diff --git a/README.md b/README.md
index 4b0dffc..077aab7 100644
--- a/README.md
+++ b/README.md
@@ -2,7 +2,7 @@
 
 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
@@ -38,7 +38,7 @@ After work, you can delete the project:
 
 ## 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.