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

Author

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

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

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

Published
2024
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3. Performance of the New FlashCam-based Camera in the 28\,m Telescope of H.E.S.S

Author

Bi, Baiyang, Barcelo, Miquel, Bauer, Christian, Benkhali, Faical Ait, Catalano, Jacqueline, Diebold, Sebastian, Föhr, Christian, Funk, Stefan, Giavitto, Gianluca, Hermann, German, Hinton, Jim, Jung-Richardt, Ira, Kalekin, Oleg, Kankanyan, Ruben, Kihm, Thomas, Leuschner, Fabian, Pfeifer, Marc, Pühlhofer, Gerd, Reimer, Olaf, Sailer, Simon, Salzmann, Heiko, Santangelo, Andrea, Steinmassl, Simon, Schanz, Thomas, Tenzer, Chris, and Werner, Felix

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

In October 2019, the central 28 m telescope of the H.E.S.S. experiment has been upgraded with a new camera. The camera is based on the FlashCam design which has been developed in view of a possible future implementation in the Medium-Sized Telescopes of the Cherenkov Telescope Array (CTA), with emphasis on cost and performance optimization and on reliability. The fully digital design of the trigger and readout system makes it possible to operate the camera at high event rates and to precisely adjust and understand the trigger system. The novel design of the front-end electronics achieves a dynamic range of over 3,000 photoelectrons with only one electronics readout circuit per pixel. Here we report on the performance parameters of the camera obtained during the first year of operation in the field, including operational stability and optimization of calibration algorithms., Comment: Proceedings of the 37th International Cosmic Ray Conference (ICRC 2021)

Published
2021
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4. The Infra-Red Telescope (IRT) on board the THESEUS mission

Author

Götz, Diego, Basa, Stéphane, Pinsard, Frédéric, Martin, Laurent, Arhancet, Axel, Bozzo, Enrico, Cara, Christophe, Sanz, Isabel Escudero, Frugier, Pierre-Antoine, Floriot, Johan, Genolet, Ludovic, Heddermann, Paul, Floc'h, Emeric Le, Mer, Isabelle Le, Paltani, Stéphane, Pamplona, Tony, Paries, Céline, Prod'homme, Thibaut, Schneider, Benjamin, Tenzer, Chris, Tourrette, Thierry, and Triou, Henri

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Infra-Red Telescope (IRT) is part of the payload of the THESEUS mission, which is one of the two ESA M5 candidates within the Cosmic Vision program, planned for launch in 2032. The THESEUS payload, composed by two high energy wide field monitors (SXI and XGIS) and a near infra-red telescope (IRT), is optimized to detect, localize and characterize Gamma-Ray Bursts and other high-energy transients. The main goal of the IRT is to identify and precisely localize the NIR counterparts of the high-energy sources and to measure their distance. Here we present the design of the IRT and its expected performance., Comment: Proceedings of the SPIE 2020, paper 11444-305

Published
2021

5. 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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6. 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

8. Multi-technique investigation of silicon nitride/aluminum membranes as optical blocking filters for high-energy space missions

Author

Sciortino, Luisa, primary, Barbera, Marco, additional, Bonura, Salvatore Ferruggia, additional, Todaro, Michela, additional, Puccio, Elena, additional, D’Anca, Fabio, additional, Cicero, Ugo Lo, additional, Törmä, Pekka T., additional, Magnano, Elena, additional, Nappini, Silvia, additional, Píš, Igor, additional, Perinati, Emanuele, additional, Diebold, Sebastian, additional, Guzman, Alejandro, additional, Tenzer, Chris, additional, Buscarino, Gianpiero, additional, Gollwitzer, Christian, additional, Handick, Evelyn, additional, Krumrey, Michael, additional, Laubis, Christian, additional, Candia, Roberto, additional, and Varisco, Salvatore, additional

Published
2024
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9. Point and Interval Estimation on the Degree and the Angle of Polarization. A Bayesian approach

