, the script makes spectra for all regions.
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Sky regions are defined in ```config.py```.
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Spectra are stored in `./products/Spec`. After spectra files are ready, go to directory `./products/Spec` and run ```perl ../../scripts/do_pha_igr_v3_mCrab.pl M81.spec```.
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