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21 results on '"burst [gamma ray]"'

1. Multicollision Internal Shock Lepto-hadronic Models for Energetic Gamma-Ray Bursts (GRBs)

Author: Rudolph, Annika, Petropoulou, Maria, Bošnjak, Željka, and Winter, Walter
Subjects: UHE [cosmic radiation], burst [gamma ray], spectrum [neutrino], feedback, dissipation, spectrum [photon], GeV, X-ray, cosmic radiation [p], electromagnetic, synchrotron, flux [energy], ddc:520, TeV, time dependence, signature
Abstract: For a subpopulation of energetic gamma-ray bursts (GRBs), a moderate baryonic loading may suffice to power ultra-high-energy cosmic rays (UHECRs). Motivated by this, we study the radiative signatures of cosmic-ray protons in the prompt phase of energetic GRBs. Our framework is the internal shock model with multicollision descriptions of the relativistic ejecta (with different emission regions along the jet), plus time-dependent calculations of photon and neutrino spectra. Our GRB prototypes are motivated by Fermi-Large Area Telescope-detected GRBs (including GRB 221009A) for which further, owing to the large energy flux, neutrino nonobservation of single events may pose a strong limit on the baryonic loading. We study the feedback of protons on electromagnetic spectra in synchrotron- and inverse Compton-dominated scenarios to identify the multiwavelength signatures, to constrain the maximally allowed baryonic loading, and to point out the differences between hadronic and inverse Compton signatures. We find that hadronic signatures appear as correlated flux increases in the optical-UV to soft X-ray and GeV–TeV gamma-ray ranges in the synchrotron scenarios, whereas they are difficult to identify in inverse Compton-dominated scenarios. We demonstrate that baryonic loadings around 10, which satisfy the UHECR energetic requirements, do not distort the predicted photon spectra in the Fermi Gamma-Ray Burst Monitor range and are consistent with constraints from neutrino data if the collision radii are large enough (i.e., the time variability is not too short). It therefore seems plausible that under the condition of large dissipation radii a population of energetic GRBs can be the origin of the UHECRs.
Published: 2023
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2. Multi-messenger Model for the Prompt Emission from GRB 221009A

Author: Annika Rudolph, Maria Petropoulou, Walter Winter, and Željka Bošnjak
Subjects: electron, velocity, UHE [cosmic radiation], burst [gamma ray], FOS: Physical sciences, feedback, gamma ray: burst, jet: relativistic, neutrino, muon, synchrotron, cosmic radiation: UHE, enhancement, High Energy Astrophysical Phenomena (astro-ph.HE), background, photon, gravitational radiation, Astronomy and Astrophysics, dissipation, UHE [p], relativistic [jet], flux, p: UHE, electromagnetic, Space and Planetary Science, ddc:520, spectral, time dependence, Astrophysics - High Energy Astrophysical Phenomena, signature, Lorentz, ejection
Abstract: The astrophysical journal / 2 944(2), L34 (2023). doi:10.3847/2041-8213/acb6d7, We present a multi-messenger model for the prompt emission from GRB 221009A within the internal shock scenario. We consider the time-dependent evolution of the outflow with its impact on the observed light curve from multiple collisions, as well as the self-consistent generation of the electromagnetic spectrum in synchrotron and inverse Compton-dominated scenarios. Our lepto-hadronic model includes UHE protons potentially accelerated in the outflow, and their feedback on spectral energy distribution and on the neutrino emission. We find that we can roughly reproduce the observed light curves with an engine with varying ejection velocity of ultrarelativistic material, which has an intermediate quiescent period of about 200 s and a variability timescale of ∼1 s. We consider baryonic loadings of 3 and 30 that are compatible with the hypothesis that the highest-energetic LHAASO photons might come from UHECR interactions with the extragalactic background light, and the paradigm that energetic GRBs may power the UHECR flux. For these values and the high dissipation radii considered, we find consistency with the nonobservation of neutrinos and no significant signatures on the electromagnetic spectrum. Inverse Compton-dominated scenarios from the prompt emission are demonstrated to lead to about an order of magnitude higher fluxes in the HE range; this enhancement is testable via its spectral impact in the Fermi-GBM and LAT ranges., Published by Institute of Physics Publ., London
Published: 2023
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3. Limits on Neutrino Emission from GRB 221009A from MeV to PeV Using the IceCube Neutrino Observatory

