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

Author

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

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

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

Published
2024
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2. Sensitivity of the GAPS Experiment to Low-energy Cosmic-ray Antiprotons

Author

Rogers, Field, Aramaki, Tsuguo, Boezio, Mirko, Boggs, Steven, Bonvicini, Valter, Bridges, Gabriel, Campana, Donatella, Craig, William W., von Doetinchem, Philip, Everson, Eric, Fabris, Lorenzo, Feldman, Sydney, Fuke, Hideyuki, Gahbauer, Florian, Gerrity, Cory, Hailey, Charles J., Hayashi, Takeru, Kawachi, Akiko, Kozai, Masayoshi, Lenni, Alex, Lowell, Alexander, Manghisoni, Massimo, Marcelli, Nadir, Mochizuki, Brent, Mognet, Isaac, Munakata, Kazuoki, Munini, Riccardo, Nakagami, Yusuke, Olson, Jerome, Ong, Rene, Osteria, Guiseppe, Perez, Kerstin M., Quinn, Sean, Re, Valerio, Riceputi, Elisa, Roach, Brandon, Ryan, Jaime, Saffold, Nathan, Scotti, Valentina, Shimizu, Yuki, Sparvoli, Roberta, Stoessl, Achim, Tiberio, Alessio, Vannuccini, Elena, Wada, Takuya, Xiao, Mengjiao, Yamatani, Masahiro, Yee, Kelsey, Yoshida, Atsumasa, Yoshida, Tetsuya, Zampa, Gianluigi, Zeng, Jiancheng, and Zweerink, Jeffrey

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

The General Antiparticle Spectrometer (GAPS) is an upcoming balloon mission to measure low-energy cosmic-ray antinuclei during at least three ~35-day Antarctic flights. With its large geometric acceptance and novel exotic atom-based particle identification, GAPS will detect ~500 cosmic antiprotons per flight and produce a precision cosmic antiproton spectrum in the kinetic energy range of ~0.07-0.21 GeV/n at the top of the atmosphere. With these high statistics extending to lower energies than any previous experiment, and with complementary sources of experimental uncertainty compared to traditional magnetic spectrometers, the GAPS antiproton measurement will be sensitive to dark matter, primordial black holes, and cosmic ray propagation. The antiproton measurement will also validate the GAPS antinucleus identification technique for the antideuteron and antihelium rare-event searches. This analysis demonstrates the GAPS sensitivity to cosmic-ray antiprotons using a full instrument simulation and event reconstruction, and including solar and atmospheric effects., Comment: 11 pages, 9 figures, revision updated with addition of Figure 5 and slight changes in the text to match the version accepted by Astroparticle Physics

Published
2022
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3. Snowmass2021 Cosmic Frontier: The landscape of cosmic-ray and high-energy photon probes of particle dark matter

Author

Aramaki, Tsuguo, Boezio, Mirko, Buckley, James, Bulbul, Esra, von Doetinchem, Philip, Donato, Fiorenza, Harding, J. Patrick, Karwin, Chris, Kumar, Jason, Leane, Rebecca K., Matsumoto, Shigeki, McEnry, Julie, Melia, Tom, Perez, Kerstin, Profumo, Stefano, Salazar-Gallegos, Daniel, Strong, Andrew W., Roach, Brandon, Sanchez-Conde, Miguel A., Shutt, Tom, Takada, Atsushi, Tanimori, Toru, Tomsick, John, Watanabe, Yu, and Williams, David A.

Subjects
High Energy Physics - Experiment, Astrophysics - High Energy Astrophysical Phenomena
Abstract

This white paper discusses the current landscape and prospects for experiments sensitive to particle dark matter processes producing photons and cosmic rays. Much of the gamma-ray sky remains unexplored on a level of sensitivity that would enable the discovery of a dark matter signal. Currently operating GeV-TeV observatories, such as Fermi-LAT, atmospheric Cherenkov telescopes, and water Cherenkov detector arrays continue to target several promising dark matter-rich environments within and beyond the Galaxy. Soon, several new experiments will continue to explore, with increased sensitivity, especially extended targets in the sky. This paper reviews the several near-term and longer-term plans for gamma-ray observatories, from MeV energies up to hundreds of TeV. Similarly, the X-ray sky has been and continues to be monitored by decade-old observatories. Upcoming telescopes will further bolster searches and allow new discovery space for lines from, e.g., sterile neutrinos and axion-photon conversion. Furthermore, this overview discusses currently operating cosmic-ray probes and the landscape of future experiments that will clarify existing persistent anomalies in cosmic radiation and spearhead possible new discoveries. Finally, the article closes with a discussion of necessary cross section measurements that need to be conducted at colliders to reduce substantial uncertainties in interpreting photon and cosmic-ray measurements in space., Comment: 61 pages, 21 figures, Snowmass2021 Cosmic Frontier White Paper

Published
2022

4. Astro 2020 Science White Paper: Cosmic-ray Antinuclei as Messengers for Dark Matter

Author

Perez, Kerstin, von Doetinchem, Philip, Aramaki, Tsuguo, Boezio, Mirko, Boggs, Steven E., Craig, William W., Fabris, Lorenzo, Fuke, Hideyuki, Gahbauer, Florian, Hailey, Charles J., and Ong, Rene

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Physics - Space Physics
Abstract

The origin of dark matter is a driving question of modern physics. Low-energy antideuterons provide a "smoking gun" signature of dark matter annihilation or decay, essentially free of astrophysical background. Low-energy antiprotons are a vital partner for this analysis, and low-energy antihelium could provide further discovery space for new physics. In the coming decade, AMS-02 will continue accumulating the large statistics and systematic understanding necessary for it to probe rare antinuclei signatures, and GAPS, which is the first experiment optimized specifically for low-energy cosmic antinuclei, will begin several Antarctic balloon campaigns. The connection of cosmic-ray antinuclei and dark matter is reviewed and the outlook in light of experimental progress is presented., Comment: 12 pages, 2 figures, Science White Paper submitted to the Astro2020 Decadal Survey. arXiv admin note: text overlap with arXiv:2002.04163

