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Roman Krivonos 2024-10-31 08:39:59 +03:00
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This repository provides the code of the IBIS/ISGRI background model used in paper [arXiv:2409.20058](https://arxiv.org/abs/2409.20058).
In addition to the code, the package contains preprocessed data in **data** directory. In particular, it contains ISGRI detector count rate cleaned from the contribution of X-ray point sources, for each INTEGRAL observation (so-called "science window", ScW) in the range of the INTEGRAL orbits 70-2740 and in different energy bands. This data set and code can be used to calibrate the ISGRI background model and measure the X-ray intensity of the Galactic background in different parts of the Milky Way.
In addition to the code, the package contains preprocessed data in `data` directory. In particular, it contains ISGRI detector count rate cleaned from the contribution of X-ray point sources, for each INTEGRAL observation (so-called "science window", ScW) in the range of the INTEGRAL orbits 70-2740 and in different energy bands. This data set and code can be used to calibrate the ISGRI background model and measure the X-ray intensity of the Galactic background in different parts of the Milky Way.
# INSTALL
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## Work with pre-processed data
Actual work with the data takes place in the **scripts** directory, where processing scripts must be run sequentially. This directory contains a detailed description of all actions.
Actual work with the data takes place in the `scripts` directory, where processing scripts must be run sequentially. This directory contains a detailed description of all actions.