Author: Abbasi, R., Ackermann, M., Adams, J., Agarwalla, S. K., Aggarwal, N., Aguilar, J. A., Ahlers, M., Alameddine, J. M., Amin, N. M., Andeen, K., Anton, G., Argüelles, C., Ashida, Y., Athanasiadou, S., Axani, S. N., Bai, X., V., A. Balagopal, Baricevic, M., Barwick, S. W., Basu, V., Bay, R., Beatty, J. J., Becker, K.-H., Tjus, J. Becker, Beise, J., Bellenghi, C., BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bontempo, F., Book, J. Y., Borowka, J., Meneguolo, C. B., Meneguolo, C. Boscolo, Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Braun, J., Brinson, B., Brostean-Kaiser, J., Burley, R. T., Busse, R. S., Campana, M. A., Carloni, K., Carnie-Bronca, E. G., Chen, C., Chen, Z., Chirkin, D., Choi, S., Clark, B. A., Classen, L., Coleman, A., Collin, G. H., Connolly, A., Conrad, J. M., Coppin, P., Correa, P., Countryman, S., Cowen, D. F., Dappen, C., Dave, P., De Clercq, C., DeLaunay, J. J., Delgado López, D., Dembinski, H., Deoskar, K., Desai, A., Desiati, P., de Vries, K. D., de Wasseige, G., DeYoung, T., Diaz, A., Díaz-Vélez, J. C., Dittmer, M., Domi, A., Dujmovic, H., DuVernois, M. A., Ehrhardt, T., Eller, P., Engel, R., Erpenbeck, H., Evans, J., Evenson, P. A., Fan, K. L., Fazely, A. R., Fedynitch, A., Feigl, N., Fiedlschuster, S., Finley, C., Fischer, L., Fox, D., Franckowiak, A., Friedman, E., Fritz, A., Fürst, P., Gaisser, T. K., Gallagher, J., Ganster, E., Garcia, A., Garrappa, S., Gerhardt, L., Ghadimi, A., Glaser, C., Glauch, T., Glüsenkamp, T., Goehlke, N., Gonzalez, J. G., Goswami, S., Grant, D., Gray, S. J., Griffin, S., Griswold, S., Günther, C., Gutjahr, P., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Hamdaoui, H., Minh, M. Ha, Hanson, K., Hardin, J., Harnisch, A. A., Hatch, P., Haungs, A., Helbing, K., Hellrung, J., Henningsen, F., Heuermann, L., Hickford, S., Hidvegi, A., Hill, C., Hill, G. C., Hoffman, K. D., Hoshina, K., Hou, W., Huber, T., Hultqvist, K., Hünnefeld, M., Hussain, R., Hymon, K., In, S., Iovine, N., Ishihara, A., Jansson, M., Japaridze, G. S., Jeong, M., Jin, M., Jones, B. J. P., Kang, D., Kang, W., Kang, X., Kappes, A., Kappesser, D., Kardum, L., Karg, T., Karl, M., Karle, A., Katz, U., Kauer, M., Kelley, J. L., Kheirandish, A., Kin, K., Kiryluk, J., Klein, S. R., Kochocki, A., Koirala, R., Kolanoski, H., Kontrimas, T., Köpke, L., Kopper, C., Koskinen, D. J., Koundal, P., Kovacevich, M., Kowalski, M., Kozynets, T., Kruiswijk, K., Krupczak, E., Kumar, A., Kun, E., Kurahashi, N., Lad, N., Lagunas Gualda, C., Lamoureux, M., Larson, M. J., Lauber, F., Lazar, J. P., Lee, J. W., DeHolton, K. L., DeHolton, K. Leonard, Leszczyńska, A., Lincetto, M., Liu, Q. R., Liubarska, M., Lohfink, E., Love, C., Mariscal, C. J. Lozano, Lu, L., Lucarelli, F., Ludwig, A., Luszczak, W., Lyu, Y., Ma, W. Y., Madsen, J., Mahn, K. B. M., Makino, Y., Mancina, S., Sainte, W. Marie, Mariş, I. C., Marka, S., Marka, Z., Marsee, M., Martinez-Soler, I., Maruyama, R., Mayhew, F., McElroy, T., McNally, F., Mead, J. V., Meagher, K., Mechbal, S., Medina, A., Meier, M., Meighen-Berger, S., Merckx, Y., Merten, L., Micallef, J., Mockler, D., Montaruli, T., Moore, R. W., Morii, Y., Morse, R., Moulai, M., Mukherjee, T., Naab, R., Nagai, R., Naumann, U., Necker, J., Neumann, M., Niederhausen, H., Nisa, M. U., Noell, A., Nowicki, S. C., Pollmann, A. Obertacke, Oehler, M., Oeyen, B., Olivas, A., Orsoe, R., Osborn, J., O’Sullivan, E., Pandya, H., Park, N., Parker, G. K., Paudel, E. N., Paul, L., de los Heros, C. Pérez, Peterson, J., Philippen, S., Pieper, S., Pizzuto, A., Plum, M., Popovych, Y., Prado Rodriguez, M., Pries, B., Procter-Murphy, R., Przybylski, G. T., Raab, C., Rack-Helleis, J., Rawlins, K., Rechav, Z., Rehman, A., Reichherzer, P., Renzi, G., Resconi, E., Reusch, S., Rhode, W., Richman, M., Riedel, B., Roberts, E. J., Robertson, S., Rodan, S., Roellinghoff, G., Rongen, M., Rott, C., Ruhe, T., Ruohan, L., Ryckbosch, D., Safa, I., Saffer, J., Salazar-Gallegos, D., Sampathkumar, P., Sanchez Herrera, S. E., Sandrock, A., Santander, M., Sarkar, S., Savelberg, J., Savina, P., Schaufel, M., Schieler, H., Schindler, S., Schlüter, B., Schmidt, T., Schneider, J., Schröder, F. G., Schumacher, L., Schwefer, G., Sclafani, S., Seckel, D., Seunarine, S., Sharma, A., Shefali, S., Shimizu, N., Silva, M., Skrzypek, B., Smithers, B., Snihur, R., Soedingrekso, J., Søgaard, A., Soldin, D., Sommani, G., Spannfellner, C., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stein, R., Stezelberger, T., Stürwald, T., Stuttard, T., Sullivan, G. W., Taboada, I., Ter-Antonyan, S., Thompson, W. G., Thwaites, J., Tilav, S., Tollefson, K., Tönnis, C., Toscano, S., Tosi, D., Trettin, A., Tung, C. F., Turcotte, R., Twagirayezu, J. P., Ty, B., Unland Elorrieta, M. A., Upshaw, K., Valtonen-Mattila, N., Vandenbroucke, J., van Eijndhoven, N., Vannerom, D., van Santen, J., Vara, J., Veitch-Michaelis, J., Venugopal, M., Verpoest, S., Veske, D., Walck, C., Watson, T. B., Weaver, C., Weigel, P., Weindl, A., Weldert, J., Wendt, C., Werthebach, J., Weyrauch, M., Whitehorn, N., Wiebusch, C. H., Willey, N., Williams, D. R., Wolf, M., Wrede, G., Wulff, J., Xu, X. W., Yanez, J. P., Yildizci, E., Yoshida, S., Yu, F., Yu, S., Yuan, T., Zhang, Z., and Zhelnin, P.
Subjects: FOS: Physical sciences, burst [gamma ray], gamma ray: burst, GLAST, High Energy Physics - Experiment, IceCube, High Energy Physics - Experiment (hep-ex), High Energy Physics - Phenomenology (hep-ph), emission, TeV, ddc:530, Cherenkov, LHAASO, High Energy Astrophysical Phenomena (astro-ph.HE), background, Physics, Astronomy and Astrophysics, redshift, neutrino: UHE, UHE [neutrino], observatory, High Energy Physics - Phenomenology, Cherenkov counter, Space and Planetary Science, correlation, ddc:520, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The astrophysical journal / 2 946(1), L26 (2023). doi:10.3847/2041-8213/acc077, Gamma-ray bursts (GRBs) have long been considered a possible source of high-energy neutrinos. While no correlations have yet been detected between high-energy neutrinos and GRBs, the recent observation of GRB 221009A—the brightest GRB observed by Fermi-GBM to date and the first one to be observed above an energy of 10 TeV—provides a unique opportunity to test for hadronic emission. In this paper, we leverage the wide energy range of the IceCube Neutrino Observatory to search for neutrinos from GRB 221009A. We find no significant deviation from background expectation across event samples ranging from MeV to PeV energies, placing stringent upper limits on the neutrino emission from this source., Published by Institute of Physics Publ., London
Published: 2023
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4. Systematic parameter space study for the UHECR origin from GRBs in models with multiple internal shocks

