Spectroscopic Time-Resolving Observatory for Broadband Energy X-ray high-energy modular array

The high-energy modular array (HEMA) is one of three instruments that compose the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) mission concept. The HEMA is a large-area, high-throughput non-imaging pointed instrument based on the large area detector (LAD) developed as part of the Large Observatory For X-ray Timing (LOFT) mission concept. It is designed for spectral timing measurements of a broad range of sources and provides a transformative increase in sensitivity to X-rays in the energy range of 2 to 30 keV compared with previous instruments, with an effective area of 3.4 m2 at 8.5 keV and an energy resolution of better than 300 at 6 keV in its nominal field of regard.

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Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2024-10-26
DOI
https://doi.org/10.1117/1.jatis.10.4.042503
Citations
1
Primary Topic
Particle Detector Development and Performance
Type
article
Field-Weighted Citation Impact
0.66

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Spectroscopic Time-Resolving Observatory for Broadband Energy X-ray high-energy modular array

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Spectroscopic Time-Resolving Observatory for Broadband Energy X-ray high-energy modular array

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article en
1 citations

Abstract

The high-energy modular array (HEMA) is one of three instruments that compose the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) mission concept. The HEMA is a large-area, high-throughput non-imaging pointed instrument based on the large area detector (LAD) developed as part of the Large Observatory For X-ray Timing (LOFT) mission concept. It is designed for spectral timing measurements of a broad range of sources and provides a transformative increase in sensitivity to X-rays in the energy range of 2 to 30 keV compared with previous instruments, with an effective area of 3.4 m2 at 8.5 keV and an energy resolution of better than 300 at 6 keV in its nominal field of regard.

Journal of Astronomical Telescopes Instruments and SystemsVol. 10(04)
University of Geneva (CH), Centrum Badań Kosmicznych (PL), United States Naval Research Laboratory (US), Southwest Research Institute (US), Istituto Nazionale di Fisica Nucleare (IT), George Mason University (US), Fondazione Bruno Kessler (IT), University of Pavia (IT), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), Czech Academy of Sciences, Astronomical Institute (CZ), Institute for Space Astrophysics and Planetology (IT), Fondazione Politecnico di Milano (IT), CEA Paris-Saclay (FR), Nicolaus Copernicus Astronomical Center (PL), Osservatorio Astronomico di Cagliari (IT), Institut de Recherche sur les Lois Fondamentales de l'Univers (FR), University of Tübingen (DE), National Institute for Astrophysics (IT), Polish Academy of Sciences (PL)
National Aeronautics and Space Administration, Office of Naval Research
Affordable and clean energy
Openalex Percentile: Top 14%
Particle Detector Development and Performance
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