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49 results on '"Gevin, Olivier"'

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. B-BOP, the SPICA Imaging Polarimeter

Author

Revéret, Vincent, Sauvage, Marc, Adami, Obaïd, Aliane, Abdelkader, Berthé, Michel, Bounissou, Sophie, de la Broïse, Xavier, Chimeno, Marcos, Demonti, Amala, Delabrouille, Jacques, Delisle, Cyrille, Doumayrou, Eric, Duband, Lionel, Dubreuil, Didier, Dussopt, Laurent, Frugier, Pierre-Antoine, Gennet, Camille, Gevin, Olivier, Goudon, Valérie, Kaya, Hacile, Marquet, Benoît, Martignac, Jérôme, Martin, Sylvain, Najarro, Paco, Navick, Xavier-François, Perez, Javier, Plesseria, Jean-Yves, Poglitsch, Albrecht, Rodriguez, Louis, Redondo, Josefina Torres, and Visticot, François

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We present the B-BOP instrument, a polarimetric camera on board the future ESA-JAXA SPICA far-infrared space observatory. B-BOP will allow the study of the magnetic field in various astrophysical environments thanks to its unprecedented ability to measure the linear polarization of the submillimeter light. The maps produced by B-BOP will contain not only information on total power, but also on the degree and the angle of polarization, simultaneously in three spectral bands (70, 200 and 350 microns). The B-BOP detectors are ultra-sensitive silicon bolometers that are intrinsically sensitive to polarization. Their NEP is close to 10E-18 W/sqrt(Hz). We will present the optical and thermal architectures of the instrument, we will detail the bolometer design and we will show the expected performances of the instrument based on preliminary lab work., Comment: 10 pages, 6 figures, SPIE proceeding: Astronomical Telescopes + Instrumentation 2020

Published
2021
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3. IDeF-X HD: a CMOS ASIC for the readout of Cd(Zn)Te Detectors for space-borne applications

Author

Gevin, Olivier, Lugiez, Francis, Michalowska, Alicja, Meuris, Aline, Limousin, Olivier, Delagnes, Eric, Lemaire, Olivier, and Pinsard, Frédéric

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Instrumentation and Detectors
Abstract

IDeF-X HD is a 32-channel analog front-end with self-triggering capability optimized for the readout of 16 x 16 pixels CdTe or CdZnTe pixelated detectors to build low power micro gamma camera. IDeF-X HD has been designed in the standard AMS CMOS 0.35 microns process technology. Its power consumption is 800 micro watt per channel. The dynamic range of the ASIC can be extended to 1.1 MeV thanks to the in-channel adjustable gain stage. When no detector is connected to the chip and without input current, a 33 electrons rms ENC level is achieved after shaping with 10.7 micro seconds peak time. Spectroscopy measurements have been performed with CdTe Schottky detectors. We measured an energy resolution of 4.2 keV FWHM at 667 keV (137-Cs) on a mono-pixel configuration. Meanwhile, we also measured 562 eV and 666 eV FWHM at 14 keV and 60 keV respectively (241-Am) with a 256 small pixel array and a low detection threshold of 1.2 keV. Since IDeF-X HD is intended for space-borne applications in astrophysics, we evaluated its radiation tolerance and its sensitivity to single event effects. We demonstrated that the ASIC remained fully functional without significant degradation of its performances after 200 krad and that no single event latch-up was detected putting the Linear Energy Transfer threshold above 110 MeV/(mg/cm2). Good noise performance and radiation tolerance make the chip well suited for X-rays energy discrimination and high-energy resolution. The chip is space qualified and flies on board the Solar Orbiter ESA mission launched in 2020.

Published
2021

4. Second generation of portable gamma camera based on Caliste CdTe hybrid technology

Author

MAIER, Daniel, BLONDEL, Claire, DELISLE, Cyrille, LIMOUSIN, Olivier, MARTIGNAC, Jerome, MEURIS, Aline, VISTICOT, Francois, DANIEL, Geoffrey, BAUSSON, Pierre-Anne, GEVIN, Olivier, AMOYAL, Guillaume, CARREL, Frederick, SCHOEPFF, Vincent, MAHE, Charly, SOUFFLET, Fabrice, and VASSAL, Marie-Cecile

Subjects
Physics - Instrumentation and Detectors, Physics - Medical Physics
Abstract

In the framework of a national funded program for nuclear safety, a first prototype of portable gamma camera was built and tested. It integrates a Caliste-HD CdTe-hybrid detector designed for space X-ray astronomy coupled with a new system-on-chip based acquisition system (FPGA and ARM microprocessor) and thermo-electrical coolers for a use at room temperature. The complete gamma part of the camera fits in a volume of 15 x 15 x 40 cm^3 for a mass lower than 1 kg and a power consumption lower than 10 W. Localization and spectro-identification of radionuclides in a contaminated scene were demonstrated during several test campaigns. A new generation of system is under development taking into account feedback experience from in-situ measurements and integrating a new generation of sensor cost-optimized by industrial applications called Caliste-O. Caliste-O holds a 16 x 16 pixel detector of 14 x 14 mm^2 and 2 mm thick with 8 full-custom front-end IDeF-X HD ASICs. Two prototypes were fabricated and tested. The paper will present the results of in-situ measurements with the first gamma camera, the spectroscopic performance of Caliste-O and the design of the second generation of gamma camera which aims for real time imaging and spectro-identification., Comment: 6 pages, 7 figures

Published
2020
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5. The enhanced X-ray Timing and Polarimetry mission - eXTP

Author

Zhang, ShuangNan, Santangelo, Andrea, Feroci, Marco, Xu, YuPeng, Lu, FangJun, Chen, Yong, Feng, Hua, Zhang, Shu, Brandt, Søren, Hernanz, Margarita, Baldini, Luca, Bozzo, Enrico, Campana, Riccardo, De Rosa, Alessandra, Dong, YongWei, Evangelista, Yuri, Karas, Vladimir, Meidinger, Norbert, Meuris, Aline, Nandra, Kirpal, Pan, Teng, Pareschi, Giovanni, Orleanski, Piotr, Huang, QiuShi, Schanne, Stephane, Sironi, Giorgia, Spiga, Daniele, Svoboda, Jiri, Tagliaferri, Gianpiero, Tenzer, Christoph, Vacchi, Andrea, Zane, Silvia, Walton, Dave, Wang, ZhanShan, Winter, Berend, Wu, Xin, Zand, Jean J. M. in 't, Ahangarianabhari, Mahdi, Ambrosi, Giovanni, Ambrosino, Filippo, Barbera, Marco, Basso, Stefano, Bayer, Jörg, Bellazzini, Ronaldo, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Borghi, Giacomo, Cao, XueLei, Cadoux, Franck, Ceraudo, Francesco, Chen, TianXiang, Chen, YuPeng, Chevenez, Jerome, Civitani, Marta, Cui, Wei, Cui, WeiWei, Dauser, Thomas, Del Monte, Ettore, Di Cosimo, Sergio, Diebold, Sebastian, Doroshenko, Victor, Dovciak, Michal, Du, YuanYuan, Ducci, Lorenzo, Fan, QingMei, Favre, Yannick, Fuschino, Fabio, Gálvez, José Luis, Gao, Min, Ge, MingYu, Gevin, Olivier, Grassi, Marco, Gu, QuanYing, Gu, YuDong, Han, DaWei, Hong, Bin, Hu, Wei, Ji, Long, Jia, ShuMei, Jiang, WeiChun, Kennedy, Thomas, Kreykenbohm, Ingo, Kuvvetli, Irfan, Labanti, Claudio, Latronico, Luca, Li, Gang, Li, MaoShun, Li, Xian, Li, Wei, Li, ZhengWei, Limousin, Olivier, Liu, HongWei, Liu, XiaoJing, Lu, Bo, Luo, Tao, Macera, Daniele, Malcovati, Piero, Martindale, Adrian, Michalska, Malgorzata, Meng, Bin, Minuti, Massimo, Morbidini, Alfredo, Muleri, Fabio, Paltani, Stephane, Perinati, Emanuele, Picciotto, Antonino, Piemonte, Claudio, Qu, JinLu, Rachevski, Alexandre, Rashevskaya, Irina, Rodriguez, Jerome, Schanz, Thomas, Shen, ZhengXiang, Sheng, LiZhi, Song, JiangBo, Song, LiMing, Sgro, Carmelo, Sun, Liang, Tan, Ying, Uttley, Phil, Wang, Juan, Wang, LangPing, Wang, YuSa, Watts, Anna L., Wen, XiangYang, Wilms, Jörn, Xiong, ShaoLin, Yang, JiaWei, Yang, Sheng, Yang, YanJi, Yu, Nian, Zhang, WenDa, Zampa, Gianluigi, Zampa, Nicola, Zdziarski, Andrzej A., Zhang, AiMei, Zhang, ChengMo, Zhang, Fan, Zhang, Long, Zhang, Tong, Zhang, Yi, Zhang, XiaoLi, Zhang, ZiLiang, Zhao, BaoSheng, Zheng, ShiJie, Zhou, YuPeng, Zorzi, Nicola, and Zwart, J. Frans