Author: A Rudolph, Jonas Heinze, Anatoli Fedynitch, Walter Winter, Denise Boncioli, and Daniel Biehl
Subjects: Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], FOS: Physical sciences, burst [gamma ray], Cosmic ray, Astrophysics, Parameter space, 7. Clean energy, 01 natural sciences, Energy requirement, Quality (physics), propagation, 0103 physical sciences, Range (statistics), stochastic, Neutrinos, Cosmic rays, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Gamma-ray burst: general, Astronomy and Astrophysics, flux [neutrino], sensitivity, messenger, injection, quality, Space and Planetary Science, stacking, ddc:520, Neutrino, Astrophysics - High Energy Astrophysical Phenomena, Gamma-ray burst
Abstract: We scrutinize the paradigm that conventional long-duration Gamma-Ray Bursts (GRBs) are the dominant source of the ultra-high energy cosmic rays (UHECRs) within the internal shock scenario by describing UHECR spectrum and composition and by studying the predicted (source and cosmogenic) neutrino fluxes. Since it has been demonstrated that the stacking searches for astrophysical GRB neutrinos strongly constrain the parameter space in single-zone models, we focus on the dynamics of multiple collisions for which different messengers are expected to come from different regions of the same object. We propose a model which can describe both stochastic and deterministic engines, which we study in a systematic way. We find that GRBs can indeed describe the UHECRs for a wide range of different model assumptions with comparable quality albeit with the previously known problematic energy requirements; the heavy mass fraction at injection is found to be larger than 70% (95% CL). We demonstrate that the post-dicted (from UHECR data) neutrino fluxes from sources and UHECR propagation are indeed below the current sensitivities but will be reached by the next generation of experiments. We finally critically review the required source energetics with the specific examples found in this study., Comment: 16 pages, 9 figures, version accepted for publication in MNRAS
Published: 2020

5. External Inverse-Compton and Proton Synchrotron Emission from the Reverse Shock as the Origin of VHE Gamma-Rays from the Hyper-Bright GRB 221009A

Author: B. Theodore Zhang, Kohta Murase, Kunihito Ioka, Deheng Song, Chengchao Yuan, and Péter Mészáros
Subjects: electron, VHE [gamma ray], gamma ray, burst, gamma ray, VHE, UHE [cosmic radiation], burst [gamma ray], FOS: Physical sciences, gamma ray: burst, GeV, synchrotron, optical, TeV, cosmic radiation: UHE, High Energy Astrophysical Phenomena (astro-ph.HE), new physics, background, photon, cosmic radiation, UHE, Astronomy and Astrophysics, acceleration, proton synchrotron, flux, gamma ray: VHE, Space and Planetary Science, ddc:520, Astrophysics - High Energy Astrophysical Phenomena, Compton scattering
Abstract: The astrophysical journal / 2 947(1), L14 (2023). doi:10.3847/2041-8213/acc79f, The detection of the hyper-bright gamma-ray burst (GRB) 221009A enables us to explore the nature of the GRB emission and the origin of very high-energy gamma rays. We analyze the Fermi Large Area Telescope (Fermi-LAT) data of this burst and investigate the GeV–TeV emission in the framework of the external reverse-shock model. We show that the early ∼1–10 GeV emission can be explained by the external inverse-Compton mechanism via upscattering MeV gamma rays by electrons accelerated at the reverse shock, in addition to the synchrotron self-Compton component. The predicted early optical flux could have been brighter than that of the naked-eye GRB 080319B. We also show that proton synchrotron emission from accelerated ultrahigh-energy cosmic rays (UHECRs) is detectable and could potentially explain ≳TeV photons detected by LHAASO or constrain the UHECR acceleration mechanism. Our model suggests that the detection of photons with energies up to ∼18 TeV is possible for reasonable models of the extragalactic background light without invoking new physics and predicts anticorrelations between MeV photons and TeV photons, which can be tested with the LHAASO data., Published by Institute of Physics Publ., London
Published: 2022
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6. Deep Learning Transient Detection with VERITAS

Author: Pfrang, Konstantin Johannes and VERITAS Collaboration
Subjects: atmosphere [Cherenkov counter], Astrophysics::High Energy Astrophysical Phenomena, Night sky, primordial [black hole], burst [gamma ray], FOS: Physical sciences, Primordial black hole, Astrophysics, Cherenkov counter: atmosphere, gamma ray: burst, GeV, Stability (probability), VHE, law.invention, blazar, evaporation, law, ddc:530, Blazar, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), background, Elevation, Astrophysics::Instrumentation and Methods for Astrophysics, imaging, stability, observatory, VERITAS, Transient (oscillation), Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, black hole: primordial, performance, Flare
Abstract: 37th International Cosmic Ray Conference, ICRC 2021, Berlin, online, Germany, 12 Jul 2021 - 23 Jul 2021; Proceedings of Science / International School for Advanced Studies (ICRC2021), 822 (2021). doi:10.22323/1.395.0822, Ground-based $\gamma$-ray observatories, such as the VERITAS array of imaging atmospheric Cherenkov telescopes, provide insight into very-high-energy (VHE, $\mathrm{E}>100\,\mathrm{GeV}$) astrophysical transient events. Examples include the evaporation of primordial black holes, gamma-ray bursts and flaring blazars. Identifying such events with a serendipitous location and time of occurrence is difficult. Thus, employing a robust search method becomes crucial. An implementation of a transient detection method based on deep-learning techniques for VERITAS will be presented. This data-driven approach significantly reduces the dependency on the characterization of the instrument response and the modelling of the expected transient signal. The response of the instrument is affected by various factors, such as the elevation of the source and the night sky background. The study of these effects allows enhancing the deep learning method with additional parameters to infer their influences on the data. This improves the performance and stability for a wide range of observational conditions. We illustrate our method for an historic flare of the blazar BL Lac that was detected by VERITAS in October 2016. We find a promising performance for the detection of such a flare in timescales of minutes that compares well with the VERITAS standard analysis., Published by SISSA, Trieste
Published: 2021

