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मुख्य लेखकों: 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
स्वरूप: Preprint
प्रकाशित: 2024
विषय:
ऑनलाइन पहुंच:https://arxiv.org/abs/2410.08346
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_version_ 1866914992781000704
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