STROBE-X Mission Logo
Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays

STROBE-X is a probe-class mission concept designed for X-ray timing and spectroscopy across the 0.2–30 keV band, with enormous collecting area, high throughput, and excellent spectral and temporal resolution. It was proposed in response to the 2023 NASA Astrophysics Probe Explorer call, following the recommendation of the Astro2020 Decadal Survey for an X-ray probe mission.

The observatory comprises three instruments—the Low Energy Modular Array (LEMA), the High Energy Modular Array (HEMA), and a Wide Field Monitor (WFM)—providing transformative capabilities for studying black holes, neutron stars, accretion physics, galaxy clusters, and time-domain and multi-messenger astrophysics.

Selections were announced in October 2024. Although STROBE-X received a Category 1 ranking and a low technical and cost risk rating, it was not selected for a Phase A study.

For detailed information on the mission as it was proposed, please see the five STROBE-X papers published in the Journal of Astronomical Telescopes, Instruments, and Systems (JATIS):
  1. Mission Overview Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays: Mission Overview Paul S. Ray, Peter W. A. Roming, Andrea Argan, Zaven Arzoumanian, et al. doi:10.1117/1.JATIS.10.4.042504
  2. LEMA Instrument STROBE-X Low-Energy Modular Array (LEMA) Instrument Keith C. Gendreau, Dominic Maes, Ronald A. Remillard, Paul S. Ray, et al. doi:10.1117/1.JATIS.10.4.042506
  3. HEMA Instrument Spectroscopic Time-Resolving Observatory for Broadband Energy X-ray High-Energy Modular Array Anthony L. Hutcheson, Marco Feroci, Andrea Argan, Matias Antonelli, et al. doi:10.1117/1.JATIS.10.4.042503
  4. WFM Instrument The STROBE-X Wide Field Monitor Instrument Ronald A. Remillard, Margarita Hernanz, Jean in't Zand, Paul S. Ray, et al. doi:10.1117/1.JATIS.10.4.042505
  5. Detector Electronics Front-End ASIC for the STROBE-X HEMA and WFM Detectors: Concept and Design Gianluigi De Geronimo, Paul S. Ray, Eric A. Wulf, Colleen A. Wilson-Hodge, et al. doi:10.1117/1.JATIS.10.4.042502