Author

Maier, Daniel, Tenzer, Chris, and Santangelo, Andrea

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

Linear polarization measurements provide access to two quantities, the degree (DOP) and the angle of polarization (AOP). The aim of this work is to give a complete and concise overview of how to analyze polarimetric measurements. We review interval estimations for the DOP with a frequentist and a Bayesian approach. Point estimations for the DOP and interval estimations for the AOP are further investigated with a Bayesian approach to match observational needs. Point and interval estimations are calculated numerically for frequentist and Bayesian statistics. Monte Carlo simulations are performed to clarify the meaning of the calculations. Under observational conditions, the true DOP and AOP are unknown, so that classical statistical considerations - based on true values - are not directly usable. In contrast, Bayesian statistics handles unknown true values very well and produces point and interval estimations for DOP and AOP, directly. Using a Bayesian approach, we show how to choose DOP point estimations based on the measured signal-to-noise ratio. Interval estimations for the DOP show great differences in the limit of low signal-to-noise ratios between the classical and Bayesian approach. AOP interval estimations that are based on observational data are presented for the first time. All results are directly usable via plots and parametric fits., Comment: 11 pages, 14 figures, 3 tables

Published
2014
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11. Calibration strategies for the LAD instrument on-board LOFT

Author

Pacciani, Luigi, Soffitta, Paolo, Argan, Andrea, Barret, Didier, Bozzo, Enrico, Feroci, Marco, Fraser, George W., Herder, Jan-Willem den, Pohl, Martin, Schmid, Christian, Tenzer, Chris, Vacchi, Andrea, Walton, Dave, Zampa, Gianluigi, and Zane, Silvia

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Scientific objectives of the LOFT mission, e.g., the study of the Neutron Star equation of state and of the Strong Gravity, require accurate energy, time and flux calibration for the 500k channels of the SDD detectors, as well as the knowledge of the detector dead-time and of the detector response with respect to the incident angle of the photons. We report here the evaluations made to asses the calibration issues for the LAD instrument. The strategies for both ground and on-board calibrations, including astrophysical observations, show that the goals are achievable within the current technologies., Comment: Proceedings of SPIE, Vol. 8443, Paper No. 8443-208, 2012

Published
2012
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13. 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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14. 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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15. SRG/eROSITA background analysis and simulation

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Perinati, Emanuele, Freyberg, Michael J., Pommranz, Christian M., Serim, M. Mirac, Yeung, Michael C. H., Dennerl, Konrad, Friedrich, Susanne, Tenzer, Chris, and Santangelo, Andrea

Published
2024
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16. eROSITA on SRG

Author

Predehl, Peter, Boehringer, Hans, Brunner, Hermann, Brusa, Marcella, Burwitz, Vadim, Cappelluti, Nico, Churazov, Evgeniy, Dennerl, Konrad, Finoguenov, Alexis, Freyberg, Michael, Friedrich, Peter, Hasinger, Guenther, Kendziorra, Eckhard, Kreykenbohm, Ingo, Schmid, Christian, Wilms, Joern, Lamer, Georg, Meidinger, Norbert, Muehlegger, Martin, Pavlinsky, Mikhail, Robrade, Jan, Santangelo, Andrea, Schmitt, Juergen, Schwope, Axel, Steinmetz, Matthias, Strueder, Lothar, Sunyaev, Rashid, and Tenzer, Chris

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

eROSITA (extended ROentgen Survey with an Imaging Telescope Array) is the core instrument on the Russian Spektrum-Roentgen-Gamma (SRG) mission which is scheduled for launch in late 2012. eROSITA is fully approved and funded by the German Space Agency DLR and the Max-Planck-Society.The design driving science is the detection of 50-100 thousands Clusters of Galaxies up to redshift z~1.3 in order to study the large scale structure in the Universe and test cosmological models, especially Dark Energy. This will be accomplished by an all-sky survey lasting for four years plus a phase of pointed observations. eROSITA consists of seven Wolter-I telescope modules, each equipped with 54 Wolter-I shells having an outer diameter of 360 mm. This would provide and effective area at 1.5 keV of ~1500 cm2 and an on axis PSF HEW of 15" which would provide an effective angular resolution of 25"-30". In the focus of each mirror module, a fast frame-store pn-CCD will provide a field of view of 1deg in diameter for an active FOV of ~0.83 deg2. At the time of writing the instrument development is currently in phase C/D., Comment: 6 Pages, 3 Figure, Proceedings of the conference "X-ray Astronomy 2009", Bologna, September 2009