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

In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources. The paper provides a detailed description of: (1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload; (2) the elements and functions of the mission, from the spacecraft to the ground segment., Comment: Accepted for publication on Sci. China Phys. Mech. Astron. (2019)

Published
2018
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6. The Large Area Detector onboard the eXTP mission

Author

Feroci, Marco, Ahangarianabhari, Mahdi, Ambrosi, Giovanni, Ambrosino, Filippo, Argan, Andrea, Barbera, Marco, Bayer, Joerg, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Borghi, Giacomo, Bozzo, Enrico, Cadoux, Franck, Campana, Riccardo, Ceraudo, Francesco, Chen, Tianxiang, Cirrincione, Daniela, De Rosa, Alessandra, Del Monte, Ettore, Di Cosimo, Sergio, Diebold, Sebastian, Evangelista, Yuri, Fan, Qingmei, Favre, Yannick, Ficorella, Francesco, Fuschino, Fabio, Gevin, Olivier, Grassi, Marco, Hong, Bin, Mao, Hanqi, Karas, Vladimir, Kennedy, Tom, Labanti, Claudio, Limousin, Olivier, Cicero, Ugo Lo, Lu, Fang-Jun, Luo, Tao, Malcovati, Piero, Martindale, Adrian, Meuris, Aline, Michalska, Malgorzata, Morbidini, Alfredo, Muleri, Fabio, Orleanski, Piotr, Paltani, Stephane, Pan, Teng, Perinati, Emanuele, Picciotto, Antonino, Pohl, Martin, Rashevskaia, Irina, Santangelo, Andrea, Schanne, Stephane, Skup, Konrad, Svoboda, Jiri, Tenzer, Chris, Vacchi, Andrea, Walton, Dave, Winter, Berend, Wu, Xin, Xu, Yupeng, Zampa, Ganluigi, Zampa, Nicola, Zane, Silvia, Zdziarski, Andrzej, Zhang, Long, Zhang, Shu, Zhang, Shuang-Nan, Zhang, Wenda, Zhang, Xiaoli, Zhou, Yupeng, and Zorzi, Nicola

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS) and China National Space Administration (CNSA) currently performing an extended phase A study and proposed for a launch by 2025 in a low-earth orbit. The eXTP scientific payload envisages a suite of instruments (Spectroscopy Focusing Array, Polarimetry Focusing Array, Large Area Detector and Wide Field Monitor) offering unprecedented simultaneous wide-band X-ray spectral, timing and polarimetry sensitivity. A large European consortium is contributing to the eXTP study and it is expected to provide key hardware elements, including a Large Area Detector (LAD). The LAD instrument for eXTP is based on the design originally proposed for the LOFT mission within the ESA context. The eXTP/LAD envisages a deployed 3.4 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 provide an overview of the LAD instrument design, including new elements with respect to the earlier LOFT configuration., Comment: Paper presented at SPIE Space Telescopes and Instrumentation 2018

Published
2018
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7. STROBE-X: A probe-class mission for X-ray spectroscopy and timing on timescales from microseconds to years

Author

Ray, Paul S., Arzoumanian, Zaven, Brandt, Søren, Burns, Eric, Chakrabarty, Deepto, Feroci, Marco, Gendreau, Keith C., Gevin, Olivier, Hernanz, Margarita, Jenke, Peter, Kenyon, Steven, Maccarone, José Luis Gálvez Thomas J., Okajima, Takashi, Remillard, Ronald A., Schanne, Stéphane, Tenzer, Chris, Vacchi, Andrea, Wilson-Hodge, Colleen A., Winter, Berend, Zane, Silvia, Ballantyne, David R., Bozzo, Enrico, Brenneman, Laura W., Cackett, Edward, De Rosa, Alessandra, Goldstein, Adam, Hartmann, Dieter H., McDonald, Michael, Stevens, Abigail L., Tomsick, John A., Watts, Anna L., Wood, Kent S., and Zoghbi, Abderahmen

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

We describe the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X), a probe-class mission concept that will provide an unprecedented view of the X-ray sky, performing timing and spectroscopy over both a broad energy band (0.2-30 keV) and a wide range of timescales from microseconds to years. STROBE-X comprises two narrow-field instruments and a wide field monitor. The soft or low-energy band (0.2-12 keV) is covered by an array of lightweight optics (3-m focal length) that concentrate incident photons onto small solid-state detectors with CCD-level (85-175 eV) energy resolution, 100 ns time resolution, and low background rates. This technology has been fully developed for NICER and will be scaled up to take advantage of the longer focal length of STROBE-X. The higher-energy band (2-30 keV) is covered by large-area, collimated silicon drift detectors that were developed for the European LOFT mission concept. Each instrument will provide an order of magnitude improvement in effective area over its predecessor (NICER in the soft band and RXTE in the hard band). Finally, STROBE-X offers a sensitive wide-field monitor (WFM), both to act as a trigger for pointed observations of X-ray transients and also to provide high duty-cycle, high time-resolution, and high spectral-resolution monitoring of the variable X-ray sky. The WFM will boast approximately 20 times the sensitivity of the RXTE All-Sky Monitor, enabling multi-wavelength and multi-messenger investigations with a large instantaneous field of view. This mission concept will be presented to the 2020 Decadal Survey for consideration., Comment: 20 pages, 10 figures, to appear in Proc. SPIE Astronomical Telescopes and Instrumentation 2018

Published
2018

9. 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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10. 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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11. SNSPD development within the SPID / IQSENS project

Author

Zmuidzinas, Jonas, Gao, Jian-Rong, Navick, Xavier-Francois, Besancon, Marc, Bounab, Ayoub, Chen, Jia-Wern, Chen, Pisin, De La Broise, Xavier, Gevin, Olivier, Glicenstein, Jean Francois, Liu, Shu-Xiao, Lu, Yu-Jung, Nam, Jiwoo, Paganis, Stathes, Peng, Tzu-Yu, Tsai, Feng-Yang, Tsiounou, Dimitra, Tuchming, Boris, Yang, Jing-Wei, and Wu, Hsin-Yeh