Published
2019

5. An Indirect Dark Matter Search Using Cosmic-Ray Antiparticles with GAPS

Author

Lowell, Alexander, Aramaki, Tsuguo, Bird, Ralph, Boezio, Mirko, Boggs, Steven, Carr, Rachel, Craig, William, von Doetinchem, Philip, Fabris, Lorenzo, Fuke, Hideyuki, Gahbauer, Florian, Gerrity, Cory, Hailey, Charles, Kato, Chihiro, Kawachi, Akiko, Kozai, Masayoshi, Mognet, Isaac, Munakata, Kazuoki, Okazaki, Shun, Ong, Rene, Osteria, Guiseppe, Perez, Kerstin, Quinn, Sean, Re, Valerio, Rogers, Field, Ryan, Jamie, Saffold, Nathan, Shimizu, Yuki, Stoessl, Achim, Yoshida, Atsumasa, Yoshida, Tetsuya, Zampa, Gianluigi, and Zweerink, Jeffrey

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract

Experiments aiming to directly detect dark matter (DM) particles have yet to make robust detections, thus underscoring the need for complementary approaches such as searches for new particles at colliders, and indirect DM searches in cosmic-ray spectra. Low energy (< 0.25 GeV/n) cosmic-ray antiparticles such as antideuterons are strong candidates for probing DM models, as the yield of these particles from DM processes can exceed the astrophysical background by more than two orders of magnitude. The General Antiparticle Spectrometer (GAPS), a balloon borne cosmic-ray detector, will perform an ultra-low background measurement of the cosmic antideuteron flux in the regime < 0.25 GeV/n, which will constrain a wide range of DM models. GAPS will also detect approximately 1000 antiprotons in an unexplored energy range throughout one long duration balloon (LDB) flight, which will constrain < 10 GeV DM models and validate the GAPS detection technique. Unlike magnetic spectrometers, GAPS relies on the formation of an exotic atom within the tracker in order to identify antiparticles. The GAPS tracker consists of ten layers of lithium-drifted silicon detectors which record dE/dx deposits from primary and nuclear annihilation product tracks, as well as measure the energy of the exotic atom deexcitation X-rays. A two-layer, plastic scintillator time of flight (TOF) system surrounds the tracker and measures the particle velocity, dE/dx deposits, and provides a fast trigger to the tracker. The nuclear annihilation product multiplicity, deexcitation X-ray energies, TOF, and stopping depth are all used together to discern between antiparticle species. This presentation provided an overview of the GAPS experiment, an update on the construction of the tracker and TOF systems, and a summary of the expected performance of GAPS in light of the upcoming LDB flight from McMurdo Station, Antarctica in 2020., Comment: 4 pages, 3 figures, The 39th International Conference on High Energy Physics (ICHEP2018), Seoul, Korea

Published
2018

7. Multi messenger astronomy and CTA: TeV cosmic rays and electrons

Author

Picozza, Piergiorgio and Boezio, Mirko

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Cosmic rays are a sample of solar, galactic and extragalactic matter. Their origin and properties are one of the most intriguing question in modern astrophysics. The most energetic events and active objects in the Universe: supernovae explosion, pulsars, relativistic jets, active galactic nuclei, have been proposed as sources of cosmic rays although unambiguous evidences have still to be found. Electrons, while comprising ~1% of the cosmic radiation, have unique features providing important information regarding the origin and propagation of cosmic rays in the Galaxy that is not accessible from the study of the cosmic-ray nuclear components due to their differing energy-loss processes. In this paper we will analyse, discussing the experimental uncertainties and challenges, the most recent measurements on cosmic-ray nuclei and, in particular, electrons with energies from tens of GeV into the TeV region., Comment: 24 pages, 10 figure, to appear in Astroparticle Physics as a special issue on CTA

Published
2012
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8. Chemical Composition of Galactic Cosmic Rays with Space Experiments

Author

Boezio, Mirko and Mocchiutti, Emiliano

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

The origin and properties of the cosmic radiation are one of the most intriguing question in modern astrophysics. The precise measurement of the chemical composition and energy spectra of the cosmic rays provides fundamental insight into these subjects. In this paper we will review the existing experimental data. Specifically, we will analyse results collected by space-born experiments discussing the experimental uncertainties and challenges with a focus on the PAMELA experiment., Comment: 42 pages, 13 figures. In Press Astrop. Phys. (2012)

Published
2012
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9. 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. Studies of cosmic-ray solar modulation with the PAMELA experiment

Author

Lenni, Alex, primary, Boezio, Mirko, additional, Munini, Riccardo, additional, Marcelli, Nadir, additional, Potgieter, Marius, additional, Ngobeni, Donald, additional, Adriani, Oscar, additional, Barbarino, Giancarlo C., additional, Bazilevskaya, Galina A., additional, Bellotti, Roberto, additional, Bogomolov, Edward A., additional, Bongi, Massimo, additional, Bonvicini, Valter, additional, Bruno, Alessandro, additional, Cafagna, Francesco, additional, Campana, Donatella, additional, Carlson, Per, additional, Casolino, Marco, additional, Castellini, Guido, additional, De Santis, Cristian, additional, Galper, Arkadiy M., additional, Koldashov, Sergey V., additional, Koldobskiy, Sergey, additional, Kvashnin, Alexander N., additional, Leonov, Alexey A., additional, Malakhov, Vitaly V., additional, Marcelli, Laura, additional, Martucci, Matteo, additional, Mayorov, Andrey G., additional, Menn, Wolfgang, additional, Mergé, Matteo, additional, Mikhailov, Vladimir V., additional, Mocchiutti, Emiliano, additional, Monaco, Alfonso, additional, Mori, Nicola, additional, Osteria, Giuseppe, additional, Panico, Beatrice, additional, Papini, Paolo, additional, Pearce, Mark, additional, Picozza, Piergiorgio, additional, Ricci, Marco, additional, Ricciarini, Sergio B., additional, Simon, Manfred, additional, Sotgiu, Alessandro, additional, Sparvoli, Roberta, additional, Spillantini, Piero, additional, Stozhkov, Yuri I., additional, Vacchi, Andrea, additional, Vannuccini, Elena, additional, Vasilyev, Gennady I., additional, Voronov, Sergey A., additional, Yurkin, Yuri T., additional, Zampa, Gianluigi, additional, and Zampa, Nicola, additional

