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201. AGILE Observations of Two Repeating Fast Radio Bursts with Low Intrinsic Dispersion Measures

Author: A. Pellizzoni, E. Costa, M. Tavani, A. Ursi, A. Giuliani, Martino Marisaldi, G. Piano, A. Morselli, M. Pilia, A. Ferrari, C. Casentini, F. Longo, F. Fuschino, A. Argan, P. W. Cattaneo, M. Feroci, Andrea Bulgarelli, L. A. Antonelli, G. Barbiellini, N. Parmiggiani, F. Paoletti, P. A. Caraveo, M. Cardillo, I. Donnarumma, F. Lazzarotto, A. W. Chen, Claudio Labanti, M. Galli, F. Verrecchia, Francesco Lucarelli, C. Pittori, S. Vercellone, P. Lipari, Casentini, C., Verrecchia, F., Tavani, M., Ursi, A., Antonelli, L. A., Argan, A., Barbiellini, G., Bulgarelli, A., Caraveo, P., Cardillo, M., Cattaneo, P. W., Chen, A., Costa, E., Donnarumma, I., Feroci, M., Ferrari, A., Fuschino, F., Galli, M., Giuliani, A., Labanti, C., Lazzarotto, F., Lipari, P., Longo, F., Lucarelli, F., Marisaldi, M., Morselli, A., Paoletti, F., Parmiggiani, N., Pellizzoni, A., Piano, G., Pilia, M., Pittori, C., and Vercellone, S.
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Radio transient sources, Millisecond, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Magnetar, Gamma-ray transient sources, Luminosity, X-ray transient, Fast radio bursts, Gamma-ray Astrophysics, Space and Planetary Science, Dispersion (optics), Magnetars, Astrophysics - High Energy Astrophysical Phenomena, Energy (signal processing), Isotropic energy, Fast radio burst
Abstract: We focus on two repeating fast radio bursts (FRBs) recently detected by the CHIME/FRB experiment in 2018--2019 (Source 1: 180916.J0158+65, and Source 2: 181030.J1054+73). These sources have low excess dispersion measures (DMs) ($ < 100 \rm \, pc \, cm^{-3}$ and $ < 20 \rm \, pc \, cm^{-3}$, respectively), implying relatively small maximal distances. They were repeatedly observed by AGILE in the MeV--GeV energy range. We do not detect prompt emission simultaneously with these repeating events. This search is particularly significant for the submillisecond and millisecond integrations obtainable by AGILE. The sources are constrained to emit a MeV-fluence in the millisecond range below $F'_{MeV} = 10^{-8} \, \rm erg \, cm^{-2}$ corresponding to an isotropic energy near $E_{MeV,UL} \simeq 2 \times 10^{46}\,$erg for a distance of 150 Mpc (applicable to Source 1). We also searched for $\gamma$-ray emission for time intervals up to 100 days, obtaining 3$\,\sigma$ upper limits (ULs) for the average isotropic luminosity above 50 MeV, $L_{\gamma,UL} \simeq \,$(5-10)$\,\times 10^{43} \rm \, erg \, s^{-1}$. For a source distance near 100 kpc (possibly applicable to Source 2), our ULs imply $E_{MeV,UL}\simeq10^{40} \rm erg$, and $L_{\gamma,UL} \simeq \,$2$\,\times 10^{37} \rm \, erg \, s^{-1}$. Our results are significant in constraining the high-energy emission of underlying sources such as magnetars, or other phenomena related to extragalactic compact objects, and show the prompt emission to be lower than the peak of the 2004 magnetar outburst of SGR 1806-20 for source distances less than about 100 Mpc., Comment: to be published in ApJL
Published: 2020

202. The LOFT Mission Concept - A Status Update

Author: Feroci, M, Bozzo, E, Brandt, S, Hernanz, M, van Der Klis, M, Liu , L. -P, Orleanski, P, Pohl, M, Santangelo, A, Schanne, S, Stella, L, Takahashi, T, Tamura, H, Watts, A, Wilms, J, Zane, S, Zhang, S. -N, Bhattacharyya, S, Agudo, I, Ahangarianabhari, M, Albertus, C, Alford, M, Alpar, A, Altamirano, D, Alvarez, L, Amati, L, Amoros, C, Andersson, N, Antonelli, A, Argan, A, Artigue, R, Artigues, B, Atteia, J. -L, Azzarello, P, Bakala, P, Ballantyne, D. R, Baldazzi, G, Baldo, M, Balman, S, Barbera, M, van Baren, C, Barret, D, Baykal, A, Begelman, M, Behar, E, Behar, O, Belloni, T, Belluti, P, Bernardini, F, Bertuccio, G, Bianchini, A, Binko, P, Blay, P, Bocchino, P, Bode, M, Bodin, P, Bombaci, I, Bonnet Bidaud, J. -M, Schnittman, Jeremy David, Borghi, G, Boutloukos, N, Bouyjou, F, Bradley, L, Braga, J, Briggs, M. S, Brown, E, Buballa, M, Bucciantini, N, Burderi, L, Burgay, M, Bursa, M, Budtz-Jorgensen, C, Cackett, E, Cadoux, F. R, Cais, P, Caliandro, G. A, Campana, R, Campana, S, Cao, X, Capitanio, F, Casares, J, Casella, P, Castro-Tirado, A. J, Cavazzuti, E, Cavechi, Y, Celestin, S, Cerda-Duran, P, Chakrabarty, D, Chamel, N, Chateau, F, Chen, C, Chen, Y, Chenevez, J, Chernyakova, M, Coker, J, Cole, R, Collura, A, Coriat, M, Cornelisse, R, Costamante, L, Cros, A, Cui, W, Cumming, A, Cusumano, G, Czerny, B, D'Ai, A, D'Ammando, J. P. C, D'Elia, V, Dai, Z, Del Monte, E, De Luca, A, De Martino, D, Dercksen, J. P. C, De Pasquale, M, De Rosa, A, Del Santo, M, Di Cosimo, S, Degenaar, N, den Herder, J. W, Diebold, S, Di Salvo, T, Dong, Y, Donnarumma, I, Doroshenko, V, Doyle, G, Drake, S. A, Durant, M, Emmanoulopoulos, D, Enoto, T, Erkut, M. H, Esposito, P, Evangelista, Y, Fabian, A, Falanga, M, Favre, Y, Feldman, C, Fender, R, Feng, H, Ferrari, V, Ferrigno, C, Ficorella, F, Finger, M, Finger, M. H, Fraser, G. W, Frericks, N, Fullekrug, M, Fuschino, F, Gabler, M, Galloway, D. K, Galvez Sanchez, J. L, Gandhi, P, Gao, Z, Garcia-Berro, E, Gendre, B, Gevin, O, Gezari, S, Giles, A. B, Gilfanov, M, Giommi, P, Giovannini, G, Giroletti, M, Gogus, E, Goldwurm, A, Goluchova, K, Gotz, D, Gou, L, Gouiffes, C, Grandi, P, Grassi, M, Greiner, J, Grinberg, V, Groot, P, Gschwender, M, Gualtieri, L, Guedel, M, Guidorzi, C, Guy, L, Haas, D, Haensel, P, Hailey, M, Hamuguchi, K, Hansen, F, Hartmann, D. H, Haswell, C. A, Hebeler, K, Heger, A, Hempel, M, Hermsen, W, Homan, J, Hornstrup, A, Hudec, R, Huovelin, J, Huppenkothen, A, Inam, S. C, Ingram, A, in't Zand, J. J. M, Israel, G, Iwasawa, K, Izzo, L, Jacobs, H. M, Jetter, F, Johannsen, T, Jenke, P. A, Jonker, P, Jose, J, Kaaret, P, Kalamkar, M, Kalemci, E, Kanbach, G, Karas, V, Karelin, D, Kataria, D, Keek, L, Kennedy, T, Klochkov, D, Kluzniak, W, Koerding, E, Kokkotas, K, Komossa, S, Korpela, S, Kouveliotou, C, Kowalski, A. F, Kreykenbohm, I, Kuiper, L. M, Kunneriath, D, Kurkela, A, Kuvvetli, I, La Franca, F, Labanti, C, Lai, D, Lamb, F. K, Lachaud, C, Laubert, P. P, Lebrun, F, Li, X, Liang, E, Limousin, O, Lin, D, Linares, M, Linder, D, Lodato, G, Longo, F, Lu, F, Lund, N, Maccarone, T. J, Macera, D, Maestre, S, Mahmoodifar, S, Maier, D, Malcovati, P, Malzac, J, Malone, C, Mandel, D, Mangano, V, Manousakis, A, Marelli, M, Margueron, J, Marisaldi, M, Markoff, S. B, Markowitz, A, Marinucci, A, Martindale, A, Martinez, G, McHardy, I. M, Medina-Tanco, G, Mehdipour, M, Melatos, A, Mendez, M, Mereghetti, S, Migliari, S, Mignani, R, Michalska, M, Mihara, T, Miller, M. C, Miller, J. M, Mineo, T, Miniutti, G, Morsink, S, Motch, C, Motta, S, Mouchet, M, Mouret, G, Mulacova, J, Muleri, F, Munoz-Darias, T, Negueruela, I, Neilsen, J, Neubert, T, Norton, A. J, Nowak, M, Nucita, A, O'Brien, P, Oertel, M, Olsen, P. E. H, Orienti, M, Orio, M, Orlandini, M, Osborne, J. P, Osten, R, Ozel, F, Pacciani, L, Paerels, F, Paltini, S, Paolillo, M, Papadakis, I, Papitto, A, Paragi, Z, Paredes, J. M, Patruno, A, Paul, B, Pederiva, F, Perinati, E, Pellizzoni, A, Penacchioni, A. V, Peretz, U, Perez, M. A, Perez-Torres, M, Petersen, B. M, Petracek, V, Picciotto, A, Piemonte, C, Pittori, C, Pons, J, Portell, J, Possenti, A, Postnov, K, Poutanen, J, Prakash, M, Prandoni, I, Provost, H. Le, Psaltis, D, Pye, J, Qu, J, Rambaud, D, Ramon, P, Ramsay, G, Rapisarda, M, Rachevski, A, Rashevskaya, I, Ray, P. S, Rea, N, Reddy, S, Reig, P, Reina, M. Aranda, Remillard, R, Reynolds, C, Rezzolla, L, Ribo, M, Rie, R. de la, Riggio, A, Rios, A, Rischke, D. H, Rodríguez-Gil, P, Rodriguez, J, Rohlfs, R, Romano, P, Rossi, E. M .R, Rozanska, A, Rousseau, A, Rudak, B, Russell, D. M, Ryde, F, Sabau-Graziati, L, Sakamoto, T, Sala, G, Salvaterra, R, Salvetti, D, Sanna, A, Sandberg, J, Savolainen, T, Scaringi, S, Schaffner-Bielich, J, Schatz, H, Schee, J, Schmid, C, Serino, M, Shakura, N, Shore, S, Schnittman, J. D, Schneider, R, Schwenk, A, Schwope, A. D, Sedrakian, A, Seyler, J.-Y, Shearer, A, Slowikowska, A, Sims, M, Smith, A, Smith, D. M, Smith, P. J, Sobolewska, M, Sochora, V, Soffitta, P, Soleri, P, Song, L, Spencer, A, Stamerra, A, Stappers, B, Staubert, R, Steiner, A. W, Stergioulas, N, Stevens, A. L, Stratta, G, Strohmayer, T. E, Stuchlik, Z, Suchy, S, Suleimanov, V, Tamburini, F, Tauris, T, Tavecchio, F, Tenzer, C, Thielemann, F. K, Tiengo, A, Tolos, L, Tombesi, F, Tomsick, J, Torok, G, Torrejon, J. M, Torres, D. F, Torresi, E, Tramacere, A, Traulsen, I, Trois, A, Turolla, R, Turriziani, S, Typel, S, Uter, P, Uttley, P, Vacchi, A, Varniere, P, Vaughan, S, Vercellone, S, Vietri, M, Vincent, F. H, Vrba, V, Walton, D, Wang, J, Wang, Z, Watanabe, S, Wawrzaszek, R, Webb, N, Weinberg, N, Wende, H, Wheatley, P, Wijers, R, Wijnands, R, Wille, M, Wilson-Hodge, C. A, Winter, B, Walk, S. J, Wood, K, Woosley, S. E, Wu, X, Xiao, L, Xu, R, Yu, W, Yuan, F, Yuan, W, Yuan, Y, Zampa, G, Zampa, N, Zampieri, L, Zdunik, L, Zdziarski, A, Zech, A, Zhang, B, Zhang, C, Zhang, S, Zingale, M, Zorzi, N, and Zwart, F
Subjects: Astrophysics
Abstract: The Large Observatory For x-ray Timing (LOFT) is a mission concept which was proposed to ESA as M3 and M4 candidate in the framework of the Cosmic Vision 2015-2025 program. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument and the uniquely large field of view of its wide field monitor, LOFT will be able to study the behaviour of matter in extreme conditions such as the strong gravitational field in the innermost regions close to black holes and neutron stars and the supra-nuclear densities in the interiors of neutron stars. The science payload is based on a Large Area Detector (LAD, is greater than 8m2 effective area, 2-30 keV, 240 eV spectral resolution, 1 degree collimated field of view) and a Wide Field Monitor (WFM, 2-50 keV, 4 steradian field of view, 1 arcmin source location accuracy, 300 eV spectral resolution). The WFM is equipped with an on-board system for bright events (e.g., GRB) localization. The trigger time and position of these events are broadcast to the ground within 30 s from discovery. In this paper we present the current technical and programmatic status of the mission.
Published: 2016
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203. Human Adenovirus 7d Strains Associated with Influenza-Like Illness, New York, USA, 2017–2019

Author: Michael Popowich, Kirsten St. George, Daryl M. Lamson, Adriana E. Kajon, and Meghan E. Fuschino
Subjects: Microbiology (medical), colleges, Variable severity, Epidemiology, 030231 tropical medicine, New York, Acute respiratory disease, influenza-like illness, lcsh:Medicine, Biology, whole-genome sequence, Human adenovirus 7, lcsh:Infectious and parasitic diseases, 03 medical and health sciences, 0302 clinical medicine, Influenza, Human, Research Letter, Humans, viruses, lcsh:RC109-216, 030212 general & internal medicine, Clade, Phylogeny, Genetic diversity, Influenza-like illness, Phylogenetic tree, Adenoviruses, Human, phylogenetic analysis, lcsh:R, Respiratory pathogen, genetic diversity, Virology, United States, Infectious Diseases, Human Adenovirus 7d Strains Associated with Influenza-like Illness, New York, USA, 2017–2019, Virus Diseases
Abstract: Human adenovirus 7d is a respiratory pathogen capable of causing acute respiratory disease of variable severity. Phylogenetic analysis of whole-genome sequences of 15 strains isolated from cases of influenza-like-illness during 2017-2019 demonstrated the circulation of 2 distinct clades of genomic variant 7d in colleges in New York, USA.
Published: 2020

204. Design and construction of the Mini-Calorimeter of the AGILE satellite

Author: Labanti, C., Marisaldi, M., Fuschino, F., Galli, M., Argan, A., Bulgarelli, A., Di Cocco, G., Gianotti, F., Tavani, M., and Trifoglio, M.
Published: 2009
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205. The XGIS imaging system onboard the THESEUS mission

Author: Gasent-Blesa, Jos�� Luis, Reglero, V��ctor, Connell, Paul, Pinazo-Herrero, Benjam��n, Navarro-Gonz��lez, Javier, Rodr��guez-Mart��nez, Pedro, Castro-Tirado, Alberto J., Caballero-Garc��a, Mar��a Dolores, Amati, Lorenzo, Labanti, Claudio, Mereghetti, Sandro, Frontera, Filippo, Campana, Riccardo, Orlandini, Mauro, Stephen, John, Terenzi, Luca, Evangelisti, Federico, Squerzanti, Stefano, Melchiorri, Michele, Fuschino, Fabio, De Rosa, Adriano, and Morgante, Gianluca
Subjects: FOS: Physical sciences, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract: Within the scientific goals of the THESEUS ESA/M5 candidate mission, a critical item is a fast (within a few s) and accurate (, Proceedings of the SPIE 2020, paper 11444-278
Published: 2021

206. Measurement of the muon transfer rate from muonic hydrogen to oxygen in the range 70-336 K

Author: Pizzolotto, C., primary, Sbrizzi, A., additional, Adamczak, A., additional, Bakalov, D., additional, Baldazzi, G., additional, Baruzzo, M., additional, Benocci, R., additional, Bertoni, R., additional, Bonesini, M., additional, Cabrera, H., additional, Cirrincione, D., additional, Clemenza, M., additional, Colace, L., additional, Danailov, M., additional, Danev, P., additional, de Bari, A., additional, De Vecchi, C., additional, De Vincenzi, M., additional, Fasci, E., additional, Fuschino, F., additional, Gadedjisso-Tossou, K.S., additional, Gianfrani, L., additional, Ishida, K., additional, Labanti, C., additional, Maggi, V., additional, Mazza, R., additional, Menegolli, A., additional, Mocchiutti, E., additional, Monzani, S., additional, Moretti, L., additional, Morgante, G., additional, Niemela, J., additional, Pullia, A., additional, Ramponi, R., additional, Rignanese, L.P., additional, Rossella, M., additional, Stoilov, M., additional, Stoychev, L., additional, Suárez-Vargas, J.J., additional, Tortora, L., additional, Vallazza, E., additional, and Vacchi, A., additional
Published: 2021
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207. Congenital Measles in a Premature 25-week Gestation Infant

Author: Hanft, Erin, primary, Brachio, Sandhya, additional, Messina, Maria, additional, Zachariah, Philip, additional, Sutton, Desmond, additional, Goffman, Dena, additional, Pike, Janett, additional, Covington, Lesley, additional, Graham, Krishika A., additional, Crouch, Bindy, additional, Adams, Eleanor, additional, Ahmad, Nina, additional, Rausch-Phung, Elizabeth, additional, Southwick, Karen, additional, Bryant, Patrick, additional, Fuschino, Meghan, additional, Khandekar, Anagha, additional, Kulas, Karen, additional, and Saiman, Lisa, additional
Published: 2021
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208. Understanding the origin of the positron annihilation line and the physics of supernova explosions

Author: Frontera, F., primary, Virgilli, E., additional, Guidorzi, C., additional, Rosati, P., additional, Diehl, R., additional, Siegert, T., additional, Fryer, C., additional, Amati, L., additional, Auricchio, N., additional, Campana, R., additional, Caroli, E., additional, Fuschino, F., additional, Labanti, C., additional, Orlandini, M., additional, Pian, E., additional, Stephen, J. B., additional, Del Sordo, S., additional, Budtz-Jorgensen, C., additional, Kuvvetli, I., additional, Brandt, S., additional, da Silva, R. M. Curado, additional, Laurent, P., additional, Bozzo, E., additional, Mazzali, P., additional, and Valle, M. Della, additional
Published: 2021
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209. XGIS Instrument Requirements

