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1. The Wide Field Monitor (WFM) of the China-Europe eXTP (enhanced X-ray Timing and Polarimetry) mission

Author

Hernanz, Margarita, Feroci, Marco, Evangelista, Yuri, Meuris, Aline, Schanne, Stéphane, Zampa, Gianluigi, Tenzer, Chris, Bayer, Jörg, Nowosielski, Witold, Michalska, Malgorzata, Kalemci, Emrah, Sungur, Müberra, Brandt, Søren, Kuvvetli, Irfan, Franco, Daniel Alvarez, Carmona, Alex, Gálvez, José-Luis, Patruno, Alessandro, Zand, Jean in' t, Zwart, Frans, Santangelo, Andrea, Bozzo, Enrico, Zhang, Shuang-Nan, Lu, Fangjun, Xu, Yupeng, Campana, Riccardo, Del Monte, Ettore, Ceraudo, Francesco, Nuti, Alessio, Della Casa, Giovanni, Argan, Andrea, Minervini, Gabriele, Antonelli, Matias, Bonvicini, Valter, Boezio, Mirko, Cirrincione, Daniela, Munini, Riccardo, Rachevski, Alexandre, Vacchi, Andrea, Zampa, Nicola, Rashevskaya, Irina, Ficorella, Francesco, Picciotto, Antonino, Zorzi, Nicola, Baudin, David, Bouyjou, Florent, Gevin, Olivier, Limousin, Olivier, Hedderman, Paul, Pliego, Samuel, Xiong, Hao, de la Rie, Rob, Laubert, Phillip, Aitink-Kroes, Gabby, Kuiper, Lucien, Orleanski, Piotr, Skup, Konrad, Tcherniak, Denis, Turhan, Onur, Bozkurt, Ayhan, and Onat, Ahmet

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

The eXTP mission is a major project of the Chinese Academy of Sciences (CAS), with a large involvement of Europe. Its scientific payload includes four instruments: SFA, PFA, LAD and WFM. They offer an unprecedented simultaneous wide-band Xray timing and polarimetry sensitivity. A large European consortium is contributing to the eXTP study, both for the science and the instrumentation. Europe is expected to provide two of the four instruments: LAD and WFM; the LAD is led by Italy and the WFM by Spain. The WFM for eXTP is based on the design originally proposed for the LOFT ESA M3 mission, that underwent a Phase A feasibility study. It will be a wide field of view X-ray monitor instrument working in the 2-50 keV energy range, achieved with large-area Silicon Drift Detectors (SDDs), similar to the ones used for the LAD but with better spatial resolution. The WFM will consist of 3 pairs of coded mask cameras with a total combined field of view (FoV) of 90x180 degrees at zero response and a source localisation accuracy of ~1 arc min. The main goal of the WFM is to provide triggers for the target of opportunity observations of the SFA, PFA and LAD, in order to perform the core science programme, dedicated to the study of matter under extreme conditions of density, gravity and magnetism. In addition, the unprecedented combination of large field of view and imaging capability, down to 2 keV, of the WFM will allow eXTP to make important discoveries of the variable and transient X-ray sky, and provide X-ray coverage of a broad range of astrophysical objects covered under 'observatory science', such as gamma-ray bursts, fast radio bursts, gravitational wave electromagnetic counterparts. In this paper we provide an overview of the WFM instrument, explaining its design, configuration, and anticipated performance., Comment: 15 pages, 13 figures, Proceedings of SPIE 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray; Proceedings Volume 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray; 130931Y (2024); doi: 10.1117/12.3020020

Published
2024
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2. A 3-step Low-latency Low-Power Multichannel Time-to-Digital Converter based on Time Residual Amplifier

Author

Bouyjou, Florent

Subjects
Electrical Engineering and Systems Science - Signal Processing
Abstract

This paper proposes and evaluates a novel architecture for a low-power Time-to-Digital Converter with high resolution, optimized for both integration in multichannel chips and high rate operation (40 Mconversion/s/channel). This converter is based on a three-step architecture. The first step uses a counter whereas the following ones are based on two kinds of Delay Line structures. A programmable time amplifier is used between the second and third steps to reach the final resolution of 24.4 ps in the standard mode of operation. The system makes use of common continuously stabilized master blocks that control trimmable slave blocks, in each channel, against the effects of global PVT variations. Thanks to this structure, the power consumption of a channel is considerably reduced when it does not process a hit, and limited to 2.2 mW when it processes a hit. In the 130 nm CMOS technology used for the prototype, the area of a TDC channel is only 0.051 mm2. This compactness combined with low power consumption is a key advantage for integration in multi-channel front-end chips. The performance of this new structure has been evaluated on prototype chips. Measurements show excellent timing performance over a wide range of operating temperatures (-40{\deg}C to 60{\deg}C) in agreement with our expectations. For example, the measured timing integral nonlinearity is better than 1 LSB (25 ps) and the overall timing precision is better than 21 ps RMS.

Published
2023

3. The Large Area Detector for the eXTP mission

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Feroci, Marco, Ambrosi, Giovanni, Antonelli, Matias, Argan, Andrea, Babinec, Viktor, Barbera, Marco, Bastia, Paolo, Bayer, Joerg, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Bonfitto, Federica, Bonvicini, Valter, Bozzo, Enrico, Baudin, David, Bouyjou, Florent, Brienza, Daniele, Cadoux, Franck, Campana, Riccardo, Candia, Roberto, Cao, Jiewei, Cavazzuti, Elisabetta, Ceraudo, Francesco, Chen, Tianxiang, Chen, Wen, Coimbra, Artur, Colucci, Angelo, Cong, Xiaoqing, Cirrincione, Daniela, De Angelis, Nicolas, De Rosa, Alessandra, Della Casa, Giovanni, Del Monte, Ettore, Di Cicca, Gaspare, Di Cosimo, Sergio, Dilillo, Giuseppe, Dohnal, Roman, Donnarumma, Immacolata, Evangelista, Yuri, Fan, Peng, Fan, Qingmei, Favre, Yannick, Fiandrini, Emanuele, Ficorella, Francesco, Gao, Na, Gevin, Olivier, Grassi, Marco, Guedel, Manuel, Guzman Cabrera, Alejandro, Han, Dong, He, Huilin, Hedderman, Paul, den Herder, Jan-Willem, Hynek, Richard, Reynaard Kole, Merlin, Karas, Vladimir, Komarek, Martin, Labanti, Claudio, La Marra, Daniel, Lesci, Giuseppe, Li, Gang, Li, Loghui, Li, Tiangtong, Limousin, Olivier, Liu, Hongwei, Liu, Rui, Liu, Yichen, Liu, Xiaojing, Lo Cicero, Ugo, Loehring, Jens, Lombardi, Giovanni, Lu, Fang-Jun, Luo, Tao, Malcovati, Piero, Marinucci, Andrea, Mele, Filippo, Mendes, Vasco, Merkl, Martin, Meuris, Aline, Michalska, Malgorzata, Morbidini, Alfredo, Morgante, Gianluca, Muleri, Fabio, Munini, Riccardo, Mussolin, Lorenzo, Negri, Barbara, Novák, Petr, Nowosielski, Witold, Nuti, Alessio, Orleanski, Piotr, Ottensamer, Roland, Pacciani, Luigi, Paltani, Stephane, Pan, Teng, Pepponi, Giancarlo, Perinati, Emanuele, Piazzolla, Raffaele, Picciotto, Antonino, Pliego, Samuel, Putz, Andreas, Rachevski, Alexandre, Rashevskaia, Irina, Samusenko, Alina, Santangelo, Andrea, Schanne, Stephane, Serafinelli, Roberto, Skup, Konrad, Sveda, Libor, Svoboda, Jiri, Tenzer, Chris, Todaro, Michela, Torok, Gabriel, Trois, Alessio, Vacchi, Andrea, Varisco, Salvatore, Villa, Francesco, Virgilli, Enrico, Xiang, Hongwen, Xiong, Hao, Wang, Jian, Wang, Xianqi, Winter, Berend, Wu, Zhenyu, Wu, Xin, Xu, Yupeng, Zampa, Gianluigi, Zampa, Nicola, Zdziarski, Andrzej A., Zhang, Long, Zhang, Shu, Zhang, Shuang-Nan, Zhang, Yonghe, Zhang, Wenda, Zhao, Qiao, Zhu, Cheng, Zhu, Xiaofei, and Zorzi, Nicola

Published
2024
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4. The Wide Field Monitor (WFM) of the China-Europe eXTP (enhanced X-ray Timing and Polarimetry) mission

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Hernanz, Margarita, Feroci, Marco, Evangelista, Yuri, Meuris, Aline, Schanne, Stéphane, Zampa, Gianluigi, Tenzer, Chris, Bayer, Jörg, Nowosielski, Witold, Michalska, Malgorzata, Kalemci, Emrah, Sungur, Müberra, Brandt, Søren, Kuvvetli, Irfan, Alvarez Franco, Daniel, Carmona, Alex, Gálvez, José-Luis, Patruno, Alessandro, In' t Zand, Jean, Zwart, Frans, Santangelo, Andrea, Bozzo, Enrico, Zhang, Shuang-Nan, Lu, Fangjun, Xu, Yupeng, Campana, Riccardo, Del Monte, Ettore, Ceraudo, Francesco, Nuti, Alessio, Della Casa, Giovanni, Argan, Andrea, Minervini, Gabriele, Antonelli, Matias, Bonvicini, Valter, Boezio, Mirko, Cirrincione, Daniela, Munini, Riccardo, Rachevski, Alexandre, Vacchi, Andrea, Zampa, Nicola, Rashevskaya, Irina, Ficorella, Francesco, Picciotto, Antonino, Zorzi, Nicola, Baudin, David, Bouyjou, Florent, Gevin, Olivier, Limousin, Olivier, Hedderman, Paul, Pliego, Samuel, Xiong, Hao, de la Rie, Rob, Laubert, Phillip, Aitink-Kroes, Gabby, Kuiper, Lucien, Orleanski, Piotr, Skup, Konrad, Tcherniak, Denis, Turhan, Onur, Bozkurt, Ayhan, and Onat, Ahmet