Published
2010
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20. 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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21. 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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23. The instrument control unit processing hardware and software of the wide field monitor on eXTP

Author

Kalemci, Emrah, primary, Turhan, Onur, additional, Kuvvetli, Irfan, additional, Schanne, Stéphane, additional, Hernanz, Margarita, additional, Orleanski, Piotr, additional, Tenzer, Chris, additional, Sungur, Müberra, additional, Onat, Ahmet, additional, Bozkurt, Ayhan, additional, Baltaci, Mehmet A., additional, Galvez, José-Luis ., additional, Brandt, Søren, additional, Skup, Konrad R., additional, Tcherniak, Denis, additional, and Michalska, Malgorzata, additional

Published
2022
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24. 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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25. 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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26. 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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27. The X/Gamma-ray Imaging Spectrometer (XGIS) for THESEUS and other mission opportunities

Author

Amati, Lorenzo, primary, Labanti, Claudio, additional, Mereghetti, Sandro, additional, Frontera, Filippo, additional, Campana, Riccardo, additional, Auricchio, Natalia, additional, Baldazzi, Giuseppe, additional, Bellutti, Pierluigi, additional, Bertuccio, Giuseppe, additional, Branchesi, Marica, additional, Butler, Reginald C., additional, Caballero-Garcia, Maria D., additional, Camisasca, Anna E., additional, Castro-Tirado, Alberto J., additional, Cavazzini, Leo, additional, Ciolfi, Riccardo, additional, De Rosa, Adriano, additional, Evangelisti, Federico, additional, Farinelli, Ruben, additional, Ferro, Lisa, additional, Ficorella, Francesco, additional, Fiorini, Mauro, additional, Fuschino, Fabio, additional, Gasent-Blesa, José L., additional, Ghirlanda, Giancarlo, additional, Grassi, Marco, additional, Guidorzi, Cristiano, additional, Hedderman, Paul, additional, Kuvvetli, Irfan, additional, La Rosa, Giovanni, additional, Lorenzi, Paolo, additional, Malcovati, Piero, additional, Marchesini, Ezequiel, additional, Marisaldi, Martino, additional, Melchiorri, Michele, additional, Mele, Filippo, additional, Mikhalska, Malgorzata, additional, Orlandini, Mauro, additional, Orleanski, Piotr, additional, Pedersen, Soren M., additional, Pizzolla, Raffaele, additional, Rachevski, Alexandre, additional, Rashevskaya, Irina, additional, Rosati, Piero, additional, Reglero, Victor, additional, Ronchini, Samuele, additional, Santangelo, Andrea, additional, Salvaterra, Ruben, additional, Sarra, Paolo, additional, Sortino, Francesca, additional, Sottile, Giuseppe, additional, Stratta, Giulia, additional, Squerzanti, Stefano, additional, Stephen, John B., additional, Tenzer, Chris, additional, Terenzi, Luca, additional, Trois, Alessio, additional, Vacchi, Andrea, additional, Virgilli, Enrico, additional, Volpe, Angela, additional, Winkler, Marek, additional, Zampa, Gianluigi, additional, Zampa, Nicola, additional, and Zdziarski, Andrzej, additional

Published
2022
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28. 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