Author: LABANTI, CLAUDIO, AMATI, LORENZO, MEREGHETTI, Sandro, Frontera, Filippo, VIRGILLI, Enrico, MARCHESINI, EZEQUIEL J., FUSCHINO, FABIO, ITA, and Amati, Lorenzo
Abstract: The purpose of this XGIS instrument requirements specification is to derive the instrument requirements based on the scientific objectives and the technical and programmatic requirements as defined in the Mission Requirement Document [AD1], the Science Requirement Document [AD2] and the Environment Specification Document [AD3]. For the purpose of this first version the requirement specifications are derived for: - The top level (level 0) Instrument Requirements Specification - Elements that are not procured by the payload consortium (TBD) In addition, a preliminary functional and performance specification shall be described for: Level 1 Requirements Specifications Elements that are subjected to technology developments in Phase B1 Note: All interface requirements to the S/C shall be summarized and presented in the EID-B and are therefore not included in this document.
Published: 2021

210. Understanding the origin of the positron annihilation line and the physics of supernova explosions

Author: Natalia Auricchio, Chris L. Fryer, R. M. Curado da Silva, Roland Diehl, M. Della Valle, Lorenzo Amati, Søren Brandt, Irfan Kuvvetli, Piero Rosati, Thomas Siegert, Enrico Bozzo, Carl Budtz-Jørgensen, Paolo A. Mazzali, Elena Pian, Claudio Labanti, Enrico Virgilli, Ezio Caroli, Mauro Orlandini, S. Del Sordo, C. Guidorzi, Riccardo Campana, F. Fuschino, F. Frontera, John B. Stephen, P. Laurent, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Subjects: Origin of positron annihilation line from Galactic bulge region, Astrophysics::High Energy Astrophysical Phenomena, Space mission concept, Population, Dark matter, Socio-culturale, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 7. Clean energy, Nucleosynthesis, 0103 physical sciences, Nuclear astrophysics, Nuclear fusion, education, 010303 astronomy & astrophysics, Physics, education.field_of_study, 010308 nuclear & particles physics, Astronomy, Astronomy and Astrophysics, Dark matter from the Galactic Center region, ESA voyage 2050, Nuclear line distribution across supernova remnants, Nucleosynthesis study in novae, Physical origin of the Phillips law, type I and core-collapse supernovae, X–/γ–ray telescopes, Galaxy, Neutron star, Supernova, Space and Planetary Science, Type I and core-collapse supernovae, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: Nuclear astrophysics, and particularly nuclear emission line diagnostics from a variety of cosmic sites, has remained one of the least developed fields in experimental astronomy, despite its central role in addressing a number of outstanding questions in modern astrophysics. Radioactive isotopes are co-produced with stable isotopes in the fusion reactions of nucleosynthesis in supernova explosions and other violent events, such as neutron star mergers. The origin of the 511 keV positron annihilation line observed in the direction of the Galactic Center is a 50-year-long mystery. In fact, we still do not understand whether its diffuse large-scale emission is entirely due to a population of discrete sources, which are unresolved with current poor angular resolution instruments at these energies, or whether dark matter annihilation could contribute to it. From the results obtained in the pioneering decades of this experimentally-challenging window, it has become clear that some of the most pressing issues in high-energy astrophysics and astro-particle physics would greatly benefit from significant progress in the observational capabilities in the keV-to-MeV energy band. Current instrumentation is in fact not sensitive enough to detect radioactive and annihilation lines from a wide variety of phenomena in our and nearby galaxies, let alone study the spatial distribution of their emission. In this White Paper (WP), we discuss how unprecedented studies in this field will become possible with a new low-energy gamma-ray space experiment, called ASTENA (Advanced Surveyor of Transient Events and Nuclear Astrophysics), which combines new imaging, spectroscopic and polarization capabilities. In a separate WP (Guidorzi et al. 39), we discuss how the same mission concept will enable new groundbreaking studies of the physics of Gamma–Ray Bursts and other high-energy transient phenomena over the next decades.
Published: 2021

211. ORION, a Multi-Chip Readout Electronics for Satellite Wide Energy Range X-/γ-Ray Imaging Spectroscopy: design and characterization of the analog section

Author: Andrea Vacchi, F. Fuschino, Ezequiel Marchesini, Lorenzo Amati, Giuseppe Bertuccio, Irina Rashevskaya, E. Demenev, Giacomo Borghi, Piero Malcovati, A. Rachevski, E. Virgilli, Nicola Zorzi, N. Zampa, Riccardo Campana, Filippo Frontera, Pierluigi Bellutti, Antonino Picciotto, Marco Grassi, M. Fiorini, Claudio Labanti, Francesco Ficorella, F. Mele, Irisa Dedolli, M. Gandola, and Gianluigi Zampa
Subjects: Nuclear and High Energy Physics, Silicon, Silicon drift detector, Chipset, Physics::Instrumentation and Detectors, Imaging spectrometer, Silicon Drift Detectors, Scintillator, Crystals, Transient analysis, Optics, ASIC, Bars, Detectors, Photonics, Radiation detectors electronics, Readout electronics, Electrical and Electronic Engineering, Physics, Scintillation, business.industry, Dynamic range, Chip, Pulse shaping, Nuclear Energy and Engineering, business
Abstract: The ORION chipset, a full-custom multi-chip readout and processing electronics for the X-γ Imaging Spectrometer (XGIS) on-board the THESEUS space mission, is presented. The XGIS detection plane is arranged in a matrix of 10×10 detection modules, each one composed by 64 CsI(Tl) scintillation bars (4.5 mm×4.5 mm×30 mm) optically coupled at the top and bottom ends to two 8×8 monolithic Silicon Drift Detector matrices. The top SDD, exposed to the X-ray entrance window, performs the double function of low-energy X-ray detection as well as scintillator’s readout, together with the bottom SDD, providing a detection and spectroscopic energy range from 2 keV up to 20 MeV. The need to achieve a high energy resolution, as well as a high sensitive area on the detection plane, led to the development of a chipset organized to have a minimum-area analog readout chip placed in close proximity of the SDD (ORION-FE) and a mixed-signal back-end (ORION-BE) placed a few centimeters further on the back-end board for the additional signal processing and digitization. The multi-chip readout electronics integrates two dedicated analog processors for low-energy photons up to 30 keV (X-processor) and high-energy photons up to 5 MeV (γ-processor), allowing a spectroscopy-grade resolution in the 4 decades energy band (2 keV–20 MeV) of the XGIS, with a simulated power consumption of 1.55 mW/pixel. The ORION prototype was bonded to two ~25mm2 SDDs, and extensively characterized in terms of pulse shaping, pulse discrimination and stretching functionality, as well as linearity, dynamic range and spectroscopic resolution. An optimum Equivalent Noise Charge (ENC) at –20°C of 24.3 el. r.m.s. on the X-channel (212 eV FWHM on Si), and 39.6 el. r.m.s. on the γ-channel (3.7 keV FWHM on CsI(Tl)) has been recorded.
Published: 2021

212. Understanding the origin of the positron annihilation line and the physics of supernova explosions

Author: Frontera, F., Virgilli, E., Guidorzi, C., Rosati, P., Diehl, R., Siegert, T., Fryer, C., Amati, L., Auricchio, N., Campana, R., Caroli, E., Fuschino, F., Labanti, C., Orlandini, M., Pian, E., Stephen, J. B., Del Sordo, S., Budtz-Jorgensen, C., Kuvvetli, I., Brandt, S., da Silva, R. M.Curado, Laurent, P., Bozzo, E., Mazzali, P., Valle, M. Della, Frontera, F., Virgilli, E., Guidorzi, C., Rosati, P., Diehl, R., Siegert, T., Fryer, C., Amati, L., Auricchio, N., Campana, R., Caroli, E., Fuschino, F., Labanti, C., Orlandini, M., Pian, E., Stephen, J. B., Del Sordo, S., Budtz-Jorgensen, C., Kuvvetli, I., Brandt, S., da Silva, R. M.Curado, Laurent, P., Bozzo, E., Mazzali, P., and Valle, M. Della
Abstract: Nuclear astrophysics, and particularly nuclear emission line diagnostics from a variety of cosmic sites, has remained one of the least developed fields in experimental astronomy, despite its central role in addressing a number of outstanding questions in modern astrophysics. Radioactive isotopes are co-produced with stable isotopes in the fusion reactions of nucleosynthesis in supernova explosions and other violent events, such as neutron star mergers. The origin of the 511 keV positron annihilation line observed in the direction of the Galactic Center is a 50-year-long mystery. In fact, we still do not understand whether its diffuse large-scale emission is entirely due to a population of discrete sources, which are unresolved with current poor angular resolution instruments at these energies, or whether dark matter annihilation could contribute to it. From the results obtained in the pioneering decades of this experimentally-challenging window, it has become clear that some of the most pressing issues in high-energy astrophysics and astro-particle physics would greatly benefit from significant progress in the observational capabilities in the keV-to-MeV energy band. Current instrumentation is in fact not sensitive enough to detect radioactive and annihilation lines from a wide variety of phenomena in our and nearby galaxies, let alone study the spatial distribution of their emission. In this White Paper (WP), we discuss how unprecedented studies in this field will become possible with a new low-energy gamma-ray space experiment, called ASTENA (Advanced Surveyor of Transient Events and Nuclear Astrophysics), which combines new imaging, spectroscopic and polarization capabilities. In a separate WP (Guidorzi et al. 39), we discuss how the same mission concept will enable new groundbreaking studies of the physics of Gamma–Ray Bursts and other high-energy transient phenomena over the next decades.
Published: 2021

213. The Large Observatory for X-ray Timing (LOFT)

Author: Feroci, M., Stella, L., van der Klis, M., Courvoisier, T. J. -L., Hernanz, M., Hudec, R., Santangelo, A., Walton, D., Zdziarski, A., Barret, D., Belloni, T., Braga, J., Brandt, S., Budtz-Jørgensen, C., Campana, S., den Herder, J. -W., Huovelin, J., Israel, G. L., Pohl, M., Ray, P., Vacchi, A., Zane, S., Argan, A., Attinà, P., Bertuccio, G., Bozzo, E., Campana, R., Chakrabarty, D., Costa, E., De Rosa, A., Del Monte, E., Di Cosimo, S., Donnarumma, I., Evangelista, Y., Haas, D., Jonker, P., Korpela, S., Labanti, C., Malcovati, P., Mignani, R., Muleri, F., Rapisarda, M., Rashevsky, A., Rea, N., Rubini, A., Tenzer, C., Wilson-Hodge, C., Winter, B., Wood, K., Zampa, G., Zampa, N., Abramowicz, M. A., Alpar, M. A., Altamirano, D., Alvarez, J. M., Amati, L., Amoros, C., Antonelli, L. A., Artigue, R., Azzarello, P., Bachetti, M., Baldazzi, G., Barbera, M., Barbieri, C., Basa, S., Baykal, A., Belmont, R., Boirin, L., Bonvicini, V., Burderi, L., Bursa, M., Cabanac, C., Cackett, E., Caliandro, G. A., Casella, P., Chaty, S., Chenevez, J., Coe, M. J., Collura, A., Corongiu, A., Covino, S., Cusumano, G., D’Amico, F., Dall’Osso, S., De Martino, D., De Paris, G., Di Persio, G., Di Salvo, T., Done, C., Dovčiak, M., Drago, A., Ertan, U., Fabiani, S., Falanga, M., Fender, R., Ferrando, P., Della Monica Ferreira, D., Fraser, G., Frontera, F., Fuschino, F., Galvez, J. L., Gandhi, P., Giommi, P., Godet, O., Göǧüş, E., Goldwurm, A., Götz, D., Grassi, M., Guttridge, P., Hakala, P., Henri, G., Hermsen, W., Horak, J., Hornstrup, A., in’t Zand, J. J. M., Isern, J., Kalemci, E., Kanbach, G., Karas, V., Kataria, D., Kennedy, T., Klochkov, D., Kluźniak, W., Kokkotas, K., Kreykenbohm, I., Krolik, J., Kuiper, L., Kuvvetli, I., Kylafis, N., Lattimer, J. M., Lazzarotto, F., Leahy, D., Lebrun, F., Lin, D., Lund, N., Maccarone, T., Malzac, J., Marisaldi, M., Martindale, A., Mastropietro, M., McClintock, J., McHardy, I., Mendez, M., Mereghetti, S., Miller, M. C., Mineo, T., Morelli, E., Morsink, S., Motch, C., Motta, S., Muñoz-Darias, T., Naletto, G., Neustroev, V., Nevalainen, J., Olive, J. F., Orio, M., Orlandini, M., Orleanski, P., Ozel, F., Pacciani, L., Paltani, S., Papadakis, I., Papitto, A., Patruno, A., Pellizzoni, A., Petráček, V., Petri, J., Petrucci, P. O., Phlips, B., Picolli, L., Possenti, A., Psaltis, D., Rambaud, D., Reig, P., Remillard, R., Rodriguez, J., Romano, P., Romanova, M., Schanz, T., Schmid, C., Segreto, A., Shearer, A., Smith, A., Smith, P. J., Soffitta, P., Stergioulas, N., Stolarski, M., Stuchlik, Z., Tiengo, A., Torres, D., Török, G., Turolla, R., Uttley, P., Vaughan, S., Vercellone, S., Waters, R., Watts, A., Wawrzaszek, R., Webb, N., Wilms, J., Zampieri, L., Zezas, A., and Ziolkowski, J.
Published: 2012
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214. Time Evolution of TGF-Producing Storms Using ERA5, GPS and Geostationary Satellites Observations

Author: Alessandra Mascitelli, Eugenio Realini, Marco Tavani, Federico Porcù, Martino Marisaldi, Stefano Federico, Andrea Gatti, A. Ursi, Leo Pio D'Adderio, Stefano Dietrich, Alessandra Tiberia, and F. Fuschino
Subjects: Meteorology, business.industry, Global Positioning System, Geostationary orbit, Environmental science, Storm, business, Lightning, atmospheric_science
Abstract: In this article we report the first investigation over time of the atmospheric conditions around TGFs occurrence, using GPS sensors in combination with geostationary satellite observations and ERA5 reanalyses data. The goal is to understand which characteristics are favourable to the development of these events and to investigate if any precursor signals can be expected. A total of 9 TGFs, occurred at a distance lower than 45 km from a GPS sensor, were analysed and two of them are shown here as an example analysis. Moreover, the lightning activity, collected by the World Wide Lightning Location Network (WWLLN) was used in order to identify any links and correlations with TGF occurrence and PWV trends. The combined use of GPS and the stroke rate trends identified, for all cases, a recurred pattern in which an increase of PWV is observed on a timescale of about two hours before the TGF occurrence that can be placed within the lightning peak. The temporal relation between the PWV trend and TGF occurrence is strictly related to the position of GPS sensors in relation to TGF coordinates. The life cycle of these storms observed by geostationary sensors, described TGFs producing clouds as intense with a wide range of extensions and, in all cases, the TGF is located at the edge of the convective cell. Furthermore, the satellite data give an added value in associating the GPS water vapor trend to the convective cell generating the TGF. The investigation with ERA5 reanalyses data showed that TGFs mainly occur in convective environment with not exceptional values with respect to the monthly average value of parameters measured in the same location. Moreover the analysis showed the strong potential of the use of GPS data for the troposphere characterization in areas with complex territorial morphology. This study provided indications on the dynamics of convective systems linked to TGFs and will certainly help refine our understanding on their production highlights a potential approach through the use of GPS data to explore the lightning activity trend and the TGFs occurrence.
Published: 2020

215. Scientific simulations and optimization of the XGIS instrument on board THESEUS

Author: Filippo Frontera, John B. Stephen, Sandro Mereghetti, J. L. Gasent-Blesa, Lorenzo Amati, Michele Lissoni, C. Guidorzi, Michela Rigoselli, Giancarlo Ghirlanda, Riccardo Campana, Ruben Farinelli, F. Fuschino, Ruben Salvaterra, Claudio Labanti, and P. Connell
Subjects: Spectrometer, Computer science, business.industry, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Monte Carlo method, Astrophysics::Instrumentation and Methods for Astrophysics, Process (computing), FOS: Physical sciences, Wide field, Redshift, On board, Sky, Aerospace engineering, Astrophysics - Instrumentation and Methods for Astrophysics, business, Gamma-ray burst, Instrumentation and Methods for Astrophysics (astro-ph.IM), media_common
Abstract: The XGIS (X and Gamma Imaging Spectrometer) is one of the three instruments onboard the THESEUS mission (ESA M5, currently in Phase-A). Thanks to its wide field of view and good imaging capabilities, it will efficiently detect and localize gamma-ray bursts and other transients in the 2-150 keV sky, and also provide spectroscopy up to 10 MeV. Its current design has been optimized by means of scientific simulations based on a Monte Carlo model of the instrument coupled to a state-of-the-art description of the populations of long and short GRBs extending to high redshifts. We describe the optimization process that led to the current design of the XGIS, based on two identical units with partially overlapping fields of view, and discuss the expected performance of the instrument., Comment: Proceedings of the SPIE 2020, paper 11444-276
Published: 2020

216. The Second AGILE MCAL Gamma-Ray Burst Catalog: 13 yr of Observations

Author: A. Ursi, M. Romani, F. Verrecchia, C. Pittori, M. Tavani, M. Marisaldi, M. Galli, C. Labanti, N. Parmiggiani, A. Bulgarelli, A. Addis, L. Baroncelli, M. Cardillo, C. Casentini, P. W. Cattaneo, A. Chen, A. Di Piano, F. Fuschino, F. Longo, F. Lucarelli, A. Morselli, G. Piano, and S. Vercellone
Subjects: Space and Planetary Science, Astronomy and Astrophysics
Abstract: We present the results of a systematic search and analysis of GRBs detected by the Astrorivelatore Gamma ad Immagini LEggero (AGILE) MiniCALorimeter (MCAL; 0.4–100 MeV) over a time frame of 13 yr, from 2007 to 2020 November. The MCAL GRB sample consists of 503 bursts triggered by MCAL, 394 of which were fully detected onboard with high time resolution. The sample consists of about 44% short GRBs and 56% long GRBs. In addition, 109 bursts triggered partial MCAL onboard data acquisitions, providing further detections that can be used for joint analyses or triangulations. More than 90% of these GRBs were also detected by the AGILE Scientific RateMeters (RMs), providing simultaneous observations between 20 keV and 100 MeV. We performed spectral analysis of these events in the 0.4–50 MeV energy range. We could fit the time-integrated spectrum of 258 GRBs with a single power-law model, resulting in a mean photon index 〈β〉of−2.3. Among them, 43 bursts could also be fitted with a Band model, with peak energy above 400 keV, resulting in a mean low-energy photon index 〈α〉 = −0.6, a mean high-energy photon index 〈β〉 = −2.5, and a mean peak energy 〈E p 〉 = 640 keV. The AGILE MCAL GRB sample mostly consists of hard-spectrum GRBs, with a large fraction of short-duration events. We discuss properties and features of the MCAL bursts, whose detections can be used to perform joint broad-band analysis with other missions, and to provide insights on the high-energy component of the prompt emission in the tens of mega electron volt energy range.
Published: 2022