Published
2024
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5. A Three-Step Low-Power Multichannel TDC Based on Time Residual Amplifier

Author

Bouyjou, Florent, Delagnes, Eric, Couderc, Fabrice, Thienpont, Damien, Gonzalez-Martinez, Jose David, Dulucq, Frederic, Guilloux, Fabrice, and Mandjavidze, Irakli

Abstract

This article proposes and evaluates an architecture for a low-power time-to-digital converter (TDC) with high resolution, optimized for high-rate operation (40 MSa/channel), and integration with analog front end in multichannel readout chips in 130-nm CMOS technology. The converter is based on a three-step architecture. The first step uses a counter and the following ones are based on two types of delay-line (DL) structures. A programmable time amplifier (TA) is used between the second and third steps to reach a final resolution of 24.4 ps in the standard mode of operation. In addition, this architecture uses common continuously stabilized reference blocks that control the channels against the effects of global process, voltage, and temperature (PVT) variations. We also propose a per-channel DL gain correction based on a trimmable block to correct the mismatch effect. The area of the TDC channel is only 0.051 mm2. For a 40-MSa/channel rate, the TDC average power consumption measured per channel is 2.2 mW for a 100% hit occupancy and decreases to 311 $\mu \text{W}$ for the 10% occupancy specified for our main application. The demonstrated compactness and low power consumption fully match our requirements for integration into multichannel front-end chips. The experimental results demonstrate good timing performance over a broad range of operating temperatures (−35 °C and 65 °C), which conforms to our expectations. For example, the measured timing integral nonlinearity (INL) is better than ±1 LSB (±25 ps), and the overall timing precision is better than 21-ps rms.

Published
2023
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7. The enhanced x-ray timing and polarimetry mission: eXTP: an update on its scientific cases, mission profile and development status

Author

Zhang, Shuang Nan, Santangelo, Andrea, Xu, Yupeng, Feroci, Marco, Hernanz, Margarita, Lu, Fangjun, Chen, Yong, Feng, Hua, Nandra, Kirpal, Jiang, Weichun, Svoboda, Jiri, Brandt, Søren, Schanne, Stéphane, Zand, Jean, Michalska, Malgorzata, Bozzo, Enrico, Kalemci, Emrah, Agudo, Ivan, Ahangarianabhari, Mahdi, Aitink-Kroes, Gabby, Ambrosi, Giovanni, Ambrosino, Filippo, An, Zhenghua, Perez Torres, Miguel Angel, Antonelli, Matias, Argan, Andrea, Babinec, Viktor, Baldini, Luca, Barbera, Marco, van Baren, Coen, Baudin, David, Bayer, Jörg, Bellazzini, Ronaldo, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Bi, Xingzi, Boezio, Mirko, Bonvicini, Valter, Bonvicini, Walter, Bordas, Pol, Borghese, Alice, Borghi, Giacomo, Bouyjou, Florent, Bozkurt, Ayhan, Brez, Alessandro, Brienza, Daniele, Cadoux, Franck, Campana, Riccardo, Cao, Jiewei, Cao, Xuelei, Casares, Jorge, Cavazzuti, Elisabetta, Ceraudo, Francesco, Chen, Tianxiang, Chen, Wen, Chen, Can, Chen, Yupeng, Chen, Xin, Chen, Yehai, Chenevez, Jerome, Cheng, Yaodong, Cirrincione, Daniela, Civitani, Marta, Cong, Min, Zelati, Francesco Coti, Cui, Weiwei, Cui, Tao, Cui, Wei, Dai, Boyu, Dauser, Thomas, De Angelis, Nicolas, De Marco, Barbara, De Rosa, Alessandra, Monte, Ettore Del, Cosimo, Sergio Di, Diebold, Sebastian, Dilillo, Giuseppe, Ding, Fei, Dohnal, Roman, Dong, Zefang, Donnarumma, Immacolata, Dovciak, Michal, Du, Yuanyuan, Ducci, Lorenzo, Evangelista, Yuri, Fan, Qingmei, Favre, Yannick, Ferrés, Patrícia, Fiandrini, Emanuele, Ficorella, Francesco, Fuschino, Fabio, Gálvez, José Luis, Gao, Na, Gao, Min, Ge, Yuqiang, Ge, Mingyu, Gevin, Olivier, Grassi, Marco, Gu, Yudong, Gu, Quanying, Guan, Ju, Guedel, Manuel, Han, Xingbo, Han, Dawei, He, Huilin, He, Junwang, Hedderman, Paul, den Herder, Jan Willem, Hong, Bin, Hormaetxe, Ander, Hou, Dongjie, Hu, Zexun, Hu, Hao, Hu, Qingbao, Hu, Yu, Huang, Yue, Huang, Jiangjiang, Huang, Qiushi, Huo, Jia, Hynek, Richard, Iwasawa, Kazumi, Izzo, Lucca, Ji, Long, Jia, Shumei, Jiang, Bowen, Jiang, Wei, Jiang, Jiechen, Jiang, Xiaowei, Jiao, Yang, Jin, Ge, Jin, Fan, Jose, Jordi, Karas, Vladimir, Kennedy, Thomas, Kirsch, Christian, Kole, Merlin, Komarek, Martin, Kreykenbohm, Ingo, Kuiper, Lucien, Kuvvetli, Irfan, Labanti, Claudio, Latronico, Luca, Laubert, Phillip, Li, Tao, Li, Longhui, Li, Hong, Li, Duo, Li, Wei, Li, Maoshun, Li, Gang, Li, Xiaobo, Li, Chengkui, Li, Bing, Li, Haibo, Liang, Hong, Liao, Qiuyan, Liao, Jinyuan, Limousin, Olivier, Lin, Yanjian, Linares, Manuel, Liu, Rui, Liu, Yichen, Liu, Zhihao, Liu, Hongwei, Liu, Xiaojing, Liu, Xiaohua, Cicero, Ugo Lo, Loehring, Jens, Lombardi, Giovanni, Lorenz, Maximilian, Lu, Bing, Lucchesi, Leonardo, Luo, Tao, Luo, Laidan, Ma, Jia, Ma, Xiang, Macera, Daniele, Malcovati, Piero, Manfreda, Alberto, Paredes, Josep Maria, Marinucci, Andrea, Martindale, Adrian, Meidinger, Norbert, Mele, Filippo, Mendes, Vasco, Meng, Bin, Merkl, Martin, Meuris, Aline, Miniutti, Giovanni, Minuti, Massimo, Morbidini, Alfredo, Morgante, Gianluca, Muleri, Fabio, Munini, Riccardo, Mussolin, Lorenzo, Negri, Barbara, Nie, Jianyin, Novák, Petr, Nowosielski, Witold, Nuti, Alessio, Onat, Ahmet, Orleanski, Piotr, Orsini, Leonardo, Ottensamer, Roland, Ou, Ge, Pacciani, Luigi, Paltani, Stephane, Pan, Teng, Pan, Kai, Pareschi, Giovanni, Patruno, Alessandro, Pepponi, Giancarlo, Perinati, Emanuele, Piazzolla, Raffaele, Picciotto, Antonino, Piemonte, Claudio, Pinchera, Michele, Pliego, Samuel, Poutanen, Juri, Qi, Liqiang, Qi, Fazhi, Qiang, Pengfei, Qiao, Fangjian, Qiao, Zheng, Qiu, Xiangbiao, Qiu, Chengbo, Qu, Jinlu, Rachevski, Alexandre, Rashevskaia, Irina, Rea, Nanda, Ribo, Marc, de la Rie, Rob, Rodriguez, Jerome, Gil, Pablo Rodríguez, Sala, Gloria, Schanz, Thomas, Serafinelli, Roberto, Sgro, Carmelo, Shen, Zhengxiang, Sheng, Lizhi, Shi, Jingyan, Sironi, Giorgia, Skup, Konrad, Song, Liming, Song, Zeyu, Song, Jiangbo, Spandre, Gloria, Spiga, Daniele, Su, Yongquan, Sun, Liang, Sungur, Müberra, Svéda, Libor, Tagliaferri, Gianpiero, Tan, Ying, Tao, Lian, Tcherniak, Denis, Tenzer, Chris, Todaro, Michela, Tolos, Laura, Torok, Gabriel, Torres, Diego F., Trois, Alessio, Turhan, Onur, Uttley, Phil, Vacchi, Andrea, Virgilli, Enrico, Vogel, Channah, Walton, Dave, Wang, Jian, Wang, Xianqi, Wang, Bo, Wang, Langping, Wang, Xiaofeng, Wang, Dianlong, Wang, Yusa, Wang, Juan, Wang, Hao, Wang, Ruijie, Wang, Ping, Wang, Lingjun, Wang, Wenshuai, Wang, Tian, Wang, Haoyu, Wang, Zhanshan, Watts, Anna L., Wen, Xiangyang, Wilms, Jörn, Winter, Berend, Wu, Xin, Wu, Chao, Wu, Zhenyu, Wu, Qiong, Wu, Kaiji, Xiong, Hao, Xiong, Shaolin, Xu, Wei, Xu, Zhao, Xu, Jingjing, Xu, Xiongwei, Xue, Jiadai, Yan, Yongqing, Yan, Xingtao, Yang, Xianghui, Yang, Yanji, Yang, Xiongtao, Yang, Sheng, Yang, Jiawei, Yang, Yingquan, Yi, Shuxu, Yu, Yonggao, Yu, Ke, Zampa, Ganluigi, Zampa, Nicola, Zane, Silvia, Zdziarski, Andrzej A., Zhang, Long, Zhang, Shu, Zhang, Wenda, Zhang, Xiaoli, Zhang, Zhen, Zhang, Jiawei, Zhang, Fan, Zhang, Ziliang, Zhang, Dali, Zhang, Honglin, Zhang, Aimei, Zhang, Tong, Zhang, Hongmei, Zhang, Juan, Zhang, Liang, Zhang, Yueting, Zhao, Li, Zhao, Baosheng, Zhao, Zijian, Zhao, Xiaofan, Zhao, Haisheng, Zhao, Xiaoyun, Zheng, Shijie, Zhou, Yupeng, Zhou, Xiaohong, Zhu, Jiahuan, Zhu, Yuxuan, Zhu, Cheng, Zhu, Zhencai, Zorzi, Nicola, Zwart, Frans, den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Chinese Academy of Sciences, Agenzia Spaziale Italiana, Ministerio de Ciencia e Innovación (España), Federal Ministry of Economics and Technology (Germany), and Foundation for Polish Science