Published
2024
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14. 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
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15. STROBE-X: A Probe-Class Mission for X-Ray Spectroscopy and Timing on Timescales from Microseconds to Years

Author

Ray, Paul S, Arzoumanian, Zaven, Brant, Soren, Burns, Eric, Chakrabarty, Deepto, Feroci, Marco, Gendreau, Keith C, Gevin, Olivier, Hernanz, Margarita, Jenke, Peter, Kenyon, Steven, Galvez, Jose Luis, Maccarone, Thomas J, Okajima, Takashi, Remillard, Ronald A, Schanne, Stephane, Tenzer, Chris, Vacchi, Andrea, Wilson-Hodge, Colleen A, Winter, Berend, Zane, Silvia, Ballantyne, David R, Bozzo, Enrico, Brenneman, Laura W, Cackett, Edward, De Rosa, Alessandra, Goldstein, Adam, Hartmann, Dieter H, McDonald, Michael, Stevens, Abigail L, Tomsick, John A, Watts, Anna L, Wood, Kent S, and Zoghbi, Abderahmen

Subjects
Astrophysics
Abstract

We describe the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X), a probe-class mission concept that will provide an unprecedented view of the X-ray sky, performing timing and spectroscopy over both a broad energy band (0.2-30 keV) and a wide range of timescales from microseconds to years. STROBE-X comprises two narrow-field instruments and a wide field monitor. The soft or low-energy band (0.2-12 keV) is covered by an array of lightweight optics (3-m focal length) that concentrate incident photons onto small solid-state detectors with CCD-level (85-175 eV) energy resolution, 100 ns time resolution, and low background rates. This technology has been fully developed for NICER and will be scaled up to take advantage of the longer focal length of STROBE-X. The higher-energy band (2-30 keV) is covered by large-area, collimated silicon drift detectors that were developed for the European LOFT mission concept. Each instrument will provide an order of magnitude improvement in effective area over its predecessor (NICER in the soft band and RXTE in the hard band). Finally, STROBE-X offers a sensitive wide-field monitor (WFM), both to act as a trigger for pointed observations of X-ray transients and also to provide high duty-cycle, high time-resolution, and high spectral-resolution monitoring of the variable X-ray sky. The WFM will boast approximately 20 times the sensitivity of the RXTE All-Sky Monitor, enabling multi-wavelength and multi-messenger investigations with a large instantaneous field of view. This mission concept will be presented to the 2020 Decadal Survey for consideration.

Published
2018
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16. The detector/readout-electronics assembly of the eXTP wide field monitor

Author

Zwart, Frans, primary, Tacken, Roland, additional, In't Zand, Jean, additional, de la Rie, Rob, additional, Limpens, Max, additional, Kochanowski, Cor, additional, Aitink-Kroes, Gabby, additional, van Baren, Coen, additional, Bayer, Jörg, additional, Baudin, David, additional, Crescenti, Fabio, additional, Evangelista, Yuri, additional, Feroci, Marco, additional, Frericks, Martin, additional, Gálvez, José-Luis, additional, Gevin, Olivier, additional, Hernanz, Margarita, additional, Hormaetxe, Ander, additional, Laubert, Phillip, additional, Meuris, Aline, additional, Nab, Jasper, additional, Neelis, John, additional, Tenzer, Chris, additional, Vogel, Channah, additional, and Zampa, Gianluigi, additional

Published
2022
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17. The wide field monitor onboard the Chinese-European x-ray mission eXTP

Author

Hernanz, Margarita, primary, Brandt, Søren, additional, In't Zand, Jean, additional, Evangelista, Yuri, additional, Meuris, Aline, additional, Tenzer, Chris, additional, Zampa, Gianluigi, additional, Orleanski, Piotr, additional, Kalemci, Emrah, additional, Sungur, Müberra, additional, Schanne, Stéphane, additional, Zwart, Frans, additional, de la Rie, Rob, additional, Laubert, Phillip, additional, van Baren, Coen, additional, Aitink-Kroes, Gabby, additional, Kuiper, Lucien, additional, Bayer, Jörg, additional, Hedderman, Paul, additional, Pliego, Samuel, additional, Xiong, Hao, additional, Campana, Riccardo, additional, Del Monte, Ettore, additional, Feroci, Marco, additional, Ceraudo, Francesco, additional, Gevin, Olivier, additional, Kuvvetli, Irfan, additional, Tcherniak, Denis, additional, Skup, Konrad, additional, Michalska, Malgorzata, additional, Nowosielski, Witold, additional, Hormaetxe, Ander, additional, Gálvez, José-Luis, additional, Ferrés, Patrícia, additional, Patruno, Alessandro, additional, Bonvicini, Walter, additional, Antonelli, Matias, additional, Boezio, Mirko, additional, Cirrincione, Daniela, additional, Munini, Riccardo, additional, Rachevski, Alexandre, additional, Vacchi, Andrea, additional, Zampa, Nicola, additional, Rashevskaya, Irina, additional, Argan, Andrea, additional, Turhan, Onur, additional, Bozkurt, Ayhan, additional, Onat, Ahmet, additional, Bozzo, Enrico, additional, Santangelo, Andrea, additional, Zhang, Shuang-Nan, additional, Lu, Fangjun, additional, and Xu, Yupeng, additional

Published
2022
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18. 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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19. 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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20. Highly sensitive and wide dynamic range polarimetric detectors arrays in the submillimeter domain

Author

Rodriguez, Louis R., primary, Adami, Obaid A., additional, Aliane, Abdelkader, additional, De la Broise, Xavier, additional, Delisle, Cyrille, additional, Demonti, Amala, additional, Desforge, Daniel, additional, Dubos, Sebastien, additional, Dussopt, Laurent, additional, Gennet, Camille, additional, Goudon, Valérie, additional, Gevin, Olivier, additional, Kaya, Hacile, additional, Lasfargues, Gilles, additional, Martignac, Jerome, additional, Navick, Xavier-François, additional, Poglitsch, Albrecht, additional, Revéret, Vincent, additional, Sauvage, Marc, additional, Tollet, Timothée, additional, and Visticot, Francois, additional

Published
2022
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21. 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