7. The H.E.S.S. Gravitational Wave Rapid Follow-up Program during O2 and O3

Author: Fabian Schüssler, Francois Brun, Patrick Reichherzer, S. Ohm, Halim Ashkar, Monica Seglar Arroyo, Sylvia Zhu, Ruslan Konno, Heike Prokoph, M. Füßling, Sylvia J. Zhu, Clemens Hoischen, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire d'Annecy de Physique des Particules (LAPP), and Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)
Subjects: data analysis method, neutron star: binary, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, VHE [gamma ray], FOS: Physical sciences, burst [gamma ray], absorption: effect, Field of view, binary [neutron star], effect [absorption], gamma ray: burst, 01 natural sciences, emission [gravitational radiation], binary: coalescence, HESS, 0103 physical sciences, Astronomical interferometer, binary [black hole], ddc:530, High Energy Stereoscopic System, LIGO, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, media_common, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Gravitational wave, Astronomy, Galaxy, Afterglow, Cherenkov counter, VIRGO, gamma ray: VHE, black hole: binary, Sky, gravitational radiation: emission, galaxy, gravitational radiation: localization, coalescence [binary], Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], localization [gravitational radiation]
Abstract: 37th International Cosmic Ray Conference, ICRC 2021, Berlin, online, Germany, 12 Jul 2021 - 23 Jul 2021; Proceedings of Science / International School for Advanced Studies (ICRC2021), 936 (2021). doi:10.22323/1.395.0936, Since 2015, the direct detection of Gravitational Waves (GWs) became possible with ground-based interferometers like LIGO and Virgo. GWs became the center of attention of the astronomical community and electromagnetic observatories took a particular interest in follow-up observations of such events. The main setback of these observations is the poor localization of GW events. In fact, GW localization uncertainties can span tens to hundreds of deg$^2$ the sky even with the advanced configurations of current GW interferometers. In this contribution, we present five follow-up strategies developed for the High Energy Stereoscopic System (H.E.S.S.) and assess their performances. We show how a 2D and 3D galaxy targeted search approach exploiting the integral probability inside the instruments field of view are best suited for medium field of view instruments like H.E.S.S. We also develop an automatic response scheme within the H.E.S.S. Transient Follow-up system that is optimized for fast response and is capable of responding promptly to all kind of GW alerts. GW events are filtered by the developed scheme and prompt and afterglow observations are automatically scheduled. The H.E.S.S. response latency to prompt alerts is measured to be less than 1 minute. With this continually optimized GW response scheme, H.E.S.S. scheduled several GW follow-up observations during the second and third LIGO/Virgo observation runs., Published by SISSA, Trieste
Published: 2021

8. VTSCat: The VERITAS Catalog of Gamma-Ray Observations

Author: Patel, Sameer, Maier, Gernot, Archer, Avery, Hona, Binita, Giuri, Chiara, Adams, Colin, McGrath, Conor, Nieto, Daniel, Hanna, David, Kieda, David, Williams, David, Ribeiro, Deivid, Kaaret, Philip, tak, donggeun, Pueschel, Elisa, Roache, Emmet, Gillanders, Gary, Sembroski, Glenn, Foote, Gregory, Sadeh, Iftach, Buckley, James, Ryan, James, Holder, Jamie, Otte, A., Christiansen, Jodi, Quinn, John, Farrell, Kayla, Ragan, Ken, Pfrang, Konstantin, Fortson, Lucy, Errando, Manel, Santander, Marcos, Lang, Mark, Pohl, Martin, Falcone, Abe, Kertzman, Mary, Capasso, Massimo, Lundy, Matthew, Nievas-Rosillo, Mireia, Hervet, Olivier, Gueta, Orel, Moriarty, Patrick, Reynolds, Paul, Feng, Qi, Prado, Raul, Gent, Alasdair E., Ong, Rene, Mukherjee, Reshmi, Shang, Ruo-Yu, Kumar, Sajan, Patel, Sonal Ramesh, O'Brien, Stephan, Humensky, Thomas Brian, Kleiner, Tobias, Williamson, Tyler, Vassiliev, Vladimir, Chromey, Alisha, Jin, Weidong, Benbow, Wystan, VERITAS Collaboration, Weinstein, Amanda, Furniss, Amy, and Brill, Aryeh
Subjects: Active galactic nucleus, atmosphere [Cherenkov counter], Astrophysics::High Energy Astrophysical Phenomena, burst [gamma ray], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Cherenkov counter: atmosphere, gamma ray: burst, GeV, star: binary, law.invention, Telescope, Pulsar, Observatory, law, Binary star, supernova, Astrophysics::Solar and Stellar Astrophysics, TeV, ddc:530, AGN, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, Astrophysics::Galaxy Astrophysics, pulsar, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), photon, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, imaging, Galaxy, observatory, Supernova, binary [star], VERITAS, galaxy, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: 37th International Cosmic Ray Conference, ICRC 2021, Berlin, online, Germany, 12 Jul 2021 - 23 Jul 2021; Proceedings of Science / International School for Advanced Studies (ICRC2021), 812 (2021). doi:10.22323/1.395.0812, We present a catalog of results of gamma-ray observations made by VERITAS, published from 2008 to 2020. VERITAS is a ground based imaging atmospheric Cherenkov telescope observatory located at the Fred Lawrence Whipple Observatory (FLWO) in southern Arizona, sensitive to gamma-ray photons with energies in the range of $\sim$ 100 GeV - 30 TeV. Its observation targets include galactic sources such as binary star systems, pulsar wind nebulae, and supernova remnants, extragalactic sources like active galactic nuclei, star forming galaxies, and gamma-ray bursts, and some unidentified objects. The catalog includes in digital form all of the high-level science results published in 112 papers using VERITAS data and currently contains data on 57 sources. The catalog has been made accessible via GitHub and at NASA's HEASARC., Published by SISSA, Trieste
Published: 2021
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9. Observation of burst activity from SGR1935+2154 associated to first galactic FRB with H.E.S.S