Subjects
Equation of state, Extreme gravity, Black hole, X-ray timing, X-ray polarimetry, Neutron star, Extreme magnetism, Extreme density
Abstract

Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray (2022), Montreal, Jul 17-22, 2022.--Proceedings of SPIE - The International Society for Optical Engineering vol. 12181 Article number 121811W.-- Full list of authors: Zhang, Shuang-Nan; Santangelo, Andrea; Xu, Yupeng; Feroci, Marco; Hernanz, Margarita; Lu, Fangjun; Chen, Yong; Feng, Hua; Nandra, Kirpal; Jiang, Weichun; Svoboda, Jiri; Brandt, Soren; Schanne, Stephane; in't Zand, Jean; Michalska, Malgorzata; Bozzo, Enrico; Kalemci, Emrah; Agudo, Ivan; Ahangarianabhari, Mahdi; Aitink-Kroes, Gabby; Ambrosi, Giovanni; Ambrosino, Filippo; An, Zhenghua; Perez Torres, Miguel Angel; Antonelli, Matias; Argan, Andrea; Babinec, Viktor; Baldini, Luca; Barbera, Marco; van Baren, Coen; Baudin, David; Bayer, Joerg; Bellazzini, Ronaldo; Bellutti, Pierluigi; Bertucci, Bruna; Bertuccio, Giuseppe; Bi, Xingzi; Boezio, Mirko; Bonvicini, Valter; Bonvicini, Walter; Bordas, Pol; Borghese, Alice; Borghi, Giacomo; Bouyjou, Florent; Bozkurt, Ayhan; Brez, Alessandro; Brienza, Daniele; Cadoux, Franck; Campana, Riccardo; Cao, Jiewei; Cao, Xuelei; Casares, Jorge; Cavazzuti, Elisabetta; Ceraudo, Francesco; Chen, Tianxiang; Chen, Wen; Chen, Can; Chen, Yupeng; Chen, Xin; Chen, Yehai; Chenevez, Jerome; Cheng, Yaodong; Cirrincione, Daniela; Civitani, Marta; Cong, Min; Coti Zelati, Francesco; Cui, Weiwei; Cui, Tao; Cui, Wei; Dai, Boyu; Dauser, Thomas; De Angelis, Nicolas; De Marco, Barbara; De Rosa, Alessandra; Del Monte, Ettore; Di Cosimo, Sergio; Diebold, Sebastian; Dilillo, Giuseppe; Ding, Fei; Dohnal, Roman; Dong, Zefang; Donnarumma, Immacolata; Dovciak, Michal; Du, Yuanyuan; Ducci, Lorenzo; Evangelista, Yuri; Fan, Qingmei; Favre, Yannick; Ferres, Patricia; Fiandrini, Emanuele; Ficorella, Francesco; Fuschino, Fabio; Luis Galvez, Jose; Gao, Na; Gao, Min; Ge, Yuqiang; Ge, Mingyu; Gevin, Olivier; Grassi, Marco; Gu, Yudong; Gu, Quanying; Guan, Ju; Guedel, Manuel; Han, Xingbo; Han, Dawei; He, Huilin; He, Junwang; Hedderman, Paul; den Herder, Jan-Willem; Hong, Bin; Hormaetxe, Ander; Hou, Dongjie; Hu, Zexun; Hu, Hao; Hu, Qingbao; Hu, Yu; Huang, Yue; Huang, Jiangjiang; Huang, Qiushi; Huo, Jia; Hynek, Richard; Iwasawa, Kazumi; Izzo, Lucca; Ji, Long; Jia, Shumei; Jiang, Bowen; Jiang, Wei; Jiang, Jiechen; Jiang, Xiaowei; Jiao, Yang; Jin, Ge; Jin, Fan; Jose, Jordi; Karas, Vladimir; Kennedy, Thomas; Kirsch, Christian; Kole, Merlin; Komarek, Martin; Kreykenbohm, Ingo; Kuiper, Lucien; Kuvvetli, Irfan; Labanti, Claudio; Latronico, Luca; Laubert, Phillip; Li, Tao; Li, Longhui; Li, Hong; Li, Duo; Li, Wei; Li, Maoshun; Li, Gang; Li, Xiaobo; Li, Chengkui; Li, Bing; Li, Haibo; Liang, Hong; Liao, Qiuyan; Liao, Jinyuan; Limousin, Olivier; Lin, Yanjian; Linares, Manuel; Liu, Rui; Liu, Yichen; Liu, Zhihao; Liu, Hongwei; Liu, Xiaojing; Liu, Xiaohua; Lo Cicero, Ugo; Loehring, Jens; Lombardi, Giovanni; Lorenz, Maximilian; Lu, Bing; Lucchesi, Leonardo; Luo, Tao; Luo, Laidan; Ma, Jia; Ma, Xiang; Macera, Daniele; Malcovati, Piero; Manfreda, Alberto; Maria Paredes, Josep; Marinucci, Andrea; Martindale, Adrian; Meidinger, Norbert; Mele, Filippo; Mendes, Vasco; Meng, Bin; Merkl, Martin; Meuris, Aline; Miniutti, Giovanni; Minuti, Massimo; Morbidini, Alfredo; Morgante, Gianluca; Muleri, Fabio; Munini, Riccardo; Mussolin, Lorenzo; Negri, Barbara; Nie, Jianyin; Novak, Petr; Nowosielski, Witold; Nuti, Alessio; Onat, Ahmet; Orleanski, Piotr; Orsini, Leonardo; Ottensamer, Roland; Ou, Ge; Pacciani, Luigi; Paltani, Stephane; Pan, Teng; Pan, Kai; Pareschi, Giovanni; Patruno, Alessandro; Pepponi, Giancarlo; Perinati, Emanuele; Piazzolla, Raffaele; Picciotto, Antonino; Piemonte, Claudio; Pinchera, Michele; Pliego, Samuel; Poutanen, Juri; Qi, Liqiang; Qi, Fazhi; Qiang, Pengfei; Qiao, Fangjian; Qiao, Zheng; Qiu, Xiangbiao; Qiu, Chengbo; Qu, Jinlu; Rachevski, Alexandre; Rashevskaia, Irina; Rea, Nanda; Ribo, Marc; de la Rie, Rob; Rodriguez, Jerome; Rodriguez Gil, Pablo; Sala, Gloria; Schanz, Thomas; Serafinelli, Roberto; Sgro, Carmelo; Shen, Zhengxiang; Sheng, Lizhi; Shi, Jingyan; Sironi, Giorgia; Skup, Konrad; Song, Liming; Song, Zeyu; Song, Jiangbo; Spandre, Gloria; Spiga, Daniele; Su, Yongquan; Sun, Liang; Sungur, Muberra; Sveda, Libor; Tagliaferri, Gianpiero; Tan, Ying; Tao, Lian; Tcherniak, Denis; Tenzer, Chris; Todaro, Michela; Tolos, Laura; Torok, Gabriel; Torres, Diego F.; Trois, Alessio; Turhan, Onur; Uttley, Phil; Vacchi, Andrea; Virgilli, Enrico; Vogel, Channah; Walton, Dave; Wang, Jian; Wang, Xianqi; Wang, Bo; Wang, Langping; Wang, Xiaofeng; Wang, Dianlong; Wang, Yusa; Wang, Juan; Wang, Hao; Wang, Ruijie; Wang, Ping; Wang, Lingjun; Wang, Wenshuai; Wang, Tian; Wang, Haoyu; Wang, Zhanshan; Watts, Anna L.; Wen, Xiangyang; Wilms, Joern; Winter, Berend; Wu, Xin; Wu, Chao; Wu, Zhenyu; Wu, Qiong; Wu, Kaiji; Xiong, Hao; Xiong, Shaolin; Xu, Wei; Xu, Zhao; Xu, Jingjing; Xu, Xiongwei; Xue, Jiadai; Yan, Yongqing; Yan, Xingtao; Yang, Xianghui; Yang, Yanji; Yang, Xiongtao; Yang, Sheng; Yang, Jiawei; Yang, Yingquan; Yi, Shuxu; Yu, Yonggao; Yu, Ke; Zampa, Ganluigi; Zampa, Nicola; Zane, Silvia; Zdziarski, Andrzej A.; Zhang, Long; Zhang, Shu; Zhang, Wenda; Zhang, Xiaoli; Zhang, Zhen; Zhang, Jiawei; Zhang, Fan; Zhang, Ziliang; Zhang, Dali; Zhang, Honglin; Zhang, Aimei; Zhang, Tong; Zhang, Hongmei; Zhang, Juan; Zhang, Liang; Zhang, Yueting; Zhao, Li; Zhao, Baosheng; Zhao, Zijian; Zhao, Xiaofan; Zhao, Haisheng; Zhao, Xiaoyun; Zheng, Shijie; Zhou, Yupeng; Zhou, Xiaohong; Zhu, Jiahuan; Zhu, Yuxuan; Zhu, Cheng; Zhu, Zhencai; Zorzi, Nicola; Zwart, Frans, The enhanced X-ray Timing and Polarimetry mission (eXTP) is a flagship observatory for X-ray timing, spectroscopy and polarimetry developed by an International Consortium. Thanks to its very large collecting area, good spectral resolution and unprecedented polarimetry capabilities, eXTP will explore the properties of matter and the propagation of light in the most extreme conditions found in the Universe. eXTP will, in addition, be a powerful X-ray observatory. The mission will continuously monitor the X-ray sky, and will enable multiwavelength and multi-messenger studies. The mission is currently in phase B, which will be completed in the middle of 2022. © 2022 SPIE. All rights reserved., The Chinese team acknowledges support by the Chinese Academy of Sciences through the Strategic Priority Research Program, Grant No. XDA15020100. The Italian authors acknowledge funding support by the Italian Space Agency (under agreement n. 2020-3-HH.0 and ASI-INAF n.2017-14-H.O) and INFN (project XRO -X-ray Observatories). The Spanish authors acknowledge funding support from the MICIN/AEI grant PID2019-108709GB-I00. The German team acknowledges support from the Bundesministerium fur Wirtschaft und Technologie through the Deutsches Zentrum fur Luft-und Raumfahrt e.V. (DLR) under the grant number FKZ 50 OO 1902. The Polish team acknowledges FNP grant POIR.04.04.00-00-5C65/17. The Czech team acknowledges support from the GACR project 21-06825X. The Turkish team acknowledges support from the Turkish Space Agency., With funding from the Spanish government through the Severo Ochoa Centre of Excellence accreditation SEV-2017-0709