22. The Wide Field Monitor onboard the Chinese-European X-ray mission eXTP

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Hernanz, Margarita, Brandt, Søren, Zand, Jeanint, Evangelista, Yuri, Meuris, Aline, Tenzer, Chris, Zampa, Gianluigi, Orleanski, Piotr, Kalemci, Emrah, Sungur, Müberra, Schanne, Stéphane, Zwart, Frans, de la Rie, Rob, Laubert, Phillip, van Baren, Coen, Aitink-Kroes, Gabby, Kuiper, Lucien, Bayer, Jörg, Hedderman, Paul, Pliego, Samuel, Xiong, Hao, Campana, Riccardo, del Monte, Ettore, Feroci, Marco, Ceraudo, Francesco, Gevin, Olivier, Kuvvetli, Irfan, Tcherniak, Denis, Skup, Konrad, Michalska, Malgorzata, Nowosielski, Witold, Hormaetxe, Ander, Gálvez, José Luis, Ferrés, Patrícia, Patruno, Alessandro, Bonvicini, Walter, Antonelli, Matias, Boezio, Mirko, Cirrincione, Daniela, Munini, Riccardo, Rachevski, Alexandre, Vacchi, Andrea, Zampa, Nicola, Rashevskaya, Irina, Argan, Andrea, Turhan, Onur, Bozkurt, Ayhan, Onat, Ahmet, Bozzo, Enrico, Santangelo, Andrea, Zhang, Shuang Nan, Lu, Fangjun, Xu, Yupeng, den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Hernanz, Margarita, Brandt, Søren, Zand, Jeanint, Evangelista, Yuri, Meuris, Aline, Tenzer, Chris, Zampa, Gianluigi, Orleanski, Piotr, Kalemci, Emrah, Sungur, Müberra, Schanne, Stéphane, Zwart, Frans, de la Rie, Rob, Laubert, Phillip, van Baren, Coen, Aitink-Kroes, Gabby, Kuiper, Lucien, Bayer, Jörg, Hedderman, Paul, Pliego, Samuel, Xiong, Hao, Campana, Riccardo, del Monte, Ettore, Feroci, Marco, Ceraudo, Francesco, Gevin, Olivier, Kuvvetli, Irfan, Tcherniak, Denis, Skup, Konrad, Michalska, Malgorzata, Nowosielski, Witold, Hormaetxe, Ander, Gálvez, José Luis, Ferrés, Patrícia, Patruno, Alessandro, Bonvicini, Walter, Antonelli, Matias, Boezio, Mirko, Cirrincione, Daniela, Munini, Riccardo, Rachevski, Alexandre, Vacchi, Andrea, Zampa, Nicola, Rashevskaya, Irina, Argan, Andrea, Turhan, Onur, Bozkurt, Ayhan, Onat, Ahmet, Bozzo, Enrico, Santangelo, Andrea, Zhang, Shuang Nan, Lu, Fangjun, and Xu, Yupeng

Abstract

The eXTP (enhanced X-ray Timing and Polarimetry) mission is a major project of the Chinese Academy of Sciences (CAS), with a large involvement of Europe. The scientific payload of eXTP includes four instruments: the SFA (Spectroscopy Focusing Array) and the PFA (Polarimetry Focusing Array) - led by China - the LAD (Large Area Detector) and the WFM (Wide Field Monitor) - led by Europe (Italy and Spain). They offer a unique simultaneous wide-band X-ray timing and polarimetry sensitivity. The WFM is a wide field X-ray monitor instrument in the 2-50 keV energy range, consisting of an array of six coded mask cameras with a field of view of 180ºx90ºat an angular resolution of 5 arcmin and 4 silicon drift detectors in each camera. Its unprecedented combination of large field of view and imaging down to 2 keV will allow eXTP to make important discoveries of the variable and transient X-ray sky and is essential in detecting transient black holes, that are part of the primary science goals of eXTP, so that they can be promptly followed up with other instruments on eXTP and elsewhere.

Published
2022

23. First Results of PEPITES, A New Transparent Profiler Based on Secondary Electrons Emission for Charged Particle Beams

Author

Thiebaux, Christophe, Bernardi, Lorenzo, Delagnes, Eric, Gastaldi, Franck, Gebreyohannes, Fikre Tsigabu, Geerebaert, Yannick, Gevin, Olivier, Guillaumat, Rémi, Haddad, Ferid, Koumeir, Charbel, Magniette, Frederic, Manigot, Pascal, Poirier, Freddy, Servagent, Noël, Verderi, Marc, Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST), Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ), GIP ARRONAX [Nantes], and Université de Nantes (UN)

Subjects
electron, radiation, detector, [PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph], vacuum, 03 Transverse Profile and Emittance Monitors, proton, Accelerator Physics
Abstract

The PEPITES project* consists of a brand new operational prototype of an ultra-thin, radiation-resistant profiler capable of continuous operation on mid-energy (O(100 MeV)) charged particle accelerators. Secondary electron emission (SEE) is used for the signal because it only requires a small amount of material (10 nm); very linear, it also offers good dynamics. The lateral beam profile is sampled using segmented electrodes, constructed by thin film methods. Gold strips, as thin as the electrical conductivity allows (~ 50 nm), are deposited on an insulating substrate as thin as possible. While crossing the gold, the beam ejects the electrons by SEE, the current thus formed in each strip allows the sampling. SEE was characterized at ARRONAX with 68 MeV proton beams and at medical energies at CPO**. Electrodes were subjected to doses of up to 10⁹ Gy without showing significant degradation. A demonstrator with dedicated electronics (CEA) is installed at ARRONAX and will be used routinely with proton beams of 17-68 MeV for intensities of 100fA to 100nA. An overview of the design and first measurements will be presented, and system performances will be assessed., Proceedings of the 11th International Beam Instrumentation Conference, IBIC2022, Kraków, Poland

Published
2022
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24. Micro hard-x ray camera: from Caliste 64 to Caliste 256

Author

Meuris, Aline, Limousin, Olivier, Lugiez, Francis, Gevin, Olivier, Delagnes, Eric, Le Mer, Isabelle, Chavassieux, Marc, Pinsard, Frederic, Blondel, Claire, Daly, F., Vassal, Marie-Cecile, Bocage, Regis, and Soufflet, Fabrice

Subjects
Business, Electronics, Electronics and electrical industries
Published
2009

25. IDeF-X ECLAIRs: a CMOS ASIC for the readout of CdTe and CdZnTe detectors for high resolution spectroscopy

Author

Gevin, Olivier, Baron, Pascal, Coppolani, Xavier, Daly, Francois, Delagnes, Eric, Limousin, Olivier, Lugiez, Francis, Meuris, Aline, Pinsard, Frederic, and Renaud, Diana

Subjects
X-ray spectroscopy, Semiconductor industry, Complementary metal oxide semiconductors, Application-specific integrated circuits, Custom integrated circuits, Detectors, Semiconductor industry, Application-specific integrated circuit, Custom IC, Business, Electronics, Electronics and electrical industries
Published
2009

26. B-BOP: the SPICA imaging polarimeter

Author

Revéret, Vincent, primary, Sauvage, Marc, additional, Adami, Obaïd, additional, Aliane, Abdelkader, additional, Berthé, Michel, additional, Bounissou, Sophie, additional, de la Broïse, Xavier, additional, Chimeno, M., additional, Demonti, Amala, additional, Delisle, Cyrille, additional, Doumayrou, Eric, additional, Duband, Lionel, additional, Dubreuil, Didier, additional, Dussopt, Laurent, additional, Frugier, Pierre-Antoine, additional, Gennet, Camille, additional, Gevin, Olivier, additional, Goudon, Valérie, additional, Kaya, Hacile, additional, Marquet, B., additional, Martignac, Jérôme, additional, Martin, Sylvain, additional, Najarro, F., additional, Navick, Xavier, additional, Perez, J., additional, Plesseria, J.-Y., additional, Poglitsch, Albrecht, additional, Rodriguez, Louis, additional, Torres Redondo, J., additional, and Visticot, François, additional

Published
2020
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27. 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
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28. 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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29. Development of a Transparent Profiler Based on Secondary Electrons Emission for Charged Particle Beams

Author

Thiebaux, Christophe, Blain, Guillaume, Boyer, Bruno, Delagnes, Eric, Gebreyohannes, Fikre Tsigabu, Geerebaert, Yannick, Gevin, Olivier, Haddad, Ferid, Koumeir, Charbel, Magniette, Frederic, Manigot, Pascal, Michel, Nathalie, Poirier, Freddy, Servagent, Noël, Sounalet, Thomas, Verderi, Marc, Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Cyclotron ARRONAX, GIP, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), and Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique)

Subjects
radiation, electron, detector, 04 Operation and Upgrades, [PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph], cyclotron, Accelerator Physics, proton
Abstract