Author: Abdalla, Hassan, Aharonian, Felix, Barbosa Martins, Victor, Lenain, Jean-Philippe, Leuschner, Fabian, Levy, Christelle, Lohse, Thomas, Luashvili, Anna, Lypova, Iryna, Mackey, Jonathan, Majumdar, Jhilik, Malyshev, Denys, Malyshev, Dmitry, Barnacka, Anna, Marandon, Vincent, Marchegiani, Paolo, Marcowith, Alexandre, Mares, Arnaud, Martí-Devesa, Guillem, Marx, Ramin, Maurin, Gilles, Meintjes, Pieter, Meyer, Manuel, Mitchell, Alison, Barnard, Monica, Moderski, Rafal, Mohrmann, Lars, Montanari, Alessandro, Moore, Chris, Morris, Paul, Moulin, Emmanuel, Muller, Jacques, Murach, Thomas, Nakashima, Kaori, Naurois , Mathieu, Batzofin, Rowan, Nayerhoda, Amid, Davids, Hambeleleni, Niemiec, Jacek, Noel, Angel, O'Brien, Paul, Oberholzer, Laenita Lorraine, Ohm, Stefan, Olivera-Nieto, Laura, Ona-Wilhelmi , Emma, Ostrowski, Michal, Becherini, Yvonne, Panny, Sebastian, Panter, Michael, Parsons, Dan, Peron, Giada, Pita, Santiago, Poireau, Vincent, Prokhorov, Dmitry, Prokoph, Heike, PUEHLHOFER, Gerd, Punch, Michael, Berge, David, Quirrenbach, Andreas, Reichherzer, Patrick, Reimer, Anita, Reimer, Olaf, Remy, Quentin, Renaud, Matthieu, Reville, Brian, Rieger, Frank, Romoli, Carlo, Rowell, Gavin, Bernloehr, Konrad, Rudak, Bronislaw, Rueda Ricarte, Hector, Ruiz Velasco, Edna, Sahakian, Vardan, Sailer, Simon, Salzmann, Heiko, Sanchez, David, Santangelo, Andrea, Sasaki, Manami, Schaefer, Johannes, Bi, Baiyang, Schutte, Hester, Schwanke, Ullrich, Schüssler, Fabian, Senniappan, Mohanraj, Seyffert, Albert, Shapopi, Jimmy N. S., Shiningayamwe, Kleopas, Simoni, Rachel, Sinha, Atreyee, Sol, Helene, Böttcher, Markus, Spackman, Hugh, Specovius, Andreas, Spencer, Samuel Timothy, Spir-Jacob, Marion, Stawarz, Lukasz, Steenkamp, Riaan, Stegmann, Christian, Steinmassl, Simon, Steppa, Constantin, Sun, Lei, Boisson, Catherine, Takahashi, Tadayuki, Tanaka, Takaaki, Tavernier, Thomas, Taylor, Andrew, Terrier, Regis, Thiersen, Hannes, Thorpe-Morgan, Charles, Tluczykont, Martin, Tomankova, Lenka, Tsirou, Michelle, Ait-Benkhali, Faical, Bolmont, Julien, Tsuji, Naomi, Tuffs, Richard, Uchiyama, Yasunobu, van der Walt, Johann, van Eldik, Christopher, van Rensburg, Carlo, van Soelen, Brian, Vasileiadis, George, Veh, Johannes, Venter, Christo, Bony , Mathieu, Vincent, Pascal, Vink, Jacco, Völk, Heinrich J., Wagner, Stefan, Watson, Jason John, Werner, Felix, White, Richard, Wierzcholska, Alicja, Wong, Yu Wun, Yassin, Hend Mahmoud, Breuhaus, Mischa, Yusafzai, Anke, Zacharias, Michael, Zanin, Roberta, Zargaryan, Davit, Zdziarski, Andrzej, Zech, Andreas, Zhu, Sylvia, Zmija, Andreas, Zouari, Samuel, Żywucka, Natalia, Brose, Robert, H. E. S. S. Collaboration, Brun, Francois, Bulik, Tomasz, Bylund, Thomas, Cangemi, Floriane, Caroff, Sami, Casanova, Sabrina, Anguener, Oguzhan, Catalano, Jaqueline, Chambery, Pauline, Chand, Tej Bahadur, Chen, Andrew, Cotter, Garret, Curlo, Malgorzata, Dalgleish, Hannah, Damascene Mbarubucyeye, Jean, Davids, Isak Delberth, Davies, James, Arcaro, Cornelia, Devin, Justine, Djannati-Ataï, Arache, Dmytriev, Anton, Donath, Axel, Doroshenko, Victor, Dreyer, Lente, Du Plessis, Louis, Duffy, Connor, Egberts, Kathrin, Einecke, Sabrina, Armand, Celine, ERNENWEIN, Jean-Pierre, Fegan, Steven, Feijen, Kirsty, Fiasson, Armand, Fichet de Clairfontaine, Gaëtan, Fontaine, Gerard, Frans, Lott, Fuessling, Matthias, Funk, Stefan, Gabici, Stefano, Armstrong, Tom, Gallant, Yves, Giavitto, Gianluca, Giunti, Luca, Glawion, Dorit, Glicenstein, Jean-Francois, Grondin, Marie-Hélène, Hattingh, Sumari, Haupt, Maria, HERMANN, German, Hinton, Jim, Ashkar, Halim, Hofmann, Werner, Hoischen, Clemens, Holch, Tim, Holler, Markus, Horns, Dieter, Huang, Zhi-Qiu, Huber, David, Hörbe, Mario, Jamrozy, Marek, Jankowsky, Felix, Backes, Michael, Joshi, Vikas, JUNG, Ira, Kasai, Eli, Katarzynski, Krzysztof, Katz, Ulì, Khangulyan, Dmitry, Khelifi, Bruno, Klepser, Stefan, Kluzniak, Wlodek, Komin, Nukri, Baghmanyan, Vardan, Konno, Ruslan, Kosack, Karl, Kostiunin, Dmitriy, Kreter, Michael, Kukec Mezek, Gašper, Kundu, Anu, Lamanna, Giovanni, Le Stum, Sébastien, Lemiere, Anne, Lemoine-Goumard, Marianne, Naurois , Mathieu, Bony , Mathieu, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, and H.E.S.S.
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Brightness, Astrophysics::High Energy Astrophysical Phenomena, atmosphere [Cherenkov counter], Soft gamma repeater, FOS: Physical sciences, burst [gamma ray], X-ray: burst, Astrophysics, gamma ray: burst, Cherenkov counter: atmosphere, Magnetar, Radio spectrum, Observational evidence, Pulsar, ddc:530, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - High Energy Astrophysical Phenomena, Cherenkov radiation, burst [X-ray]
Abstract: 37th International Cosmic Ray Conference, ICRC2021, Berlin, Germany - Online, 12 Jul 2021 - 23 Jul 2021; Proceedings of Science / International School for Advanced Studies (ICRC2021), 777 (2021). doi:10.22323/1.395.0777, Fast radio bursts (FRB) are enigmatic powerful single radio pulses with durations of several milliseconds and high brightness temperatures suggesting coherent emission mechanism. For the time being a number of extragalactic FRBs have been detected in the high-frequency radio band including repeating ones. The most plausible explanation for these phenomena is magnetar hyperflares. The first observational evidence of this scenario was obtained in April 2020 when an FRB was detected from the direction of the Galactic magnetar and soft gamma repeater SGR1935+2154. The FRB was preceded with a number of soft gamma-ray bursts observed by Swift-BAT satellite, which triggered the follow-up program of the H.E.S.S. imaging atmospheric Cherenkov telescopes (IACTs). H.E.S.S. has observed SGR1935+2154 over a 2 hour window few hours prior to the FRB detection by STARE2 and CHIME. The observations overlapped with other X-ray bursts from the magnetar detected by INTEGRAL and Swift-BAT, thus providing first observations of a magnetar in a flaring state in the very-high energy domain. We present the analysis of these observations, discuss the obtained results and prospects of the H.E.S.S. follow-up program for soft gamma repeaters and anomalous X-ray pulsars., Published by SISSA, Trieste
Published: 2021
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10. Realtime follow-up of astrophysical transients with the IceCube Neutrino Observatory