217. The AGILE space mission

Author: Tavani, M., Barbiellini, G., Argan, A., Bulgarelli, A., Caraveo, P., Chen, A., Cocco, V., Costa, E., De Paris, G., Del Monte, E., Di Cocco, G., Donnarumma, I., Feroci, M., Fiorini, M., Froysland, T., Fuschino, F., Galli, M., Gianotti, F., Giuliani, A., Evangelista, Y., Labanti, C., Lapshov, I., Lazzarotto, F., Lipari, P., Longo, F., Marisaldi, M., Mastropietro, M., Mauri, F., Mereghetti, S., Morelli, E., Morselli, A., Pacciani, L., Pellizzoni, A., Perotti, F., Picozza, P., Pontoni, C., Porrovecchio, G., Prest, M., Pucella, G., Rapisarda, M., Rossi, E., Rubini, A., Soffitta, P., Trifoglio, M., Trois, A., Vallazza, E., Vercellone, S., Zambra, A., Zanello, D., Giommi, P., Antonelli, A., and Pittori, C.
Published: 2008
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218. Search of GRB with AGILE Minicalorimeter

Author: Fuschino, F., Labanti, C., Galli, M., Marisaldi, M., Bulgarelli, A., Gianotti, F., Trifoglio, M., Argan, A., Del Monte, E., Donnarumma, I., Feroci, M., Lazzarotto, F., Pacciani, L., Tavani, M., and Trois, A.
Published: 2008
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219. A broad energy range wide field monitor for next generation gamma-ray burst experiments

Author: Marisaldi, M., Labanti, C., Fuschino, F., and Amati, L.
Published: 2008
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220. THESEUS: A key space mission concept for Multi-Messenger Astrophysics

Author: F. Fuschino, Ruben Salvaterra, F. Frontera, M. Branchesi, Bruce Gendre, U. Maio, Stefano Covino, Tomaz Rodic, Giancarlo Ghirlanda, Serena Vinciguerra, D. Mereghetti, Andrea Rossi, Lorenzo Amati, Diego Götz, M. H. P. M. van Putten, Monica Colpi, Roberto Mignani, P. D'Avanzo, Riccardo Campana, Eliana Palazzi, Andrea Bulgarelli, M. G. Bernardini, Valerio D'Elia, Jochen Greiner, Elisabetta Maiorano, Enzo Brocato, Joseph Caruana, Piero Rosati, R. L. C. Starling, Nial Tanvir, Riccardo Ciolfi, G. Stratta, S. D. Vergani, S. Colafrancesco, Claudio Labanti, Bing Zhang, Dorottya Szécsi, M. Razzano, Enrico Bozzo, Antonio Stamerra, D. Malesani, René Hudec, Francesco Longo, Luciano Rezzolla, S. Piranomonte, M. de Pasquale, Richard Willingale, B. Patricelli, J. P. Osborne, P. T. O'Brien, Peter G. Jonker, Luciano Nicastro, C. Guidorzi, Aniello Grado, M. Boer, Alessandro Drago, Maria Giovanna Dainotti, Carole Mundell, Centre d'étude spatiale des rayonnements (CESR), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Istituto di Astrofisica Spaziale e Fisica Cosmica - Milano (IASF-MI), Istituto Nazionale di Astrofisica (INAF), ISDC Data Centre for Astrophysics, University of Geneva [Switzerland], INAF - Osservatorio Astronomico di Brera (OAB), University of Ferrara [Ferrara], Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Department of Physics and Astronomy [Leicester], University of Leicester, Max-Planck-Institut für Extraterrestrische Physik (MPE), Mullard Space Science Laboratory (MSSL), University College of London [London] (UCL), INAF - Osservatorio Astronomico di Roma (OAR), INAF-IASF Milano, Observatoire de Haute-Provence (OHP), Institut Pythéas (OSU PYTHEAS), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Centre National de la Recherche Scientifique (CNRS), ASI-Science Data Center, Rome, Laboratori Nazionali di Frascati (LNF), National Institute for Nuclear Physics (INFN), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Astronomical Institute of the Czech Academy of Sciences, Czech Academy of Sciences [Prague] (ASCR), Department of Astrophysics [Nijmegen], Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud university [Nijmegen]-Radboud university [Nijmegen], Dark Cosmology Centre (DARK), Niels Bohr Institute [Copenhagen] (NBI), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), CNR Institute of Atmospheric Sciences and Climate (ISAC), Consiglio Nazionale delle Ricerche (CNR), Observatoire de Paris - Site de Meudon (OBSPM), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université de Genève = University of Geneva (UNIGE), Università degli Studi di Ferrara = University of Ferrara (UniFE), Istituto Nazionale di Fisica Nucleare (INFN), Astronomical Institute of the Czech Academy of Sciences (ASU / CAS), Czech Academy of Sciences [Prague] (CAS), Radboud University [Nijmegen]-Radboud University [Nijmegen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Département d'Astrophysique (ex SAP) (DAP), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015 - 2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), THESEUS, Stratta, G., Ciolfi, R., Amati, L., Bozzo, E., Ghirlanda, G., Maiorano, E., Nicastro, L., Rossi, A., Vinciguerra, S., Frontera, F., Götz, D., Guidorzi, C., O'Brien, P., Osborne, J. P., Tanvir, N., Branchesi, M., Brocato, E., Dainotti, M. G., De Pasquale, M., Grado, A., Greiner, J., Longo, F., Maio, U., Mereghetti, D., Mignani, R., Piranomonte, S., Rezzolla, L., Salvaterra, R., Starling, R., Willingale, R., Böer, M., Bulgarelli, A., Caruana, J., Colafrancesco, S., Colpi, M., Covino, S., D'Avanzo, P., D'Elia, V., Drago, A., Fuschino, F., Gendre, B., Hudec, R., Jonker, P., Labanti, C., Malesani, D., Mundell, C. G., Palazzi, E., Patricelli, B., Razzano, M., Campana, R., Rosati, P., Rodic, T., Szécsi, D., Stamerra, A., van Putten, M., Vergani, S., Zhang, B., Bernardini, M., Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Università degli Studi di Ferrara (UniFE), Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Centre National de la Recherche Scientifique (CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Institut de Recherche pour le Développement (IRD), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Stratta, G, Ciolfi, R, Amati, L, Bozzo, E, Ghirlanda, G, Maiorano, E, Nicastro, L, Rossi, A, Vinciguerra, S, Frontera, F, Götz, D, Guidorzi, C, O'Brien, P, Osborne, J, Tanvir, N, Branchesi, M, Brocato, E, Dainotti, M, De Pasquale, M, Grado, A, Greiner, J, Longo, F, Maio, U, Mereghetti, D, Mignani, R, Piranomonte, S, Rezzolla, L, Salvaterra, R, Starling, R, Willingale, R, Böer, M, Bulgarelli, A, Caruana, J, Colafrancesco, S, Colpi, M, Covino, S, D'Avanzo, P, D'Elia, V, Drago, A, Fuschino, F, Gendre, B, Hudec, R, Jonker, P, Labanti, C, Malesani, D, Mundell, C, Palazzi, E, Patricelli, B, Razzano, M, Campana, R, Rosati, P, Rodic, T, Szécsi, D, Stamerra, A, van Putten, M, Vergani, S, Zhang, B, and Bernardini, M
Subjects: Atmospheric Science, Computer science, Astronomy, Astronomical and space-research instrumentation, Gamma-ray bursts, Gamma-ray sources, X-ray bursts, X-ray sources, Aerospace Engineering, Space and Planetary Science, Astrophysics, 01 natural sciences, Economica, astronomical and space-research instrumentation, 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS, media_common, High Energy Astrophysical Phenomena (astro-ph.HE), [PHYS]Physics [physics], energy: high, gamma-ray bursts, Gamma-ray source, neutrino: detector, Geophysics, Upgrade, Neutrino detector, upgrade, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Cosmic Vision, media_common.quotation_subject, FOS: Physical sciences, Context (language use), frequency: high, X-ray source, 0103 physical sciences, gravitational radiation: frequency, Gamma-ray burst, X-ray burst, gamma-ray sources, 010308 nuclear & particles physics, Gravitational wave, family: 3, Astronomy and Astrophysics, gravitational radiation detector, Universe, messenger, electromagnetic, General Earth and Planetary Sciences, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: The recent discovery of the electromagnetic counterpart of the gravitational wave source GW170817, has demonstrated the huge informative power of multi-messenger observations. During the next decade the nascent field of multi-messenger astronomy will mature significantly. Around 2030, third generation gravitational wave detectors will be roughly ten times more sensitive than the current ones. At the same time, neutrino detectors currently upgrading to multi km^3 telescopes, will include a 10 km^3 facility in the Southern hemisphere that is expected to be operational around 2030. In this review, we describe the most promising high frequency gravitational wave and neutrino sources that will be detected in the next two decades. In this context, we show the important role of the Transient High Energy Sky and Early Universe Surveyor (THESEUS), a mission concept proposed to ESA by a large international collaboration in response to the call for the Cosmic Vision Programme M5 missions. THESEUS aims at providing a substantial advancement in early Universe science as well as playing a fundamental role in multi-messenger and time-domain astrophysics, operating in strong synergy with future gravitational wave and neutrino detectors as well as major ground- and space-based telescopes. This review is an extension of the THESEUS white paper (Amati et al. 2017), also in light of the discovery of GW170817/GRB170817A that was announced on October 16th, 2017., Comment: 25 pages, 13 figures, accepted to Advances in Space Research with minor revisions. Details on the THESEUS instrumentation, science case and expected performances can also be found in Amati et al. 2017 (arXiv:1710.04638) and in the presentations of the THESEUS Workshop 2017 (http://www.isdc.unige.ch/theseus/workshop2017-programme.html). v2 few typos corrected
Published: 2018

221. First FAMU observation of muon transfer from μp atoms to higher-Z elements

Author: L. Tortora, A. Vacchi, L. Colace, Maurizio Bonesini, A. Tomaselli, M. Rossella, Anselmo Margotti, E. Vallazza, Claudio Labanti, D. Guffanti, G. Zampa, R. Mazza, A. Curioni, T. Cervi, P. Danev, R. Carbone, Germano Baldazzi, Ezio Previtali, Paolo Rossi, Roberto Benocci, R. Bertoni, M. Furini, K. S. Gadedjisso-Tossou, L. Stoychev, Miltcho B. Danailov, Dimitar Bakalov, Giovanni Baccolo, M. Stoilov, K. Ishida, F. Fuschino, E. Furlanetto, L. P. Rignanese, M. Moretti, Gianluca Morgante, R. Nardò, Massimiliano Nastasi, G. Campana, C. De Vecchi, F. Chignoli, M. De Vincenzi, I. D'Antone, Andrzej Adamczak, C. Pizzolotto, E. Mocchiutti, A. Iaciofano, S. Meneghini, F. Somma, Valter Maggi, M. Zuffa, Alessandro Menegolli, A. Rachevski, A. de Bari, M. Clemenza, V. Bonvicini, Joseph Niemela, Roberta Ramponi, Mocchiutti, E., Bonvicini, V., Carbone, R., Danailov, M., Furlanetto, E., Gadedjisso-Tossou, K.S., Guffanti, D., Pizzolotto, C., Rachevski, A., Stoychev, L., Vallazza, E., Zampa, G., Niemela, J., Ishida, K., Adamczak, A., Baccolo, G., Benocci, R., Bertoni, R., Bonesini, M., Chignoli, F., Clemenza, M., Curioni, A., Maggi, V., Mazza, R., Moretti, M., Nastasi, M., Previtali, E., Bakalov, D., Danev, P., Stoilov, M., Baldazzi, G., Campana, G., D'Antone, I., Furini, M., Fuschino, F., Labanti, C., Margotti, A., Meneghini, S., Morgante, G., Rignanese, L.P., Rossi, P.L., Zuffa, M., Cervi, T., Bari, A.D., Menegolli, A., Vecchi, C.D., Nardò, R., Rossella, M., Tomaselli, A., Colace, L., Vincenzi, M.D., Iaciofano, A., Somma, F., Tortora, L., Ramponi, R., Vacchi, A., Gadedjisso-Tossou, K. S., Baldazzi, Germano, Rignanese, L. P., Rossi, P. L., Bari, A. De, Vecchi, C. De, Vincenzi, M. De, Iaciofano, Alfredo, Mocchiutti, E, Bonvicini, V, Carbone, R, Danailov, M, Furlanetto, E, Gadedjisso-Tossou, K, Guffanti, D, Pizzolotto, C, Rachevski, A, Stoychev, L, Vallazza, E, Zampa, G, Niemela, J, Ishidaf, K, Adamczak, A, Baccolo, G, Benocci, R, Bertoni, R, Bonesini, M, Chignoli, F, Clemenza, M, Curioni, A, Maggi, V, Mazza, R, Moretti, M, Nastasi, M, Previtali, E, Bakalov, D, Danev, P, Stoilov, M, Baldazzi, G, Campana, G, D'Antone, I, Furini, M, Fuschino, F, Labanti, C, Margotti, A, Meneghini, S, Morgante, G, Rignanese, L, Rossi, P, Zuffa, M, Cervi, T, De Bari, A, Menegolli, A, De Vecchi, C, Nardò, R, Rossella, M, Tomaselli, A, Colace, L, De Vincenzi, M, Iaciofano, A, Somma, F, Tortora, L, and Vacchi, R
Subjects: X-ray detector, Pressurized ga, Ground state, chemistry.chemical_element, Charged particle, Measurements of, Atom, 01 natural sciences, Timing detectors, Nuclear physics, 0103 physical sciences, 010306 general physics, Instrumentation, Hyperfine structure, Mathematical Physics, Exotic atom, X rays, Hyperfine splitting, Physics, Kinetic, Argon, Muon, Rutherford appleton laboratorie, 010308 nuclear & particles physics, Muonic hydrogen, X-ray detectors, Transfer rates, X ray detector, Carbon, chemistry, Carbon dioxide, Timing detector, Excited state, Analysis and statistical methods, Physics::Accelerator Physics, X ray apparatu, Analysis and statistical method, Kinetic energy, Beam (structure), Muon transfer rate
Abstract: The FAMU experiment aims to accurately measure the hyperfine splitting of the ground state of the muonic hydrogen atom. A measurement of the transfer rate of muons from hydrogen to heavier gases is necessary for this purpose. In June 2014, within a preliminary experiment, a pressurized gas-target was exposed to the pulsed low-energy muon beam at the RIKEN RAL muon facility (Rutherford Appleton Laboratory, U.K.). The main goal of the test was the characterization of both the noise induced by the pulsed beam and the X-ray detectors. The apparatus, to some extent rudimental, has served admirably to this task. Technical results have been published that prove the validity of the choices made and pave the way for the next steps. This paper presents the results of physical relevance of measurements of the muon transfer rate to carbon dioxide, oxygen, and argon from non-thermalized excited μp atoms. The analysis methodology and the approach to the systematics errors are useful for the subsequent study of the transfer rate as function of the kinetic energy of the μp currently under way. © 2018 The Author(s).
Published: 2018