29. The X/Gamma-ray Imaging Spectrometer (XGIS) for THESEUS and other mission opportunities

Author

den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Amati, Lorenzo, Labanti, Claudio, Mereghetti, Sandro, Frontera, Filippo, Campana, Riccardo, Auricchio, Natalia, Baldazzi, Giuseppe, Bellutti, Pierluigi, Bertuccio, Giuseppe, Branchesi, Marica, Butler, Reginald C., Caballero-Garcia, Maria D., Camisasca, Anna E., Castro-Tirado, Alberto J., Cavazzini, Leo, Ciolfi, Riccardo, De Rosa, Adriano, Evangelisti, Federico, Farinelli, Ruben, Ferro, Lisa, Ficorella, Francesco, Fiorini, Mauro, Fuschino, Fabio, Gasent-Blesa, José L., Ghirlanda, Giancarlo, Grassi, Marco, Guidorzi, Cristiano, Hedderman, Paul, Kuvvetli, Irfan, Rosa, Giovanni La, Lorenzi, Paolo, Malcovati, Piero, Marchesini, Ezequiel, Marisaldi, Martino, Melchiorri, Michele, Mele, Filippo, Michalska, Malgorzata, Orlandini, Mauro, Orleanski, Piotr, Pedersen, Søren Møller, Piazzolla, Raffaele, Rachevski, Alexandre, Rashevskaya, Irina, Rosati, Piero, Reglero, Victor, Ronchini, Samuele, Santangelo, Andrea, Salvaterra, Ruben, Sarra, Paolo, Sortino, Francesca, Sottile, Giuseppe, Stratta, Giulia, Squerzanti, Stefano, Stephen, John B., Tenzer, Chris, Terenzi, Luca, Trois, Alessio, Vacchi, Andrea, Virgilli, Enrico, Volpe, Angela, Winkler, Marek, Zampa, Gianluigi, Zampa, Nicola, Zdziarski, Andrzej, den Herder, Jan-Willem A., Nikzad, Shouleh, Nakazawa, Kazuhiro, Amati, Lorenzo, Labanti, Claudio, Mereghetti, Sandro, Frontera, Filippo, Campana, Riccardo, Auricchio, Natalia, Baldazzi, Giuseppe, Bellutti, Pierluigi, Bertuccio, Giuseppe, Branchesi, Marica, Butler, Reginald C., Caballero-Garcia, Maria D., Camisasca, Anna E., Castro-Tirado, Alberto J., Cavazzini, Leo, Ciolfi, Riccardo, De Rosa, Adriano, Evangelisti, Federico, Farinelli, Ruben, Ferro, Lisa, Ficorella, Francesco, Fiorini, Mauro, Fuschino, Fabio, Gasent-Blesa, José L., Ghirlanda, Giancarlo, Grassi, Marco, Guidorzi, Cristiano, Hedderman, Paul, Kuvvetli, Irfan, Rosa, Giovanni La, Lorenzi, Paolo, Malcovati, Piero, Marchesini, Ezequiel, Marisaldi, Martino, Melchiorri, Michele, Mele, Filippo, Michalska, Malgorzata, Orlandini, Mauro, Orleanski, Piotr, Pedersen, Søren Møller, Piazzolla, Raffaele, Rachevski, Alexandre, Rashevskaya, Irina, Rosati, Piero, Reglero, Victor, Ronchini, Samuele, Santangelo, Andrea, Salvaterra, Ruben, Sarra, Paolo, Sortino, Francesca, Sottile, Giuseppe, Stratta, Giulia, Squerzanti, Stefano, Stephen, John B., Tenzer, Chris, Terenzi, Luca, Trois, Alessio, Vacchi, Andrea, Virgilli, Enrico, Volpe, Angela, Winkler, Marek, Zampa, Gianluigi, Zampa, Nicola, and Zdziarski, Andrzej

Abstract

We describe the science case, design and expected performances of the X/Gamma-ray Imaging Spectrometer (XGIS), a GRB and transients monitor developed and studied for the THESEUS mission project, capable of covering an exceptionally wide energy band (2 keV – 10 MeV), with imaging capabilities and location accuracy <15 arcmin up to 150 keV over a Field of View of 2sr, a few hundreds eV energy resolution in the X-ray band (<30 keV) and few micro seconds time resolution over the whole energy band. Thanks to a design based on a modular approach, the XGIS can be easily re-scaled and adapted for fitting the available resources and specific scientific objectives of future high-energy astrophysics missions, and especially those aimed at fully exploiting GRBs and high-energy transients for multi-messenger astrophysics and fundamental physics.