Author: IceCube Collaboration, Pizzuto, Alex, Abbasi, Rasha, Ackermann, Markus, Adams, Jenni, Aguilar, Juanan, Ahlers, M., Ahrens, Maryon, Alispach, Cyril Martin, Alves Junior, Antonio Augusto, Amin, Najia Moureen Binte, An, Rui, Andeen, Karen, Anderson, Tyler, Anton, Gisela, Arguelles, Carlos, Ashida, Yosuke, Axani, Spencer, Bai, Xinhua, Balagopal V., Aswathi, Barbano, Anastasia Maria, Barwick, S. W., Bastian, Benjamin, Basu, Vedant, Baur, Sebastian, Bay, R. C., Beatty, J. J., Becker, K. H., Becker Tjus, Julia, Bellenghi, Chiara, BenZvi, Segev, Berley, D., Bernardini, Elisa, Besson, D. Z., Binder, Gary, Bindig, Daniel, Blaufuss, E., Blot, Summer, Boddenberg, Matthias, Bontempo, Federico, Borowka, Jürgen, Boser, S., Botner, Olga, Böttcher, Jakob, Bourbeau, Etienne, Bradascio, Federica, Braun, J., Bron, Stephanie, Brostean-Kaiser, Jannes, Browne, Sally-Ann, Burgman, Alexander, Burley, Ryan, Busse, Raffaela, Campana, Michael, Carnie-Bronca, Erin, Chen, Chujie, Chirkin, Dmitry, Choi, Koun, Clark, Bryanlee, Clark, Kenneth, Classen, Lew, Coleman, Alan, Collin, Gabriel, Conrad, J. M., Coppin, Paul, Correa, Pablo, Cowen, D. F., Cross, R., Dappen, Christian, Dave, Pranav, DE CLERCQ, Catherine, DeLaunay, James, Dembinski, Hans, Deoskar, Kunal, De Ridder, Sam, Desai, Abhishek, Desiati, Paolo, de Vries, Krijn, de Wasseige, Gwenhaël, De With, Meike, DeYoung, Tyce, Dharani, Sukeerthi, Diaz, Alejandro, Diaz-Velez, Juan Carlos, Dittmer, Markus, Dujmovic, Hrvoje, Dunkman, Matt, DuVernois, Michael, Dvorak, Emily, Ehrhardt, Thomas, Eller, Philipp, Engel, Ralph, Erpenbeck, Hannah, Evans, John, Evenson, P. A., Fan, Kwok Lung, Fazely, A. R., Fiedlschuster, Sebastian, Fienberg, Aaron, Filimonov, Kirill, Finley, Chad, Fischer, Leander, Fox, Derek B., Franckowiak, Anna, Friedman, Elizabeth, Fritz, Alexander, Fürst, Philipp, Gaisser, T. K., Gallagher, Jay, Ganster, Erik, Garcia, Alfonso, Garrappa, Simone, Gerhardt, L., Ghadimi, Ava, Glaser, Christian, Glauch, Theo, Glusenkamp, Thorsten, Goldschmidt, A., Gonzalez, Javier, Goswami, Sreetama, Grant, Darren, Grégoire, Timothée, Griswold, Spencer, Gunduz, Mehmet, Günther, Christoph, Haack, Christian, Hallgren, Allan, Halliday, R., Halve, Lasse Yannik, Halzen, F., Ha Minh, Martin, Hanson, Kael, Hardin, John, Harnisch, Alexander A., Haungs, Andreas, Hauser, Simon, Hebecker, Dustin, Helbing, K., Henningsen, Felix, Hettinger, Emma C., Hickford, Stephanie, Hignight, Joshua, Hill, Colton, Hill, G. C., Hoffman, Kara, Hoffmann, Ruth, Hoinka, Tobias, Hokanson-Fasig, Benjamin, Hoshina, K., Huang, Feifei, Huber, Matthias, Huber, Thomas, Hultqvist, Klas, Hunnefeld, Mirco, Hussain, Raamis, In, Seongjin, Iovine, Nadège, Ishihara, Aya, Jansson, Matti, Japaridze, George, Jeong, Minjin, Jones, Ben, Kang, Donghwa, Kang, Woosik, Kang, Xinyue, Kappes, Alexander, Kappesser, David, Karg, Timo, Karl, Martina, Karle, A., Katz, U., Kauer, M., Kellermann, Moritz, Kelley, J. L., Kheirandish, Ali, Kin, Ken'ichi, Kintscher, Thomas, Kiryluk, Joanna, Klein, Spencer, Koirala, Ramesh, Kolanoski, Hermann, Kontrimas, Tomas, Kopke, Lutz, Kopper, Claudio, Kopper, Sandro, Koskinen, D. J., Koundal, Paras, Kovacevich, Michael, Kowalski, Marek, Kozynets, Tetiana, Kun, Emma, Kurahashi, Naoko, Lad, Neha, Lagunas Gualda, Cristina, Lanfranchi, Justin, Larson, Michael J., Lauber, Frederik Hermann, Lazar, Jeffrey, Lee, Jiwoong, Leonard, Kayla, Leszczyńska, Agnieszka, Li, Yijia, Lincetto, Massimiliano, Liu, Qinrui, Liubarska, Maria, Lohfink, Elisa, Lozano Mariscal, Cristian Jesus, Lu, Lu, Lucarelli, Francesco, Ludwig, Andrew, Luszczak, William, Lyu, Yang, Ma, Wing Yan, Madsen, James, Mahn, Kendall, Makino, Yuya, Mancina, Sarah, Maris, Ioana Codrina, Maruyama, Reina H., Mase, K., McElroy, Thomas, McNally, Frank, Mead, James