222. The THESEUS space mission concept: science case, design and expected performances

Author: Martino Marisaldi, Enrico Bozzo, Valerie Connaughton, Dorottya Szécsi, D. Malesani, L. Maraschi, B. Cordier, P. D'Avanzo, Salvatore Capozziello, Darach Watson, C. Contini, Maryam Modjaz, Pierluigi Bellutti, M. de Pasquale, C. Guidorzi, Colleen A. Wilson-Hodge, O. Boulade, C. Adami, Y. Evangelista, A. Argan, Johan P. U. Fynbo, Y.-W. Dong, Poshak Gandhi, Allan Hornstrup, Eliana Palazzi, Andrea Bulgarelli, Andrea Comastri, E. Geza, Luciano Burderi, Giuseppe Malaguti, D. de Martino, Irfan Kuvvetli, S.-N. Zhang, Claudio Labanti, Fiamma Capitanio, Luca Izzo, Bradley Cenko, A. Melandri, Umberto Maio, Nicola Omodei, Stefano Ettori, C. Butler, S. D. Vergani, S. Zhang, Lajos G. Balázs, Patricia Schady, Federica B. Bianco, M. Branchesi, Jens Hjorth, Jochen Greiner, Felix Ryde, Jean-Gabriel Cuby, Piero Malcovati, Lorraine Hanlon, Peter G. Jonker, M. Della Valle, Elena Pian, Piotr Orleanski, Etienne Renotte, W. Skidmore, L. Sabau-Graziati, Mauro Dadina, Carl Budtz-Jørgensen, Tomaz Rodic, Giancarlo Ghirlanda, Luigi Piro, Sheila McBreen, M. Fiorini, M. Topinka, Jan Harms, Riccardo Ciolfi, Yi Chen, Giacomo Vianello, Ester Piedipalumbo, Zsolt Bagoly, Aniello Grado, Yuki Kaneko, Vito Sguera, B. Morelli, E. Le Floc'h, Luciano Rezzolla, K. Wiersema, Remo Ruffini, E. Del Monte, J. P. Osborne, M. G. Bernardini, A. Gomboc, A. De Luca, Stefano Covino, Ian Hutchinson, A. Antonelli, Enzo Brocato, Mark R. Sims, M. Razzano, Elisabetta Maiorano, Jean-Luc Atteia, J. Zicha, S. Korpela, Eros Vanzella, V. D'Elia, M. H. P. M. van Putten, Marco Feroci, Carole Mundell, A. V. Penacchioni, J. Soomin, Gabriele Ghisellini, Sandra Savaglio, N. Shigehiro, Andrea Santangelo, Antonio Martin-Carrillo, Avishay Gal-Yam, A. M. Read, Piergiorgio Casella, Giuseppe Baldazzi, B. Ciardi, Pawan Kumar, Li Song, V. Lebrun, G. Zampa, Daisuke Yonetoku, S. Vojtech, Gregor Rauw, Piero Rosati, A. J. Castro-Tirado, Bruce Gendre, Tsvi Piran, A. Rachevski, S. Basa, T. Li, Michela Uslenghi, Gianluca Morgante, Michèle Lavagna, Pascal Chardonnet, Andrew MacFadyen, Asaf Pe'er, Sandro Mereghetti, Alessandro Drago, M. Hafizi, Richard Willingale, D. Morris, Bing Zhang, Paolo Giommi, Andrea Ferrara, Mauro Orlandini, Maria Giovanna Dainotti, N. Masetti, Yuji Urata, Maxim Lyutikov, A. Vacchi, László L. Kiss, E. Campolongo, M. Boer, Lorenzo Amati, Diego Götz, Andrew Blain, M. T. Botticella, C. Tenzer, Monica Colpi, Victor Reglero, Roberto Mignani, Michael S. Briggs, Joseph Caruana, Elizabeth R. Stanway, S. Colafrancesco, Francesca Panessa, H. U. Nargaard-Nielsen, F. Lu, Giuseppe Bertuccio, A. Paizis, P. Romano, S. Vercellone, Luciano Nicastro, S. Paltani, G. Pareschi, G. Stratta, V. Petrosian, João Braga, N. Zampa, Nial Tanvir, James E. Rhoads, Raffaella Margutti, Luca Valenziano, Søren Brandt, S. Boci, Andrea Rossi, Paul J. Callanan, Annalisa Celotti, N. Kawai, René Hudec, Francesco Longo, Primo Attina, G. L. Israel, F. Fuschino, Fabio Finelli, M. Hernanz, Ruben Salvaterra, F. Frontera, P. T. O'Brien, Sergio Campana, Rupal Basak, Riccardo Campana, Eleonora Troja, Jordan Camp, Petr Páta, S. Piranomonte, G. Tagliaferri, Sylvain Guiriec, R. L. C. Starling, B. B. Zhang, Natalia Auricchio, Serena Vinciguerra, Département d'Astrophysique (ex SAP) (DAP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Agenzia Spaziale Italiana, European Commission, Czech Grant Agency, ITA, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), THESEUS, Amati, L, O'Brien, P, Götz, D, Bozzo, E, Tenzer, C, Frontera, F, Ghirlanda, G, Labanti, C, Osborne, J, Stratta, G, Tanvir, N, Willingale, R, Attina, P, Campana, R, Castro-Tirado, A, Contini, C, Fuschino, F, Gomboc, A, Hudec, R, Orleanski, P, Renotte, E, Rodic, T, Bagoly, Z, Blain, A, Callanan, P, Covino, S, Ferrara, A, Le Floch, E, Marisaldi, M, Mereghetti, S, Rosati, P, Vacchi, A, D'Avanzo, P, Giommi, P, Piranomonte, S, Piro, L, Reglero, V, Rossi, A, Santangelo, A, Salvaterra, R, Tagliaferri, G, Vergani, S, Vinciguerra, S, Briggs, M, Campolongo, E, Ciolfi, R, Connaughton, V, Cordier, B, Morelli, B, Orlandini, M, Adami, C, Argan, A, Atteia, J, Auricchio, N, Balazs, L, Baldazzi, G, Basa, S, Basak, R, Bellutti, P, Bernardini, M, Bertuccio, G, Braga, J, Branchesi, M, Brandt, S, Brocato, E, Budtz-Jorgensen, C, Bulgarelli, A, Burderi, L, Camp, J, Capozziello, S, Caruana, J, Casella, P, Cenko, B, Chardonnet, P, Ciardi, B, Colafrancesco, S, Dainotti, M, D'Elia, V, De Martino, D, De Pasquale, M, Del Monte, E, Della Valle, M, Drago, A, Evangelista, Y, Feroci, M, Finelli, F, Fiorini, M, Fynbo, J, Gal-Yam, A, Gendre, B, Ghisellini, G, Grado, A, Guidorzi, C, Hafizi, M, Hanlon, L, Hjorth, J, Izzo, L, Kiss, L, Kumar, P, Kuvvetli, I, Lavagna, M, Li, T, Longo, F, Lyutikov, M, Maio, U, Maiorano, E, Malcovati, P, Malesani, D, Margutti, R, Martin-Carrillo, A, Masetti, N, Mcbreen, S, Mignani, R, Morgante, G, Mundell, C, Nargaard-Nielsen, H, Nicastro, L, Palazzi, E, Paltani, S, Panessa, F, Pareschi, G, Pe'Er, A, Penacchioni, A, Pian, E, Piedipalumbo, E, Piran, T, Rauw, G, Razzano, M, Read, A, Rezzolla, L, Romano, P, Ruffini, R, Savaglio, S, Sguera, V, Schady, P, Skidmore, W, Song, L, Stanway, E, Starling, R, Topinka, M, Troja, E, van Putten, M, Vanzella, E, Vercellone, S, Wilson-Hodge, C, Yonetoku, D, Zampa, G, Zampa, N, Zhang, B, Zhang, S, Antonelli, A, Bianco, F, Boci, S, Boer, M, Botticella, M, Boulade, O, Butler, C, Campana, S, Capitanio, F, Celotti, A, Chen, Y, Colpi, M, Comastri, A, Cuby, J, Dadina, M, De Luca, A, Dong, Y, Ettori, S, Gandhi, P, Geza, E, Greiner, J, Guiriec, S, Harms, J, Hernanz, M, Hornstrup, A, Hutchinson, I, Israel, G, Jonker, P, Kaneko, Y, Kawai, N, Wiersema, K, Korpela, S, Lebrun, V, Lu, F, Macfadyen, A, Malaguti, G, Maraschi, L, Melandri, A, Modjaz, M, Morris, D, Omodei, N, Paizis, A, Páta, P, Petrosian, V, Rachevski, A, Rhoads, J, Ryde, F, Sabau-Graziati, L, Shigehiro, N, Sims, M, Soomin, J, Szécsi, D, Urata, Y, Uslenghi, M, Valenziano, L, Vianello, G, Vojtech, S, Watson, D, Zicha, J, Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Gian Luca, Israel, Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., Mcbreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'Er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., Macfadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., Zicha, J., Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), ANR-16-CE31-0003,BEaPro,Using the most powerful explosion as probes of the high-redshift Universe(2016), Galaxies, Etoiles, Physique, Instrumentation ( GEPI ), Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Astrophysique de Marseille ( LAM ), Aix Marseille Université ( AMU ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National d'Etudes Spatiales ( CNES ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de recherche en astrophysique et planétologie ( IRAP ), Université Paul Sabatier - Toulouse 3 ( UPS ) -Observatoire Midi-Pyrénées ( OMP ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy-le-Vieux de Physique Théorique ( LAPTH ), Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux ( ARTEMIS ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de la Côte d'Azur, Université Côte d'Azur ( UCA ) -Centre National de la Recherche Scientifique ( CNRS ), Gotz, D., Pata, P., Szecsi, D., Department of Physics, and Amati, L. and O'Brien, P. and Götz, D. and Bozzo, E. and Tenzer, C. and Frontera, F. and Ghirlanda, G. and Labanti, C. and Osborne, J.P. and Stratta, G. and Tanvir, N. and Willingale, R. and Attina, P. and Campana, R. and Castro-Tirado, A.J. and Contini, C. and Fuschino, F. and Gomboc, A. and Hudec, R. and Orleanski, P. and Renotte, E. and Rodic, T. and Bagoly, Z. and Blain, A. and Callanan, P. and Covino, S. and Ferrara, A. and Le Floch, E. and Marisaldi, M. and Mereghetti, S. and Rosati, P. and Vacchi, A. and D'Avanzo, P. and Giommi, P. and Piranomonte, S. and Piro, L. and Reglero, V. and Rossi, A. and Santangelo, A. and Salvaterra, R. and Tagliaferri, G. and Vergani, S. and Vinciguerra, S. and Briggs, M. and Campolongo, E. and Ciolfi, R. and Connaughton, V. and Cordier, B. and Morelli, B. and Orlandini, M. and Adami, C. and Argan, A. and Atteia, J.-L. and Auricchio, N. and Balazs, L. and Baldazzi, G. and Basa, S. and Basak, R. and Bellutti, P. and Bernardini, M.G. and Bertuccio, G. and Braga, J. and Branchesi, M. and Brandt, S. and Brocato, E. and Budtz-Jorgensen, C. and Bulgarelli, A. and Burderi, L. and Camp, J. and Capozziello, S. and Caruana, J. and Casella, P. and Cenko, B. and Chardonnet, P. and Ciardi, B. and Colafrancesco, S. and Dainotti, M.G. and D'Elia, V. and De Martino, D. and De Pasquale, M. and Del Monte, E. and Della Valle, M. and Drago, A. and Evangelista, Y. and Feroci, M. and Finelli, F. and Fiorini, M. and Fynbo, J. and Gal-Yam, A. and Gendre, B. and Ghisellini, G. and Grado, A. and Guidorzi, C. and Hafizi, M. and Hanlon, L. and Hjorth, J. and Izzo, L. and Kiss, L. and Kumar, P. and Kuvvetli, I. and Lavagna, M. and Li, T. and Longo, F. and Lyutikov, M. and Maio, U. and Maiorano, E. and Malcovati, P. and Malesani, D. and Margutti, R. and Martin-Carrillo, A. and Masetti, N. and McBreen, S. and Mignani, R. and Morgante, G. and Mundell, C. and Nargaard-Nielsen, H.U. and Nicastro, L. and Palazzi, E. and Paltani, S. and Panessa, F. and Pareschi, G. and Pe'er, A. and Penacchioni, A.V. and Pian, E. and Piedipalumbo, E. and Piran, T. and Rauw, G. and Razzano, M. and Read, A. and Rezzolla, L. and Romano, P. and Ruffini, R. and Savaglio, S. and Sguera, V. and Schady, P. and Skidmore, W. and Song, L. and Stanway, E. and Starling, R. and Topinka, M. and Troja, E. and van Putten, M. and Vanzella, E. and Vercellone, S. and Wilson-Hodge, C. and Yonetoku, D. and Zampa, G. and Zampa, N. and Zhang, B. and Zhang, B.B. and Zhang, S. and Zhang, S.-N. and Antonelli, A. and Bianco, F. and Boci, S. and Boer, M. and Botticella, M.T. and Boulade, O. and Butler, C. and Campana, S. and Capitanio, F. and Celotti, A. and Chen, Y. and Colpi, M. and Comastri, A. and Cuby, J.-G. and Dadina, M. and De Luca, A. and Dong, Y.-W. and Ettori, S. and Gandhi, P. and Geza, E. and Greiner, J. and Guiriec, S. and Harms, J. and Hernanz, M. and Hornstrup, A. and Hutchinson, I. and Israel, G. and Jonker, P. and Kaneko, Y. and Kawai, N. and Wiersema, K. and Korpela, S. and Lebrun, V. and Lu, F. and MacFadyen, A. and Malaguti, G. and Maraschi, L. and Melandri, A. and Modjaz, M. and Morris, D. and Omodei, N. and Paizis, A. and Páta, P. and Petrosian, V. and Rachevski, A. and Rhoads, J. and Ryde, F. and Sabau-Graziati, L. and Shigehiro, N. and Sims, M. and Soomin, J. and Szécsi, D. and Urata, Y. and Uslenghi, M. and Valenziano, L. and Vianello, G. and Vojtech, S. and Watson, D. and Zicha, J.
Subjects: Ionization, Atmospheric Science, cosmological model, Cherenkov Telescope Array, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Astronomy, Dark age, MASSIVE SINGLE STARS, Star formation rates, Gamma ray, 01 natural sciences, Cosmology: observation, localization, law.invention, Astrophysic, Einstein Telescope, observational cosmology, law, Observational cosmology, Re-ionization, Cosmology: observations, Dark ages, First stars, Gamma-ray: bursts, LIGO, observations [Cosmology], Telescope, 010303 astronomy & astrophysics, High sensitivity, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Multi-wavelength, energy: high, sezele, gamma-ray bursts, Aerospace Engineering, Space and Planetary Science, Astrophysics::Instrumentation and Methods for Astrophysics, imaging, star: formation, burst [Gamma-ray], observatory, Geophysics, X rays, Cosmology: observation, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, signature, Star, TIDAL DISRUPTION, Gamma-ray: burst, Astrophysics::High Energy Astrophysical Phenomena, SIMILAR-TO 6, Socio-culturale, FOS: Physical sciences, observation [Cosmology], galaxy: luminosity, X-ray astronomy: instrumentation, 7 CANDIDATE GALAXIES, Astrophysics::Cosmology and Extragalactic Astrophysics, gamma ray: burst, 114 Physical sciences, Settore FIS/03 - Fisica della Materia, X-ray, bursts [Gamma-ray], FIS/05 - ASTRONOMIA E ASTROFISICA, Settore FIS/05 - Astronomia e Astrofisica, First star, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], KAGRA, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, LIGHT CURVES, 010308 nuclear & particles physics, Gravitational wave, gravitational radiation, Astronomy and Astrophysics, 115 Astronomy, Space science, redshift, sensitivity, Redshift, NEUTRON-STAR MERGER, messenger, VIRGO, electromagnetic, LUMINOSITY FUNCTION, BLACK-HOLE, General Earth and Planetary Sciences, Gamma-ray burst, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift 10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ¿20s/early ¿30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).© 2018 COSPAR, S.E. acknowledges the financial support from contracts ASI-INAF 1/009/10/0, NARO15 ASI-INAF 1/037/12/0 and ASI 2015-046-R.0. R.H. acknowledges GACR grant 13-33324S. S.V. research leading to these results has received funding from the European Union's Seventh Framework Programme for research, technological development and demonstration under grant agreement no 606176. D.S. was supported by the Czech grant 1601116S GA CR. Maria Giovanna Dainotti acknowledges funding from the European Union through the Marie Curie Action FP7-PEOPLE-2013-IOF, under grant agreement No. 626267 (>Cosmological Candles>).
Published: 2018

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

Author: ShuangNan Zhang, Andrea Santangelo, Marco Feroci, YuPeng Xu, FangJun Lu, Yong Chen, Hua Feng, Shu Zhang, Søren Brandt, Margarita Hernanz, Luca Baldini, Enrico Bozzo, Riccardo Campana, Alessandra De Rosa, YongWei Dong, Yuri Evangelista, Vladimir Karas, Norbert Meidinger, Aline Meuris, Kirpal Nandra, Teng Pan, Giovanni Pareschi, Piotr Orleanski, QiuShi Huang, Stephane Schanne, Giorgia Sironi, Daniele Spiga, Jiri Svoboda, Gianpiero Tagliaferri, Christoph Tenzer, Andrea Vacchi, Silvia Zane, Dave Walton, ZhanShan Wang, Berend Winter, Xin Wu, Jean J. M. in’ t Zand, Mahdi Ahangarianabhari, Giovanni Ambrosi, Filippo Ambrosino, Marco Barbera, Stefano Basso, Jörg Bayer, Ronaldo Bellazzini, Pierluigi Bellutti, Bruna Bertucci, Giuseppe Bertuccio, Giacomo Borghi, XueLei Cao, Franck Cadoux, Francesco Ceraudo, TianXiang Chen, YuPeng Chen, Jerome Chevenez, Marta Civitani, Wei Cui, WeiWei Cui, Thomas Dauser, Ettore Del Monte, Sergio Di Cosimo, Sebastian Diebold, Victor Doroshenko, Michal Dovciak, YuanYuan Du, Lorenzo Ducci, QingMei Fan, Yannick Favre, Fabio Fuschino, José Luis Gálvez, Min Gao, MingYu Ge, Olivier Gevin, Marco Grassi, QuanYing Gu, YuDong Gu, DaWei Han, Bin Hong, Wei Hu, Long Ji, ShuMei Jia, WeiChun Jiang, Thomas Kennedy, Ingo Kreykenbohm, Irfan Kuvvetli, Claudio Labanti, Luca Latronico, Gang Li, MaoShun Li, Xian Li, Wei Li, ZhengWei Li, Olivier Limousin, HongWei Liu, XiaoJing Liu, Bo Lu, Tao Luo, Daniele Macera, Piero Malcovati, Adrian Martindale, Malgorzata Michalska, Bin Meng, Massimo Minuti, Alfredo Morbidini, Fabio Muleri, Stephane Paltani, Emanuele Perinati, Antonino Picciotto, Claudio Piemonte, JinLu Qu, Alexandre Rachevski, Irina Rashevskaya, Jerome Rodriguez, Thomas Schanz, ZhengXiang Shen, LiZhi Sheng, JiangBo Song, LiMing Song, Carmelo Sgro, Liang Sun, Ying Tan, Phil Uttley, Bo Wang, DianLong Wang, GuoFeng Wang, Juan Wang, LangPing Wang, YuSa Wang, Anna L. Watts, XiangYang Wen, Jörn Wilms, ShaoLin Xiong, JiaWei Yang, Sheng Yang, YanJi Yang, Nian Yu, WenDa Zhang, Gianluigi Zampa, Nicola Zampa, Andrzej A. Zdziarski, AiMei Zhang, ChengMo Zhang, Fan Zhang, Long Zhang, Tong Zhang, Yi Zhang, XiaoLi Zhang, ZiLiang Zhang, BaoSheng Zhao, ShiJie Zheng, YuPeng Zhou, Nicola Zorzi, J. Frans Zwart, ITA, GBR, FRA, DEU, ESP, DNK, POL, CZE, CHN, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, eXTP, Zhang, ShuangNan, Santangelo, Andrea, Feroci, Marco, Xu, YuPeng, Lu, FangJun, Chen, Yong, Feng, Hua, Zhang, Shu, Brandt, Søren, Hernanz, Margarita, Baldini, Luca, Bozzo, Enrico, Campana, Riccardo, De Rosa, Alessandra, Dong, YongWei, Evangelista, Yuri, Karas, Vladimir, Meidinger, Norbert, Meuris, Aline, Nandra, Kirpal, Pan, Teng, Pareschi, Giovanni, Orleanski, Piotr, Huang, QiuShi, Schanne, Stephane, Sironi, Giorgia, Spiga, Daniele, Svoboda, Jiri, Tagliaferri, Gianpiero, Tenzer, Christoph, Vacchi, Andrea, Zane, Silvia, Walton, Dave, Wang, ZhanShan, Winter, Berend, Wu, Xin, in’ t Zand, Jean J. M., Ahangarianabhari, Mahdi, Ambrosi, Giovanni, Ambrosino, Filippo, Barbera, Marco, Basso, Stefano, Bayer, Jörg, Bellazzini, Ronaldo, Bellutti, Pierluigi, Bertucci, Bruna, Bertuccio, Giuseppe, Borghi, Giacomo, Cao, XueLei, Cadoux, Franck, Ceraudo, Francesco, Chen, TianXiang, Chen, YuPeng, Chevenez, Jerome, Civitani, Marta, Cui, Wei, Cui, WeiWei, Dauser, Thoma, Del Monte, Ettore, Di Cosimo, Sergio, Diebold, Sebastian, Doroshenko, Victor, Dovciak, Michal, Du, YuanYuan, Ducci, Lorenzo, Fan, QingMei, Favre, Yannick, Fuschino, Fabio, Gálvez, José Lui, Gao, Min, Ge, MingYu, Gevin, Olivier, Grassi, Marco, Gu, QuanYing, Gu, YuDong, Han, DaWei, Hong, Bin, Hu, Wei, Ji, Long, Jia, ShuMei, Jiang, WeiChun, Kennedy, Thoma, Kreykenbohm, Ingo, Kuvvetli, Irfan, Labanti, Claudio, Latronico, Luca, Li, Gang, Li, MaoShun, Li, Xian, Li, Wei, Li, ZhengWei, Limousin, Olivier, Liu, HongWei, Liu, XiaoJing, Lu, Bo, Luo, Tao, Macera, Daniele, Malcovati, Piero, Martindale, Adrian, Michalska, Malgorzata, Meng, Bin, Minuti, Massimo, Morbidini, Alfredo, Muleri, Fabio, Paltani, Stephane, Perinati, Emanuele, Picciotto, Antonino, Piemonte, Claudio, Qu, JinLu, Rachevski, Alexandre, Rashevskaya, Irina, Rodriguez, Jerome, Schanz, Thoma, Shen, ZhengXiang, Sheng, LiZhi, Song, JiangBo, Song, LiMing, Sgro, Carmelo, Sun, Liang, Tan, Ying, Uttley, Phil, Wang, Bo, Wang, DianLong, Wang, GuoFeng, Wang, Juan, Wang, LangPing, Wang, YuSa, Watts, Anna L., Wen, XiangYang, Wilms, Jörn, Xiong, ShaoLin, Yang, JiaWei, Yang, Sheng, Yang, YanJi, Yu, Nian, Zhang, WenDa, Zampa, Gianluigi, Zampa, Nicola, Zdziarski, Andrzej A., Zhang, AiMei, Zhang, ChengMo, Zhang, Fan, Zhang, Long, Zhang, Tong, Zhang, Yi, Zhang, XiaoLi, Zhang, ZiLiang, Zhao, BaoSheng, Zheng, ShiJie, Zhou, YuPeng, Zorzi, Nicola, Zwart, J. Frans, and High Energy Astrophys. & Astropart. Phys (API, FNWI)
Subjects: Gravity (chemistry), Computer science, space mission: eXTP, X-ray timing, Polarimetry, General Physics and Astronomy, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, Physics and Astronomy (all), Settore FIS/05 - Astronomia E Astrofisica, Observatory, X-ray instrumentation, 0103 physical sciences, X-ray polarimetry, Ground segment, Aerospace engineering, 010306 general physics, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), High Energy Astrophysical Phenomena (astro-ph.HE), Spacecraft, sezele, business.industry, Payload, Gravitational wave, Astrophysics::Instrumentation and Methods for Astrophysics, Space Science, business, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: In this paper we present the enhanced X-ray Timing and Polarimetry mission - eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources. The paper provides a detailed description of: (1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload; (2) the elements and functions of the mission, from the spacecraft to the ground segment., Accepted for publication on Sci. China Phys. Mech. Astron. (2019)
Published: 2019