Published
2022

8. The digital data processing concepts of the large area detector and the wide field monitor onboard eXTP

Author

Xiong, Hao, primary, Argan, Andrea, additional, Baudin, David, additional, Bayer, Jörg, additional, Bouyjou, Florent, additional, De Angelis, Nicolas, additional, Del Monte, Ettore, additional, Evangelista, Yuri, additional, Favre, Yannick, additional, Feroci, Marco, additional, Galvez, José-Luis, additional, Gevin, Olivier, additional, Hedderman, Paul, additional, Hernanz, Margarita, additional, Kole, Merlin R., additional, Meuris, Aline, additional, Pliego-Caballero, Samuel, additional, Santangelo, Andrea, additional, Tenzer, Chris, additional, Trois, Alessio, additional, Wang, Xianqi, additional, and Zampa, Gianluigi, additional

Published
2022
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9. The large area detector onboard the eXTP mission

Author

Feroci, Marco, primary, Ambrosi, Giovanni, additional, Ambrosino, Filippo, additional, Antonelli, Matias, additional, Argan, Andrea, additional, Babinec, Viktor, additional, Barbera, Marco, additional, Bayer, Jörg, additional, Bellutti, Pierluigi, additional, Bertucci, Bruna, additional, Bertuccio, Giuseppe, additional, Bi, Xingzi, additional, Boezio, Mirko, additional, Bonvicini, Walter, additional, Borghi, Giacomo, additional, Bozzo, Enrico, additional, Baudin, David, additional, Bouyjou, Florent, additional, Brienza, Daniele, additional, Cadoux, Franck, additional, Campana, Riccardo, additional, Cao, Jiewei, additional, Cavazzuti, Elisabetta, additional, Ceraudo, Francesco, additional, Chen, Tianxiang, additional, Chen, Wen, additional, Cirrincione, Daniela, additional, De Angelis, Nicolas, additional, De Rosa, Alessandra, additional, Del Monte, Ettore, additional, Di Cosimo, Sergio, additional, Dilillo, Giuseppe, additional, Dohnal, Roman, additional, Donnarumma, Immacolata, additional, Evangelista, Yuri, additional, Fan, Qingmei, additional, Favre, Yannick, additional, Fiandrini, Emanuele, additional, Ficorella, Francesco, additional, Fuschino, Fabio, additional, Gao, Na, additional, Gevin, Olivier, additional, Grassi, Marco, additional, Guedel, Manuel, additional, Han, Xingbo, additional, He, Huilin, additional, Hedderman, Paul, additional, den herder, jan-willem, additional, Hynek, Richard, additional, Hong, Bing, additional, Jin, Ge, additional, Kole, Merlin, additional, Karas, Vladimír, additional, Komarek, Martin, additional, Labanti, Claudio, additional, Li, Loghui, additional, Li, Tianming, additional, Liang, Hong, additional, Limousin, Olivier, additional, Liu, Rui, additional, Lo Cicero, Ugo, additional, Lohering, Jens, additional, Lombardi, Giovanni, additional, Lu, Fang-Jun, additional, Luo, Tao, additional, Malcovati, Piero, additional, Mao, Hanqi, additional, Marinucci, Andrea, additional, Mele, Filippo, additional, Mendes, Vasco, additional, Merkl, Martin, additional, Meuris, Aline, additional, Michalska, Małgorzata, additional, Morbidini, Alfredo, additional, Morgante, Gianluca, additional, Muleri, Fabio, additional, Munini, Riccardo, additional, Mussolin, Lorenzo, additional, Negri, Barbara, additional, Novak, Petr, additional, Nowosielski, Witold, additional, Nuti, Alessio, additional, Orleanski, Piotr, additional, Ottensamer, Roland, additional, Pacciani, Luigi, additional, Paltani, Stephane, additional, Pan, Teng, additional, Pepponi, Giancarlo, additional, Perinati, Emanuele, additional, Piazzolla, Raffaele, additional, Picciotto, Antonino, additional, Pliego, Samuel, additional, Rachevski, Alexandre, additional, Rashevskaia, Irina, additional, Santangelo, Andrea, additional, Serafinelli, Roberto, additional, Schanne, Stéphane, additional, Skup, Konrad, additional, Sveda, Libor, additional, Svoboda, Jiri, additional, Tenzer, Christopher, additional, Todaro, Michela, additional, Torok, Gabreil, additional, Trois, Alessio, additional, Vacchi, Andrea, additional, Virgilli, Enrico, additional, Xiong, Hao, additional, Wang, Jian, additional, Wang, Xianqi, additional, Winter, Berend, additional, Wu, Xin, additional, Xu, Yupeng, additional, Zampa, Gianluigi, additional, Zampa, Nicola, additional, Zdziarski, Andrei, additional, Zhang, Long, additional, Zhang, Shu, additional, Zhang, Shuang-Nan, additional, Zhang, Wenda, additional, Zhang, Xiaoli, additional, Zhang, Zhen, additional, Zhou, Yupeng, additional, and Zorzi, Nicola, additional

Published
2022
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10. The enhanced X-ray Timing and Polarimetry mission – eXTP:an update on its scientific cases, mission profile and development status

