The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase
Didier Barret (IRAP), Vincent Albouys (CNES), Jan-Willem den Herder, (SRON), Luigi Piro (INAF-IAPS), Massimo Cappi (INAF-OAS Bologna), Juhani, Huovelin (Univ. Helsinki), Richard Kelley (NASA/GSFC), J. Miguel Mas-Hesse, (CAB (CSIC-INTA)), St\'ephane Paltani (Univ. Gen\`eve)

TL;DR
The paper details the design and review process of the Athena X-ray Integral Field Unit (X-IFU), highlighting its capabilities, subsystems, budgets, and ongoing technology development to ensure it meets scientific goals despite redesign challenges.
Contribution
It provides a comprehensive overview of the X-IFU's consolidated design, subsystem requirements, and development status during its System Requirement Review, ensuring flagship scientific capabilities are maintained.
Findings
X-IFU offers 2.5 eV spectral resolution up to 7 keV.
The design aims to retain scientific objectives despite cost-driven redesigns.
Ongoing technology demonstrations support the instrument's performance goals.
Abstract
The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer, studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory, a versatile observatory designed to address the Hot and Energetic Universe science theme, selected in November 2013 by the Survey Science Committee. Based on a large format array of Transition Edge Sensors (TES), it aims to provide spatially resolved X-ray spectroscopy, with a spectral resolution of 2.5 eV (up to 7 keV) over an hexagonal field of view of 5 arc minutes (equivalent diameter). The X-IFU entered its System Requirement Review (SRR) in June 2022, at about the same time when ESA called for an overall X-IFU redesign (including the X-IFU cryostat and the cooling chain), due to an unanticipated cost overrun of Athena. In this paper, after illustrating the breakthrough capabilities of the X-IFU, we describe the…
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