224. On the High‐Energy Spectral Component and Fine Time Structure of Terrestrial Gamma Ray Flashes

Author: Alessio Trois, Martino Marisaldi, Marco Tavani, Nikolai Østgaard, David Sarria, Riccardo Campana, A. Ursi, Fanchao Lyu, Steven A. Cummer, C. Pittori, Anders Lindanger, M. Galli, F. Verrecchia, C. Labanti, A. Argan, F. Fuschino, ITA, USA, NOR, Marisaldi, M., Galli, M., Labanti, C., Ostgaard, N., Sarria, D., Cummer, S. A., Lyu, F., Lindanger, A., Campana, R., Ursi, A., Tavani, M., Fuschino, F., Argan, A., Trois, A., Pittori, C., and Verrecchia, F.
Subjects: Atmospheric Science, Photon, 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, FOS: Physical sciences, Astrophysics, 7. Clean energy, 01 natural sciences, Spectral line, atmospheric electricity, Physics - Space Physics, 0103 physical sciences, Earth and Planetary Sciences (miscellaneous), high-energy atmospheric physics, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, high-energy atmospheric physic, Gamma ray, Spectral component, AGILE satellite, high-energy radiation, lightning, terrestrial gamma ray flash, Lightning, Space Physics (physics.space-ph), Particle acceleration, Geophysics, Relativistic runaway electron avalanche, Space and Planetary Science, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Terrestrial gamma ray flashes (TGFs) are very short bursts of gamma radiation associated to thunderstorm activity and are the manifestation of the highest-energy natural particle acceleration phenomena occurring on Earth. Photon energies up to several tens of megaelectronvolts are expected, but the actual upper limit and high-energy spectral shape are still open questions. Results published in 2011 by the AGILE team proposed a high-energy component in TGF spectra extended up to $\approx$100 MeV, which is difficult to reconcile with the predictions from the Relativistic Runaway Electron Avalanche (RREA) mechanism at the basis of many TGF production models. Here we present a new set of TGFs detected by the AGILE satellite and associated to lightning measurements capable to solve this controversy. Detailed end-to-end Monte Carlo simulations and an improved understanding of the instrument performance under high-flux conditions show that it is possible to explain the observed high-energy counts by a standard RREA spectrum at the source, provided that the TGF is sufficiently bright and short. We investigate the possibility that single high-energy counts may be the signature of a fine-pulsed time structure of TGFs on time scales $\approx$4 {\mu}s, but we find no clear evidence for this. The presented data set and modeling results allow also for explaining the observed TGF distribution in the (Fluence x duration) parameter space and suggest that the AGILE TGF detection rate can almost be doubled. Terrestrial gamma ray flashes (TGFs) are very short bursts of gamma radiation associated to thunderstorm activity and are the manifestation of the highest-energy natural particle acceleration phenomena occurring on Earth. (...continues)
Published: 2019

225. GPM‐DPR Observations on TGFs Producing Storms

Author: Tiberia, A., primary, Porcú, F., additional, Marisaldi, M., additional, Tavani, M., additional, Lapierre, J., additional, Ursi, A., additional, Fuschino, F., additional, D'Adderio, L. P., additional, and Dietrich, S., additional
Published: 2021
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226. Time Evolution of Storms Producing Terrestrial Gamma-Ray Flashes Using ERA5 Reanalysis Data, GPS, Lightning and Geostationary Satellite Observations

Author: Tiberia, Alessandra, primary, Mascitelli, Alessandra, additional, D’Adderio, Leo Pio, additional, Federico, Stefano, additional, Marisaldi, Martino, additional, Porcù, Federico, additional, Realini, Eugenio, additional, Gatti, Andrea, additional, Ursi, Alessandro, additional, Fuschino, Fabio, additional, Tavani, Marco, additional, and Dietrich, Stefano, additional
Published: 2021
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227. THESEUS: A key space mission concept for Multi-Messenger Astrophysics

Author: Stratta, G, Ciolfi, R, Amati, L, Bozzo, E, Ghirlanda, G, Maiorano, E, Nicastro, L, Rossi, A, Vinciguerra, S, Frontera, F, Götz, D, Guidorzi, C, O'Brien, P, Osborne, J, Tanvir, N, Branchesi, M, Brocato, E, Dainotti, M, De Pasquale, M, Grado, A, Greiner, J, Longo, F, Maio, U, Mereghetti, D, Mignani, R, Piranomonte, S, Rezzolla, L, Salvaterra, R, Starling, R, Willingale, R, Böer, M, Bulgarelli, A, Caruana, J, Colafrancesco, S, Colpi, M, Covino, S, D'Avanzo, P, D'Elia, V, Drago, A, Fuschino, F, Gendre, B, Hudec, R, Jonker, P, Labanti, C, Malesani, D, Mundell, C, Palazzi, E, Patricelli, B, Razzano, M, Campana, R, Rosati, P, Rodic, T, Szécsi, D, Stamerra, A, van Putten, M, Vergani, S, Zhang, B, Bernardini, M, Stratta, G., Ciolfi, R., Amati, L., Bozzo, E., Ghirlanda, G., Maiorano, E., Nicastro, L., Rossi, A., Vinciguerra, S., Frontera, F., Götz, D., Guidorzi, C., O'Brien, P., Osborne, J. P., Tanvir, N., Branchesi, M., Brocato, E., Dainotti, M. G., De Pasquale, M., Grado, A., Greiner, J., Longo, F., Maio, U., Mereghetti, D., Mignani, R., Piranomonte, S., Rezzolla, L., Salvaterra, R., Starling, R., Willingale, R., Böer, M., BULGARELLI, ALICE, Caruana, J., Colafrancesco, S., Colpi, M., Covino, S., D'Avanzo, P., D'Elia, V., Drago, A., Fuschino, F., Gendre, B., Hudec, R., Jonker, P., Labanti, C., Malesani, D., Mundell, C. G., Palazzi, E., Patricelli, B., Razzano, M., Campana, R., Rosati, P., Rodic, T., Szécsi, D., Stamerra, A., van Putten, M., Vergani, S., Zhang, B., Bernardini, M., Stratta, G, Ciolfi, R, Amati, L, Bozzo, E, Ghirlanda, G, Maiorano, E, Nicastro, L, Rossi, A, Vinciguerra, S, Frontera, F, Götz, D, Guidorzi, C, O'Brien, P, Osborne, J, Tanvir, N, Branchesi, M, Brocato, E, Dainotti, M, De Pasquale, M, Grado, A, Greiner, J, Longo, F, Maio, U, Mereghetti, D, Mignani, R, Piranomonte, S, Rezzolla, L, Salvaterra, R, Starling, R, Willingale, R, Böer, M, Bulgarelli, A, Caruana, J, Colafrancesco, S, Colpi, M, Covino, S, D'Avanzo, P, D'Elia, V, Drago, A, Fuschino, F, Gendre, B, Hudec, R, Jonker, P, Labanti, C, Malesani, D, Mundell, C, Palazzi, E, Patricelli, B, Razzano, M, Campana, R, Rosati, P, Rodic, T, Szécsi, D, Stamerra, A, van Putten, M, Vergani, S, Zhang, B, Bernardini, M, Stratta, G., Ciolfi, R., Amati, L., Bozzo, E., Ghirlanda, G., Maiorano, E., Nicastro, L., Rossi, A., Vinciguerra, S., Frontera, F., Götz, D., Guidorzi, C., O'Brien, P., Osborne, J. P., Tanvir, N., Branchesi, M., Brocato, E., Dainotti, M. G., De Pasquale, M., Grado, A., Greiner, J., Longo, F., Maio, U., Mereghetti, D., Mignani, R., Piranomonte, S., Rezzolla, L., Salvaterra, R., Starling, R., Willingale, R., Böer, M., BULGARELLI, ALICE, Caruana, J., Colafrancesco, S., Colpi, M., Covino, S., D'Avanzo, P., D'Elia, V., Drago, A., Fuschino, F., Gendre, B., Hudec, R., Jonker, P., Labanti, C., Malesani, D., Mundell, C. G., Palazzi, E., Patricelli, B., Razzano, M., Campana, R., Rosati, P., Rodic, T., Szécsi, D., Stamerra, A., van Putten, M., Vergani, S., Zhang, B., and Bernardini, M.
Abstract: The recent discovery of the electromagnetic counterpart of the gravitational wave source GW170817, has demonstrated the huge informative power of multi-messenger observations. During the next decade the nascent field of multi-messenger astronomy will mature significantly. Around 2030 and beyond, third generation ground-based gravitational wave detectors will be roughly ten times more sensitive than the current ones. At the same time, neutrino detectors currently upgrading to multi km3 telescopes, will include a 10 km3 facility in the Southern hemisphere. In this review, we describe the most promising sources of high frequency gravitational waves and neutrinos that will be detected in the next two decades. In this context, we show the important role of the Transient High Energy Sky and Early Universe Surveyor (THESEUS), a mission concept accepted by ESA for phase A study and proposed by a large international collaboration in response to the call for the Cosmic Vision Programme M5 missions. THESEUS aims at providing a substantial advancement in early Universe science as well as in multi–messenger and time–domain astrophysics, operating in strong synergy with future gravitational wave and neutrino detectors as well as major ground- and space-based telescopes. This review is an extension of the THESEUS white paper (Amati et al., 2017), also in light of the discovery of GW170817/GRB170817A that was announced on October 16th, 2017.
Published: 2018

228. The THESEUS space mission concept: science case, design and expected performances

Author: Amati, L, O'Brien, P, Götz, D, Bozzo, E, Tenzer, C, Frontera, F, Ghirlanda, G, Labanti, C, Osborne, J, Stratta, G, Tanvir, N, Willingale, R, Attina, P, Campana, R, Castro-Tirado, A, Contini, C, Fuschino, F, Gomboc, A, Hudec, R, Orleanski, P, Renotte, E, Rodic, T, Bagoly, Z, Blain, A, Callanan, P, Covino, S, Ferrara, A, Le Floch, E, Marisaldi, M, Mereghetti, S, Rosati, P, Vacchi, A, D'Avanzo, P, Giommi, P, Piranomonte, S, Piro, L, Reglero, V, Rossi, A, Santangelo, A, Salvaterra, R, Tagliaferri, G, Vergani, S, Vinciguerra, S, Briggs, M, Campolongo, E, Ciolfi, R, Connaughton, V, Cordier, B, Morelli, B, Orlandini, M, Adami, C, Argan, A, Atteia, J, Auricchio, N, Balazs, L, Baldazzi, G, Basa, S, Basak, R, Bellutti, P, Bernardini, M, Bertuccio, G, Braga, J, Branchesi, M, Brandt, S, Brocato, E, Budtz-Jorgensen, C, Bulgarelli, A, Burderi, L, Camp, J, Capozziello, S, Caruana, J, Casella, P, Cenko, B, Chardonnet, P, Ciardi, B, Colafrancesco, S, Dainotti, M, D'Elia, V, De Martino, D, De Pasquale, M, Del Monte, E, Della Valle, M, Drago, A, Evangelista, Y, Feroci, M, Finelli, F, Fiorini, M, Fynbo, J, Gal-Yam, A, Gendre, B, Ghisellini, G, Grado, A, Guidorzi, C, Hafizi, M, Hanlon, L, Hjorth, J, Izzo, L, Kiss, L, Kumar, P, Kuvvetli, I, Lavagna, M, Li, T, Longo, F, Lyutikov, M, Maio, U, Maiorano, E, Malcovati, P, Malesani, D, Margutti, R, Martin-Carrillo, A, Masetti, N, Mcbreen, S, Mignani, R, Morgante, G, Mundell, C, Nargaard-Nielsen, H, Nicastro, L, Palazzi, E, Paltani, S, Panessa, F, Pareschi, G, Pe'Er, A, Penacchioni, A, Pian, E, Piedipalumbo, E, Piran, T, Rauw, G, Razzano, M, Read, A, Rezzolla, L, Romano, P, Ruffini, R, Savaglio, S, Sguera, V, Schady, P, Skidmore, W, Song, L, Stanway, E, Starling, R, Topinka, M, Troja, E, van Putten, M, Vanzella, E, Vercellone, S, Wilson-Hodge, C, Yonetoku, D, Zampa, G, Zampa, N, Zhang, B, Zhang, S, Antonelli, A, Bianco, F, Boci, S, Boer, M, Botticella, M, Boulade, O, Butler, C, Campana, S, Capitanio, F, Celotti, A, Chen, Y, Colpi, M, Comastri, A, Cuby, J, Dadina, M, De Luca, A, Dong, Y, Ettori, S, Gandhi, P, Geza, E, Greiner, J, Guiriec, S, Harms, J, Hernanz, M, Hornstrup, A, Hutchinson, I, Israel, G, Jonker, P, Kaneko, Y, Kawai, N, Wiersema, K, Korpela, S, Lebrun, V, Lu, F, Macfadyen, A, Malaguti, G, Maraschi, L, Melandri, A, Modjaz, M, Morris, D, Omodei, N, Paizis, A, Páta, P, Petrosian, V, Rachevski, A, Rhoads, J, Ryde, F, Sabau-Graziati, L, Shigehiro, N, Sims, M, Soomin, J, Szécsi, D, Urata, Y, Uslenghi, M, Valenziano, L, Vianello, G, Vojtech, S, Watson, D, Zicha, J, Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., Zicha, J., Amati, L, O'Brien, P, Götz, D, Bozzo, E, Tenzer, C, Frontera, F, Ghirlanda, G, Labanti, C, Osborne, J, Stratta, G, Tanvir, N, Willingale, R, Attina, P, Campana, R, Castro-Tirado, A, Contini, C, Fuschino, F, Gomboc, A, Hudec, R, Orleanski, P, Renotte, E, Rodic, T, Bagoly, Z, Blain, A, Callanan, P, Covino, S, Ferrara, A, Le Floch, E, Marisaldi, M, Mereghetti, S, Rosati, P, Vacchi, A, D'Avanzo, P, Giommi, P, Piranomonte, S, Piro, L, Reglero, V, Rossi, A, Santangelo, A, Salvaterra, R, Tagliaferri, G, Vergani, S, Vinciguerra, S, Briggs, M, Campolongo, E, Ciolfi, R, Connaughton, V, Cordier, B, Morelli, B, Orlandini, M, Adami, C, Argan, A, Atteia, J, Auricchio, N, Balazs, L, Baldazzi, G, Basa, S, Basak, R, Bellutti, P, Bernardini, M, Bertuccio, G, Braga, J, Branchesi, M, Brandt, S, Brocato, E, Budtz-Jorgensen, C, Bulgarelli, A, Burderi, L, Camp, J, Capozziello, S, Caruana, J, Casella, P, Cenko, B, Chardonnet, P, Ciardi, B, Colafrancesco, S, Dainotti, M, D'Elia, V, De Martino, D, De Pasquale, M, Del Monte, E, Della Valle, M, Drago, A, Evangelista, Y, Feroci, M, Finelli, F, Fiorini, M, Fynbo, J, Gal-Yam, A, Gendre, B, Ghisellini, G, Grado, A, Guidorzi, C, Hafizi, M, Hanlon, L, Hjorth, J, Izzo, L, Kiss, L, Kumar, P, Kuvvetli, I, Lavagna, M, Li, T, Longo, F, Lyutikov, M, Maio, U, Maiorano, E, Malcovati, P, Malesani, D, Margutti, R, Martin-Carrillo, A, Masetti, N, Mcbreen, S, Mignani, R, Morgante, G, Mundell, C, Nargaard-Nielsen, H, Nicastro, L, Palazzi, E, Paltani, S, Panessa, F, Pareschi, G, Pe'Er, A, Penacchioni, A, Pian, E, Piedipalumbo, E, Piran, T, Rauw, G, Razzano, M, Read, A, Rezzolla, L, Romano, P, Ruffini, R, Savaglio, S, Sguera, V, Schady, P, Skidmore, W, Song, L, Stanway, E, Starling, R, Topinka, M, Troja, E, van Putten, M, Vanzella, E, Vercellone, S, Wilson-Hodge, C, Yonetoku, D, Zampa, G, Zampa, N, Zhang, B, Zhang, S, Antonelli, A, Bianco, F, Boci, S, Boer, M, Botticella, M, Boulade, O, Butler, C, Campana, S, Capitanio, F, Celotti, A, Chen, Y, Colpi, M, Comastri, A, Cuby, J, Dadina, M, De Luca, A, Dong, Y, Ettori, S, Gandhi, P, Geza, E, Greiner, J, Guiriec, S, Harms, J, Hernanz, M, Hornstrup, A, Hutchinson, I, Israel, G, Jonker, P, Kaneko, Y, Kawai, N, Wiersema, K, Korpela, S, Lebrun, V, Lu, F, Macfadyen, A, Malaguti, G, Maraschi, L, Melandri, A, Modjaz, M, Morris, D, Omodei, N, Paizis, A, Páta, P, Petrosian, V, Rachevski, A, Rhoads, J, Ryde, F, Sabau-Graziati, L, Shigehiro, N, Sims, M, Soomin, J, Szécsi, D, Urata, Y, Uslenghi, M, Valenziano, L, Vianello, G, Vojtech, S, Watson, D, Zicha, J, Amati, L., O'Brien, P., Götz, D., Bozzo, E., Tenzer, C., Frontera, F., Ghirlanda, G., Labanti, C., Osborne, J. P., Stratta, G., Tanvir, N., Willingale, R., Attina, P., Campana, R., Castro-Tirado, A. J., Contini, C., Fuschino, F., Gomboc, A., Hudec, R., Orleanski, P., Renotte, E., Rodic, T., Bagoly, Z., Blain, A., Callanan, P., Covino, S., Ferrara, A., Le Floch, E., Marisaldi, M., Mereghetti, S., Rosati, P., Vacchi, A., D'Avanzo, P., Giommi, P., Piranomonte, S., Piro, L., Reglero, V., Rossi, A., Santangelo, A., Salvaterra, R., Tagliaferri, G., Vergani, S., Vinciguerra, S., Briggs, M., Campolongo, E., Ciolfi, R., Connaughton, V., Cordier, B., Morelli, B., Orlandini, M., Adami, C., Argan, A., Atteia, J. -L., Auricchio, N., Balazs, L., Baldazzi, G., Basa, S., Basak, R., Bellutti, P., Bernardini, M. G., Bertuccio, G., Braga, J., Branchesi, M., Brandt, S., Brocato, E., Budtz-Jorgensen, C., Bulgarelli, A., Burderi, L., Camp, J., Capozziello, S., Caruana, J., Casella, P., Cenko, B., Chardonnet, P., Ciardi, B., Colafrancesco, S., Dainotti, M. G., D'Elia, V., De Martino, D., De Pasquale, M., Del Monte, E., Della Valle, M., Drago, A., Evangelista, Y., Feroci, M., Finelli, F., Fiorini, M., Fynbo, J., Gal-Yam, A., Gendre, B., Ghisellini, G., Grado, A., Guidorzi, C., Hafizi, M., Hanlon, L., Hjorth, J., Izzo, L., Kiss, L., Kumar, P., Kuvvetli, I., Lavagna, M., Li, T., Longo, F., Lyutikov, M., Maio, U., Maiorano, E., Malcovati, P., Malesani, D., Margutti, R., Martin-Carrillo, A., Masetti, N., McBreen, S., Mignani, R., Morgante, G., Mundell, C., Nargaard-Nielsen, H. U., Nicastro, L., Palazzi, E., Paltani, S., Panessa, F., Pareschi, G., Pe'er, A., Penacchioni, A. V., Pian, E., Piedipalumbo, E., Piran, T., Rauw, G., Razzano, M., Read, A., Rezzolla, L., Romano, P., Ruffini, R., Savaglio, S., Sguera, V., Schady, P., Skidmore, W., Song, L., Stanway, E., Starling, R., Topinka, M., Troja, E., van Putten, M., Vanzella, E., Vercellone, S., Wilson-Hodge, C., Yonetoku, D., Zampa, G., Zampa, N., Zhang, B., Zhang, B. B., Zhang, S., Zhang, S. -N., Antonelli, A., Bianco, F., Boci, S., Boer, M., Botticella, M. T., Boulade, O., Butler, C., Campana, S., Capitanio, F., Celotti, A., Chen, Y., Colpi, M., Comastri, A., Cuby, J. -G., Dadina, M., De Luca, A., Dong, Y. -W., Ettori, S., Gandhi, P., Geza, E., Greiner, J., Guiriec, S., Harms, J., Hernanz, M., Hornstrup, A., Hutchinson, I., Israel, G., Jonker, P., Kaneko, Y., Kawai, N., Wiersema, K., Korpela, S., Lebrun, V., Lu, F., MacFadyen, A., Malaguti, G., Maraschi, L., Melandri, A., Modjaz, M., Morris, D., Omodei, N., Paizis, A., Páta, P., Petrosian, V., Rachevski, A., Rhoads, J., Ryde, F., Sabau-Graziati, L., Shigehiro, N., Sims, M., Soomin, J., Szécsi, D., Urata, Y., Uslenghi, M., Valenziano, L., Vianello, G., Vojtech, S., Watson, D., and Zicha, J.
Abstract: THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5–1 arcmin localization, an energy band extending from several MeV down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift ∼10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late ’20s/early ’30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA).
Published: 2018