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Zhang, Shuang Nan, Santangelo, Andrea, Xu, Yupeng, Feroci, Marco, Hernanz, Margarita, Lu, Fangjun, Chen, Yong, Feng, Hua, Nandra, Kirpal, Jiang, Weichun, Svoboda, Jiri, Brandt, Søren, Schanne, Stéphane, Zand, Jean, Michalska, Malgorzata, Bozzo, Enrico, Kalemci, Emrah, Agudo, Ivan, Ahangarianabhari, Mahdi, Aitink-Kroes, Gabby, Ambrosi, Giovanni, Ambrosino, Filippo, An, Zhenghua, Perez Torres, Miguel Angel, Antonelli, Matias, Argan, Andrea, Babinec, Viktor, Baldini, Luca, Barbera, Marco, van Baren, Coen, Baudin, David, Bayer, Jörg, Bellazzini, Ronaldo, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Bi, Xingzi, Boezio, Mirko, Bonvicini, Valter, Bonvicini, Walter, Bordas, Pol, Borghese, Alice, Borghi, Giacomo, Bouyjou, Florent, Bozkurt, Ayhan, Brez, Alessandro, Brienza, Daniele, Cadoux, Franck, Campana, Riccardo, Cao, Jiewei, Cao, Xuelei, Casares, Jorge, Cavazzuti, Elisabetta, Ceraudo, Francesco, Chen, Tianxiang, Chen, Wen, Chen, Can, Chen, Yupeng, Chen, Xin, Chen, Yehai, Chenevez, Jerome, Cheng, Yaodong, Cirrincione, Daniela, Civitani, Marta, Cong, Min, Zelati, Francesco Coti, Cui, Weiwei, Cui, Tao, Cui, Wei, Dai, Boyu, Dauser, Thomas, De Angelis, Nicolas, De Marco, Barbara, De Rosa, Alessandra, Monte, Ettore Del, Cosimo, Sergio Di, Diebold, Sebastian, Dilillo, Giuseppe, Ding, Fei, Dohnal, Roman, Dong, Zefang, Donnarumma, Immacolata, Dovciak, Michal, Du, Yuanyuan, Ducci, Lorenzo, Evangelista, Yuri, Fan, Qingmei, Favre, Yannick, Ferrés, Patrícia, Fiandrini, Emanuele, Ficorella, Francesco, Fuschino, Fabio, Gálvez, José Luis, Gao, Na, Gao, Min, Ge, Yuqiang, Ge, Mingyu, Gevin, Olivier, Grassi, Marco, Gu, Yudong, Gu, Quanying, Guan, Ju, Guedel, Manuel, Han, Xingbo, Han, Dawei, He, Huilin, He, Junwang, Hedderman, Paul, den Herder, Jan Willem, Hong, Bin, Hormaetxe, Ander, Hou, Dongjie, Hu, Zexun, Hu, Hao, Hu, Qingbao, Hu, Yu, Huang, Yue, Huang, Jiangjiang, Huang, Qiushi, Huo, Jia, Hynek, Richard, Iwasawa, Kazumi, Izzo, Lucca, Ji, Long, Jia, Shumei, Jiang, Bowen, Jiang, Wei, Jiang, Jiechen, Jiang, Xiaowei, Jiao, Yang, Jin, Ge, Jin, Fan, Jose, Jordi, Karas, Vladimir, Kennedy, Thomas, Kirsch, Christian, Kole, Merlin, Komarek, Martin, Kreykenbohm, Ingo, Kuiper, Lucien, Kuvvetli, Irfan, Labanti, Claudio, Latronico, Luca, Laubert, Phillip, Li, Tao, Li, Longhui, Li, Hong, Li, Duo, Li, Wei, Li, Maoshun, Li, Gang, Li, Xiaobo, Li, Chengkui, Li, Bing, Li, Haibo, Liang, Hong, Liao, Qiuyan, Liao, Jinyuan, Limousin, Olivier, Lin, Yanjian, Linares, Manuel, Liu, Rui, Liu, Yichen, Liu, Zhihao, Liu, Hongwei, Liu, Xiaojing, Liu, Xiaohua, Cicero, Ugo Lo, Loehring, Jens, Lombardi, Giovanni, Lorenz, Maximilian, Lu, Bing, Lucchesi, Leonardo, Luo, Tao, Luo, Laidan, Ma, Jia, Ma, Xiang, Macera, Daniele, Malcovati, Piero, Manfreda, Alberto, Paredes, Josep Maria, Marinucci, Andrea, Martindale, Adrian, Meidinger, Norbert, Mele, Filippo, Mendes, Vasco, Meng, Bin, Merkl, Martin, Meuris, Aline, Miniutti, Giovanni, Minuti, Massimo, Morbidini, Alfredo, Morgante, Gianluca, Muleri, Fabio, Munini, Riccardo, Mussolin, Lorenzo, Negri, Barbara, Nie, Jianyin, Novák, Petr, Nowosielski, Witold, Nuti, Alessio, Onat, Ahmet, Orleanski, Piotr, Orsini, Leonardo, Ottensamer, Roland, Ou, Ge, Pacciani, Luigi, Paltani, Stephane, Pan, Teng, Pan, Kai, Pareschi, Giovanni, Patruno, Alessandro, Pepponi, Giancarlo, Perinati, Emanuele, Piazzolla, Raffaele, Picciotto, Antonino, Piemonte, Claudio, Pinchera, Michele, Pliego, Samuel, Poutanen, Juri, Qi, Liqiang, Qi, Fazhi, Qiang, Pengfei, Qiao, Fangjian, Qiao, Zheng, Qiu, Xiangbiao, Qiu, Chengbo, Qu, Jinlu, Rachevski, Alexandre, Rashevskaia, Irina, Rea, Nanda, Ribo, Marc, de la Rie, Rob, Rodriguez, Jerome, Gil, Pablo Rodríguez, Sala, Gloria, Schanz, Thomas, Serafinelli, Roberto, Sgro, Carmelo, Shen, Zhengxiang, Sheng, Lizhi, Shi, Jingyan, Sironi, Giorgia, Skup, Konrad, Song, Liming, Song, Zeyu, Song, Jiangbo, Spandre, Gloria, Spiga, Daniele, Su, Yongquan, Sun, Liang, Sungur, Müberra, Svéda, Libor, Tagliaferri, Gianpiero, Tan, Ying, Tao, Lian, Tcherniak, Denis, Tenzer, Chris, Todaro, Michela, Tolos, Laura, Torok, Gabriel, Torres, Diego F., Trois, Alessio, Turhan, Onur, Uttley, Phil, Vacchi, Andrea, Virgilli, Enrico, Vogel, Channah, Walton, Dave, Wang, Jian, Wang, Xianqi, Wang, Bo, Wang, Langping, Wang, Xiaofeng, Wang, Dianlong, Wang, Yusa, Wang, Juan, Wang, Hao, Wang, Ruijie, Wang, Ping, Wang, Lingjun, Wang, Wenshuai, Wang, Tian, Wang, Haoyu, Wang, Zhanshan, Watts, Anna L., Wen, Xiangyang, Wilms, Jörn, Winter, Berend, Wu, Xin, Wu, Chao, Wu, Zhenyu, Wu, Qiong, Wu, Kaiji, Xiong, Hao, Xiong, Shaolin, Xu, Wei, Xu, Zhao, Xu, Jingjing, Xu, Xiongwei, Xue, Jiadai, Yan, Yongqing, Yan, Xingtao, Yang, Xianghui, Yang, Yanji, Yang, Xiongtao, Yang, Sheng, Yang, Jiawei, Yang, Yingquan, Yi, Shuxu, Yu, Yonggao, Yu, Ke, Zampa, Ganluigi, Zampa, Nicola, Zane, Silvia, Zdziarski, Andrzej A., Zhang, Long, Zhang, Shu, Zhang, Wenda, Zhang, Xiaoli, Zhang, Zhen, Zhang, Jiawei, Zhang, Fan, Zhang, Ziliang, Zhang, Dali, Zhang, Honglin, Zhang, Aimei, Zhang, Tong, Zhang, Hongmei, Zhang, Juan, Zhang, Liang, Zhang, Yueting, Zhao, Li, Zhao, Baosheng, Zhao, Zijian, Zhao, Xiaofan, Zhao, Haisheng, Zhao, Xiaoyun, Zheng, Shijie, Zhou, Yupeng, Zhou, Xiaohong, Zhu, Jiahuan, Zhu, Yuxuan, Zhu, Cheng, Zhu, Zhencai, Zorzi, Nicola, Zwart, Frans, den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Zhang, Shuang Nan, Santangelo, Andrea, Xu, Yupeng, Feroci, Marco, Hernanz, Margarita, Lu, Fangjun, Chen, Yong, Feng, Hua, Nandra, Kirpal, Jiang, Weichun, Svoboda, Jiri, Brandt, Søren, Schanne, Stéphane, Zand, Jean, Michalska, Malgorzata, Bozzo, Enrico, Kalemci, Emrah, Agudo, Ivan, Ahangarianabhari, Mahdi, Aitink-Kroes, Gabby, Ambrosi, Giovanni, Ambrosino, Filippo, An, Zhenghua, Perez Torres, Miguel Angel, Antonelli, Matias, Argan, Andrea, Babinec, Viktor, Baldini, Luca, Barbera, Marco, van Baren, Coen, Baudin, David, Bayer, Jörg, Bellazzini, Ronaldo, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Bi, Xingzi, Boezio, Mirko, Bonvicini, Valter, Bonvicini, Walter, Bordas, Pol, Borghese, Alice, Borghi, Giacomo, Bouyjou, Florent, Bozkurt, Ayhan, Brez, Alessandro, Brienza, Daniele, Cadoux, Franck, Campana, Riccardo, Cao, Jiewei, Cao, Xuelei, Casares, Jorge, Cavazzuti, Elisabetta, Ceraudo, Francesco, Chen, Tianxiang, Chen, Wen, Chen, Can, Chen, Yupeng, Chen, Xin, Chen, Yehai, Chenevez, Jerome, Cheng, Yaodong, Cirrincione, Daniela, Civitani, Marta, Cong, Min, Zelati, Francesco Coti, Cui, Weiwei, Cui, Tao, Cui, Wei, Dai, Boyu, Dauser, Thomas, De Angelis, Nicolas, De Marco, Barbara, De Rosa, Alessandra, Monte, Ettore Del, Cosimo, Sergio Di, Diebold, Sebastian, Dilillo, Giuseppe, Ding, Fei, Dohnal, Roman, Dong, Zefang, Donnarumma, Immacolata, Dovciak, Michal, Du, Yuanyuan, Ducci, Lorenzo, Evangelista, Yuri, Fan, Qingmei, Favre, Yannick, Ferrés, Patrícia, Fiandrini, Emanuele, Ficorella, Francesco, Fuschino, Fabio, Gálvez, José Luis, Gao, Na, Gao, Min, Ge, Yuqiang, Ge, Mingyu, Gevin, Olivier, Grassi, Marco, Gu, Yudong, Gu, Quanying, Guan, Ju, Guedel, Manuel, Han, Xingbo, Han, Dawei, He, Huilin, He, Junwang, Hedderman, Paul, den Herder, Jan Willem, Hong, Bin, Hormaetxe, Ander, Hou, Dongjie, Hu, Zexun, Hu, Hao, Hu, Qingbao, Hu, Yu, Huang, Yue, Huang, Jiangjiang, Huang, Qiushi, Huo, Jia, Hynek, Richard, Iwasawa, Kazumi, Izzo, Lucca, Ji, Long, Jia, Shumei, Jiang, Bowen, Jiang, Wei, Jiang, Jiechen, Jiang, Xiaowei, Jiao, Yang, Jin, Ge, Jin, Fan, Jose, Jordi, Karas, Vladimir, Kennedy, Thomas, Kirsch, Christian, Kole, Merlin, Komarek, Martin, Kreykenbohm, Ingo, Kuiper, Lucien, Kuvvetli, Irfan, Labanti, Claudio, Latronico, Luca, Laubert, Phillip, Li, Tao, Li, Longhui, Li, Hong, Li, Duo, Li, Wei, Li, Maoshun, Li, Gang, Li, Xiaobo, Li, Chengkui, Li, Bing, Li, Haibo, Liang, Hong, Liao, Qiuyan, Liao, Jinyuan, Limousin, Olivier, Lin, Yanjian, Linares, Manuel, Liu, Rui, Liu, Yichen, Liu, Zhihao, Liu, Hongwei, Liu, Xiaojing, Liu, Xiaohua, Cicero, Ugo Lo, Loehring, Jens, Lombardi, Giovanni, Lorenz, Maximilian, Lu, Bing, Lucchesi, Leonardo, Luo, Tao, Luo, Laidan, Ma, Jia, Ma, Xiang, Macera, Daniele, Malcovati, Piero, Manfreda, Alberto, Paredes, Josep Maria, Marinucci, Andrea, Martindale, Adrian, Meidinger, Norbert, Mele, Filippo, Mendes, Vasco, Meng, Bin, Merkl, Martin, Meuris, Aline, Miniutti, Giovanni, Minuti, Massimo, Morbidini, Alfredo, Morgante, Gianluca, Muleri, Fabio, Munini, Riccardo, Mussolin, Lorenzo, Negri, Barbara, Nie, Jianyin, Novák, Petr, Nowosielski, Witold, Nuti, Alessio, Onat, Ahmet, Orleanski, Piotr, Orsini, Leonardo, Ottensamer, Roland, Ou, Ge, Pacciani, Luigi, Paltani, Stephane, Pan, Teng, Pan, Kai, Pareschi, Giovanni, Patruno, Alessandro, Pepponi, Giancarlo, Perinati, Emanuele, Piazzolla, Raffaele, Picciotto, Antonino, Piemonte, Claudio, Pinchera, Michele, Pliego, Samuel, Poutanen, Juri, Qi, Liqiang, Qi, Fazhi, Qiang, Pengfei, Qiao, Fangjian, Qiao, Zheng, Qiu, Xiangbiao, Qiu, Chengbo, Qu, Jinlu, Rachevski, Alexandre, Rashevskaia, Irina, Rea, Nanda, Ribo, Marc, de la Rie, Rob, Rodriguez, Jerome, Gil, Pablo Rodríguez, Sala, Gloria, Schanz, Thomas, Serafinelli, Roberto, Sgro, Carmelo, Shen, Zhengxiang, Sheng, Lizhi, Shi, Jingyan, Sironi, Giorgia, Skup, Konrad, Song, Liming, Song, Zeyu, Song, Jiangbo, Spandre, Gloria, Spiga, Daniele, Su, Yongquan, Sun, Liang, Sungur, Müberra, Svéda, Libor, Tagliaferri, Gianpiero, Tan, Ying, Tao, Lian, Tcherniak, Denis, Tenzer, Chris, Todaro, Michela, Tolos, Laura, Torok, Gabriel, Torres, Diego F., Trois, Alessio, Turhan, Onur, Uttley, Phil, Vacchi, Andrea, Virgilli, Enrico, Vogel, Channah, Walton, Dave, Wang, Jian, Wang, Xianqi, Wang, Bo, Wang, Langping, Wang, Xiaofeng, Wang, Dianlong, Wang, Yusa, Wang, Juan, Wang, Hao, Wang, Ruijie, Wang, Ping, Wang, Lingjun, Wang, Wenshuai, Wang, Tian, Wang, Haoyu, Wang, Zhanshan, Watts, Anna L., Wen, Xiangyang, Wilms, Jörn, Winter, Berend, Wu, Xin, Wu, Chao, Wu, Zhenyu, Wu, Qiong, Wu, Kaiji, Xiong, Hao, Xiong, Shaolin, Xu, Wei, Xu, Zhao, Xu, Jingjing, Xu, Xiongwei, Xue, Jiadai, Yan, Yongqing, Yan, Xingtao, Yang, Xianghui, Yang, Yanji, Yang, Xiongtao, Yang, Sheng, Yang, Jiawei, Yang, Yingquan, Yi, Shuxu, Yu, Yonggao, Yu, Ke, Zampa, Ganluigi, Zampa, Nicola, Zane, Silvia, Zdziarski, Andrzej A., Zhang, Long, Zhang, Shu, Zhang, Wenda, Zhang, Xiaoli, Zhang, Zhen, Zhang, Jiawei, Zhang, Fan, Zhang, Ziliang, Zhang, Dali, Zhang, Honglin, Zhang, Aimei, Zhang, Tong, Zhang, Hongmei, Zhang, Juan, Zhang, Liang, Zhang, Yueting, Zhao, Li, Zhao, Baosheng, Zhao, Zijian, Zhao, Xiaofan, Zhao, Haisheng, Zhao, Xiaoyun, Zheng, Shijie, Zhou, Yupeng, Zhou, Xiaohong, Zhu, Jiahuan, Zhu, Yuxuan, Zhu, Cheng, Zhu, Zhencai, Zorzi, Nicola, and Zwart, Frans