The PEPITES project* aims at realizing an operational prototype of an ultra-thin, radiation-resistant profiler able to permanently operate on mid-energy (O(100 MeV)) charged particle accelerators. PEPITES uses secondary electron emission (SEE) for the signal because it requires only a minimal thickness of material (10 nm); very linear, it also offers a great dynamic. The lateral beam profile is sampled using segmented electrodes, constructed by thin film methods. Gold strips, as thin as the electrical conductivity allows (~ 50 nm), are deposited on an as thin as possible insulating substrate. When crossing the gold, the beam ejects the electrons by SEE, the current thus formed in each strip allows the sampling. The technique was validated at ARRONAX with 68 MeV proton beams for intensities from 100 fA to 10 nA. SEE is characterized up to 100 nA at ARRONAX and medical energies at CPO**. Electrodes were subjected to doses of up to 10⁹ Gy without showing significant degradation. A demonstrator with dedicated electronics (CEA) will be installed at ARRONAX and used routinely. The performances of the system and its behavior over time will thus be characterized., Proceedings of the 22nd International Conference on Cyclotrons and their Applications, Cyclotrons2019, Cape Town, South Africa

Published
2019
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30. The enhanced X-ray Timing and Polarimetry mission—eXTP

Author

Zhang, ShuangNan, primary, Santangelo, Andrea, additional, Feroci, Marco, additional, Xu, YuPeng, additional, Lu, FangJun, additional, Chen, Yong, additional, Feng, Hua, additional, Zhang, Shu, additional, Brandt, Søren, additional, Hernanz, Margarita, additional, Baldini, Luca, additional, Bozzo, Enrico, additional, Campana, Riccardo, additional, De Rosa, Alessandra, additional, Dong, YongWei, additional, Evangelista, Yuri, additional, Karas, Vladimir, additional, Meidinger, Norbert, additional, Meuris, Aline, additional, Nandra, Kirpal, additional, Pan, Teng, additional, Pareschi, Giovanni, additional, Orleanski, Piotr, additional, Huang, QiuShi, additional, Schanne, Stephane, additional, Sironi, Giorgia, additional, Spiga, Daniele, additional, Svoboda, Jiri, additional, Tagliaferri, Gianpiero, additional, Tenzer, Christoph, additional, Vacchi, Andrea, additional, Zane, Silvia, additional, Walton, Dave, additional, Wang, ZhanShan, additional, Winter, Berend, additional, Wu, Xin, additional, in’ t Zand, Jean J. M., additional, Ahangarianabhari, Mahdi, additional, Ambrosi, Giovanni, additional, Ambrosino, Filippo, additional, Barbera, Marco, additional, Basso, Stefano, additional, Bayer, Jörg, additional, Bellazzini, Ronaldo, additional, Bellutti, Pierluigi, additional, Bertucci, Bruna, additional, Bertuccio, Giuseppe, additional, Borghi, Giacomo, additional, Cao, XueLei, additional, Cadoux, Franck, additional, Ceraudo, Francesco, additional, Chen, TianXiang, additional, Chen, YuPeng, additional, Chevenez, Jerome, additional, Civitani, Marta, additional, Cui, Wei, additional, Cui, WeiWei, additional, Dauser, Thomas, additional, Del Monte, Ettore, additional, Di Cosimo, Sergio, additional, Diebold, Sebastian, additional, Doroshenko, Victor, additional, Dovciak, Michal, additional, Du, YuanYuan, additional, Ducci, Lorenzo, additional, Fan, QingMei, additional, Favre, Yannick, additional, Fuschino, Fabio, additional, Gálvez, José Luis, additional, Gao, Min, additional, Ge, MingYu, additional, Gevin, Olivier, additional, Grassi, Marco, additional, Gu, QuanYing, additional, Gu, YuDong, additional, Han, DaWei, additional, Hong, Bin, additional, Hu, Wei, additional, Ji, Long, additional, Jia, ShuMei, additional, Jiang, WeiChun, additional, Kennedy, Thomas, additional, Kreykenbohm, Ingo, additional, Kuvvetli, Irfan, additional, Labanti, Claudio, additional, Latronico, Luca, additional, Li, Gang, additional, Li, MaoShun, additional, Li, Xian, additional, Li, Wei, additional, Li, ZhengWei, additional, Limousin, Olivier, additional, Liu, HongWei, additional, Liu, XiaoJing, additional, Lu, Bo, additional, Luo, Tao, additional, Macera, Daniele, additional, Malcovati, Piero, additional, Martindale, Adrian, additional, Michalska, Malgorzata, additional, Meng, Bin, additional, Minuti, Massimo, additional, Morbidini, Alfredo, additional, Muleri, Fabio, additional, Paltani, Stephane, additional, Perinati, Emanuele, additional, Picciotto, Antonino, additional, Piemonte, Claudio, additional, Qu, JinLu, additional, Rachevski, Alexandre, additional, Rashevskaya, Irina, additional, Rodriguez, Jerome, additional, Schanz, Thomas, additional, Shen, ZhengXiang, additional, Sheng, LiZhi, additional, Song, JiangBo, additional, Song, LiMing, additional, Sgro, Carmelo, additional, Sun, Liang, additional, Tan, Ying, additional, Uttley, Phil, additional, Wang, Bo, additional, Wang, DianLong, additional, Wang, GuoFeng, additional, Wang, Juan, additional, Wang, LangPing, additional, Wang, YuSa, additional, Watts, Anna L., additional, Wen, XiangYang, additional, Wilms, Jörn, additional, Xiong, ShaoLin, additional, Yang, JiaWei, additional, Yang, Sheng, additional, Yang, YanJi, additional, Yu, Nian, additional, Zhang, WenDa, additional, Zampa, Gianluigi, additional, Zampa, Nicola, additional, Zdziarski, Andrzej A., additional, Zhang, AiMei, additional, Zhang, ChengMo, additional, Zhang, Fan, additional, Zhang, Long, additional, Zhang, Tong, additional, Zhang, Yi, additional, Zhang, XiaoLi, additional, Zhang, ZiLiang, additional, Zhao, BaoSheng, additional, Zheng, ShiJie, additional, Zhou, YuPeng, additional, Zorzi, Nicola, additional, and Zwart, J. Frans, additional

Published
2018
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31. STROBE-X: A probe-class mission for X-ray spectroscopy and timing on timescales from microseconds to years

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Ray, Paul S., Arzoumanian, Zaven, Brandt, Søren, Burns, Eric, Chakrabarty, Deepto, Feroci, Marco, Gendreau, Keith C., Gevin, Olivier, Hernanz, Margarita, Jenke, Peter, Kenyon, Steven, Maccarone, José Luis Gálvez Thomas J., Okajima, Takashi, Remillard, Ronald A., Schanne, Stéphane, Tenzer, Chris, Vacchi, Andrea, Wilson-Hodge, Colleen A., Winter, Berend, Zane, Silvia, Ballantyne, David R., Bozzo, Enrico, Brenneman, Laura W., Cackett, Edward, De Rosa, Alessandra, Goldstein, Adam, Hartmann, Dieter H., McDonald, Michael, Stevens, Abigail L., Tomsick, John A., Watts, Anna L., Wood, Kent S., Zoghbi, Abderahmen, den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Ray, Paul S., Arzoumanian, Zaven, Brandt, Søren, Burns, Eric, Chakrabarty, Deepto, Feroci, Marco, Gendreau, Keith C., Gevin, Olivier, Hernanz, Margarita, Jenke, Peter, Kenyon, Steven, Maccarone, José Luis Gálvez Thomas J., Okajima, Takashi, Remillard, Ronald A., Schanne, Stéphane, Tenzer, Chris, Vacchi, Andrea, Wilson-Hodge, Colleen A., Winter, Berend, Zane, Silvia, Ballantyne, David R., Bozzo, Enrico, Brenneman, Laura W., Cackett, Edward, De Rosa, Alessandra, Goldstein, Adam, Hartmann, Dieter H., McDonald, Michael, Stevens, Abigail L., Tomsick, John A., Watts, Anna L., Wood, Kent S., and Zoghbi, Abderahmen

