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# Galactic diffuse emission with INTEGRAL/IBIS
This repository provides the code of the IBIS/ISGRI background model used in paper "The properties of the Galactic Hard X-Ray and soft gamma-ray Background based on 20 years of INTEGRAL/IBIS observations" by Krivonos et al., (2024) [arXiv:2409.20058](https://arxiv.org/abs/2409.20058).
This repository provides the code of the IBIS/ISGRI background model used in the paper "The properties of the Galactic Hard X-Ray and soft gamma-ray Background based on 20 years of INTEGRAL/IBIS observations" by Krivonos et al., (2024) [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.