Abstract

The enhanced X-ray Timing and Polarimetry mission (eXTP) is a flagship observatory for X-ray timing, spectroscopy and polarimetry developed by an International Consortium. Thanks to its very large collecting area, good spectral resolution and unprecedented polarimetry capabilities, eXTP will explore the properties of matter and the propagation of light in the most extreme conditions found in the Universe. eXTP will, in addition, be a powerful X-ray observatory. The mission will continuously monitor the X-ray sky, and will enable multiwavelength and multi-messenger studies. The mission is currently in phase B, which will be completed in the middle of 2022.

Published
2022

11. The digital data processing concepts of the large area detector and the wide field monitor onboard eXTP

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Xiong, Hao, Argan, Andrea, Baudin, David, Bayer, Jörg, Bouyjou, Florent, De Angelis, Nicolas, Del Monte, Ettore, Evangelista, Yuri, Favre, Yannick, Feroci, Marco, Galvez, José-Luis, Gevin, Olivier, Hedderman, Paul, Hernanz, Margarita, Kole, Merlin Reynaard, Meuris, Aline, Pliego-Caballero, Samuel, Santangelo, Andrea, Tenzer, Chris, Trois, Alessio, Wang, Xianqi, and Zampa, Gianluigi

Published
2022
Full Text
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12. The large area detector onboard the eXTP mission