Published
2023
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12. A 32-Channel Readout ASIC for X-Ray Spectrometry and Tracking in the GAPS Experiment

Author

Manghisoni, Massimo, Ghislotti, Luca, Lazzaroni, Paolo, Re, Valerio, Riceputi, Elisa, Ratti, Lodovico, Fabris, Lorenzo, Boezio, Mirko, and Zampa, Gianluigi

Abstract

This work describes the architecture and the experimental results from the characterization of a 32-channel mixed-signal application-specific integrated circuit (ASIC) developed for the readout of the lithium-drifted silicon (Si(Li)), detectors of the general antiparticle spectrometer (GAPS) experiment dedicated to searching for dark matter. The instrument is designed for the identification of antiprotons, antideuterons, and antihelium nuclei from cosmic rays during an Antarctic balloon mission scheduled for late 2024. A full-custom integrated circuit, named SLIDER32 (32-channel Si-Li detector readout) ASIC, has been produced in a commercial 180-nm CMOS technology. The ASIC comprises 32 low-noise analog readout channels featuring dynamic signal compression to comply with the wide input range, an 11-bit successive approximation register (SAR) analog-to-digital converter (ADC), and a digital back-end section which is responsible for channel setting and for sending digital information to the data acquisition system (DAQ). The circuit design criteria and the experimental results are discussed in this article.

Published
2024
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14. 南極周回気球による宇宙線反粒子探索実験GAPSの現状報告

Author

HAILEY, Charles, BOEZIO, Mirko, SHIMIZU, Yuki, IRIE, Yuka, SUZUKI, Shunsuke, WADA, Takuya, YOSHIDA, Atsumasa, FUKE, Hideyuki, MIZUKOSHI, keita, OGAWA, Hiroyuki, OKAZAKI, Shun, SHIRATORI, Hirohide, TOKUNAGA, Kakeru, YAMATANI, Masahiro, YOSHIDA, Tetsuya, KOZAI, Masayoshi, KATO, Chihiro, MUNAKATA, Kazuoki, KAWACHI, Akiko, KAWAMATA, Syusuke, KAWAMOTO, Yuki, NARA, Shotaro, and TAKAHASHI, Shun

Abstract

大気球シンポジウム 2022年度（2022年11月7-8日. ハイブリッド開催（JAXA相模原キャンパス& オンライン)), Balloon Symposium 2022 (November 7-8, 2022. Hybrid(in-person & online) Conference (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan, 著者人数: 26名, 資料番号: SA6000177012, レポート番号: isas22-sbs-012

Published
2022

15. 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

16. 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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17. 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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19. 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

20. 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

21. Design of an Antimatter Large Acceptance Detector In Orbit (ALADInO)

Author

Adriani, Oscar, primary, Altomare, Corrado, additional, Ambrosi, Giovanni, additional, Azzarello, Philipp, additional, Barbato, Felicia Carla Tiziana, additional, Battiston, Roberto, additional, Baudouy, Bertrand, additional, Bergmann, Benedikt, additional, Berti, Eugenio, additional, Bertucci, Bruna, additional, Boezio, Mirko, additional, Bonvicini, Valter, additional, Bottai, Sergio, additional, Burian, Petr, additional, Buscemi, Mario, additional, Cadoux, Franck, additional, Calvelli, Valerio, additional, Campana, Donatella, additional, Casaus, Jorge, additional, Contin, Andrea, additional, D’Alessandro, Raffaello, additional, Dam, Magnus, additional, De Mitri, Ivan, additional, de Palma, Francesco, additional, Derome, Laurent, additional, Di Felice, Valeria, additional, Di Giovanni, Adriano, additional, Donnini, Federico, additional, Duranti, Matteo, additional, Fiandrini, Emanuele, additional, Follega, Francesco Maria, additional, Formato, Valerio, additional, Gargano, Fabio, additional, Giovacchini, Francesca, additional, Graziani, Maura, additional, Ionica, Maria, additional, Iuppa, Roberto, additional, Loparco, Francesco, additional, Marín, Jesús, additional, Mariotto, Samuele, additional, Marsella, Giovanni, additional, Martínez, Gustavo, additional, Martínez, Manel, additional, Martucci, Matteo, additional, Masi, Nicolò, additional, Mazziotta, Mario Nicola, additional, Mergé, Matteo, additional, Mori, Nicola, additional, Munini, Riccardo, additional, Musenich, Riccardo, additional, Mussolin, Lorenzo, additional, Nozzoli, Francesco, additional, Oliva, Alberto, additional, Osteria, Giuseppe, additional, Pacini, Lorenzo, additional, Paniccia, Mercedes, additional, Papini, Paolo, additional, Pearce, Mark, additional, Perrina, Chiara, additional, Picozza, Piergiorgio, additional, Pizzolotto, Cecilia, additional, Pospíšil, Stanislav, additional, Pozzato, Michele, additional, Quadrani, Lucio, additional, Ricci, Ester, additional, Rico, Javier, additional, Rossi, Lucio, additional, Schioppa, Enrico Junior, additional, Serini, Davide, additional, Smolyanskiy, Petr, additional, Sotgiu, Alessandro, additional, Sparvoli, Roberta, additional, Surdo, Antonio, additional, Tomassetti, Nicola, additional, Vagelli, Valerio, additional, Velasco, Miguel Ángel, additional, Wu, Xin, additional, and Zuccon, Paolo, additional

