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Line Emission Mapper (LEM): Probing the physics of cosmic ecosystems
Ralph Kraft, Maxim Markevitch, Caroline Kilbourne +107
The Line Emission Mapper (LEM) is an X-ray Probe for the 2030s that will answer the outstanding questions of the Universe's structure formation. It will also provide transformative…
XSLIDE (X-Ray Spectral Line IDentifier and Explorer): a quick-look tool for XRISM
Efrem Braun, Chris Baluta, Trisha F. Doyle +7
We present XSLIDE (X-Ray Spectral Line IDentifier and Explorer), a graphical user interface that has been designed as a quick-look tool for the upcoming X-Ray Imaging and Spectrosc…
The XRISM Pipeline Software System: Connecting Continents, Processes, Testing, and Scientists
Trisha F. Doyle, Matthew P. Holland, Robert S. Hill +6
XRISM (X-Ray Imaging and Spectroscopy Mission), with the Resolve high-resolution spectrometer and the Xtend wide-field imager on-board, is designed to build on the successes of the…
Understanding the effects of charge diffusion in next-generation soft X-ray imagers
Eric D. Miller, Gregory Y. Prigozhin, Beverly J. LaMarr +6
To take advantage of high-resolution optics sensitive to a broad energy range, future X-ray imaging instruments will require thick detectors with small pixels. This pixel aspect ra…
Towards precision particle background estimation for future X-ray missions: correlated variability between Chandra ACIS and AMS
Catherine E. Grant, Eric D. Miller, Marshall W. Bautz +4
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 p…
Mitigating the effects of particle background on the Athena Wide-Field Imager
Eric D. Miller, Catherine E. Grant, Marshall W. Bautz +16
The Wide Field Imager (WFI) flying on Athena will usher in the next era of studying the hot and energetic Universe. WFI observations of faint, diffuse sources will be limited by un…