AHEAD2020 · Horizon 2020 Research and Innovation Programme · GA 871158
WP 9.3.c "Understanding the interaction between soft protons and X-ray mirrors"
WP 9.8 "Understanding the interaction between soft protons and X-ray mirrors"
* Authors: V.Fioretti(1), T. Mineo(2), R. Amato(2), S. Lotti(3), C. Macculi(3), S. Molendi(4), F. Gastaldello(4), M. Cappi(1), M. Dadina(1), S. Ettori(1)
* Authors: V.Fioretti(1), T. Mineo(2), R. Amato(2), S. Lotti(3), C. Macculi(3), S. Molendi(4), F. Gastaldello(4), G. Lanzuisi(1), M. Cappi(1), M. Dadina(1), S. Ettori(1)
* Description: The proton response matrix for the XMM-Newton telescope is composed by a Redistribution Matrix File (RMF)
@@ -41,6 +41,12 @@ collecting the grasp of the optics, the filter transmission efficiency and the d
* 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.
### Documentation
The
### 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]
@@ -65,8 +71,6 @@ Due to biases at the boundary of the RMF modeling, induced by features in the in