Abstract

We describe the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X), a probe-class mission concept that will provide an unprecedented view of the X-ray sky, performing timing and spectroscopy over both a broad energy band (0.2-30 keV) and a wide range of timescales from microseconds to years. STROBE-X comprises two narrow-field instruments and a wide field monitor. The soft or low-energy band (0.2-12 keV) is covered by an array of lightweight optics (3-m focal length) that concentrate incident photons onto small solid-state detectors with CCD-level (85-175 eV) energy resolution, 100 ns time resolution, and low background rates. This technology has been fully developed for NICER and will be scaled up to take advantage of the longer focal length of STROBE-X. The higher-energy band (2-30 keV) is covered by large-area, collimated silicon drift detectors that were developed for the European LOFT mission concept. Each instrument will provide an order of magnitude improvement in effective area over its predecessor (NICER in the soft band and RXTE in the hard band). Finally, STROBE-X offers a sensitive wide-field monitor (WFM), both to act as a trigger for pointed observations of X-ray transients and also to provide high duty-cycle, high time-resolution, and high spectral-resolution monitoring of the variable X-ray sky. The WFM will boast approximately 20 times the sensitivity of the RXTE All-Sky Monitor, enabling multi-wavelength and multi-messenger investigations with a large instantaneous field of view. This mission concept will be presented to the 2020 Decadal Survey for consideration.

Published
2018

32. The large area detector onboard the eXTP mission

Author

Feroci, Marco, primary, Karas, Vladimir, primary, Orleański, Piotr, primary, Santangelo, Andrea, primary, Schanne, Stéphane, primary, Wu, Xin, primary, Zane, Silvia, primary, Zhang, Shuangnan, primary, Vacchi, Andrea, primary, Paltani, Stephane, primary, Bellutti, Pierluigi, primary, Ambrosi, Giovanni, primary, Bozzo, Enrico, primary, XU, Yupeng, primary, Zdziarski, Andrzej, primary, De Rosa, Alessandra, primary, Ambrosino, Filippo, primary, Barbera, Marco, primary, Limousin, Olivier, primary, Ahangarianabhari, Mahdi, primary, Argan, Andrea, primary, Bertucci, Bruna, primary, Bertuccio, Giuseppe, primary, Bayer, Joerg, primary, Borghi, Giacomo, primary, Cadeaux, Franck, primary, Campana, Riccardo, primary, Ceraudo, Francesco, primary, Cirrincione, Daniela, primary, Del Monte, Ettore, primary, Di Cosimo, Sergio, primary, Evangelista, Yuri, primary, diebold, Sebastian, primary, Favre, Yannick, primary, Ficorella, Francesco, primary, Fuschino, Fabio, primary, Gevin, Olivier, primary, Grassi, Marco, primary, Kennedy, Tom, primary, Labanti, Claudio, primary, Lo Cicero, Ugo, primary, Malcovati, Piero, primary, Martindale, Adrian, primary, Meuris, Aline, primary, Michalska, Malgrozata, primary, Morbidini, Alfredo, primary, Muleri, Fabio, primary, perinati, emanuele, primary, Picciotto, Antonino, primary, Pohl, Martin, primary, Rashvskaya, Irina, primary, Svoboda, Jiri, primary, Skup, Kornad, primary, Tenzer, Chris, primary, Walton, Dave, primary, Winter, Berend, primary, Zampa, Gianluigi, primary, Zampa, Nicola, primary, Zorzi, Nicola, primary, Zhang, Shu, primary, Chen, Tianxiang, primary, Fan, Qingmei, primary, Hong, Bin, primary, Mao, Hanqi, primary, Lu, Fangjun, primary, Luo, Tao, primary, Zhou, Yupeng, primary, Zhang, Long, primary, Zhang, Wenda, primary, Pan, Teng, primary, and zhang, xiaoli, primary

Published
2018
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34. BRAHMS: polarimetric bolometer arrays for the SPICA observatory camera (Conference Presentation)

Author

Rodriguez, Louis R., primary, Poglitsch, Albrecht, additional, Aliane, Abdelkader, additional, Revéret, Vincent, additional, Gevin, Olivier, additional, Goudon, Valérie, additional, Bounissou, Sophie, additional, Adami, Obaïd-Allah, additional, de la Broïse, Xavier, additional, Martignac, Jérôme, additional, Delisle, Cyrille, additional, Sauvageot, Jean-Luc, additional, Dussopt, Laurent, additional, and Thabet, Hanan, additional

Published
2018
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37. Flight production of Caliste-SO: the hard x-ray spectrometers for solar orbiter/STIX instrument

Author

Limousin, Olivier, additional, Meuris, Aline, additional, Gevin, Olivier, additional, Blondel, Claire, additional, Donati, Modeste, additional, Dumaye, Luc, additional, Le Mer, Isabelle, additional, Martignac, Jérôme, additional, Tourrette, Thierry, additional, Vassal, Marie-Cécile, additional, Blain, Dominique, additional, Boussadia, Mohamed, additional, Fiant, Nicolas, additional, Soufflet, Fabrice, additional, Bednarzik, Martin, additional, Birrer, Guy, additional, Stutz, Stefan, additional, Wild, Christopher, additional, Billot, Marc, additional, Fratter, Isabelle, additional, Grimm, Oliver, additional, and Krucker, Säm, additional

Published
2016
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38. The enhanced X-ray Timing and Polarimetry mission—eXTP