Published
2022

30. 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

32. Performance of the new FlashCam-based camera in the 28m telescope of H.E.S.S.

Author

Bi, Baiyang, primary, Barcelo, Miquel, additional, Bauer, Christian, additional, Benkhali, Faical Ait, additional, Catalano, Jacqueline, additional, Diebold, Sebastian, additional, Föhr, Christian, additional, Funk, Stefan, additional, Giavitto, Gianluca, additional, HERMANN, German, additional, Hinton, Jim, additional, Jung-Richardt, Ira, additional, KALEKIN, Oleg, additional, Kankanyan, Ruben, additional, KIHM, Thomas, additional, Leuschner, Fabian, additional, Pfeifer, Marc, additional, Pühlhofer, Gerd, additional, Reimer, Olaf, additional, Sailer, Simon, additional, Salzmann, Heiko, additional, Santangelo, Andrea, additional, Steinmassl, Simon, additional, SCHANZ, Thomas, additional, Tenzer, Chris, additional, and Werner, Felix, additional

Published
2021
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34. The Infra-Red Telescope (IRT) on board the THESEUS mission

Author

Götz, Diego, primary, Basa, Stéphane, additional, Pinsard, Frédéric, additional, Martin, Laurent, additional, Arhancet, Axel, additional, Bozzo, Enrico, additional, Cara, Christophe, additional, Escudero Sanz, Isabel, additional, Frugier, Pierre-Antoine, additional, Floriot, Johan, additional, Genolet, Ludovic, additional, Heddermann, Paul, additional, Le Floc'h, Emeric, additional, Le Mer, Isabelle, additional, Paltani, Stéphane, additional, Pamplona, Tony, additional, Paries, Céline, additional, Prod'homme, Thibaut, additional, Schneider, Benjamin, additional, Tenzer, Chris, additional, Tourrette, Thierry, additional, and Triou, Henri, additional

Published
2020
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35. SRG/eROSITA in-flight background at L2

Author

Freyberg, Michael, primary, Perinati, Emanuele, additional, Pacaud, Florian, additional, Eraerds, Tanja, additional, Churazov, Eugene, additional, Dennerl, Konrad, additional, Predehl, Peter, additional, Merloni, Andrea, additional, Meidinger, Norbert, additional, Bulbul, Esra, additional, Friedrich, Susanne, additional, Gilfanov, Marat, additional, Tenzer, Chris, additional, Pommranz, Christian, additional, Eckert, Dominique, additional, Schmitt, Juergen, additional, Brusa, Marcella, additional, and Santangelo, Andrea, additional

Published
2020
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37. 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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38. 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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39. 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, in't Zand, Jean, Michalska, Malgosia, Bozzo, Enrico, Kalemci, Emrah, Agudo, Ivan, Ahangarianabhari, Mahdi, Aitink-Kroes, Gabby, An, Zhenghua, Cao, Jiewei, Cao, Xuelei, Chen, Tianxiang, Chen, Can, Chen, Yupeng, Cheng, Yaodong, Cong, Min, Cui, Weiwei, Cui, Tao, Wu, Zhenyu, Liu, Yichen, Su, Yongquan, Wang, Jian, Zhang, Zhen, Jin, Ge, Li, Longhui, Qiu, Xiangbiao, Lin, Yanjian, Li, Tao, Zhang, Jiawei, Wu, Chao, Xu, Wei, Hu, Zexun, Xu, Zhao, Qiao, Fangjian, Pan, Kai, Zhang, Shu, Song, Liming, He, Huilin, Zhang, Fan, Liu, Hongwei, Liu, Xiaojing, Yang, Yanji, Song, Zeyu, Zhang, Jiawei, Yu, Ke, Wang, Yusa, Li, Wei, Han, Dawei, Wang, Juan, Zhang, Ziliang, Wang, Hao, Zhang, Dali, Gao, Min, Ma, Jia, Huo, Jia, Li, Maoshun, Hou, Dongjie, Yang, Xiongtao, Zhao, Zijian, Zhao, Xiaofan, Xu, Jingjing, Luo, Laidan, Zhu, Yuxuan, Zhang, Honglin, Liu, Xiaohua, Gu, Yudong, Du, Yuanyuan, Yang, Sheng, Sun, Liang, Jiang, Jiechen, Yang, Jiawei, Dong, Zefang, Dai, Boyu, Jiao, Yang, Wen, Xiangyang, Meng, Bin, Zhang, Aimei, Wang, Ruijie, Zhang, Tong, Lu, Bing, Gao, Na, Xu, Xiongwei, Luo, Tao, Qi, Liqiang, Li, Gang, Qu, Jinlu, Xiong, Shaolin, Tao, Liao, Jia, Shumei, Ge, Mingyu, Zheng, Shijie, Li, Xiaobo, Ma, Xiang, Huang, Yue, Li, Chengkui, Nie, Jianyin, Zhao, Haisheng, Guan, Ju, Liao, Jinyuan, Zhang, Hongmei, Zhang, Juan, Wang, Ping, Zhao, Xiaoyun, Wang, Lingjun, Zhang, Liang, Yi, Shuxu, Li, Bing, Tan, Ying, Qi, Fazhi, Wang, Wenshuai, Ou, Ge, Hu, Hao, Shi, Jingyan, Hu, Qingbao, Jiang, Xiaowei, Li, Haibo, Hu, Yu, Jiang, Bowen, Tenzer, Chris, Perinati, Emanuele, and Pliego, Samuel