Published
2022
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26. The GAPS experiment to search for dark matter using low-energy antimatter

Author

Massachusetts Institute of Technology. Department of Physics, Ong, Rene, Aramaki, Tsuguo, Bird, Ralph, Boezio, Mirko, Boggs, Steve E., Carr, Rachel, Craig, William, Von Doetinchem, Philip, Fabris, Lorenzo, Gahbauer, Florian, Gerrity, Cory, Fuke, Hideyuki, Hailey, Charles, Kato, Chihiro, Kawachi, Akiko, Kozai, Masayoshi, Mognet, Samuel Isaac, Munakata, K., Okazaki, Shun, Osteria, Giuseppe, Perez, Kerstin, Re, Valerio, Rogers, Field, Saffold, Nate, Shimizu, Yuki, Yoshida, Atsumasa, Yoshida, Tetsuya, Zampa, Gianluigi, Zweerink, Jeff, Massachusetts Institute of Technology. Department of Physics, Ong, Rene, Aramaki, Tsuguo, Bird, Ralph, Boezio, Mirko, Boggs, Steve E., Carr, Rachel, Craig, William, Von Doetinchem, Philip, Fabris, Lorenzo, Gahbauer, Florian, Gerrity, Cory, Fuke, Hideyuki, Hailey, Charles, Kato, Chihiro, Kawachi, Akiko, Kozai, Masayoshi, Mognet, Samuel Isaac, Munakata, K., Okazaki, Shun, Osteria, Giuseppe, Perez, Kerstin, Re, Valerio, Rogers, Field, Saffold, Nate, Shimizu, Yuki, Yoshida, Atsumasa, Yoshida, Tetsuya, Zampa, Gianluigi, and Zweerink, Jeff

Abstract

© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0). The GAPS experiment is designed to carry out a sensitive dark matter search by measuring low-energy cosmic ray antideuterons and antiprotons. GAPS will provide a new avenue to access a wide range of dark matter models and masses that is complementary to direct detection techniques, collider experiments and other indirect detection techniques. Well-motivated theories beyond the Standard Model contain viable dark matter candidates which could lead to a detectable signal of antideuterons resulting from the annihilation or decay of dark matter particles. The dark matter contribution to the antideuteron flux is believed to be especially large at low energies (E < 1 GeV), where the predicted flux from conventional astrophysical sources (i.e. from secondary interactions of cosmic rays) is very low. The GAPS low-energy antiproton search will provide stringent constraints on less than 10 GeV dark matter, will provide the best limits on primordial black hole evaporation on Galactic length scales, and will explore new discovery space in cosmic ray physics. Unlike other antimatter search experiments such as BESS and AMS that use magnetic spectrometers, GAPS detects antideuterons and antiprotons using an exotic atom technique. This technique, and its unique event topology, will give GAPS a nearly background-free detection capability that is critical in a rare-event search. GAPS is designed to carry out its science program using long-duration balloon flights in Antarctica. A prototype instrument was successfully flown from Taiki, Japan in 2012. GAPS has now been approved by NASA to proceed towards the full science instrument, with the possibility of a first long-duration balloon flight in late 2020. This presentation will motivate low-energy cosmic ray antimatter searches and it will discuss the current status of the GAP

Published
2021

27. 宇宙線反粒子探索GAPS実験計画の近況報告

Author

HAILEY, Charles, PEREZ, Kerstin, FABRIS, Lorenzo, CRAIG, William, ONG, Rene, BOGGS, Steven, DOETINCHEM, Philip von, BOEZIO, Mirko, FUKE, Hideyuki, KOZAI, Masayoshi, OGAWA, Hiroyuki, OKAZAKI, Shun, SAIJO, Masaru, TOKUNAGA, Kakeru, YAMATANI, Masahiro, YOSHIDA, Tetsuya, NAKAGAMI, Yusuke, WADA, Takuya, YOSHIDA, Atsumasa, IMAMURA, Hikaru, SHIMIZU, Yuki, YAMADA, Noboru, KOIKE, Takahisa, KATO, Chihiro, MUNAKATA, Kazuoki, NAGAI, Hiroki, IMANISHI, Yuka, KAWACHI, Akiko, KOBAYASHI, Shohei, MOTOKI, Makoto, NARA, Shotaro, TAKAHASHI, Shun, TAKEMURA, Kaoru, and INOUE, Takayoshi

Abstract

大気球シンポジウム 2020年度（2020年11月5-6日. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)）, 相模原市, 神奈川県, Balloon Symposium 2020 (November 5-6, 2020. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)), Sagamihara, Kanagawa Japan, 著者人数: 34名, 資料番号: SA6000151006, レポート番号: isas20-sbs-006

Published
2020

29. 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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30. 宇宙線反粒子探索GAPS実験計画の(特に日本チームの)現状報告