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Feroci, Marco, Ambrosi, Giovanni, Ambrosino, Filippo, Antonelli, Matias, Argan, Andrea, Babinec, Viktor, Barbera, Marco, Bayer, Joerg, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Bi, Xingzi, Boezio, Mirko, Bonvicini, Walter, Borghi, Giacomo, Bozzo, Enrico, Baudin, David, Bouyjou, Florent, Brienza, Daniele, Cadoux, Franck, Campana, Riccardo, Cao, Jiewei, Cavazzuti, Elisabetta, Ceraudo, Francesco, Chen, Tianxiang, Chen, Wen, Cirrincione, Daniela, De Angelis, Nicolas, De Rosa, Alessandra, Del Monte, Ettore, Di Cosimo, Sergio, Dilillo, Giuseppe, Dohnal, Roman, Donnarumma, Immacolata, Evangelista, Yuri, Fan, Qingmei, Favre, Yannick, Fiandrini, Emanuele, Ficorella, Francesco, Fuschino, Fabio, Gao, Na, Gevin, Olivier, Grassi, Marco, Guedel, Manuel, Han, Xingbo, He, Huilin, Hedderman, Paul, den Herder, Jan-Willem, Hynek, Richard, Hong, Bin, Jin, Ge, Kole, Merlin, Karas, Vladimir, Komarek, Martin, Labanti, Claudio, Li, Loghui, Li, Tianming, Liang, Hong, Limousin, Olivier, Liu, Rui, Lo Cicero, Ugo, Lohering, Jens, Lombardi, Giovanni, Lu, Fang-Jun, Luo, Tao, Malcovati, Piero, Mao, Hanqi, Marinucci, Andrea, Mele, Filippo, Mendes, Vasco, Merkl, Martin, Meuris, Aline, Michalska, Malgorzata, Morbidini, Alfredo, Morgante, Gianluca, Muleri, Fabio, Munini, Riccardo, Mussolin, Lorenzo, Negri, Barbara, Novák, Petr, Nowosielski, Witold, Nuti, Alessio, Orleanski, Piotr, Ottensamer, Roland, Pacciani, Luigi, Paltani, Stephane, Pan, Teng, Pepponi, Giancarlo, Perinati, Emanuele, Piazzolla, Raffaele, Picciotto, Antonino, Pliego, Samuel, Rachevski, Alexandre, Rashevskaia, Irina, Santangelo, Andrea, Schanne, Stéphane, Serafinelli, Roberto, Skup, Konrad, Sveda, Libor, Svoboda, Jiri, Tenzer, Chris, Todaro, Michela, Torok, Gabriel, Trois, Alessio, Vacchi, Andrea, Virgilli, Enrico, Xiong, Hao, Wang, Jian, Wang, Xianqi, Winter, Berend, Wu, Xin, Xu, Yupeng, Zampa, Ganluigi, Zampa, Nicola, Zdziarski, Andrzej A., Zhang, Long, Zhang, Shu, Zhang, Shuang-Nan, Zhang, Wenda, Zhang, Xiaoli, Zhang, Zhen, Zhou, Yupeng, and Zorzi, Nicola

Published
2022
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14. CMOS Analog Front End Design for Particle Energy Measurement in Space Environment

Author

Bouyjou, Florent, Bernal, Olivier, Tap, Hélène, Sauvaud, Jean-André, Jean, Pierre, Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Équipe Optoélectronique pour les Systèmes Embarqués (LAAS-OSE), Laboratoire d'analyse et d'architecture des systèmes (LAAS), Université Toulouse - Jean Jaurès (UT2J)-Université Toulouse 1 Capitole (UT1), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université Fédérale Toulouse Midi-Pyrénées-Université Toulouse - Jean Jaurès (UT2J)-Université Toulouse 1 Capitole (UT1), Université Fédérale Toulouse Midi-Pyrénées, Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse Capitole (UT Capitole), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Université Toulouse - Jean Jaurès (UT2J), Université de Toulouse (UT)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université de Toulouse (UT)-Université Toulouse Capitole (UT Capitole), Université de Toulouse (UT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), and Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)

Subjects
[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics
Abstract

International audience; In situ studies of the geospace environment, including space weather monitoring, is mainly based on the measurements of particles and fields. The particle content of the Earth’s magnetosphere is studied with electron and ion detectors in various energy ranges, from the cold and dense eV solar wind to the MeV radiation belts. Here, the in situ high-energy (50 keV to 725keV) electron measurement is targeted. The design and development of space embedded electronic equipment require a specific approach . An Analog-Front-End (AFE) design methodology is proposed to optimizenoise, bandwidth, consumption, crosstalk and radiation hardness performances of such AFEs for Si semiconductor detectors. The conception ofan Analog-Front-End optimized in noise, band width, consumption, crosstalk and radiation hardness, dedicated to a silicon (SiA) detector. Each channel includes an 8 bits successive approximation register (SAR) ADC in order to digitize the incident electron energy. The chip was designed in a0.35 μm HV CMOS process. The ASIC measurements have shown that for a charge range of 0.6 fC to 32 fC , the charge - to - voltage conversion gainis approximately 60 mV/fC. The equivalent noise charge (ENC) is 3119 e- for 40pF input parasitic capacitance while consuming 2.5 mW. The circuitcan perform measurements up to a 650 kHz rate. The next step is to characterize the ASIC associated with the SC detector in a vacuum chamber. Furthermore, the total ionisation dose (TID) and the single event effect ( SEE ) tolerances must also be evaluated

Published
2014

15. Qualifying a CMOS Instrumentation Chain for Charged Particles Detection in the Space Environment

Author

Bouyjou, Florent, Bernal, Olivier, Tap, Hélène, Picaut, Guillaume, Sauvaud, Jean-André, Équipe Optoélectronique pour les Systèmes Embarqués (LAAS-OSE), Laboratoire d'analyse et d'architecture des systèmes (LAAS), Université Toulouse - Jean Jaurès (UT2J)-Université Toulouse 1 Capitole (UT1), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université Fédérale Toulouse Midi-Pyrénées-Université Toulouse - Jean Jaurès (UT2J)-Université Toulouse 1 Capitole (UT1), Université Fédérale Toulouse Midi-Pyrénées, Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), RTRA-STAE, ESA, Université Toulouse Capitole (UT Capitole), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Université Toulouse - Jean Jaurès (UT2J), Université de Toulouse (UT)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université de Toulouse (UT)-Université Toulouse Capitole (UT Capitole), Université de Toulouse (UT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), and Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)

Subjects
CMOS ASIC, AFE, particle detection, Top hat electrosctatic analyser, [SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics, charge conversion
Abstract

7 pages; International audience; For the solar system exploration and the distant universe study, the in-situ particle energy measurement and/or the electron/ion event detection are needed. For our on-board satellite application, the particle sensor that is used to convert particle momentum into measurable electrical charges is a Microchannel plate (MCP). The performances of such a sensor depend on the Analog-Front-End (AFE) circuit used to process the incoming charges. Consequently, a CMOS instrumentation chain for charged particle detection has been designed and tested under space environment. This AFE contains 16 channels, all of which includes a charge pre-amplifier (CPA), a pulse shaper (PS) and a monostable circuit to perform the detection. Using a standard 0.35 μm CMOS process, the proposed AFE has a conversion gain of 0.9mV/fC for electrons and a power consumption of 2.15 mW per channel. Its dynamic range is 79 dB and it is possible to convert charges up to 1.5 pC. The circuit works properly from -20 to 80°C with a measured analog gain variation of 1μV.fC-1.K-1. As far as crosstalk is concerned, experiments show that the proposed instrumentation chain can detect negative charges down to 122 fC without any ambiguity. Further, the proposed chain was irradiated at an average rate of 140 rads (Si) per hour up to 360 krad without any functionality loss.

Published
2012

16. Nouvelles chaînes d'instrumentation intégrées multivoies pour l'astrophysique

Author

Bouyjou, Florent, Institut National Polytechnique de Toulouse - INPT (FRANCE), Équipe Optoélectronique pour les Systèmes Embarqués (LAAS-OSE), Laboratoire d'analyse et d'architecture des systèmes (LAAS), Université Toulouse - Jean Jaurès (UT2J)-Université Toulouse 1 Capitole (UT1), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université Fédérale Toulouse Midi-Pyrénées-Université Toulouse - Jean Jaurès (UT2J)-Université Toulouse 1 Capitole (UT1), Université Fédérale Toulouse Midi-Pyrénées, Institut National Polytechnique de Toulouse - INPT, H.TAP-BETEILLE, Université Toulouse Capitole (UT Capitole), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Université Toulouse - Jean Jaurès (UT2J), Université de Toulouse (UT)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université de Toulouse (UT)-Université Toulouse Capitole (UT Capitole), Université de Toulouse (UT), and Institut National Polytechnique de Toulouse - Toulouse INP (FRANCE)

Subjects
Technologie CMOS et ASIC analogique / numérique, Chaînes d'instrumentation intégrées, numérique, Technologie CMOS, Détecteurs MCP et Semi-conducteurs, ASIC analogique, Environnement spatial, [SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/Microelectronics, Chaînes d’instrumentation intégrées
Abstract

L'exploration du système solaire et l'étude de l'univers lointain sont encore sources de découvertes et de mystère pour la communauté scientifique et pour l’humanité en général. Ces observations sont actuellement principalement basées sur la mesure d’ions et de particules in-situ qui constituent ces milieux. Les instruments d’observation intègrent des détecteurs spatiaux, utilisés pour convertir l'énergie des particules en charges électriques mesurables. Ces derniers sont étroitement liés à leur électronique analogique ou Analog-Front-End (AFE) et cette combinaison forme des chaines astrophysiques de détection appelées « sensor heads ». Depuis quelques années, la volonté d’améliorer les résolutions spatiale et spectrale des détecteurs nécessite la conception d’une électronique intégrée multivoies. Ainsi, une électronique spatiale de type Application Specific Integrated Circuit (ASIC) doit être développée. Cela permet d’une part de s’adapter au mieux à chaque détecteur pour en optimiser les performances ; et d’autre part de bénéficier des multiples avantages inhérents à l’utilisation d’une technologie CMOS : diminuer les dimensions et les temps de transit des signaux, intégration multifonctions, réduction des coûts pour une fabrication de masse et effets parasites étudiés et bien connus. Cependant les contraintes spatiales exigent une qualification draconienne du circuit. En effet, ces environnent radiatifs peuvent endommager les systèmes électroniques embarqués à bord des missions spatiales. Grâce à la réduction des dimensions, il ne semble plus opportun aujourd’hui d’utiliser des technologies dédiées au spatial (type SOI ou biCMOS spécifiques) mais plutôt de mettre en œuvre des techniques de durcissement par design (RHBD) sur des technologies standards qui sont moins onéreuses et plus performantes. L’objectif de cette thèse est la conception de nouvelles chaînes d’instrumentations intégrées multivoies pour le spatial. Ce travail, co-financé par le CNES et le CNRS, s’est inscrit dans le cadre d’un projet soutenu par le Réseau Thématique de Recherche Avancée Sciences et Technologies pour l’Aéronautique et l’Espace (RTRA STAE) entre 2008 et 2011, intitulé CASA (Chaines AStrophysiques et leur instrumentation Associée). Au cours de cette thèse nous avons conçu 2 ASICs associés à 2 types de détecteurs spatiaux bien distincts. Le premier permet de compter les électrons en sortie d’une microchannel plate (MCP) tandis que le deuxième permet de quantifier le niveau d’énergie perdu par les e- en pénétrant dans un SC. L’étude de ces différents détecteurs doit d’abord être faite afin de les modéliser pour une parfaite adéquation avec leur électronique de détection. Ensuite, une optimisation des chaînes de conversion en vitesse, bruit et consommation est réalisée. Enfin, une méthodologie de savoir faire au niveau du traitement des informations doit être développée pour pérenniser l’expérience emmagasinée durant ces travaux.

