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| स्वरूप: | Preprint |
| प्रकाशित: |
2024
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| विषय: | |
| ऑनलाइन पहुंच: | https://arxiv.org/abs/2410.08346 |
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| _version_ | 1866914992781000704 |
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| author | Hutcheson, Anthony L. Feroci, Marco Argan, Andrea Antonelli, Matias Barbera, Marco Bayer, Jorg Bellutti, Pierluigi Bertuccio, Giuseppe Bonvicini, Valter Cadoux, Franck Campana, Riccardo Vignali, Matteo Centis Ceraudo, Francesco Christophersen, Marc Cirrincione, Daniela D'Anca, Fabio De Angelis, Nicolas De Rosa, Alessandra Della Casa, Giovanni Del Monte, Ettore Dilillo, Giuseppe Evangelista, Yuri Favre, Yannick Ficorella, Francesco Fiorini, Mauro Ford, Jeremy J. Grassi, Marco Grove, J. Eric Guzman, Alejandro Heddermann, Paul Kole, Merlin R. Cicero, Ugo Lo Lombardi, Giovanni Malcovati, Piero Michalska, Malgorzata Meuris, Aline Minervini, Gabriele Nowosielski, Witold Nuti, Alessio Pacciani, Luigi Pepponi, Giancarlo Persyn, Steven C. Picciotto, Antonino Pliego, Samuel Rachevski, Alexander Rashevskaya, Irina Ray, Paul S. Samusenko, Alina Santangelo, Andrea Schanne, Stephane Schwendeman, Carl L. Sleator, Clio Smith, Jacob R. Sveda, Libor Svoboda, Jiri Tenzer, Christoph Todaro, Michela Trois, Alessio Vacchi, Andrea Xiong, Hao Wang, Xianqi Wu, Xin Wulf, Eric A. Zampa, Gianluigi Zampa, Nicola Zdziarski, Andrzej Zorzi, Nicola |
| author_facet | Hutcheson, Anthony L. Feroci, Marco Argan, Andrea Antonelli, Matias Barbera, Marco Bayer, Jorg Bellutti, Pierluigi Bertuccio, Giuseppe Bonvicini, Valter Cadoux, Franck Campana, Riccardo Vignali, Matteo Centis Ceraudo, Francesco Christophersen, Marc Cirrincione, Daniela D'Anca, Fabio De Angelis, Nicolas De Rosa, Alessandra Della Casa, Giovanni Del Monte, Ettore Dilillo, Giuseppe Evangelista, Yuri Favre, Yannick Ficorella, Francesco Fiorini, Mauro Ford, Jeremy J. Grassi, Marco Grove, J. Eric Guzman, Alejandro Heddermann, Paul Kole, Merlin R. Cicero, Ugo Lo Lombardi, Giovanni Malcovati, Piero Michalska, Malgorzata Meuris, Aline Minervini, Gabriele Nowosielski, Witold Nuti, Alessio Pacciani, Luigi Pepponi, Giancarlo Persyn, Steven C. Picciotto, Antonino Pliego, Samuel Rachevski, Alexander Rashevskaya, Irina Ray, Paul S. Samusenko, Alina Santangelo, Andrea Schanne, Stephane Schwendeman, Carl L. Sleator, Clio Smith, Jacob R. Sveda, Libor Svoboda, Jiri Tenzer, Christoph Todaro, Michela Trois, Alessio Vacchi, Andrea Xiong, Hao Wang, Xianqi Wu, Xin Wulf, Eric A. Zampa, Gianluigi Zampa, Nicola Zdziarski, Andrzej Zorzi, Nicola |
| contents | The High Energy Modular Array (HEMA) is one of three instruments that compose the STROBE-X mission concept. The HEMA is a large-area, high-throughput non-imaging pointed instrument based on the Large Area Detector developed as part of the 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--30 keV compared to previous instruments, with an effective area of 3.4 m$^{2}$ at 8.5 keV and an energy resolution of better than 300 eV at 6 keV in its nominal field of regard. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_08346 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | STROBE-X High Energy Modular Array (HEMA) Hutcheson, Anthony L. Feroci, Marco Argan, Andrea Antonelli, Matias Barbera, Marco Bayer, Jorg Bellutti, Pierluigi Bertuccio, Giuseppe Bonvicini, Valter Cadoux, Franck Campana, Riccardo Vignali, Matteo Centis Ceraudo, Francesco Christophersen, Marc Cirrincione, Daniela D'Anca, Fabio De Angelis, Nicolas De Rosa, Alessandra Della Casa, Giovanni Del Monte, Ettore Dilillo, Giuseppe Evangelista, Yuri Favre, Yannick Ficorella, Francesco Fiorini, Mauro Ford, Jeremy J. Grassi, Marco Grove, J. Eric Guzman, Alejandro Heddermann, Paul Kole, Merlin R. Cicero, Ugo Lo Lombardi, Giovanni Malcovati, Piero Michalska, Malgorzata Meuris, Aline Minervini, Gabriele Nowosielski, Witold Nuti, Alessio Pacciani, Luigi Pepponi, Giancarlo Persyn, Steven C. Picciotto, Antonino Pliego, Samuel Rachevski, Alexander Rashevskaya, Irina Ray, Paul S. Samusenko, Alina Santangelo, Andrea Schanne, Stephane Schwendeman, Carl L. Sleator, Clio Smith, Jacob R. Sveda, Libor Svoboda, Jiri Tenzer, Christoph Todaro, Michela Trois, Alessio Vacchi, Andrea Xiong, Hao Wang, Xianqi Wu, Xin Wulf, Eric A. Zampa, Gianluigi Zampa, Nicola Zdziarski, Andrzej Zorzi, Nicola Instrumentation and Methods for Astrophysics The High Energy Modular Array (HEMA) is one of three instruments that compose the STROBE-X mission concept. The HEMA is a large-area, high-throughput non-imaging pointed instrument based on the Large Area Detector developed as part of the 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--30 keV compared to previous instruments, with an effective area of 3.4 m$^{2}$ at 8.5 keV and an energy resolution of better than 300 eV at 6 keV in its nominal field of regard. |
| title | STROBE-X High Energy Modular Array (HEMA) |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2410.08346 |