Kavli Affiliate: Richard Foster | Summary:A science goal of many future X-ray observatories is mapping the cosmic web through deep exposures of faint diffuse sources. Such observations require low background and the best possible knowledge of the remaining unrejected background. The dominant contribution to the background above 1-2 keV is from Galactic Cosmic Ray protons. […]
Continue.. Towards precision particle background estimation for future X-ray missions: correlated variability between Chandra ACIS and AMS