Published
2011

19. The digital data processing concepts of the large area detector and the wide field monitor onboard eXTP.

Author

Xiong, Hao, Argan, Andrea, Baudin, David, Bayer, Jörg, Bouyjou, Florent, De Angelis, Nicolas, Del Monte, Ettore, Evangelista, Yuri, Favre, Yannick, Feroci, Marco, Galvez, José-Luis, Gevin, Olivier, Hedderman, Paul, Hernanz, Margarita, Kole, Merlin Reynaard, Meuris, Aline, Pliego-Caballero, Samuel, Santangelo, Andrea, Tenzer, Chris, and Trois, Alessio

Published
2022
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20. The large area detector onboard the eXTP mission.

Author

Feroci, Marco, Ambrosi, Giovanni, Ambrosino, Filippo, Antonelli, Matias, Argan, Andrea, Babinec, Viktor, Barbera, Marco, Bayer, Joerg, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Bi, Xingzi, Boezio, Mirko, Bonvicini, Walter, Borghi, Giacomo, Bozzo, Enrico, Baudin, David, Bouyjou, Florent, Brienza, Daniele, and Cadoux, Franck

Published
2022
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21. The Large Area Detector onboard the eXTP mission

Author

Marco Feroci, Giovanni Ambrosi, Filippo Ambrosino, Matias Antonelli, Andrea Argan, Viktor Babinec, Marco Barbera, Jörg Bayer, Pierluigi Bellutti, Bruna Bertucci, Giuseppe Bertuccio, Xingzi Bi, Mirko Boezio, Walter Bonvicini, Giacomo Borghi, Enrico Bozzo, David Baudin, Florent Bouyjou, Daniele Brienza, Franck Cadoux, Riccardo Campana, Jiewei Cao, Elisabetta Cavazzuti, Francesco Ceraudo, Tianxiang Chen, Wen Chen, Daniela Cirrincione, Nicolas De Angelis, Alessandra De Rosa, Ettore Del Monte, Sergio Di Cosimo, Giuseppe Dilillo, Roman Dohnal, Immacolata Donnarumma, Yuri Evangelista, Qingmei Fan, Yannick Favre, Emanuele Fiandrini, Francesco Ficorella, Fabio Fuschino, Na Gao, Olivier Gevin, Marco Grassi, Manuel Guedel, Xingbo Han, Huilin He, Paul Hedderman, jan-willem den herder, Richard Hynek, Bing Hong, Ge Jin, Merlin Kole, Vladimír Karas, Martin Komarek, Claudio Labanti, Loghui Li, Tianming Li, Hong Liang, Olivier Limousin, Rui Liu, Ugo Lo Cicero, Jens Lohering, Giovanni Lombardi, Fang-Jun Lu, Tao Luo, Piero Malcovati, Hanqi Mao, Andrea Marinucci, Filippo Mele, Vasco Mendes, Martin Merkl, Aline Meuris, Małgorzata Michalska, Alfredo Morbidini, Gianluca Morgante, Fabio Muleri, Riccardo Munini, Lorenzo Mussolin, Barbara Negri, Petr Novak, Witold Nowosielski, Alessio Nuti, Piotr Orleanski, Roland Ottensamer, Luigi Pacciani, Stephane Paltani, Teng Pan, Giancarlo Pepponi, Emanuele Perinati, Raffaele Piazzolla, Antonino Picciotto, Samuel Pliego, Alexandre Rachevski, Irina Rashevskaia, Andrea Santangelo, Roberto Serafinelli, Stéphane Schanne, Konrad Skup, Libor Sveda, Jiri Svoboda, Christopher Tenzer, Michela Todaro, Gabreil Torok, Alessio Trois, Andrea Vacchi, Enrico Virgilli, Hao Xiong, Jian Wang, Xianqi Wang, Berend Winter, Xin Wu, Yupeng Xu, Gianluigi Zampa, Nicola Zampa, Andrei Zdziarski, Long Zhang, Shu Zhang, Shuang-Nan Zhang, Wenda Zhang, Xiaoli Zhang, Zhen Zhang, Yupeng Zhou, Nicola Zorzi, den Herder, Jan-Willem A., Feroci, Marco, Ambrosi, Giovanni, Ambrosino, Filippo, Antonelli, Matia, Argan, Andrea, Babinec, Viktor, Barbera, Marco, Bayer, Jörg, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Bi, Xingzi, Boezio, Mirko, Bonvicini, Walter, Borghi, Giacomo, Bozzo, Enrico, Baudin, David, Bouyjou, Florent, Brienza, Daniele, Cadoux, Franck, Campana, Riccardo, Cao, Jiewei, Cavazzuti, Elisabetta, Ceraudo, Francesco, Chen, Tianxiang, Chen, Wen, Cirrincione, Daniela, De Angelis, Nicola, De Rosa, Alessandra, Del Monte, Ettore, Di Cosimo, Sergio, Dilillo, Giuseppe, Dohnal, Roman, Donnarumma, Immacolata, Evangelista, Yuri, Fan, Qingmei, Favre, Yannick, Fiandrini, Emanuele, Ficorella, Francesco, Fuschino, Fabio, Gao, Na, Gevin, Olivier, Grassi, Marco, Guedel, Manuel, Han, Xingbo, He, Huilin, Hedderman, Paul, den herder, jan-willem, Hynek, Richard, Hong, Bing, Jin, Ge, Kole, Merlin, Karas, Vladimír, Komarek, Martin, Labanti, Claudio, Li, Loghui, Li, Tianming, Liang, Hong, Limousin, Olivier, Liu, Rui, Lo Cicero, Ugo, Lohering, Jen, Lombardi, Giovanni, Lu, Fang-Jun, Luo, Tao, Malcovati, Piero, Mao, Hanqi, Marinucci, Andrea, Mele, Filippo, Mendes, Vasco, Merkl, Martin, Meuris, Aline, Michalska, Małgorzata, Morbidini, Alfredo, Morgante, Gianluca, Muleri, Fabio, Munini, Riccardo, Mussolin, Lorenzo, Negri, Barbara, Novak, Petr, Nowosielski, Witold, Nuti, Alessio, Orleanski, Piotr, Ottensamer, Roland, Pacciani, Luigi, Paltani, Stephane, Pan, Teng, Pepponi, Giancarlo, Perinati, Emanuele, Piazzolla, Raffaele, Picciotto, Antonino, Pliego, Samuel, Rachevski, Alexandre, Rashevskaia, Irina, Santangelo, Andrea, Serafinelli, Roberto, Schanne, Stéphane, Skup, Konrad, Sveda, Libor, Svoboda, Jiri, Tenzer, Christopher, Todaro, Michela, Torok, Gabreil, Trois, Alessio, Vacchi, Andrea, Virgilli, Enrico, Xiong, Hao, Wang, Jian, Wang, Xianqi, Winter, Berend, Wu, Xin, Xu, Yupeng, Zampa, Gianluigi, Zampa, Nicola, Zdziarski, Andrei, Zhang, Long, Zhang, Shu, Zhang, Shuang-Nan, Zhang, Wenda, Zhang, Xiaoli, Zhang, Zhen, Zhou, Yupeng, and Zorzi, Nicola

Subjects
Settore FIS/05 - Astronomia E Astrofisica, EXTP, LAD, Silicon Drift Detector, X-ray timing
Abstract

The Large Area Detector (LAD) is the high-throughput, spectral-timing instrument onboard the eXTP mission, a flagship mission of the Chinese Academy of Sciences and the China National Space Administration, with a large European participation coordinated by Italy and Spain. The eXTP mission is currently performing its phase B study, with a target launch at the end-2027. The eXTP scientific payload includes four instruments (SFA, PFA, LAD and WFM) offering unprecedented simultaneous wide-band X-ray timing and polarimetry sensitivity. The LAD instrument is based on the design originally proposed for the LOFT mission. It envisages a deployed 3.2 m2 effective area in the 2-30 keV energy range, achieved through the technology of the large-area Silicon Drift Detectors - offering a spectral resolution of up to 200 eV FWHM at 6 keV - and of capillary plate collimators - limiting the field of view to about 1 degree. In this paper we will provide an overview of the LAD instrument design, its current status of development and anticipated performance.

Published
2022

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