Published
2022
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40. 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

41. 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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42. The wide field monitor onboard the eXTP mission

Author

Brandt, Søren K., primary, Hernanz, Margarita, primary, Feroci, Marco, primary, Orleański, Piotr, primary, Santangelo, Andrea, primary, Schanne, Stéphane, primary, Wu, Xin, primary, in't Zand, Jean, primary, Zhang, Shuangnan, primary, Olsen, Poul Erik, primary, Mansanet, Carlos, primary, Campana, Riccardo, primary, Fuschino, F., primary, Labanti, Claudio, primary, Zampa, Gianluigi, primary, Zampa, Nicola, primary, Bellutti, Pierluigi, primary, Borghi, Giacomo, primary, Ficorella, Francesco, primary, Picciotto, Antonino, primary, Zorzi, Nicola, primary, Limousin, Olivier, primary, Meris, Aline, primary, Xu, Yupeng, primary, Bozzo, Enrico, primary, Evangelista, Yuri, primary, Gálvez, José Luis, primary, Tenzer, Chris, primary, Zwart, Frans, primary, Lu, Fanjung, primary, Zhang, Shu, primary, Cheng, Tianxiang, primary, Ambrosino, F., primary, Argan, Andrea, primary, Del Monte, Ettore, primary, Budtz-Jorgensen, Carl, primary, Lund, Niels, primary, Rachevski, Alexander, primary, Vacchi, Andrea, primary, and Rashevskaya, Irina, primary

Published
2018
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44. Readout electronics testing during mass production of FlashCam cameras for the Cherenkov Telescope Array

Author

Diebold, Sebastian, primary, Tenzer, Chris, primary, Bauer, Christian, primary, Bernhard, Sabrina, primary, Biegger, Matthias, primary, Capasso, Massimo, primary, Eschbach, Stefan, primary, Florin, Daniel, primary, Föhr, Christian, primary, Funk, Stefan, primary, Gadola, Arno, primary, Marszalek, Adam, primary, Pfeifer, Marc, primary, Principe, Giacomo, primary, Pürckhauer, Sabina, primary, Rajda, Pawel J., primary, Reimer, Olaf, primary, Sailer, Simon, primary, Schwab, Thomas, primary, Steiner, Stefan, primary, Straumann, Ulrich, primary, Vollhardt, Achim, primary, Werner, Felix, primary, Wolf, David, primary, Zietara, Krzysztof, primary, Eisenkolb, Felix, primary, Kalkuhl, Christoph, primary, Puehlhofer, Gerd, primary, Santangelo, Andrea, primary, Schanz, Thomas, primary, Garrecht, Frank, primary, Hermann, German, primary, Jung, Ira, primary, Kalekin, Oleg, primary, Kasperek, Jerzy, primary, Kihm, Thomas, primary, Lahmann, Robert, primary, and Barcelo, Miquel, primary

Published
2017
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45. WFI electronics and on-board data processing