Author

Hailey, Charles, Perez, Kerstin, Fabris, Lorenzo, Craig, William, Ong, Rene, Boggs, Steven, Doetinchem, Philip von, Boezio, Mirko, 他GAPS, Collaboration, Fuke, Hideyuki, Kozai, Masayoshi, Ogawa, Hiroyuki, Okazaki, Shun, Sakimoto, Kazuhiro, Yoshida, Tetsuya, Konada, Takuya, Takeuchi, Shuto, Wada, Takuya, Watanabe, Tsubasa, Yoshida, Atsumasa, Shimizu, Yuki, Yamada, Noboru, Koike, Takahisa, Kato, Chihiro, Munakata, Kazuoki, Nagai, Hiroki, Kawachi, Akiko, Kondo, Manami, Miyazaki, Yousuke, Sato, Kaori, Takahashi, Shun, Takemura, Kaoru, Inoue, Takayoshi, and GAPS, Collaboration

Abstract

第19回宇宙科学シンポジウム (2019年1月9日-10日. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)相模原キャンパス), 相模原市, 神奈川県, 19th Space Science Symposium (January 9-10, 2019. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS)Sagamihara Campus), Sagamihara, Kanagawa Japan, 著者人数: 32名, 資料番号: SA6000144072, レポート番号: P-037

Published
2019

34. Cosmic Ray Electron and Positron Spectrum with the PAMELA Experiment

Author

Mikhailov, Vladimir, primary, Adriani, O., additional, Barbarino, G., additional, A. Bazilevskaya, G, additional, Bellotti, R., additional, Boezio, Mirko, additional, A. Bogomolov, E, additional, Bongi, M., additional, Bonvicini, V., additional, Bruno, A., additional, S. Cafagna, F, additional, Campana, D., additional, Carlson, P., additional, Casolino, M., additional, Castellini, G., additional, De Santis, C, additional, Di Felice, V, additional, M. Galper, A, additional, V. Karelin, A, additional, V. Koldashov, S, additional, A. Koldobsky, S, additional, A. Kvashnin, A, additional, N. Kvashnin, A, additional, A. Leonov, A, additional, V. Malakhov, V, additional, Marcell, L., additional, Martucci, M., additional, G. Mayorov, A, additional, Menn, W., additional, Mergé, M., additional, Mocchiutti, E., additional, Monaco, A., additional, Mori, N., additional, Munin, R., additional, Osteria, G., additional, Papini, P., additional, Panico, B., additional, Pearce, M., additional, Picozza, P., additional, Ricci, Marco, additional, B. Ricciarini, S, additional, Simon, M., additional, Sparvoli, R., additional, Spillantini, P., additional, I. Stozhkov, Yu, additional, Vacchi, A., additional, Vannuccini, E., additional, Vasilyev, I., additional, A. Voronov, S, additional, T. Yurkin, Yu, additional, Zampa, G., additional, and Zampa, N., additional

Published
2019
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35. Short-term variation in the galactic cosmic ray intensity measured with the PAMELA experiment

Author

Riccardo Munini, Alessandro Bruno, Christian Eric, Georgia A. De Nolfo, Martucci Matteo, Merge Matteo, Ryan James, Stochaj Steve, di Felice Valeria, Boezio Mirko, Potgieter Marius, Valeria Di Felice, Mirko Boezio, Oscar Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, E. A. Bogomolov, Massimo Bongi, Giovanni Bonvicini, S. Bottai, A. Bruno, Francesco Cafagna, D. Campana, Marco Casolino, Guido Castellini, C. De Santis, A. M. Galper, A. V. Karelin, S. V. Koldashov, S. Y. Krutkov, A. N. Kvashnin, A. Leonov, V. Malakhov, L. Marcelli, M. Martucci, A.G Mayorov, W. Menn, Mirko Merge', V. V. Mikhailov, E. Mocchiutti, A. Monaco, N. Mori, G. Osteria, Beatrice Panico, P. Papini, Mark Pearce, P. Picozza, Marco Ricci, Sergio B. Ricciarini, M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. A. Voronov, Y. T. Yurkin, G. Zampa, N. Zampa, M. S. Potgieter, E. C. Christian, I. Richardson, J.M Ryan, and S. Stochaj

Subjects
Physics, Solar wind, Neutron monitor, Amplitude, Physics::Space Physics, Coronal mass ejection, Forbush decrease, Cosmic ray, Astrophysics, Heliospheric current sheet, Heliosphere
Abstract

New results on the galactic cosmic ray (GCR) short-term intensity variation associated with Forbush decrease and co-rotating interaction regions (CIRs) measured by the PAMELA instrument between November 2006 and March 2007 are presented. Most of the past measurements on Forbush decrease events were carried out with neutron monitor detector. This tecnique allows only indirect detection of the overall GCR intensity over an integrated energy range. For the first time, thanks to the unique features of the PAMELA magnetic spectrometer, the Forbush decrease associated with the December 13th coronal mass ejection (CME) was studied in a wide rigidity range (0.4-20 GV) and for different species of GCRs detected directly in space. Using GCR protons, the amplitude and the recovery time of the Forbush decrease were studied for ten rigidity interval with a temporal resolution of one day. For comparison the helium and the electron intensity over time were also studied. The temporal evolution of the helium and proton intensity was found in good agreement while the electrons show, on average, a faster recovery time. This was interpreted as a charge-sign dependence introduced by drift motion experienced by the low rigidity (

