The role of the background in past and future X-ray missions

Abstract

Background has played an important role in X-ray missions, limiting the exploitation of science data in several and sometimes unexpected ways. In this presentation I review past X-ray missions focusing on some important lessons we can learn from them. I then go on discussing prospects for overcoming background related limitations in future ones.

arXiv commentTo Appear in Experimental Astronomy. Invited Review presented at the AHEAD Background Workshop, 28-30 November 2016, Rome, Italy

References in corpus (6)

• The European Photon Imaging Camera on XMM-Newton: The MOS Cameras
• The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission
• The 2-8 keV cosmic X-ray background spectrum as observed with XMM-Newton
• The gas distribution in the outer regions of galaxy clusters
• The XMM Cluster Outskirts Project (X-COP): Physical conditions to the virial radius of Abell 2142
• A critical assessment of the metal content of the ICM

Cited by in corpus (4)

• The Demonstration Model of the ATHENA X-IFU Cryogenic AntiCoincidence Detector
• Analysis of the unconcentrated background of the EPIC-pn camera on board XMM-Newton
• Advancing Precision Particle Background Estimation for Future X-ray Missions: Correlated Variability between AMS and Chandra/XMM-Newton
• The origin of the unfocused XMM-Newton background, its variability and lessons learned for ATHENA