Development of Space Qualified Signal Processing Readout Electronics for HabWorlds and Origins Space Telescope Detector and Arrays

editorAstrobiology22 hours ago3 Views

Development of Space Qualified Signal Processing Readout Electronics for HabWorlds and Origins Space Telescope Detector and Arrays

The proposed readout system builds upon high-TRL modular SpaceCube hardware. Left panel: The readout system uses a build-to-print SpaceCube v3.0 Mini where the FPGA card (primary side pictured) houses a Xilinx Kintex KU060 chip. Right panel: Photograph of a full SpaceCube electronics system with 1U CubeSat cards inserted into a backplane.– astro-ph.IM

The Habitable Worlds Observatory (HWO) — a flagship ultraviolet/optical/infrared space telescope recommended by the National Academies’ Pathways to Discovery in Astronomy and Astrophysics — will require detector technologies capable of supporting significantly larger pixel-count arrays than previous missions.

Microwave Kinetic Inductance Detectors (MKIDs), naturally suited to microwave multiplexing readout, are already in use across several balloon-borne missions with FPGA based systems. To transition this capability to space, we are developing a radiation-hardened detector readout system that builds directly on the technical and environmental requirements defined by the PRIMA mission.

PRIMA serves as a critical pathfinder, informing the radiation tolerance, resource constraints, and on-board processing capabilities needed for HWO. In this work, we present our current results on algorithm implementation, hardware architecture, and firmware development using the radiation-hardened AMD Kintex Ultrascale FPGA, aligning with PRIMA’s stringent specifications to ensure compatibility with future space-based observatories like HWO.

Tracee Jamison-Hooks, Lynn Miles, Sanetra Newman-Bailey, Oketa Basha, Abarna Karthikeyan, Sarah E. Kay, Sean Bryan, Philip Mauskopf, Thomas Essinger-Hileman, Jason Glen, Sumit Dahal, Adrian Sinclair, Kathryn Chamberlain

Comments: 4 pages, 6 figures, presented at The International Symposium on Space Terahertz Technology (ISSTT) 2025, Berlin, Germany (Apr 6th-9th, 2025). It is submitted as part of the conference proceedings
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); Instrumentation and Detectors (physics.ins-det); Space Physics (physics.space-ph)
Cite as: arXiv:2508.00322 [astro-ph.IM] (or arXiv:2508.00322v2 [astro-ph.IM] for this version)
https://doi.org/10.48550/arXiv.2508.00322
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Submission history
From: Sarah Kay
[v1] Fri, 1 Aug 2025 05:11:53 UTC (1,751 KB)
[v2] Wed, 6 Aug 2025 03:13:17 UTC (676 KB)
https://arxiv.org/abs/2508.00322

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