26 October 2024 Spectroscopic Time-Resolving Observatory for Broadband Energy X-ray high-energy modular array
Anthony L. Hutcheson, Marco Feroci, Andrea Argan, Matias Antonelli, Marco Barbera, Jörg Bayer, Pierluigi Bellutti, Giuseppe Bertuccio, Valter Bonvicini, Franck Cadoux, Riccardo Campana, Matteo Centis Vignali, Francesco Ceraudo, Marc Christophersen, Daniela Cirrincione, Fabio D’Anca, Nicolas De Angelis, Alessandra DeRosa, Giovanni Della Casa, Ettore Del Monte, Giuseppe Dilillo, Yuri Evangelista, Yannick Favre, Francesco Ficorella, Mauro Fiorini, Jeremy J. Ford, Paul Hedderman, Marco Grassi, J. Eric Grove, Alejandro Guzmán, Merlin R. Kole, Ugo Lo Cicero, Giovanni Lombardi, Piero Malcovati, Malgorzata Michalska, Aline Meuris, Gabriele Minervini, Witold Nowosielski, Alessio Nuti, Luigi Pacciani, Giancarlo Pepponi, Steven C. Persyn, Antonino Picciotto, Samuel Pliego, Alexander Rashevsky, Irina Rashevskaya, Paul S. Ray, Alina Samusenko, Andrea Santangelo, Stéphane Schanne, Carl L. Schwendeman, Clio Sleator, Jacob R. Smith, Libor Sveda, Jiri Svoboda, Christopher Tenzer, Michela Todaro, Alessio Trois, Andrea Vacchi, Hao Xiong, Xianqi Wang, Xin Wu, Eric A. Wulf, Gianluigi Zampa, Nicola Zampa, Andrzej Zdziarski, Nicola Zorzi
Author Affiliations +
Funded by: Office of Naval Research, NASA James Webb Space Telescope
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.

© 2024 Society of Photo-Optical Instrumentation Engineers (SPIE)
Anthony L. Hutcheson, Marco Feroci, Andrea Argan, Matias Antonelli, Marco Barbera, Jörg Bayer, Pierluigi Bellutti, Giuseppe Bertuccio, Valter Bonvicini, Franck Cadoux, Riccardo Campana, Matteo Centis Vignali, Francesco Ceraudo, Marc Christophersen, Daniela Cirrincione, Fabio D’Anca, Nicolas De Angelis, Alessandra DeRosa, Giovanni Della Casa, Ettore Del Monte, Giuseppe Dilillo, Yuri Evangelista, Yannick Favre, Francesco Ficorella, Mauro Fiorini, Jeremy J. Ford, Paul Hedderman, Marco Grassi, J. Eric Grove, Alejandro Guzmán, Merlin R. Kole, Ugo Lo Cicero, Giovanni Lombardi, Piero Malcovati, Malgorzata Michalska, Aline Meuris, Gabriele Minervini, Witold Nowosielski, Alessio Nuti, Luigi Pacciani, Giancarlo Pepponi, Steven C. Persyn, Antonino Picciotto, Samuel Pliego, Alexander Rashevsky, Irina Rashevskaya, Paul S. Ray, Alina Samusenko, Andrea Santangelo, Stéphane Schanne, Carl L. Schwendeman, Clio Sleator, Jacob R. Smith, Libor Sveda, Jiri Svoboda, Christopher Tenzer, Michela Todaro, Alessio Trois, Andrea Vacchi, Hao Xiong, Xianqi Wang, Xin Wu, Eric A. Wulf, Gianluigi Zampa, Nicola Zampa, Andrzej Zdziarski, and Nicola Zorzi "Spectroscopic Time-Resolving Observatory for Broadband Energy X-ray high-energy modular array," Journal of Astronomical Telescopes, Instruments, and Systems 10(4), 042503 (26 October 2024). https://doi.org/10.1117/1.JATIS.10.4.042503
Received: 14 May 2024; Accepted: 23 September 2024; Published: 26 October 2024
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KEYWORDS
Sensors

X-rays

Equipment

Observatories

Collimators

Design

Spectroscopes

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