Published
2017

36. Time dependence of the helium flux measured by PAMELA

Author

Panico, Beatrice, primary, Campana, D., additional, Osteria, G., additional, Barbarino, G. C, additional, Adriani, Oscar, additional, Bongi, Massimo, additional, Spillantini, P., additional, Mori, N., additional, Papini, P., additional, Vannuccini, E., additional, Bazilevskaya, G. A, additional, Kvashnin, A. N, additional, Stozhkov, Y. I, additional, Bellotti, R., additional, Monaco, A., additional, Bruno, A., additional, Cafagna, Francesco, additional, Boezio, Mirko, additional, Bonvicini, V., additional, Mocchiutti, E., additional, Vacchi, A., additional, Zampa, G., additional, Zampa, N., additional, Bogomolov, E. A, additional, Krutkov, S. Y, additional, Vasilyev, G. I, additional, Carlson, P., additional, Pearce, M., additional, Casolino, M., additional, Castellini, Guido, additional, Marcelli, L., additional, De Santis, C., additional, Mergé, M., additional, Picozza, P., additional, Sparvoli, R., additional, Munini, Riccardo, additional, Galper, A. M, additional, Karelin, A. V, additional, Koldashov, S. V, additional, Koldobskiy, S., additional, Yurkin, Y. T, additional, Malakhov, V., additional, Leonov, A., additional, Mayorov, A. G, additional, Mikhailov, V. V, additional, Voronov, S. A, additional, Martucci, M., additional, Menn, W., additional, Simon, M., additional, Ricci, Marco, additional, and Ricciarini, Sergio B., additional

Published
2017
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37. The PAMELA Experiment: A Cosmic Ray Experiment Deep Inside the Heliosphere

Author

Boezio, Mirko, primary, Munini, Riccardo, additional, Adriani, Oscar, additional, Barbarino, G. C., additional, Bazilevskaya, G. A., additional, Bellotti, R., additional, Bogomolov, E. A., additional, Bongi, Massimo, additional, Bonvicini, Giovanni, additional, Bottai, S., additional, Bruno, A., additional, Cafagna, Francesco, additional, Campana, D., additional, Carlson, P., additional, Casolino, M., additional, Castellini, Guido, additional, De Santis, C., additional, Di Felice, V., additional, Galper, A. M., additional, Karelin, A. V., additional, Koldashov, S. V., additional, Koldobskiy, S., additional, Krutkov, S. Y., additional, Kvashnin, A. N., additional, Leonov, A., additional, Malakhov, V., additional, Marcelli, L., additional, Martucci, M., additional, Mayorov, A. G., additional, Menn, W., additional, Merge', M., additional, Mikhailov, V. V., additional, Mocchiutti, E., additional, Monaco, A., additional, Mori, N., additional, Osteria, G., additional, Panico, B., additional, Papini, P., additional, Pearce, Mark, additional, Picozza, P., additional, Ricci, Marco, additional, Ricciarini, Sergio B., additional, Simon, M., additional, Sparvoli, R., additional, Spillantini, P., additional, Stozhkov, Y. I., additional, Vacchi, A., additional, Vannuccini, E., additional, Vasilyev, G., additional, Voronov, S. A., additional, Yurkin, Y. T., additional, Zampa, G., additional, and Zampa, N., additional

Published
2017
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38. Short-term variation in the galactic cosmic ray intensity measured with the PAMELA experiment

Author

Munini, Riccardo, primary, Bruno, Alessandro, additional, Eric, Christian, additional, De Nolfo, Georgia A., additional, Matteo, Martucci, additional, Matteo, Merge, additional, James, Ryan, additional, Steve, Stochaj, additional, Valeria, di Felice, additional, Mirko, Boezio, additional, Marius, Potgieter, additional, Di Felice, Valeria, additional, Boezio, Mirko, additional, Adriani, Oscar, additional, Barbarino, G. C., additional, Bazilevskaya, G. A., additional, Bellotti, R., additional, Bogomolov, E. A., additional, Bongi, Massimo, additional, Bonvicini, Giovanni, additional, Bottai, S., additional, Bruno, A., additional, Cafagna, Francesco, additional, Campana, D., additional, Casolino, Marco, additional, Castellini, Guido, additional, De Santis, C., additional, Galper, A. M., additional, Karelin, A. V., additional, Koldashov, S. V., additional, Krutkov, S. Y., additional, Kvashnin, A. N., additional, Leonov, A., additional, Malakhov, V., additional, Marcelli, L., additional, Martucci, M., additional, Mayorov, A.G, additional, Menn, W., additional, Merge', Mirko, additional, Mikhailov, V. V., additional, Mocchiutti, E., additional, Monaco, A., additional, Mori, N., additional, Osteria, G., additional, Panico, Beatrice, additional, Papini, P., additional, Pearce, Mark, additional, Picozza, P., additional, Ricci, Marco, additional, Ricciarini, Sergio B., additional, Simon, M., additional, Sparvoli, R., additional, Spillantini, P., additional, Stozhkov, Y. I., additional, Vacchi, A., additional, Vannuccini, E., additional, Vasilyev, G., additional, Voronov, S. A., additional, Yurkin, Y. T., additional, Zampa, G., additional, Zampa, N., additional, Potgieter, M. S., additional, Christian, E. C., additional, Richardson, I., additional, Ryan, J.M, additional, and Stochaj, S., additional

Published
2017
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39. PAMELA measurements of solar energetic particle spectra

Author

Mergé, Matteo, primary, Bruno, Alessandro, additional, Martucci, Matteo, additional, Adriani, Oscar, additional, Barbarino, Giancarlo, additional, Bazilevskaya, G. A., additional, Bellotti, Roberto, additional, Boezio, Mirko, additional, Bogomolov, E. A., additional, Bongi, Massimo, additional, Bonvicini, Giovanni, additional, Cafagna, Francesco, additional, Campana, Donatella, additional, Carlson, Per, additional, Casolino, Marco, additional, Castellini, Guido, additional, Christian, Eric, additional, De Santis, Cristian, additional, De Donato, Cinzia, additional, De Nolfo, Georgia A., additional, Di Felice, Valeria, additional, Galper, A. M., additional, Karelin, Alexander, additional, Koldashov, Sergey, additional, Koldobskiy, Sergey, additional, Krutkov, S. Y., additional, Kvashnin, Alexander, additional, Leonov, Alexey, additional, Malakhov, V., additional, Marcelli, Laura, additional, Marcelli, Nadir, additional, Mayorov, Andrey, additional, Mayorov, A. G., additional, Mikhailov, Vladimir, additional, Mocchiutti, Emiliano, additional, Monaco, Alfonso, additional, Mori, Nicola, additional, Munini, Riccardo, additional, Osteria, Giuseppe, additional, Panico, Beatrice, additional, Papini, Paolo, additional, Pearce, Mark, additional, Picozza, Piergiorgio, additional, Ricci, Marco, additional, Ricciarini, Sergio B., additional, Richardson, Ian, additional, Ryan, James, additional, Simon, Manfred, additional, Sparvoli, Roberta, additional, Spillantini, P., additional, Stochaj, Steven J., additional, Stozhkov, Yuriy, additional, Vacchi, Andrea, additional, Vannuccini, Elena, additional, Vasilyev, Gennady, additional, Voronov, Sergey, additional, Yurkin, Yuri, additional, Zampa, Gianluigi, additional, and Zampa, Nicola, additional