229. The FAMU experiment at RIKEN-RAL to study the muon transfer rate from hydrogen to other gases

Author: Adamczak, A, Baccolo, G, Banfi, S, Bakalov, D, Baldazzi, G, Benocci, R, Bertoni, R, Bonesini, M, Bonvicini, V, Chignoli, F, Clemenza, M, Colace, L, Danailov, M, Danev, P, de Bari, A, Vecchi, C, Vincenzi, M, Furlanetto, E, Fuschino, F, Gadedjisso-Tossou, K, Guffanti, D, Iaciofano, A, Ishida, K, Labanti, C, Maggi, V, Margotti, A, Mazza, R, Menegolli, A, Mocchiutti, E, Moretti, M, Morgante, G, Nastasi, M, Niemela, J, Pizzolotto, C, Previtali, E, Pullia, A, Ramponi, R, Rachevski, A, Rignanese, L, Rossella, M, Rossi, N, Sarkar, R, Stoilov, M, Stoychev, L, Tomaselli, A, Tortora, L, Vallazza, E, Zampa, G, Vacchi, A, Adamczak, A., Baccolo, G., Banfi, S., Bakalov, D., Baldazzi, G., Benocci, R., Bertoni, R., Bonesini, M., Bonvicini, V., Chignoli, F., Clemenza, M., Colace, L., Danailov, M., Danev, P., de Bari, A., Vecchi, C. De, Vincenzi, M. De, Furlanetto, E., Fuschino, F., Gadedjisso-Tossou, K. S., Guffanti, D., Iaciofano, A., Ishida, K., Labanti, C., Maggi, V., Margotti, A., Mazza, R., Menegolli, A., Mocchiutti, E., Moretti, M., Morgante, G., Nastasi, M., Niemela, J., Pizzolotto, C., Previtali, E., Pullia, A., Ramponi, R., Rachevski, A., Rignanese, L. P., Rossella, M., Rossi, N., Sarkar, R., Stoilov, M., Stoychev, L., Tomaselli, A., Tortora, L., Vallazza, E., Zampa, G., Vacchi, A., Adamczak, A, Baccolo, G, Banfi, S, Bakalov, D, Baldazzi, G, Benocci, R, Bertoni, R, Bonesini, M, Bonvicini, V, Chignoli, F, Clemenza, M, Colace, L, Danailov, M, Danev, P, de Bari, A, Vecchi, C, Vincenzi, M, Furlanetto, E, Fuschino, F, Gadedjisso-Tossou, K, Guffanti, D, Iaciofano, A, Ishida, K, Labanti, C, Maggi, V, Margotti, A, Mazza, R, Menegolli, A, Mocchiutti, E, Moretti, M, Morgante, G, Nastasi, M, Niemela, J, Pizzolotto, C, Previtali, E, Pullia, A, Ramponi, R, Rachevski, A, Rignanese, L, Rossella, M, Rossi, N, Sarkar, R, Stoilov, M, Stoychev, L, Tomaselli, A, Tortora, L, Vallazza, E, Zampa, G, Vacchi, A, Adamczak, A., Baccolo, G., Banfi, S., Bakalov, D., Baldazzi, G., Benocci, R., Bertoni, R., Bonesini, M., Bonvicini, V., Chignoli, F., Clemenza, M., Colace, L., Danailov, M., Danev, P., de Bari, A., Vecchi, C. De, Vincenzi, M. De, Furlanetto, E., Fuschino, F., Gadedjisso-Tossou, K. S., Guffanti, D., Iaciofano, A., Ishida, K., Labanti, C., Maggi, V., Margotti, A., Mazza, R., Menegolli, A., Mocchiutti, E., Moretti, M., Morgante, G., Nastasi, M., Niemela, J., Pizzolotto, C., Previtali, E., Pullia, A., Ramponi, R., Rachevski, A., Rignanese, L. P., Rossella, M., Rossi, N., Sarkar, R., Stoilov, M., Stoychev, L., Tomaselli, A., Tortora, L., Vallazza, E., Zampa, G., and Vacchi, A.
Abstract: The aim of the FAMU (Fisica degli Atomi Muonici) experiment is to realize the first measurement of the hyperfine splitting (hfs) in the 1S state of muonic hydrogen Delta E-1S(hfs), by using the RIKEN-RAL intense pulsed muon beam and a high-energy mid-infrared tunable laser. This requires a detailed study of the muon transfer mechanism at different temperatures and hence at different epithermal states of the muonic system. The experimental setup involves a cryogenic pressurized gas target and a detection system based on silicon photomultipliers-fiber beam hodoscopes and high purity Germanium detectors and Cerium doped Lanthanium Bromide crystals, for X-rays detection at energies around 100 keV.Simulation, construction and detector performances of the FAMU apparatus at RAL are reported in this paper.
Published: 2018

230. Monitoring Coronavirus Disease 2019 (COVID-19) Through Trends in Influenza-like Illness, Laboratory-confirmed Influenza, and COVID-19—New York State, Excluding New York City, 1 January 2020–12 April 2020

Author: Rosenberg, Eli S, Hall, Eric W, Rosenthal, Elizabeth M, Maxted, Angela M, Gowie, Donna L, Dufort, Elizabeth M, Blog, Debra S, Hoefer, Dina, George, Kirsten St, Hutton, Brad J, Zucker, Howard A, Anand, Madhu, Backenson, Bryon, Kaufman, Alison, Kuhles, Daniel, Muse, Alison, Newman, Alexandra, Pulver, Wendy, Smith, Lou, Sommer, Jamie, White, Jennifer, Dean, Amy, Derbyshire, Victoria, Egan, Christina, Fuschino, Meghan, Griesemer, Sara, Hull, Rene, Lamson, Daryl, Laplante, Jennifer, McDonough, Kathleen, Mitchell, Kara, Nazarian, Elizabeth, Popowich, Michael, Taylor, Jill, Walsh, Anne, Amler, Sherlita, Huang, Ada, Recchia, Renee, Whalen, Elizabeth, Lewis, Elizabeth, Friedman, Cynthia, Carrera, Sandra, Eisenstein, Lawrence, DeSimone, Ann, Morne, Johanne, Johnson, Megan, Navarette, Kristen, Kumar, Jessica, Ostrowski, Stephanie, Mazeau, Andrienne, Dreslin, Sally, Yates, Nora, Greene, Danielle, Heslin, Eugene, Lutterloh, Emily, Holtgrave, David, and Barranco, Meredith
Subjects: Microbiology (medical), 2019-20 coronavirus outbreak, Coronavirus disease 2019 (COVID-19), Severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2), New York, Psychological intervention, 03 medical and health sciences, 0302 clinical medicine, Environmental health, Influenza, Human, Humans, Medicine, 030212 general & internal medicine, Flu-like illness, epidemiological monitoring, Influenza-like illness, SARS-CoV-2, business.industry, Brief Report, virus diseases, COVID-19, Outbreak, 030208 emergency & critical care medicine, AcademicSubjects/MED00290, Infectious Diseases, New York City, Epidemiological Monitoring, influenza, Laboratories, business
Abstract: Innovative monitoring approaches are needed to track the coronavirus disease 2019 (COVID-19) epidemic and potentially assess the impact of community mitigation interventions. We present temporal data on influenza-like illness, influenza diagnosis, and COVID-19 cases for all 4 regions of New York State through the first 6 weeks of the outbreak.
Published: 2020

231. COVID-19 Testing, Epidemic Features, Hospital Outcomes, and Household Prevalence, New York State—March 2020

Author: Rosenberg, Eli S, Dufort, Elizabeth M, Blog, Debra S, Hall, Eric W, Hoefer, Dina, Backenson, Bryon P, Muse, Alison T, Kirkwood, James N, St. George, Kirsten, Holtgrave, David R, Hutton, Brad J, Zucker, Howard A, Anand, Madhu, Kaufman, Alison, Kuhles, Daniel, Maxted, Angie, Newman, Alexandra, Pulver, Wendy, Smith, Lou, Sommer, Jamie, White, Jennifer, Dean, Amy, Derbyshire, Victoria, Egan, Christina, Fuschino, Meghan, Griesemer, Sara, Hull, Rene, Lamson, Daryl, Laplante, Jennifer, McDonough, Kathleen, Mitchell, Kara, Musser, Kimberlee, Nazarian, Elizabeth, Popowich, Michael, Taylor, Jill, Walsh, Anne, Amler, Sherlita, Huang, Ada, Recchia, Renee, Whalen, Elizabeth, Lewis, Elizabeth, Friedman, Cynthia, Carrera, Sandra, Eisenstein, Lawrence, DeSimone, Ann, Morne, Johanne, Johnson, Megan, Navarette, Kristen, Kumar, Jessica, Ostrowski, Stephanie, Mazeau, Adrienne, Dreslin, Sally, Yates, Nora, Greene, Danielle, Heslin, Eugene, Lutterloh, Emily, Rosenthal, Elizabeth, and Barranco, Meredith
Subjects: Adult, Male, 0301 basic medicine, Microbiology (medical), medicine.medical_specialty, Adolescent, Coronavirus disease 2019 (COVID-19), Pneumonia, Viral, 030106 microbiology, New York, Young Adult, 03 medical and health sciences, Age Distribution, COVID-19 Testing, 0302 clinical medicine, Risk Factors, Epidemiology, Prevalence, medicine, Humans, 030212 general & internal medicine, Child, Pandemics, Aged, Estimation, Family Characteristics, Spatial Analysis, Clinical Laboratory Techniques, business.industry, Medical record, Infant, Newborn, COVID-19, Infant, Outbreak, Middle Aged, Metropolitan area, Hospitalization, Infectious Diseases, Hospital outcomes, Specimen collection, Child, Preschool, Female, Coronavirus Infections, business, Demography
Abstract: Background The US’ coronavirus disease 2019 (COVID-19) epidemic has grown extensively since February 2020, with substantial associated hospitalizations and mortality; New York State has emerged as the national epicenter. We report on the extent of testing and test results during the month of March in New York State, along with risk factors, outcomes, and household prevalence among initial cases subject to in-depth investigations. Methods Specimen collection for COVID-19 testing was conducted in healthcare settings, community-based collection sites, and by home testing teams. Information on demographics, risk factors, and hospital outcomes of cases was obtained through epidemiological investigations and an electronic medical records match, and summarized descriptively. Active testing of initial case’s households enabled estimation of household prevalence. Results During March in New York State, outside of New York City, a total of 47 326 persons tested positive for severe acute respiratory syndrome coronavirus 2, out of 141 495 tests (33% test-positive), with the highest number of cases located in the metropolitan region counties. Among 229 initial cases diagnosed through 12 March, by 30 March 13% were hospitalized and 2% died. Testing conducted among 498 members of these case’s households found prevalent infection among 57%, excluding first-reported cases 38%. In these homes, we found a significant age gradient in prevalence, from 23% among those Conclusions New York State faced a substantial and increasing COVID-19 outbreak during March 2020. The earliest cases had high levels of infection in their households and by the end of the month, the risks of hospitalization and death were high.
Published: 2020
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232. X-/γ-Ray Detection Instrument for the HERMES Nano-Satellites Based on SDDs Read-Out by the LYRA Mixed-Signal ASIC Chipset

Author: A. Rachevski, P. Bellutti, Francesco Ficorella, Piero Malcovati, Raffaele Piazzolla, F. Mele, M. Fiorini, Riccardo Campana, Miriam Grassi, Claudio Labanti, F. Fuschino, Nicola Zorzi, N. Zampa, Giuseppe Bertuccio, Marco Feroci, I. Rashevskaya, E. Demenev, A. Vacchi, G. Zampa, Giacomo Borghi, Y. Evangelista, Fabrizio Fiore, A. Picciotto, M. Gandola, and Luciano Burderi
Subjects: Interconnection, Silicon drift detector, Chipset, 010308 nuclear & particles physics, business.industry, Detector, Electrical engineering, 01 natural sciences, 030218 nuclear medicine & medical imaging, Power (physics), Section (fiber bundle), 03 medical and health sciences, 0302 clinical medicine, Application-specific integrated circuit, CMOS, 0103 physical sciences, Medicine, business
Abstract: This paper presents the front-end section of the X-/γ-ray detection instrument of the HERMES mission, whose goal is to observe and localize γ-ray bursts, through a constellation of more than one hundred nano-satellites. Considering the severe volume and power consumption constraints of the nano-satellites, in the HERMES X-/γ-ray detection instrument, silicon drift detectors are read out through a mixed-signal ASIC chipset, called LYRA, based on a peculiar architecture. In particular, a small front-end ASIC (LYRA-FE), placed close to each silicon drift detector, is connected, through a current-mode link, to a multi-channel back-end ASIC (LYRA-BE). The LYRA ASIC chipset, implemented in a 0.35µm CMOS technology, achieves less than $22{\text{e}}_{{\text{rms}}}^ - $ of equivalent noise charge, with a power consumption lower than 600µW/channel from a 3.3V power supply. Thanks to the current-mode link between the LYRA-FE and the LYRA-BE ASICs, no significant crosstalk among channels can be observed, in spite of the length of the interconnection wires as large as 12cm.
Published: 2020

