diff --git a/README.md b/README.md
index 963247d117bccdd698354daa13d5bc1f35c0db17..88266560d7eb0c8010dd1936a581cb8152aabee4 100644
--- a/README.md
+++ b/README.md
@@ -3,16 +3,13 @@
<!-- PROJECT LOGO -->
<br />
<p align="CENTER">
- <a href="https://www.ict.inaf.it/gitlab/xmm-newton-proton-response-files/ProtonRMFSimAnalysis">
+ <a href="https://www.ict.inaf.it/gitlab/proton_response_matrix/xmm-newton-proton-response-files">
<img src="AHEAD2020_logo.png" alt="AHEAD2020_logo" height="130">
<img src="HORIZON2020_logo.png" alt="AHEAD2020_logo" height="130">
<img src="INAF_logo.png" alt="INAF_logo" height="130">
</a>
<h3 align="center">XMM-Newton proton response files</h3>
- <p align="center">
- XMM-Newton proton RMF and ARF files
- </p>
</p>
@@ -21,7 +18,7 @@
## Table of Contents
* [About the Project](#about-the-project)
- * [Built With](#built-with)
+ * [Built with](#built-with)
* [Usage](#usage)
* [License](#license)
* [Contact](#contact)
@@ -40,11 +37,11 @@ WP 9.3.c "Understanding the interaction between soft protons and X-ray mirrors"
* Description: The proton response matrix for the XMM-Newton telescope is composed by a Redistribution Matrix File (RMF)
mapping the proton energy space (from 2 to 300 keV) into detector pulse height and an Auxiliary Response File (ARF)
-collecting the grasp of the optics, the filter transmission efficiency and the detector quantum efficiency.
+collecting the grasp of the optics, the filter transmission efficiency and the detector quantum efficiency. A PATTERN selection of 0 (only events that generate 1 pixel or Singles counts) is used.
-The files are formatted according to the NASA OGIP (Office of Guest Investigators Program) calibration database (caldb) format, and they are tested with the NASA HEASARC XSPEC analysis software tool.
+* The files are formatted according to the NASA OGIP (Office of Guest Investigators Program) calibration database (caldb) format, and they are tested with the NASA HEASARC XSPEC analysis software tool.
-### Built With
+### Built with
The current release of the proton response files is based on:
* Geant4 v10.4 [Agostinelli et al. NIMPA, 506, 250, 2003; Allison et al. ITNS, 53, 270, 2006; Allison et al. NIMPA, 835, 186, 2016]
* BoGEMMS v2.1 [Fioretti et al., Proc. SPIE, 118221F, 2021]
@@ -63,15 +60,12 @@ The current release of the proton response files is based on:
<!-- LICENSE -->
## License
-* copyright : (C) 2022 Valentina Fioretti INAF/OAS
-* email : valentina.fioretti@inaf.it
-
-
+* Copyright (C) 2022 INAF - see LICENSE.rst
<!-- CONTACT -->
## Contact
-Valentina Fioretti (INAF OAS) - valentina.fioretti@inaf.it
+Valentina Fioretti (INAF OAS Bologna) - valentina.fioretti<at>inaf.it
Project Link: [https://ahead.iaps.inaf.it/](https://ahead.iaps.inaf.it/)