Published
2017
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40. Ten years of positron and electron solar modulation measured by the PAMELA experiment.

Author

Munini, Riccardo, primary, Boezio, Mirko, additional, Potgieter, Marius, additional, Di Felice, Valeria, additional, Adriani, Oscar, additional, Barbarino, G. C., additional, Bazilevskaya, G. A., additional, Bellotti, R., additional, Bogomolov, E. A., additional, Bongi, Massimo, additional, Bonvicini, Giovanni, additional, Bottai, S., additional, Bruno, A., additional, Cafagna, Francesco, additional, Campana, D., additional, Casolino, Marco, additional, Castellini, Guido, additional, Santis, C. de, additional, Galper, A. M., additional, Karelin, A. V., additional, Koldashov, S. V., additional, Krutkov, S. Y., additional, Kvashnin, A. N., additional, Leonov, A., additional, Malakhov, V., additional, Marcelli, L., additional, Martucci, M., additional, Mayorov, A.G, additional, Menn, W., additional, Merge', M., additional, Mikhailov, V. V., additional, Mocchiutti, E., additional, Monaco, A., additional, Mori, N., additional, Osteria, G., additional, Panico, Beatrice, additional, Papini, P., additional, Pearce, Mark, additional, Picozza, P., additional, Ricci, Marco, additional, Ricciarini, Sergio B., additional, Simon, M., additional, Sparvoli, R., additional, Spillantini, P., additional, Stozhkov, Y. I., additional, Vacchi, A., additional, Vannuccini, E., additional, Vasilyev, G., additional, Voronov, S. A., additional, Yurkin, Y. T., additional, Zampa, G., additional, Zampa, N., additional, Potgieter, M. S., additional, and Raath, J. L., additional

Published
2017
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42. Effect of the Jupiter magnetosphere on the cosmic ray protons measured with the PAMELA experiment

Author

Ricci, Marco, primary, Pizzella, Guido, additional, Martucci, Matteo, additional, Bruno, Alessandro, additional, Di Felice, Valeria, additional, Marcelli, Nadir, additional, Adriani, Oscar, additional, Barbarino, Giancarlo, additional, Bazilevskaya, G. A., additional, Bellotti, Roberto, additional, Boezio, Mirko, additional, Bogomolov, E. A., additional, Bongi, Massimo, additional, Bonvicini, Giovanni, additional, Cafagna, Francesco, additional, Campana, Donatella, additional, Carlson, Per, additional, Casolino, Marco, additional, Castellini, Guido, additional, De Santis, Cristian, additional, Galper, A. M., additional, Karelin, Alexander, additional, Koldashov, Sergey, additional, Koldobskiy, Sergey, additional, Krutkov, S. Y., additional, Kvashnin, Alexander, additional, Leonov, Alexey, additional, Malakhov, V., additional, Marcelli, Laura, additional, Mayorov, Andrey, additional, Mayorov, A. G., additional, Mergé, Matteo, additional, Mikhailov, Vladimir, additional, Mocchiutti, Emiliano, additional, Monaco, Alfonso, additional, Mori, Nicola, additional, Munini, Riccardo, additional, Osteria, Giuseppe, additional, Panico, Beatrice, additional, Papini, Paolo, additional, Pearce, Mark, additional, Picozza, Piergiorgio, additional, Ricciarini, Sergio B., additional, Simon, Manfred, additional, Sparvoli, Roberta, additional, Spillantini, P., additional, Stozhkov, Yuriy, additional, Vacchi, Andrea, additional, Vannuccini, Elena, additional, Vasilyev, Gennady, additional, Voronov, Sergey, additional, Yurkin, Yuri, additional, Zampa, Gianluigi, additional, and Zampa, Nicola, additional

Published
2017
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43. Time dependence of the proton and helium flux measured by PAMELA

Author

Panico, Beatrice, primary, Osteria, Giuseppe, additional, Campana, Donatella, additional, Barbarino, Giancarlo, additional, Adriani, Oscar, additional, Bongi, Massimo, additional, Spillantini, Piero, additional, Mori, Nicola, additional, Papini, Paolo, additional, Vannuccini, Elena, additional, Bazilevskaya, Galina, additional, Kvashnin, Anatolii, additional, Stozhkov, Yul, additional, Bellotti, Riccardo, additional, Monaco, Alfonso, additional, Bruno, Alessandro, additional, Cafagna, Francesco, additional, Boezio, Mirko, additional, Bonvicini, Valter, additional, Mocchiutti, Emiliano, additional, Munini, Riccardo, additional, Zampa, Nicola, additional, Zampa, Gianluigi, additional, Vacchi, Andrea, additional, Bogomolov, Eduard, additional, Krutkov, Sergey, additional, Vasilyev, Sergey, additional, Carlson, Per, additional, Pearce, Mark, additional, Casolino, Marco, additional, Castellini, Sergio, additional, De Santis, Cristian, additional, Sparvoli, Roberta, additional, Marcelli, Laura, additional, Mergé, Matteo, additional, Picozza, Piergiorgio, additional, Di Felice, Valeria, additional, Galper, Arkadiy, additional, Karelin, Alexander, additional, Koldashov, Sergey, additional, Koldobskiy, Sergey, additional, Yurkin, Yuriy T., additional, Malakhov, Vitaly, additional, Leonov, Alexey, additional, Mayorov, A.G, additional, Mikhailov, Vladimir, additional, Voronov, Sergey, additional, Martucci, Matteo, additional, Menn, Wolfgang, additional, Simon, Manfred, additional, Ricci, Marco, additional, and Ricciarini, Sergio B., additional