233. An innovative architecture for a wide band transient monitor on board the HERMES nano-satellite constellation

Author: G. Dilillo, A. Rachevski, P. Bellutti, I. Rashevskaya, Francesco Ficorella, Y. Evangelista, G. Zampa, Yupeng Xu, Gianluca Morgante, Fabrizio Fiore, G. La Rosa, Giuseppe Bertuccio, G. Pauletta, P. Nogara, Piero Malcovati, Miriam Grassi, A. Vacchi, M. Feroci, F. Ceraudo, Raffaele Piazzolla, Claudio Labanti, M. Fiorini, E. Virgilli, T. Chen, Nicola Zorzi, Giacomo Borghi, N. Zampa, M. Gandola, F. Mele, Giuseppe Sottile, J. Cao, L. Wang, Filippo Ambrosino, N. Gao, E. Demenev, A. Picciotto, F. Fuschino, Riccardo Campana, ITA, DEU, and CHN
Subjects: Photon, Physics - Instrumentation and Detectors, Computer science, Physics::Instrumentation and Detectors, FOS: Physical sciences, Scintillator Detectors, Silicon Drift Detectors, 02 engineering and technology, Scintillator, 7. Clean energy, 01 natural sciences, 010309 optics, Application-specific integrated circuit, 0103 physical sciences, Electronic engineering, Sensitivity (control systems), Instrumentation and Methods for Astrophysics (astro-ph.IM), Constellation, High Energy Astrophysical Phenomena (astro-ph.HE), Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), 021001 nanoscience & nanotechnology, Nanosatellites, Gamma-ray Burst, Transient (oscillation), 0210 nano-technology, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Energy (signal processing)
Abstract: The HERMES-TP/SP mission, based on a nanosatellite constellation, has very stringent constraints of sensitivity and compactness, and requires an innovative wide energy range instrument. The instrument technology is based on the "siswich" concept, in which custom-designed, low-noise Silicon Drift Detectors are used to simultaneously detect soft X-rays and to readout the optical light produced by the interaction of higher energy photons in GAGG:Ce scintillators. To preserve the inherent excellent spectroscopic performances of SDDs, advanced readout electronics is necessary. In this paper, the HERMES detector architecture concept will be described in detail, as well as the specifically developed front-end ASICs (LYRA-FE and LYRA-BE) and integration solutions. The experimental performance of the integrated system composed by scintillator+SDD+LYRA ASIC will be discussed, demonstrating that the requirements of a wide energy range sensitivity, from 2 keV up to 2 MeV, are met in a compact instrument., Comment: 12 pages, 10 figures. Proceedings of SPIE "Astronomical Telescopes and Instrumentation" 2020
Published: 2020

234. The Payload Data Handling Unit (PDHU) on-board the HERMES-TP and HERMES-SP CubeSat Missions

Author: Raffaele Piazzolla, Andrea Colagrossi, Riccardo Campana, G. La Rosa, Andrea Santangelo, Jörg Bayer, Michele Fiorito, C. Tenzer, F. Fuschino, Francesco G. Russo, S. Pliego, S. Curzel, P. Nogara, Y. Evangelista, A. Guzman, Giuseppe Sottile, and Fabrizio Fiore
Subjects: On-board computer, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Field of view, 02 engineering and technology, 7. Clean energy, 01 natural sciences, 010309 optics, 0103 physical sciences, CubeSat, Aerospace engineering, Instrumentation and Methods for Astrophysics (astro-ph.IM), Constellation, Physics, business.industry, Payload, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, 021001 nanoscience & nanotechnology, Pathfinder, Satellite bus, Nanosatellites, Gamma Ray Bursts, Astrophysics - Instrumentation and Methods for Astrophysics, 0210 nano-technology, business, Gamma-ray burst
Abstract: The High Energy Rapid Modular Ensemble of Satellites (HERMES) Technological and Scientific pathfinder is a space borne mission based on a constellation of LEO nanosatellites. The payloads of these CubeSats consist of miniaturized detectors designed for bright high-energy transients such as Gamma-Ray Bursts (GRBs). This platform aims to impact Gamma Ray Burst (GRB) science and enhance the detection of Gravitational Wave (GW) electromagnetic counterparts. This goal will be achieved with a field of view of several steradians, arcmin precision and state of the art timing accuracy. The localization performance for the whole constellation is proportional to the number of components and inversely proportional to the average baseline between them, and therefore is expected to increase as more. In this paper we describe the Payload Data Handling Unit (PDHU) for the HERMES-TP and HERMES SP mission. The PDHU is the main interface between the payload and the satellite bus. The PDHU is also in charge of the on-board control and monitoring of the scintillating crystal detectors. We will explain the TM/TC design and the distinct modes of operation. We also discuss the on-board data processing carried out by the PDHU and its impact on the output data of the detector., Comment: 11 pages, 10 figures. Proceedings of SPIE "Astronomical Telescopes and Instrumentation" 2020
Published: 2020
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235. The XGIS instrument on-board THESEUS: the detection plane and on-board electronics

Author: Paolo Lorenzi, G. Zampa, Miriam Grassi, I. Rashevskaya, M. Winkler, Lorenzo Amati, Piero Malcovati, Lucas Christoffer Bune Jensen, P. Bellutti, Giacomo Borghi, Francesco Ficorella, Giuseppe Sottile, A. Picciotto, Alessandro Gemelli, F. Mele, E. Virgilli, Riccardo Campana, Søren Møller Pedersen, F. Fuschino, Ifran Kuvvetli, G. La Rosa, Piotr Orleanski, Claudio Labanti, Andrea Santangelo, Denis Tcherniak, Paul Hedderman, A. Rachevski, Luca Terenzi, C. Tenzer, A. Vacchi, M. Gandola, Nicola Zorzi, Paolo Sarra, N. Zampa, Giuseppe Bertuccio, A. den Herder, Jan-Willem, Nikzad, Shouleh, and Nakazawa, Kazuhiro
Subjects: Scintillation, Cosmic Vision, Spectrometer, Physics::Instrumentation and Detectors, business.industry, Computer science, ASIC, Detector, Electrical engineering, FOS: Physical sciences, Photodetector, Chipset, Integrated circuit, law.invention, ORION, law, Scintillator crystals, Silicon Drift Detector, THESEUS mission, Redundancy (engineering), Electronics, Astrophysics - Instrumentation and Methods for Astrophysics, business, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract: The X and Gamma Imaging Spectrometer instrument on-board the THESEUS mission (selected by ESA in the framework of the Cosmic Vision M5 launch opportunity, currently in phase A) is based on a detection plane composed of several thousands of single active elements. Each element comprises a 4.5x4.5x30 mm 3 CsI(Tl) scintillator bar, optically coupled at both ends to Silicon Drift Detectors (SDDs). The SDDs acts both as photodetectors for the scintillation light and as direct X-ray sensors. In this paper the design of the XGIS detection plane is reviewed, outlining the strategic choices in terms of modularity and redundancy of the system. Results on detector-electronics prototypes are also described. Moreover, the design and development of the low-noise front-end electronics is presented, emphasizing the innovative architectural design based on custom-designed Application-Specific Integrated Circuits (ASICs)., Comment: Proceedings of the SPIE 2020, paper 11444-277
Published: 2020

236. The XGIS instrument on-board THESEUS: Monte Carlo simulations for response, background, and sensitivity

Author: Valentina Fioretti, Enrico Virgilli, Riccardo Campana, Mauro Orlandini, F. Fuschino, John B. Stephen, Claudio Labanti, Sandro Mereghetti, Lorenzo Amati, and ITA
Subjects: Physics, Photon, Cosmic Vision, Spectrometer, business.industry, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Albedo, Universe, Sky, Physics::Space Physics, Transient (oscillation), Astrophysics::Earth and Planetary Astrophysics, Aerospace engineering, business, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), media_common
Abstract: The response of the X and Gamma Imaging Spectrometer (XGIS) instrument onboard the Transient High Energy Sky and Early Universe Surveyor (THESEUS) mission, selected by ESA for an assessment phase in the framework of the Cosmic Vision M5 launch opportunity, has been extensively modeled with a Monte Carlo Geant-4 based software. In this paper, the expected sources of background in the Low Earth Orbit foreseen for THESEUS are described (e.g. diffuse photon backgrounds, cosmic-ray populations, Earth albedo emission) and the simulated on-board background environment and its effects on the instrumental performance is shown., Proceedings of the SPIE 2020, paper 11444-275. arXiv admin note: text overlap with arXiv:2101.03017
Published: 2020

237. The XGIS imaging system on board the THESEUS mission

Author: Lorenzo Amati, F. Fuschino, F. Evangelisti, Sandro Mereghetti, Luca Terenzi, M. D. Caballero-Garcia, Riccardo Campana, J. L. Gasent-Blesa, Victor Reglero, Pedro Rodríguez-Martínez, Mauro Orlandini, A. de Rosa, Filippo Frontera, J. Navarro-González, John B. Stephen, S. Squerzanti, Claudio Labanti, M. Melchiorri, P. Connell, Benjamin Pinazo-Herrero, A. J. Castro-Tirado, Gianluca Morgante, Istituto Nazionale di Astrofisica, European Space Agency, European Commission, Ministerio de Ciencia e Innovación (España), National Science Centre (Poland), and Foundation for Polish Science
Subjects: 010504 meteorology & atmospheric sciences, Computer science, Imaging techniques, X-ray transients, 01 natural sciences, Multiplexing, law.invention, X-ray astronomy, law, 0103 physical sciences, International Space Station, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, COSMIC cancer database, business.industry, Detector, Collimator, Upgrade, Signal multiplexing, Electromagnetic shielding, Gamma-ray bursts, Coded mask, business, Computer hardware
Abstract: Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray; Virtual, Online; United States; 14 December 2020 through 18 December 2020; Code 166330.--Proceedings of SPIE - The International Society for Optical Engineering Volume 11444, 2020, Article number 114448S.--Full list of authors: Gasent-Blesa, J. L.; Reglero, V.; Connell, P.; Pinazo-Herrero, B.; Navarro-González, J.; Rodríguez-Martínez, P.; Castro-Tirado, A. J.; Caballero-García, M. D.; Amati, L.; Labanti, C.; Mereghetti, S.; Frontera, F.; Campana, R.; Orlandini, M.; Stephen, J.; Terenzi, L.; Evangelisti, F.; Squerzanti, S.; Melchiorri, M.; Fuschino, F. De Rosa, A.; Morgante, G., Within the scientific goals of the THESEUS ESA/M5 candidate mission, a critical item is a fast (within a few s) and accurate (, THESEUS/XGIS instrument is supported by: the ASI-INAF Agreement n. 2018-29-HH.0; the OHB Italia/INAF-OASBo Agreement n.2331/2020/01; the European Space Agency ESA through the M5/NPMC Programme; the AHEAD2020 project funded by the UE through H2020-INFRAIA-2018-2020; the Spanish Ministerio de Ciencia e Innovaci?n, PID2019 109269RB-C41; the Polish National Science Centre, Project 2019/35/B/ST9/03944 and Foundation for Polish Science, Project POIR.04.04.00-00-5C65/17-00. The authors thank all the members of the THESEUS team involved in the development of XGIS instrument.
Published: 2020

238. Evidence that accumulation of mutants in a biofilm reflects natural selection rather than stress-induced adaptive mutation

Author: Banas, Jeffrey A., Miller, Justin D., Fuschino, Meghan E., Hazlett, Karsten R.O., Toyofuku, Wendy, Porter, Kristen A., Reutzel, Sarah B., Florczyk, Matthew A., McDonough, Kathleen A., and Michalek, Suzanne M.
Subjects: Microbial mats -- Research, Streptococcus mutans -- Research, Virulence (Microbiology) -- Research, Biological sciences
Abstract: The deletion mutants of dental pathogen Streptococcus mutants were studied for the virulence. The accumulation of the virulent strains in the biofilm was quantitatively determined to be occurring due to natural selection.
Published: 2007

239. The X/Gamma-ray Imaging Spectrometer (XGIS) on-board THESEUS: design, main characteristics, and concept of operation

Author: Herder, Jan-Willem A. den, Nikzad, Shouleh, Nakazawa, Kazuhiro, Labanti, C., Amati, L., Frontera, F., Mereghetti, S., Gasent-Blesa, J. L., Tenzer, C., Orleanski, P., Kuvvetli, I., Campana, R., Fuschino, F., Terenzi, L., Virgilli, E., Morgante, G., Orlandini, M., Butler, R. C., Stephen, J. B., Auricchio, N., Rosa, A. De, Ronco, V. Da, Evangelisti, F., Melchiorri, M., Squerzanti, S., Fiorini, M., Bertuccio, G., Mele, F., Gandola, M., Malcovati, P., Grassi, M., Bellutti, P., Borghi, G., Ficorella, F., Picciotto, A., Zanini, V., Zorzi, N., Demenev, E., Rashevskaya, I., Rachevski, A., Zampa, G., Vacchi, A., Zampa, N., Baldazzi, G., Rosa, G. La, Sottile, G., Volpe, A., Winkler, M., Reglero, V., Connell, P. H., Pinazo-Herrero, B., Navarro-González, J., Rodríguez-Martínez, P., Castro-Tirado, A. J., Santangelo, A., Hedderman, P., Lorenzi, P., Sarra, P., Pedersen, S. M., Tcherniak, D., Guidorzi, C., Rosati, P., Trois, A., Piazzolla, R., Herder, Jan-Willem A. den, Nikzad, Shouleh, Nakazawa, Kazuhiro, Labanti, C., Amati, L., Frontera, F., Mereghetti, S., Gasent-Blesa, J. L., Tenzer, C., Orleanski, P., Kuvvetli, I., Campana, R., Fuschino, F., Terenzi, L., Virgilli, E., Morgante, G., Orlandini, M., Butler, R. C., Stephen, J. B., Auricchio, N., Rosa, A. De, Ronco, V. Da, Evangelisti, F., Melchiorri, M., Squerzanti, S., Fiorini, M., Bertuccio, G., Mele, F., Gandola, M., Malcovati, P., Grassi, M., Bellutti, P., Borghi, G., Ficorella, F., Picciotto, A., Zanini, V., Zorzi, N., Demenev, E., Rashevskaya, I., Rachevski, A., Zampa, G., Vacchi, A., Zampa, N., Baldazzi, G., Rosa, G. La, Sottile, G., Volpe, A., Winkler, M., Reglero, V., Connell, P. H., Pinazo-Herrero, B., Navarro-González, J., Rodríguez-Martínez, P., Castro-Tirado, A. J., Santangelo, A., Hedderman, P., Lorenzi, P., Sarra, P., Pedersen, S. M., Tcherniak, D., Guidorzi, C., Rosati, P., Trois, A., and Piazzolla, R.
Abstract: THESEUS (Transient High Energy Sky and Early Universe Surveyor) is one of the three missions selected by ESA as fifth medium class mission (M5) candidates in its Cosmic Vision science program, currently under assessment in a phase A study with a planned launch date in 2032. THESEUS is designed to carry on-board two wide and deep sky monitoring instruments for X/gamma-ray transients detection: a wide-field soft X-ray monitor with imaging capability (Soft X-ray Imager, SXI, 0.3 – 5 keV), a hard X-ray, partially-imaging spectroscopic instrument (X and Gamma Imaging Spectrometer, XGIS, 2 keV – 10 MeV), and an optical/near-IR telescope with both imaging and spectroscopic capability (InfraRed Telescope, IRT, 0.7 – 1.8 μm). The spacecraft will be capable of performing fast repointing of the IRT to the error region provided by the monitors, thus allowing it to detect and localize the transient sources down to a few arcsec accuracy, for immediate identification and redshift determination. The prime goal of the XGIS will be to detect transient sources, with monitoring timescales down to milliseconds, both independently of, or following up, SXI detections, and identify the sources performing localisation at <15 arcmin and characterize them over a broad energy band, thus providing also unique clues to their emission physics. The XGIS system consists of two independent but identical coded mask cameras, arranged to cover 2 steradians. The XGIS will exploit an innovative technology coupling Silicon Drift Detectors (SDD) with crystal scintillator bars and a very low-noise distributed front-end electronics (ORION ASICs), which will produce a position sensitive detection plane, with a large effective area over a huge energy band (from soft X-rays to soft gamma-rays) with timing resolution down to a few µs. Here is presented an overview of the XGIS instrument design, its configuration, and capabilities.
Published: 2020

240. The XGIS instrument on-board THESEUS: The detection plane and on-board electronics

Author: A. den Herder, Jan-Willem, Nikzad, Shouleh, Nakazawa, Kazuhiro, Fuschino, F., Campana, R., Labanti, C., Amati, L., Virgilli, E., Terenzi, L., Bellutti, P., Bertuccio, G., Borghi, G., Bune Jensen, L. C., Ficorella, F., Gandola, M., Gemelli, A., Grassi, M., Hedderman, P., Kuvvetli, I., la Rosa, G., Lorenzi, P., Malcovati, P., Mele, F., Orleanski, P., Pedersen, M., Picciotto, A., Rachevski, A., Rashevskaya, I., Santangelo, A., Sarra, P., Sottile, G., Tcherniak, D., Tenzer, C., Vacchi, A., Winkler, M., Zampa, G., Zampa, N., Zorzi, N., A. den Herder, Jan-Willem, Nikzad, Shouleh, Nakazawa, Kazuhiro, Fuschino, F., Campana, R., Labanti, C., Amati, L., Virgilli, E., Terenzi, L., Bellutti, P., Bertuccio, G., Borghi, G., Bune Jensen, L. C., Ficorella, F., Gandola, M., Gemelli, A., Grassi, M., Hedderman, P., Kuvvetli, I., la Rosa, G., Lorenzi, P., Malcovati, P., Mele, F., Orleanski, P., Pedersen, M., Picciotto, A., Rachevski, A., Rashevskaya, I., Santangelo, A., Sarra, P., Sottile, G., Tcherniak, D., Tenzer, C., Vacchi, A., Winkler, M., Zampa, G., Zampa, N., and Zorzi, N.
Abstract: The X and Gamma Imaging Spectrometer instrument on-board the THESEUS mission (selected by ESA in the framework of the Cosmic Vision M5 launch opportunity, currently in phase A) is based on a detection plane composed of several thousands of single active elements. Each element comprises a 4.5×4.5×30 mm3 CsI(Tl) scintillator bar, optically coupled at both ends to Silicon Drift Detectors (SDDs). The SDDs acts both as photodetectors for the scintillation light and as direct X-ray sensors. In this paper the design of the XGIS detection plane is reviewed, outlining the strategic choices in terms of modularity and redundancy of the system. Results on detector-electronics prototypes are also described. Moreover, the design and development of the low-noise front-end electronics is presented, emphasizing the innovative architectural design based on custom-designed Application-Specific Integrated Circuits (ASICs).
Published: 2020

241. Azacytidine Treatment in Patients with Acute Myeloid Leukemia/High-Risk Myelodysplastic Syndrome: Day-Hospital Management Compared to Home Care Setting