Vincent, Meagher, K., Medina, Andres, Meier, Maximilian, Meighen-Berger, Stephan, Micallef, Jessie, Mockler, Daniela, Montaruli, Teresa, Moore, Roger, Morse, R., Moulai, Marjon, Naab, Richard, Nagai, Ryo, Naumann, Uwe, Necker, Jannis, Nguyen, Le Viet, Niederhausen, Hans, Nisa, Mehr, Nowicki, Sarah, Nygren, Dave, Obertacke Pollmann, Anna, Oehler, Marie, Olivas, A., O'Sullivan, Erin, Pandya, Hershal, Pankova, Daria, Park, Nahee, Parker, Grant, Paudel, Ek Narayan, Paul, Larissa, Perez de los Heros, Carlos, Peters, Lilly, Peterson, Josh, Philippen, Saskia, Pieloth, Damian, Pieper, Sarah, Pittermann, Martin, Pizzuto, A., Plum, M., Popovych, Yuiry, Porcelli, Alessio, Prado Rodriguez, Maria, Price, P. Buford, Pries, Brandom, Przybylski, Gerald, Raab, Christoph, Raissi, Amirreza, Rameez, Mohamed, Rawlins, K., Rea, Immacolata Carmen, Rehman, Abdul, Reichherzer, Patrick, Reimann, René, Renzi, Giovanni, Resconi, Elisa, Reusch, Simeon, Rhode, Wolfgang, Richman, Mike, Riedel, Benedikt, Roberts, Ella, Robertson, Sally, Roellinghoff, Gerrit, Rongen, Martin, Rott, Carsten, Ruhe, Tim, Ryckbosch, Dirk, Rysewyk Cantu, Devyn, Safa, Ibrahim, Saffer, Julian, Sanchez Herrera, Sebastian, Sandrock, Alexander, Sandroos, Joakim, Santander, Marcos, Sarkar, Subir, Sarkar, Sourav, Satalecka, Konstancja, Scharf, Maximilian Karl, Schaufel, Merlin, Schieler, Harald, Schindler, Sebastian, Schlunder, P., Schmidt, Torsten, Schneider, Austin, Schneider, Judith, Schröder, Frank G., Schumacher, Lisa Johanna, Schwefer, Georg, Sclafani, Steve, Seckel, D., Seunarine, Surujhdeo, Sharma, Ankur, Shefali, Shefali, Silva, Manuel, Skrzypek, Barbara, Smithers, Ben, Snihur, Robert, Soedingrekso, Jan, Soldin, Dennis, Spannfellner, Christian, Spiczak, Glenn, Spiering, Christian, Stachurska, Juliana, Stamatikos, Michael, Stanev, T., Stein, Robert, Stettner, Jöran Benjamin, Steuer, A., Stezelberger, T., Sturwald, Timo, Stuttard, Thomas, Sullivan, G. W., Taboada, I., Tenholt, Frederik, Ter-Antonyan, Samvel, Tilav, S., Tischbein, Franziska, Tollefson, Kirsten, Tomankova, Lenka, Tönnis, Christoph, Toscano, Simona, Tosi, Delia, Trettin, Alexander, Tselengidou, Maria, Tung, Chunfai, Turcati, Andrea, Turcotte, Roxanne, Turley, Colin, Twagirayezu, Jean Pierre, Ty, Bunheng, Unland Elorrieta, Martin, Valtonen-Mattila, Nora, Vandenbroucke, Justin, van Eijndhoven, Nick, Vannerom, David, van Santen, Jakob, Verpoest, Stef, Vraeghe, Matthias, Walck, C., Watson, Timothyblake, Weaver, Chris, Weigel, Philip, Weindl, Andreas, Weiss, Matthew, Weldert, Jan, Wendt, Chris, Werthebach, Johannes, Weyrauch, Mark, Whitehorn, Nathan, Wiebusch, Christopher, Williams, Dawn, Wolf, Martin, Woschnagg, Kurt, Wrede, Gerrit, Wulff, Johan, Xu, Xianwu, Xu, Yiqian, Yanez, Juan Pablo, Yoshida, S., Yu, Shiqi, Yuan, Tianlu, and Zhang, Zelong
Subjects: burst [radio wave], High energy, cosmic radiation [neutrino], neutrino: energy: high, Astrophysics::High Energy Astrophysical Phenomena, Pipeline (computing), burst [gamma ray], Field of view, gamma ray: burst, GLAST, IceCube Neutrino Observatory, IceCube, blazar, Observatory, Cherenkov [radiation], optical, ddc:530, energy: high [neutrino], Physics, radio wave: burst, Gravitational wave, background, photon, Astrophysics::Instrumentation and Methods for Astrophysics, gravitational radiation, Astronomy, temperature, radiation: Cherenkov, sensitivity, messenger, observatory, atmosphere, neutrino: cosmic radiation, Neutrino
Abstract: 37. International Cosmic Ray Conference, ICRC 2021, Berlin, Germany, 15 Jul 2021 - 22 Jul 2021; Proceedings of Science 395, 952 (2022). doi:10.22323/1.395.0952 special issue: "37th International Cosmic Ray Conference : ICRC2021 : 12-23 July 2021 : Berlin, Germany - Online / Editorial Board: Alexander Kappes, Institut für Kernphysik, Westfälische Wilhelms-Universität Münster, D-48149 Münster, Germany ; Bianca Keilhauer, Karlsruhe Institute of Technology, Institute for Astroparticle Physics (IAP)", Published by SISSA, Trieste
Published: 2021