Published
2017
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44. The GAPS experiment to search for dark matter using low-energy antimatter

Author

Ong, Rene, primary, Aramaki, Tsuguo, additional, Bird, Ralph, additional, Boezio, Mirko, additional, Boggs, Steve E., additional, Carr, Rachel, additional, Craig, William, additional, Von Doetinchem, Philip, additional, Fabris, Lorenzo, additional, Gahbauer, Florian, additional, Gerrity, Cory, additional, Fuke, Hideyuki, additional, Hailey, Charles, additional, Kato, Chihiro, additional, Kawachi, Akiko, additional, Kozai, Masayoshi, additional, Mognet, Samuel Isaac, additional, Munakata, K., additional, Okazaki, Shun, additional, Osteria, Giuseppe, additional, Perez, Kerstin, additional, Re, Valerio, additional, Rogers, Field, additional, Saffold, Nate, additional, Shimizu, Yuki, additional, Yoshida, Atsumasa, additional, Yoshida, Tetsuya, additional, Zampa, Gianluigi, additional, and Zweerink, Jeff, additional

Published
2017
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48. The electron-hadron separation performance of the PAMELA electromagnetic calorimeter

Author

Boezio, Mirko, Pearce, Mark, Albi, M., Bonvicini, V., Lund, Jens, Lundquist, J., Mocchiutti, Emiliano, Vacchi, A., Zampa, G., Zampa, N., Boezio, Mirko, Pearce, Mark, Albi, M., Bonvicini, V., Lund, Jens, Lundquist, J., Mocchiutti, Emiliano, Vacchi, A., Zampa, G., and Zampa, N.

Abstract

A silicon-tungsten sampling imaging calorimeter has been designed and built for thePAMELA satellite-borne experiment. The main physics goals of the experiment are themeasurement of the flux of antiprotons (80 MeV-190 GeV) and positrons (50 MeV-270 GeV) in the cosmic radiation. The calorimeter has been designed to identify antiprotons from an electron background and positrons in a background of protons with a high efficiency and rejection power. This work presents the electron-hadron separationcapabilities of the calorimeter as obtained using both Monte Carlo and test beam data.The calorimeter is found to have sufficient performance to reach the primary scientific objectives of PAMELA, providing a proton rejection factor of ∼105 while keeping a ∼90% efficiency in selecting electrons and positrons. From simulations, an electron rejection factor of ∼105 in antiproton measurements (∼90% antiproton identification efficiency) is demonstrated., QC 20120228

Published
2006
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49. Preliminary results of studying the effect of heavy charged particles on the human central nervous system in experiments SilEye and Alteino

Author

Avdeev, S. V., Galper, A. M., Korotkov, M. G., Popov, A. V., Ivanova, A. V., Picozza, P., Bidoli, V., Casolino, M., de Pascale, M. P., Furano, G., Modena, I., Morselli, A., Narici, L., Reali, E., Sparvoli, R., Ricci, M., Spillantini, P., Castellini, G., Bonvicini, W., Vacchi, A., Zampa, N., Carlson, Per J., Boezio, Mirko, Fuglesang, C., Salnitsky, V. P., Trukhanov, K. A., Shevchenko, O. I., Avdeev, S. V., Galper, A. M., Korotkov, M. G., Popov, A. V., Ivanova, A. V., Picozza, P., Bidoli, V., Casolino, M., de Pascale, M. P., Furano, G., Modena, I., Morselli, A., Narici, L., Reali, E., Sparvoli, R., Ricci, M., Spillantini, P., Castellini, G., Bonvicini, W., Vacchi, A., Zampa, N., Carlson, Per J., Boezio, Mirko, Fuglesang, C., Salnitsky, V. P., Trukhanov, K. A., and Shevchenko, O. I.

Abstract

A series of experiments were carried out in the period 1995 to 2002 to study the phenomenon of light flashes (LFs) which arose in the eyes of astronauts. These experiments were made onboard the Mir orbital station (SilEye, SilEye-2) and on the Russian segment of the International Space Station (SilEye-3/Alteino). As a result of investigation it is reliably demonstrated that the majority of light flashes under conditions of a space flight are caused by nuclei of cosmic rays. Electric signals from brain, recorded during LF occurrence, were an important final result of these studies., QC 20141201

Published
2005

50. Measuring the size of the proton

Author

Vacchi, Andrea, primary, Adamczak, Andrzej, additional, Andreson, Benjamin, additional, Bakalov, Dimitar, additional, Stoilov, Michail, additional, Battistoni, Giuseppe, additional, Bhattacharya, Nandini, additional, Urbach, Paul, additional, Boezio, Mirko, additional, Bonvicini, Walter, additional, Zampa, Nicola, additional, Bonesini, Maurizio, additional, Danailov, Miltcho, additional, Demidovich, Alexander, additional, Dzagli, Milohum, additional, Gadedjisso-Tossou, Komlan, additional, Niemela, Joe, additional, Stoychev, Lyubomir, additional, Sumeet, Kumar, additional, and Ramponi, Roberta, additional

Published
2012
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