Author: Roberto Latagliata, Loredana Bassi, Monica Poscente, Silvia Ciambella, Giulio Trapè, Michela Tarnani, Michela Fuschino, Raffaella Isidori, Silvia Bertelli, Cristina Mastino, Giuseppe Topini, Valentina Panichi, Roberta Talucci, Cinzia De Gregoris, Alessandra Crocicchia, Gloria Pessina, Vincenza Innocenti, Gioia De Angelis, Elisa Emanueli Cippitelli, Ambra Di Veroli, Marco Montanaro, Marco Morucci, Raffaella Randi, Giulia Pezzuti, and Annalisa Lippi
Subjects: Care setting, medicine.medical_specialty, business.industry, Internal medicine, Immunology, Myeloid leukemia, Medicine, In patient, Day hospital, Cell Biology, Hematology, business, Biochemistry
Abstract: Introduction Treatment with Hypometilating Agents (HMA) of unfit patients (pts) with Acute Myelogenous Leukemia (AML) and High-Risk Myelodysplastic Syndromes (HR-MDS) is often difficult in the standard Day-Hospital (DH) setting, due to the number of hospital admissions required and the frail clinical conditions of pts. In the Viterbo province, accounting for 3612 Km 2 divided into 60 municipalities, is operative an Unit of Domiciliary Hematologic Care (UDHC) for clinical assistance to frail pts with hemopathies. Aims To evaluate the role of the UDHC compared to standard DH setting in the active frontline treatment with HMA +/- venetoclax (VTX) of pts with AML/HR-MDS. Methods All pts with newly diagnosed AML/HR-MDS unfit for intensive care and treated frontline with HMA from 1/2010 to 4/2021 were analysed. Results In this study period, 112 pts (62 AML/50 HR-MDS) received HMA (azacytidine in 105 cases and decitabine in 7 cases): six pts added VTX to HMA. As concern therapy management, 69 pts (61.6%) were treated in a standard DH setting and 43 (38.4%) were followed by UDHC: pts were allocated to DH or home care setting by responsible physician based on clinical conditions, comorbidities, caregiver availability and distance from hospital. The main features at baseline of HMA in the whole cohort and according to management are reported in the Table 1. Median interval from diagnosis to HMA initiation was 0.9 months (IQR 0.5 - 3.0). Median number of HMA cycles administered was 9 (IQR 4 - 16). The overall response rate (ORR), including complete response, partial response and hematologic improvement, was 43.7% (48/112 pts) in the whole cohort, without differences according to management [29/69 (42.0%) in DH vs 19/43 (44.1%) in home care, p=0.797]. Infections were also equally reported [46/69 pts (66.6%) in DH vs 31/43 (72.0%) in home care setting had at least 1 infection, p=0.362]. Median response duration of the whole cohort was 10.0 months (95%CI 5.7 - 14.2), without differences according to management [8.7 months (95%CI 7.0 - 10.3) in DH vs 13.0 months (95%CI 8.3 - 17.6) in home care, p=0.460]. Median Overall Survival (OS) of the whole cohort was 13.0 months (95%CI 9.7 - 16.2): median OS of pts treated in DH was 13.7 months (95%CI 9.9 - 17.4) compared to 13.0 months (95%CI 6.7 - 19.3) of pts managed by UDHC (p=0.753) (Figure 1). Conclusions Home care management of HMA for unfit AML/HR-MDS pts is feasible and effective, with results similar to those achievable in a standard DH setting: this approach is thus adequate to offer active therapies in a fraction of frail pts with AML/HR-MDS considered up to now ineligible. Figure 1 Figure 1. Disclosures Latagliata: Novartis: Honoraria; Pfizer: Honoraria; BMS Cellgene: Honoraria.
Published: 2021

242. GrailQuest and HERMES: hunting for gravitational wave electromagnetic counterparts and probing space-time quantum foam

Author: Burderi, Luciano, primary, Di Salvo, Tiziana, additional, Riggio, Alessandro, additional, Gambino, Angelo Francesco, additional, Sanna, Andrea, additional, Fiore, Fabrizio, additional, Amarilli, Fabrizio, additional, Amati, Lorenzo, additional, Ambrosino, Filippo, additional, Amelino-Camelia, Giovanni, additional, Anitra, Alessio, additional, Barbera, Marco, additional, Bechini, Michele, additional, Bellutti, Paolo, additional, Bertaccin, Roberto, additional, Bertuccio, Giuseppe, additional, Campana, Riccardo, additional, Cao, Jiewei, additional, Capozziello, Salvatore, additional, Ceraudo, Francesco, additional, Chen, Tianxiang, additional, Cinelli, Marco, additional, Citossi, Marco, additional, Clerici, Aurora, additional, Colagrossi, Andrea, additional, Costa, Enrico, additional, Curzel, Serena, additional, De Laurentis, Mariafelicia, additional, Della Casa, Giovanni, additional, Della Valle, Massimo, additional, Demenev, Evgeny, additional, Del Santo, Melania, additional, Dilillo, Giuseppe, additional, Efremov, Pavel, additional, Evangelista, Yuri, additional, Feroci, Marco, additional, Ferruglio, Chiara, additional, Ferrandi, Fabrizio, additional, Fiorini, Mauro, additional, Fiorito, Michele, additional, Frontera, Filippo, additional, Fuschino, Fabio, additional, Gacnik, Dejan, additional, Galgoczi, Gabor, additional, Gao, Na, additional, Gandola, Massimo, additional, Ghirlanda, Giancarlo, additional, Gamboc, Andreja, additional, Grassi, Marco, additional, Guidorzi, Cristiano, additional, Guzman, Alejandro, additional, Iaria, Rosario, additional, Karlica, Mile, additional, Kostic, Uros, additional, Labanti, Claudio, additional, La Rosa, Giovanni, additional, Lo Cicero, Ugo, additional, Lopez Fernandez, Borja, additional, Lunghi, Paolo, additional, Malcovati, Piero, additional, Maselli, Alessandro, additional, Manca, Arianna, additional, Mele, Filippo, additional, Milankovich, Dorottya, additional, Monge, Angel, additional, Morgante, Gianluca, additional, Nava, Lara, additional, Negri, Barbara, additional, Nogara, Paolo, additional, Ohno, Masanori, additional, Ottolina, Daniele, additional, Pasquale, Andrea, additional, Pal, Andras, additional, Perri, Matteo, additional, Piccinin, Margherita, additional, Piazzolla, Raffaele, additional, Pirrotta, Simone, additional, Pliego-Caballero, Samuel, additional, Prinetto, Jacopo, additional, Pucacco, Giuseppe, additional, Puccetti, Simonetta, additional, Rapisarda, Massimo, additional, Rashevskaya, Irina, additional, Rashevsky, Alexander, additional, Ripa, Jakub, additional, Russo, Francesco, additional, Papitto, Alessandro, additional, Piranomonte, Silvia, additional, Santangelo, Andrea, additional, Scala, Francesca, additional, Sciarrone, Giulia, additional, Selcan, David, additional, Silvestrini, Stefano, additional, Sottile, Giuseppe, additional, Rotovnik, Tomaz, additional, Tenzer, Christoph, additional, Troisi, Ivan, additional, Vacchi, Andrea, additional, Virgilli, Enrico, additional, Werner, Norbert, additional, Wang, Lingjun, additional, Xu, Yupeng, additional, Zampa, Gianluigi, additional, Zampa, Nicola, additional, Zane, Silvia, additional, and Zanotti, Giovanni, additional
Published: 2021
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243. Time Evolution of TGF-Producing Storms Using ERA5, GPS and Geostationary Satellites Observations

Author: Tiberia, Alessandra, primary, Mascitelli, A., additional, D’Adderio, Leo Pio, additional, Federico, Stefano, additional, Marisaldi, Martino, additional, Porcù, Federico, additional, Realini, Eugenio, additional, Gatti, Andrea, additional, Ursi, Alessandro, additional, Fuschino, Fabio, additional, Tavani, Marco, additional, and Dietrich, Stefano, additional
Published: 2020
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244. Timing techniques applied to distributed modular high-energy astronomy: the H.E.R.M.E.S. project

Author: Sanna, Andrea, primary, Burderi, Luciano, additional, Di Salvo, Tiziana, additional, Fiore, Fabrizio, additional, Riggio, Alessandro, additional, Gambino, Angelo, additional, Lavagna, Michèle, additional, Bertacin, Roberto, additional, Evangelista, Yuri, additional, Campana, Riccardo, additional, Fuschino, Fabio, additional, Lunghi, Paolo, additional, Monge, Ángel, additional, Negri, Barbara, additional, Pirrotta, Simone, additional, Puccetti, Simonetta, additional, Amarilli, Fabrizio, additional, Ambrosino, Filippo, additional, Amelino-Camelia, Giavanni, additional, Anitra, Alessio, additional, Barbera, Marco, additional, Bechini, Michele, additional, Bellutti, Paolo, additional, Bertuccio, Giuseppe, additional, Cao, Jiewei, additional, Ceraudo, Francesco, additional, Chen, Tianxiang, additional, Cinelli, Matteo, additional, Citossi, Marco, additional, Clerici, Aurora, additional, Colagrossi, Andrea, additional, Curzel, Serena, additional, Della Casa, Giovanni, additional, Demenev, Evgeny, additional, Del Santo, Melania, additional, Dilillo, Giuseppe, additional, Efremov, Pavel, additional, Feroci, Marco, additional, Feruglio, Chiara, additional, Ferrandi, Fabrizio, additional, Fiorini, Mauro, additional, Fiorito, Michele, additional, Gacnik, Dejan, additional, Galgoczi, Gabor, additional, Gao, Na, additional, Gandola, Massimo, additional, Ghirlanda, Giancarlo, additional, Gamboc, Andreja, additional, Grassi, Marco, additional, Guidorzi, Cristiano, additional, Guzman, Alejandro, additional, Iaria, Rosario, additional, Karlica, Mile, additional, Kostic, Uros, additional, Labanti, Claudio, additional, La Rosa, Giovanni, additional, Lo Cicero, Ugo, additional, Loper Fernandez, Borja, additional, Malcovati, Piero, additional, Maselli, Alessandro, additional, Manca, Arianna, additional, Mele, Filippo, additional, Milankovich, Dorottya, additional, Morgante, Gianluca, additional, Nava, Lara, additional, Nogara, Paolo, additional, Ohno, Masanori, additional, Ottolina, Daniele, additional, Pasquale, Andrea, additional, Pal, Andras, additional, Perri, Matteo, additional, Piccinin, Margherita, additional, Piazzolla, Raffaele, additional, Pliego-Caballero, Samuel, additional, Prinetto, Jacopo, additional, Pucacco, Giuseppe, additional, Rashevskaya, Irina, additional, Rashevsky, Alexander, additional, Ripa, Jakub, additional, Russo, Francesco, additional, Papitto, Alessandro, additional, Piranamonte, Silvia, additional, Santangelo, Andrea, additional, Scala, Francesca, additional, Sciarrone, Giulia, additional, Selcan, David, additional, Silvestrini, Stefano, additional, Sottile, Giuseppe, additional, Rotovnik, Tomaz, additional, Tenzer, Christoph, additional, Troisi, Ivan, additional, Vacchi, Andrea, additional, Virgili, Enrico, additional, Werner, Norbert, additional, Wang, Lingjun, additional, Xu, Yupeng, additional, Zampa, Gianluigi, additional, Zampa, Nicola, additional, and Zanotti, Giovanni, additional
Published: 2020
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245. The X/Gamma-ray Imaging Spectrometer (XGIS) on-board THESEUS: design, main characteristics, and concept of operation

Author: Labanti, Claudio, primary, Amati, Lorenzo, additional, Frontera, Filippo, additional, Mereghetti, Sandro, additional, Gasent-Blesa, José Luis, additional, Tenzer, Christoph, additional, Orleanski, Piotr, additional, Kuvvetli, Irfan, additional, Campana, Riccardo, additional, Fuschino, Fabio, additional, Terenzi, Luca, additional, Virgilli, Enrico, additional, Morgante, Gianluca, additional, Orlandini, Mauro, additional, Butler, Reginald C., additional, Stephen, John B., additional, Auricchio, Natalia, additional, De Rosa, Adriano, additional, Da Ronco, Vanni, additional, Evangelisti, Federico, additional, Melchiorri, Michele, additional, Squerzanti, Stefano, additional, Fiorini, Mauro, additional, Bertuccio, Giuseppe, additional, Mele, Filippo, additional, Gandola, Massimo, additional, Malcovati, Piero, additional, Grassi, Marco, additional, Bellutti, Pierluigi, additional, Borghi, Giacomo, additional, Ficorella, Francesco, additional, Picciotto, Antonino, additional, Zanini, Vittorio, additional, Zorzi, Nicola, additional, Demenev, Evgeny, additional, Rashevskaya, Irina, additional, Rachevski, Alexander, additional, Zampa, Gianluigi, additional, Vacchi, Andrea, additional, Zampa, Nicola, additional, Baldazzi, Giuseppe, additional, La Rosa, Giovanni, additional, Sottile, Giuseppe, additional, Volpe, Angela, additional, Winkler, Marek, additional, Reglero, Victor, additional, Connell, Paul H., additional, Pinazo-Herrero, Benjamin, additional, Navarro-González, Javier, additional, Rodríguez-Martínez, Pedro, additional, Castro-Tirado, Alberto J., additional, Santangelo, Andrea, additional, Hedderman, Paul, additional, Lorenzi, Paolo, additional, Sarra, Paolo, additional, Pedersen, Søren M., additional, Tcherniak, Denis, additional, Guidorzi, Cristiano, additional, Rosati, Piero, additional, Trois, Alessio, additional, and Piazzolla, Raffaele, additional
Published: 2020
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246. The scientific payload on-board the HERMES-TP and HERMES-SP CubeSat missions

Author: Evangelista, Yuri, primary, Fiore, Fabrizio, additional, Fuschino, Fabio, additional, Campana, Riccardo, additional, Ceraudo, Francesco, additional, Demenev, Evgeny, additional, Guzman, Alejandro, additional, Labanti, Claudio, additional, La Rosa, Giovanni, additional, Fiorini, Mauro, additional, Gandola, Massimo, additional, Grassi, Marco, additional, Mele, Filippo, additional, Morgante, Gianluca, additional, Nogara, Paolo, additional, Piazzolla, Raffaele, additional, Pliego Caballero, Samuel, additional, Rashevskaya, Irina, additional, Russo, Francesco, additional, Sciarrone, Giulia, additional, Sottile, Giuseppe, additional, Milankovich, Dorottya, additional, Pál, András, additional, Ambrosino, Filippo, additional, Auricchio, Natalia, additional, Barbera, Marco, additional, Bellutti, Pierluigi, additional, Bertuccio, Giuseppe, additional, Borghi, Giacomo, additional, Cao, Jiewei, additional, Chen, Tianxiang, additional, Dilillo, Giuseppe, additional, Feroci, Marco, additional, Ficorella, Francesco, additional, Lo Cicero, Ugo, additional, Malcovati, Piero, additional, Morbidini, Alfredo, additional, Pauletta, Giovanni, additional, Picciotto, Antonino, additional, Rachevski, Alexandre, additional, Santangelo, Andrea, additional, Tenzer, Chistoph, additional, Vacchi, Andrea, additional, Wang, Lingjun, additional, Xu, Yupeng, additional, Zampa, Gianluigi, additional, Zampa, Nicola, additional, Zorzi, Nicola, additional, Burderi, Luciano, additional, Lavagna, Michèle, additional, Bertacin, Roberto, additional, Lunghi, Paolo, additional, Monge, Angel, additional, Negri, Barbara, additional, Pirrotta, Simone, additional, Puccetti, Simonetta, additional, Sanna, Andrea, additional, Amarilli, Fabrizio, additional, Amelino-Camelia, Giovanni, additional, Bechini, Michele, additional, Citossi, Marco, additional, Colagrossi, Andrea, additional, Curzel, Serena, additional, Della Casa, Giovanni, additional, Cinelli, Marco, additional, Del Santo, Melania, additional, Di Salvo, Tiziana, additional, Feruglio, Chiara, additional, Ferrandi, Fabrizio, additional, Fiorito, Michele, additional, Gacnik, Dejan, additional, Galgóczi, Gabor, additional, Gambino, Angelo Francesco, additional, Ghirlanda, Giancarlo, additional, Gomboc, Andreja, additional, Karlica, Mile, additional, Efremov, Pavel, additional, Kostic, Uros, additional, Clerici, Aurora, additional, Lopez Fernandez, Borja, additional, Maselli, Alessandro, additional, Nava, Lara, additional, Ohno, Masanori, additional, Ottolina, Daniele, additional, Pasquale, Andrea, additional, Perri, Matteo, additional, Piccinin, Margherita, additional, Prinetto, Jacopo, additional, Riggio, Alessandro, additional, Ripa, Jakub, additional, Papitto, Alessandro, additional, Piranomonte, Silvia, additional, Scala, Francesca, additional, Selcan, David, additional, Silvestrini, Stefano, additional, Rotovnik, Tomaz, additional, Virgilli, Enrico, additional, Troisi, Ivan, additional, Werner, Norbert, additional, Zanotti, Giovanni, additional, Anitra, Alessio, additional, and Manca, Arianna, additional
Published: 2020
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247. Scientific simulations and optimization of the XGIS instrument on board THESEUS

Author: Mereghetti, Sandro, primary, Ghirlanda, Giancarlo, additional, Salvaterra, Ruben, additional, Campana, Riccardo, additional, Labanti, Claudio, additional, Connell, Paul H., additional, Farinelli, Ruben, additional, Frontera, Filippo, additional, Fuschino, Fabio, additional, Gasent-Blesa, Jose L., additional, Guidorzi, Cristiano, additional, Lissoni, Michele, additional, Rigoselli, Michela, additional, Stephen, John B., additional, and Amati, Lorenzo, additional
Published: 2020
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248. The XGIS imaging system on board the Theseus mission

Author: Gasent-Blesa, José Luis, primary, Reglero, Víctor, additional, Connell, Paul, additional, Pinazo-Herrero, Benjamín, additional, Navarro-González, Javier, additional, Rodríguez-Martínez, Pedro, additional, Castro-Tirado, Alberto J., additional, Caballero-García, María Dolores, additional, Amati, Lorenzo, additional, Labanti, Claudio, additional, Mereghetti, Sandro, additional, Frontera, Filippo, additional, Campana, Riccardo, additional, Orlandini, Mauro, additional, Stephen, John, additional, Terenzi, Luca, additional, Evangelisti, Federico, additional, Squerzanti, Stefano, additional, Melchiorri, Michele, additional, Fuschino, Fabio, additional, De Rosa, Adriano, additional, and Morgante, Gianluca, additional
Published: 2020
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249. The Payload Data Handling Unit (PDHU) on-board the HERMES-TP and HERMES-SP CubeSat Missions

Author: Guzman Cabrera, Alejandro, primary, Pliego-Caballero, Samuel, additional, Bayer, Joerg, additional, Evangelista, Yuri, additional, La Rosa, Giovanni, additional, Sottile, Giuseppe, additional, Curzel, Serena, additional, Campana, Riccardo, additional, Fiore, Fabrizio, additional, Fuschino, Fabio, additional, Colagrossi, Andrea, additional, Fiorito, Michele, additional, Nogara, Paolo, additional, Piazzolla, Raffaele, additional, Russo, Francesco, additional, Santangelo, Andrea, additional, and Tenzer, Jan Christoph, additional
Published: 2020
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250. The XGIS instrument on-board THESEUS: Monte Carlo simulations for response, background, and sensitivity

Author: Campana, Riccardo, primary, Fuschino, Fabio, additional, Labanti, Claudio, additional, Mereghetti, Sandro, additional, Virgilli, Enrico, additional, Fioretti, Valentina, additional, Orlandini, Mauro, additional, Stephen, John B., additional, and Amati, Lorenzo, additional
Published: 2020
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