Author

den Herder, Jan-Willem A., Takahashi, Tadayuki, Bautz, Marshall, Plattner, Markus, Albrecht, Sebastian, Bayer, Jörg, Brandt, Søren, Drumm, Paul, Hälker, Olaf, Kerschbaum, Franz, Koch, Anna, Kuvvetli, Irfan, Meidinger, Norbert, Ott, Sabine, Ottensamer, Roland, Reiffers, Jonas, Schanz, Thomas, Skup, Konrad, Steller, Manfred, Tenzer, Chris, Thomas, Chris, den Herder, Jan-Willem A., Takahashi, Tadayuki, Bautz, Marshall, Plattner, Markus, Albrecht, Sebastian, Bayer, Jörg, Brandt, Søren, Drumm, Paul, Hälker, Olaf, Kerschbaum, Franz, Koch, Anna, Kuvvetli, Irfan, Meidinger, Norbert, Ott, Sabine, Ottensamer, Roland, Reiffers, Jonas, Schanz, Thomas, Skup, Konrad, Steller, Manfred, Tenzer, Chris, and Thomas, Chris

Published
2016

46. eROSITA on SRG

Author

Predehl, Peter, additional, Andritschke, Robert, additional, Babyshkin, Vladimir, additional, Becker, Werner, additional, Bornemann, Walter, additional, Bräuninger, Heinrich, additional, Brunner, Hermann, additional, Boller, Thomas, additional, Burwitz, Vadim, additional, Burkert, Wolfgang, additional, Clerc, Nicolas, additional, Churazov, Eugene, additional, Coutinho, Diogo, additional, Dennerl, Konrad, additional, Dwelly, Tom, additional, Eder, Josef, additional, Emberger, Valentin, additional, Freyberg, Michael, additional, Friedrich, Peter, additional, Fürmetz, Maria, additional, Georgakakis, Antonis, additional, Gilfanov, Marat, additional, Grossberger, Christoph, additional, Haberl, Frank, additional, Hälker, Olaf, additional, Hartner, Gisela, additional, v. Kienlin, Andreas, additional, Kink, Walter, additional, Kreykenbohm, Ingo, additional, Lamer, Georg, additional, Lomakin, Ilya, additional, Lapshov, Igor, additional, Meidinger, Norbert, additional, Merloni, Andrea, additional, Mican, Benjamin, additional, Müller, Siegfried, additional, Nandra, Kirpal, additional, Pavlinsky, Mikhail, additional, Pfeffermann, Elmar, additional, Pietschner, Daniel, additional, Robrade, Jan, additional, Salvato, Mara, additional, Santangelo, Andrea, additional, Sasaki, Manami, additional, Scheuerle, Hartmut, additional, Schmitt, Jürgen, additional, Schwope, Axel, additional, Sunyaev, Rashid, additional, Tenzer, Chris, additional, Yaroshenko, Valeri, additional, and Wilms, Jörn, additional

Published
2016
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47. WFI electronics and on-board data processing

Author

Plattner, Markus, additional, Albrecht, Sebastian, additional, Bayer, Jörg, additional, Brandt, Soeren, additional, Drumm, Paul, additional, Hälker, Olaf, additional, Kerschbaum, Franz, additional, Koch, Anna, additional, Kuvvetli, Irfan, additional, Meidinger, Norbert, additional, Ott, Sabine, additional, Ottensamer, Roland, additional, Reiffers, Jonas, additional, Schanz, Thomas, additional, Skup, Konrad, additional, Steller, Manfred, additional, Tenzer, Chris, additional, and Thomas, Chris, additional

Published
2016
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48. Multi-technique investigation of silicon nitride/aluminum membranes as optical blocking filters for high-energy space missions

Author

Sciortino, Luisa, Barbera, Marco, Bonura, Salvatore Ferruggia, Todaro, Michela, Puccio, Elena, D’Anca, Fabio, Cicero, Ugo Lo, Törmä, Pekka T., Magnano, Elena, Nappini, Silvia, Píš, Igor, Perinati, Emanuele, Diebold, Sebastian, Guzman, Alejandro, Tenzer, Chris, Buscarino, Gianpiero, Gollwitzer, Christian, Handick, Evelyn, Krumrey, Michael, Laubis, Christian, Candia, Roberto, and Varisco, Salvatore

Published
2023
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