From c98da48a171c19f82ad6970dde19b7b7f9451f8f Mon Sep 17 00:00:00 2001 From: Roman Krivonos Date: Thu, 5 Dec 2024 17:14:04 +0300 Subject: [PATCH] Acknowledgements --- README.md | 2 +- 1 file changed, 1 insertion(+), 1 deletion(-) diff --git a/README.md b/README.md index 961b20f..9aa3a0a 100644 --- a/README.md +++ b/README.md @@ -1,6 +1,6 @@ # 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.