Author

Zhang, ShuangNan, Santangelo, Andrea, Feroci, Marco, Xu, YuPeng, Lu, FangJun, Chen, Yong, Feng, Hua, Zhang, Shu, Brandt, Søren, Hernanz, Margarita, Baldini, Luca, Bozzo, Enrico, Campana, Riccardo, Rosa, Alessandra, Dong, YongWei, Evangelista, Yuri, Karas, Vladimir, Meidinger, Norbert, Meuris, Aline, Nandra, Kirpal, Pan, Teng, Pareschi, Giovanni, Orleanski, Piotr, Huang, QiuShi, Schanne, Stephane, Sironi, Giorgia, Spiga, Daniele, Svoboda, Jiri, Tagliaferri, Gianpiero, Tenzer, Christoph, Vacchi, Andrea, Zane, Silvia, Walton, Dave, Wang, ZhanShan, Winter, Berend, Wu, Xin, in’ t Zand, Jean, Ahangarianabhari, Mahdi, Ambrosi, Giovanni, Ambrosino, Filippo, Barbera, Marco, Basso, Stefano, Bayer, Jörg, Bellazzini, Ronaldo, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Borghi, Giacomo, Cao, XueLei, Cadoux, Franck, Campana, Riccardo, Ceraudo, Francesco, Chen, TianXiang, Chen, YuPeng, Chevenez, Jerome, Civitani, Marta, Cui, Wei, Cui, WeiWei, Dauser, Thomas, Monte, Ettore, Cosimo, Sergio, Diebold, Sebastian, Doroshenko, Victor, Dovciak, Michal, Du, YuanYuan, Ducci, Lorenzo, Fan, QingMei, Favre, Yannick, Fuschino, Fabio, Gálvez, José, Gao, Min, Ge, MingYu, Gevin, Olivier, Grassi, Marco, Gu, QuanYing, Gu, YuDong, Han, DaWei, Hong, Bin, Hu, Wei, Ji, Long, Jia, ShuMei, Jiang, WeiChun, Kennedy, Thomas, Kreykenbohm, Ingo, Kuvvetli, Irfan, Labanti, Claudio, Latronico, Luca, Li, Gang, Li, MaoShun, Li, Xian, Li, Wei, Li, ZhengWei, Limousin, Olivier, Liu, HongWei, Liu, XiaoJing, Lu, Bo, Luo, Tao, Macera, Daniele, Malcovati, Piero, Martindale, Adrian, Michalska, Malgorzata, Meng, Bin, Minuti, Massimo, Morbidini, Alfredo, Muleri, Fabio, Paltani, Stephane, Perinati, Emanuele, Picciotto, Antonino, Piemonte, Claudio, Qu, JinLu, Rachevski, Alexandre, Rashevskaya, Irina, Rodriguez, Jerome, Schanz, Thomas, Shen, ZhengXiang, Sheng, LiZhi, Song, JiangBo, Song, LiMing, Sgro, Carmelo, Sun, Liang, Tan, Ying, Uttley, Phil, Wang, Bo, Wang, DianLong, Wang, GuoFeng, Wang, Juan, Wang, LangPing, Wang, YuSa, Watts, Anna, Wen, XiangYang, Wilms, Jörn, Xiong, ShaoLin, Yang, JiaWei, Yang, Sheng, Yang, YanJi, Yu, Nian, Zhang, WenDa, Zampa, Gianluigi, Zampa, Nicola, Zdziarski, Andrzej, Zhang, AiMei, Zhang, ChengMo, Zhang, Fan, Zhang, Long, Zhang, Tong, Zhang, Yi, Zhang, XiaoLi, Zhang, ZiLiang, Zhao, BaoSheng, Zheng, ShiJie, Zhou, YuPeng, Zorzi, Nicola, and Zwart, J.

Abstract

In this paper we present the enhanced X-ray Timing and Polarimetry mission—eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources. The paper provides a detailed description of: (1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload; (2) the elements and functions of the mission, from the spacecraft to the ground segment.

Published
2019
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39. Caliste-SO: the x-ray spectrometer unit of the STIX instrument onboard the Solar Orbiter space mission

Author

Meuris, Aline, additional, Limousin, Olivier, additional, Gevin, Olivier, additional, Vassal, Marie-Cécile, additional, Soufflet, Fabrice, additional, Fiant, Nicolas, additional, Bednarzik, Martin, additional, Wild, Christopher, additional, Stutz, Stefan, additional, Birrer, Guy, additional, Blondel, Claire, additional, Le Mer, Isabelle, additional, Huynh, Duc-Dat, additional, Donati, Modeste, additional, Grimm, Oliver, additional, Commichau, Volker, additional, Hurford, Gordon, additional, Krucker, Säm, additional, Gonzalez, François, additional, and Billot, Marc, additional

Published
2014
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40. The Large Area Detector onboard the eXTP mission

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Feroci, Marco, Ahangarianabhari, Mahdi, Ambrosi, Giovanni, Ambrosino, Filippo, Argan, Andrea, Barbera, Marco, Bayer, Joerg, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Borghi, Giacomo, Bozzo, Enrico, Cadeaux, Franck, Campana, Riccardo, Ceraudo, Francesco, Chen, Tianxiang, Cirrincione, Daniela, De Rosa, Alessandra, Del Monte, Ettore, Di Cosimo, Sergio, Diebold, Sebastian, Evangelista, Yuri, Fan, Qingmei, Favre, Yannick, Ficorella, Francesco, Fuschino, Fabio, Gevin, Olivier, Grassi, Marco, Hong, Bin, Mao, Hanqi, Karas, Vladimir, Kennedy, Tom, Labanti, Claudio, Limousin, Olivier, Lo Cicero, Ugo, Lu, Fangjun, Luo, Tao, Malcovati, Piero, Martindale, Adrian, Meuris, Aline, Michalska, Malgrozata, Morbidini, Alfredo, Muleri, Fabio, Orleański, Piotr, Paltani, Stephane, Pan, Teng, Perinati, Emanuele, Picciotto, Antonino, Pohl, Martin, Rashvskaia, Irina, Santangelo, Andrea, Schanne, Stéphane, Skup, Kornad, Svoboda, Jiri, Tenzer, Chris, Vacchi, Andrea, Walton, Dave, Winter, Berend, Wu, Xin, Xu, Yupeng, Zampa, Gianluigi, Zampa, Nicola, Zane, Silvia, Zdziarski, Andrzej, Zhang, Long, Zhang, Shu, Zhang, Shuangnan, Zhang, Wenda, Zhang, Xiaoli, Zhou, Yupeng, and Zorzi, Nicola

Published
2018
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44. Caliste HD: A new fine pitch Cd(Zn)Te imaging spectrometer from 2 keV up to 1 MeV

Author

Meuris, Aline, primary, Limousin, Olivier, additional, Gevin, Olivier, additional, Lugiez, Francis, additional, Le Mer, Isabelle, additional, Pinsard, Frederic, additional, Donati, Modeste, additional, Blondel, Claire, additional, Michalowska, Alicja, additional, Delagnes, Eric, additional, Vassal, Marie-Cecile, additional, and Soufflet, Fabrice, additional

Published
2011
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45. 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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46. Flight production of Caliste-SO: the hard x-ray spectrometers for solar orbiter/STIX instrument

Author

den Herder, Jan-Willem A., Takahashi, Tadayuki, Bautz, Marshall, Limousin, Olivier, Meuris, Aline, Gevin, Olivier, Blondel, Claire, Donati, Modeste, Dumaye, Luc, Le Mer, Isabelle, Martignac, Jérôme, Tourrette, Thierry, Vassal, Marie-Cécile, Blain, Dominique, Boussadia, Mohamed, Fiant, Nicolas, Soufflet, Fabrice, Bednarzik, Martin, Birrer, Guy, Stutz, Stefan, Wild, Christopher, Billot, Marc, Fratter, Isabelle, Grimm, Oliver, and Krucker, Säm

Published
2016
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47. Caliste-SO: the x-ray spectrometer unit of the STIX instrument onboard the Solar Orbiter space mission

Author

Holland, Andrew D., Beletic, James, Meuris, Aline, Limousin, Olivier, Gevin, Olivier, Vassal, Marie-Cécile, Soufflet, Fabrice, Fiant, Nicolas, Bednarzik, Martin, Wild, Christopher, Stutz, Stefan, Birrer, Guy, Blondel, Claire, Le Mer, Isabelle, Huynh, Duc-Dat, Donati, Modeste, Grimm, Oliver, Commichau, Volker, Hurford, Gordon, Krucker, Säm, Gonzalez, François, and Billot, Marc

Published
2013
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48. 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

