Ground calibration plan for the Athena/X-IFU microcalorimeter spectrometer
/ Authors
A. Molin, F. Pajot, M. Audard, M. Barbera, Sophie Beaumont, E. Cucchetti, M. D’Andrea, Christophe Daniel, R. D. Hartog, M. Eckart
and 17 more authors
Philippe Ferrando, L. Gottardi, M. Leutenegger, S. Lotti, Lorenzo Natalucci, P. Peille, J. Plaa, E. Pointecouteau, Scott Porter, Kosuke Sato, J. Wilms, V. Albouys, D. Barret, Massimo Cappi, J. D. Herder, L. Piro, A. Simionescu
/ Abstract
The X-ray Integral Field Unit is the X-ray imaging spectrometer on-board one of ESA's next large missions, Athena. Athena is set to investigate the theme of the Hot and Energetic Universe, with a launch planned in the late-2030s. Based on a high sensitivity Transition Edge Sensor (TES) detector array operated at very low temperature (50 mK), X-IFU will provide spatially resolved high resolution spectroscopy of the X-ray sky in the 0.2-12 keV energy band, with an energy resolution goal of 4 eV up to 7 keV [3 eV design goal]. This paper presents the current calibration plan of the X-IFU. It provides the requirements applicable to the X-IFU calibration, describes the overall calibration strategy, and details the procedure and sources needed for the ground calibration of each parameter or characteristics of the X-IFU.
Journal: Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray
DOI: 10.1117/12.3020082