49. The enhanced X-ray Timing and Polarimetry mission—eXTP

Author

ShuangNan Zhang, Andrea Santangelo, Marco Feroci, YuPeng Xu, FangJun Lu, Yong Chen, Hua Feng, Shu Zhang, Søren Brandt, Margarita Hernanz, Luca Baldini, Enrico Bozzo, Riccardo Campana, Alessandra De Rosa, YongWei Dong, Yuri Evangelista, Vladimir Karas, Norbert Meidinger, Aline Meuris, Kirpal Nandra, Teng Pan, Giovanni Pareschi, Piotr Orleanski, QiuShi Huang, Stephane Schanne, Giorgia Sironi, Daniele Spiga, Jiri Svoboda, Gianpiero Tagliaferri, Christoph Tenzer, Andrea Vacchi, Silvia Zane, Dave Walton, ZhanShan Wang, Berend Winter, Xin Wu, Jean J. M. in’ t Zand, Mahdi Ahangarianabhari, Giovanni Ambrosi, Filippo Ambrosino, Marco Barbera, Stefano Basso, Jörg Bayer, Ronaldo Bellazzini, Pierluigi Bellutti, Bruna Bertucci, Giuseppe Bertuccio, Giacomo Borghi, XueLei Cao, Franck Cadoux, Francesco Ceraudo, TianXiang Chen, YuPeng Chen, Jerome Chevenez, Marta Civitani, Wei Cui, WeiWei Cui, Thomas Dauser, Ettore Del Monte, Sergio Di Cosimo, Sebastian Diebold, Victor Doroshenko, Michal Dovciak, YuanYuan Du, Lorenzo Ducci, QingMei Fan, Yannick Favre, Fabio Fuschino, José Luis Gálvez, Min Gao, MingYu Ge, Olivier Gevin, Marco Grassi, QuanYing Gu, YuDong Gu, DaWei Han, Bin Hong, Wei Hu, Long Ji, ShuMei Jia, WeiChun Jiang, Thomas Kennedy, Ingo Kreykenbohm, Irfan Kuvvetli, Claudio Labanti, Luca Latronico, Gang Li, MaoShun Li, Xian Li, Wei Li, ZhengWei Li, Olivier Limousin, HongWei Liu, XiaoJing Liu, Bo Lu, Tao Luo, Daniele Macera, Piero Malcovati, Adrian Martindale, Malgorzata Michalska, Bin Meng, Massimo Minuti, Alfredo Morbidini, Fabio Muleri, Stephane Paltani, Emanuele Perinati, Antonino Picciotto, Claudio Piemonte, JinLu Qu, Alexandre Rachevski, Irina Rashevskaya, Jerome Rodriguez, Thomas Schanz, ZhengXiang Shen, LiZhi Sheng, JiangBo Song, LiMing Song, Carmelo Sgro, Liang Sun, Ying Tan, Phil Uttley, Bo Wang, DianLong Wang, GuoFeng Wang, Juan Wang, LangPing Wang, YuSa Wang, Anna L. Watts, XiangYang Wen, Jörn Wilms, ShaoLin Xiong, JiaWei Yang, Sheng Yang, YanJi Yang, Nian Yu, WenDa Zhang, Gianluigi Zampa, Nicola Zampa, Andrzej A. Zdziarski, AiMei Zhang, ChengMo Zhang, Fan Zhang, Long Zhang, Tong Zhang, Yi Zhang, XiaoLi Zhang, ZiLiang Zhang, BaoSheng Zhao, ShiJie Zheng, YuPeng Zhou, Nicola Zorzi, J. Frans Zwart, ITA, GBR, FRA, DEU, ESP, DNK, POL, CZE, CHN, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, eXTP, Zhang, ShuangNan, Santangelo, Andrea, Feroci, Marco, Xu, YuPeng, Lu, FangJun, Chen, Yong, Feng, Hua, Zhang, Shu, Brandt, Søren, Hernanz, Margarita, Baldini, Luca, Bozzo, Enrico, Campana, Riccardo, De Rosa, Alessandra, Dong, YongWei, Evangelista, Yuri, Karas, Vladimir, Meidinger, Norbert, Meuris, Aline, Nandra, Kirpal, Pan, Teng, Pareschi, Giovanni, Orleanski, Piotr, Huang, QiuShi, Schanne, Stephane, Sironi, Giorgia, Spiga, Daniele, Svoboda, Jiri, Tagliaferri, Gianpiero, Tenzer, Christoph, Vacchi, Andrea, Zane, Silvia, Walton, Dave, Wang, ZhanShan, Winter, Berend, Wu, Xin, in’ t Zand, Jean J. M., Ahangarianabhari, Mahdi, Ambrosi, Giovanni, Ambrosino, Filippo, Barbera, Marco, Basso, Stefano, Bayer, Jörg, Bellazzini, Ronaldo, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Borghi, Giacomo, Cao, XueLei, Cadoux, Franck, Ceraudo, Francesco, Chen, TianXiang, Chen, YuPeng, Chevenez, Jerome, Civitani, Marta, Cui, Wei, Cui, WeiWei, Dauser, Thoma, Del Monte, Ettore, Di Cosimo, Sergio, Diebold, Sebastian, Doroshenko, Victor, Dovciak, Michal, Du, YuanYuan, Ducci, Lorenzo, Fan, QingMei, Favre, Yannick, Fuschino, Fabio, Gálvez, José Lui, Gao, Min, Ge, MingYu, Gevin, Olivier, Grassi, Marco, Gu, QuanYing, Gu, YuDong, Han, DaWei, Hong, Bin, Hu, Wei, Ji, Long, Jia, ShuMei, Jiang, WeiChun, Kennedy, Thoma, Kreykenbohm, Ingo, Kuvvetli, Irfan, Labanti, Claudio, Latronico, Luca, Li, Gang, Li, MaoShun, Li, Xian, Li, Wei, Li, ZhengWei, Limousin, Olivier, Liu, HongWei, Liu, XiaoJing, Lu, Bo, Luo, Tao, Macera, Daniele, Malcovati, Piero, Martindale, Adrian, Michalska, Malgorzata, Meng, Bin, Minuti, Massimo, Morbidini, Alfredo, Muleri, Fabio, Paltani, Stephane, Perinati, Emanuele, Picciotto, Antonino, Piemonte, Claudio, Qu, JinLu, Rachevski, Alexandre, Rashevskaya, Irina, Rodriguez, Jerome, Schanz, Thoma, Shen, ZhengXiang, Sheng, LiZhi, Song, JiangBo, Song, LiMing, Sgro, Carmelo, Sun, Liang, Tan, Ying, Uttley, Phil, Wang, Bo, Wang, DianLong, Wang, GuoFeng, Wang, Juan, Wang, LangPing, Wang, YuSa, Watts, Anna L., Wen, XiangYang, Wilms, Jörn, Xiong, ShaoLin, Yang, JiaWei, Yang, Sheng, Yang, YanJi, Yu, Nian, Zhang, WenDa, Zampa, Gianluigi, Zampa, Nicola, Zdziarski, Andrzej A., Zhang, AiMei, Zhang, ChengMo, Zhang, Fan, Zhang, Long, Zhang, Tong, Zhang, Yi, Zhang, XiaoLi, Zhang, ZiLiang, Zhao, BaoSheng, Zheng, ShiJie, Zhou, YuPeng, Zorzi, Nicola, Zwart, J. Frans, and High Energy Astrophys. & Astropart. Phys (API, FNWI)

Subjects
Gravity (chemistry), Computer science, space mission: eXTP, X-ray timing, Polarimetry, General Physics and Astronomy, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, Physics and Astronomy (all), Settore FIS/05 - Astronomia E Astrofisica, Observatory, X-ray instrumentation, 0103 physical sciences, X-ray polarimetry, Ground segment, Aerospace engineering, 010306 general physics, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), High Energy Astrophysical Phenomena (astro-ph.HE), Spacecraft, sezele, business.industry, Payload, Gravitational wave, Astrophysics::Instrumentation and Methods for Astrophysics, Space Science, business, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources. The paper provides a detailed description of: (1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload; (2) the elements and functions of the mission, from the spacecraft to the ground segment., Accepted for publication on Sci. China Phys. Mech. Astron. (2019)

Published
2019
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