11. Ultra-high-energy cosmic-ray nuclei and neutrinos in models of gamma-ray bursts and extragalactic propagation

Author: Heinze, Jonas, Winter, Walter, Lohse, Thomas, and Sigl, Günter
Subjects: geometry, accelerator, energy loss, UHE [cosmic radiation], nuclear cascades, burst [gamma ray], gamma-ray-bursts, gamma ray: burst, power spectrum, nucleus: cosmic radiation, nucleus: cascade, neutrino: flux, Kosmische Strahlung, neutrino: production, mass spectrum, photo-hadronic interactions, production [neutrino], propagation, radiation modelling, US 1670, ddc:530, numerisch [Methoden], cosmic radiation: UHE, Strahlungsmodellierung, plasma, Photohadronische Wechselwirkungen, Nukleare Kaskaden, secondary [neutrino], ultra-high-energy cosmic rays, showers: atmosphere, photon, numerical [methods], flux [neutrino], extragalactic propagation, astrophysical neutrinos, 530 Physik, Gammastrahlenblitze, angular dependence, neutrino: secondary, cosmic radiation [nucleus], hydrodynamics, Astrophysikalische Neutrinos, Extragalaktische Propagation, cascade [nucleus], atmosphere [showers]
Abstract: Dissertation, Humboldt University, 2020; Humboldt-Universität zu Berlin 194 pp. (2020). doi:10.18452/21386 = Dissertation, Humboldt University, 2020, Utrahochenergetische kosmische Strahlung (ultra-high-energy cosmic rays -- UHECR) besteht aus ionisierten Atomkernen mit den höchsten Teilchenergien, die je gemessen wurden. Zwar wurden die Quellen von UHECRs noch nicht eindeutig identifiziert, doch gibt es deutliche Anzeichen, dass sie extragalaktisch sind. Um die Beobachtungen zu interpretieren, wird ein Modell der Wechselwirkungen mit Photofeldern sowohl in der Quelle als auch während der extragalaktischen Propagation benötigt. Bei diesen Wechselwirkungen werden sekundäre Neutrinos erzeugt. Diese Dissertation behandelt Modelle der Quellen von UHECRs und die damit verbundene Produktion von Neutrinos sowohl in den Quellen als auch während der Propagation. Dafür wurde ein neuer Code, PriNCe, für die Propagation von UHECRs entwickelt. Dieser Code wird in einem umfangreichen Parameterscan für ein generisches Quellenmodell angewendet, welches mit dem Spektralindex, der maximalen Rigidität, der kosmologischen Quellenverteilung und der chemischen Komposition als freie Parameter definiert ist. Dabei wird der Einfluss von verschiedenen Photodisintegrations- und Luftschauermodellen auf die erwarteten Eigenschaften der Quellen demonstriert. Der Fluss kosmogenischer Neutrinos, der sich daraus robust vorhersagen lässt, liegt außerhalb der Reichweite aller derzeit geplanten Neutrinodetektoren. GRBs als mögliche Quellen von UHECRs werden im Multi-Collision Internal-Shock Modell simuliert, welches die Abhängigkeit der Strahlungsprozesse von den verschiedenen Dissipationsradien im Plasmajet berücksichtigt. Für dieses Modell wird der Effekt demonstriert, den verschiedene Annahmen über die anfängliche Verteilung des Plasmajets und das hydrodynamische Modell auf die resultierende UHECR- und Neutrinosstrahlung haben. Für den Gammastrahlenblitz GRB170817A, welcher zusammen mit einem Gravitationswellensignal beobachtet wurde, werden Vorhersagen für den Neutrinofluss und ihre Abhängigkeit vom Beobachtungswinkel gemacht.Ultra-high-energy cosmic rays (UHECRs) are the most energetic particles observed in the Universe. While the astrophysical sources of UHECRs have not yet been uniquely identified, there are strong indications for an extragalactic origin. The interpretation of the observations requires both simulations of UHECR acceleration and energy losses inside the source environment as well as interactions during extragalactic propagation. Due to their extreme energies, UHECR will interact with photons in these environments, producing a flux of secondary neutrinos. This dissertation deals with models of UHECR sources and the accompanying neutrino production in the source environment and during extragalactic propagation. We have developed a new, computationally efficient code, PriNCe, for the extragalactic propagation of UHECR nuclei. The PriNCe code is applied for an extensive parameter scan of a generic source model that is described by the spectral index, the maximal rigidity, the cosmological source evolution and the injected mass composition. In this scan, we demonstrate the impact of different disintegration and air-shower models on the inferred source properties. A prediction for the expected flux of cosmogenic neutrinos is also derived. GRBs are discussed as specific UHECR source candidates in the multi-collision internal-shock model. This model takes the radiation from different radii in the GRB outflow into account. We demonstrate how different assumptions about the initial setup of the jet and the hydrodynamic collision model impact the production of UHECRs and neutrinos. Motivated by the multi-messenger observation of GRB170817A, we discuss the expected neutrino production from this GRB and its dependence on the observation angle. We show that the neutrino flux for this event is at least four orders of magnitude below the detection limit for different geometries of the plasma jet., Published by Humboldt-Universität zu Berlin
Published: 2020

12. Probing the Magnetic Field in the GW170817 Outflow Using H.E.S.S. Observations

Author: Collaboration, H. E. S. S., Abdalla, H., Adam, R., Aharonian, F., Benkhali, F. Ait, Ang��ner, E. O., Arakawa, M., Arcaro, C., Armand, C., Armstrong, T., Ashkar, H., Backes, M., Baghmanyan, V., Barbosa-Martins, V., Barnacka, A., Barnard, M., Becherini, Y., Berge, D., Bernl��hr, K., Blackwell, R., B��ttcher, M., Boisson, C., Bolmont, J., Bonnefoy, S., Bregeon, J., Breuhaus, M., Brun, F., Brun, P., Bryan, M., B��chele, M., Bulik, T., Bylund, T., Caroff, S., Carosi, A., Casanova, S., Cerruti, M., Chand, T., Chandra, S., Chen, A., Cotter, G., Cury��o, M., Davids, I. D., Davies, J., Deil, C., Devin, J., deWilt, P., Dirson, L., Djannati-Ata��, A., Dmytriiev, A., Donath, A., Doroshenko, V., Dyks, J., Egberts, K., Eichhorn, F., Emery, G., Ernenwein, J. -P., Eschbach, S., Feijen, K., Fegan, S., Fiasson, A., Fontaine, G., Funk, S., F��ling, M., Gabici, S., Gallant, Y. A., Giavitto, G., Giunti, L., Glawion, D., Glicenstein, J. F., Gottschall, D., Grondin, M. -H., Hahn, J., Haupt, M., Heinzelmann, G., Hermann, G., Hinton, J. A., Hofmann, W., Hoischen, C., Holch, T. L., Holler, M., H��rbe, M., Horns, D., Huber, D., Iwasaki, H., Jamrozy, M., Jankowsky, D., Jankowsky, F., Jardin-Blicq, A., Joshi, V., Jung-Richardt, I., Kastendieck, M. A., Katarzy��ski, K., Katsuragawa, M., Katz, U., Khangulyan, D., Kh��lifi, B., Klepser, S., Klu��niak, W., Komin, Nu., Konno, R., Kosack, K., Kostunin, D., Kreter, M., Lamanna, G., Lemi��re, A., Lemoine-Goumard, M., Lenain, J. -P., Leser, E., Levy, C., Lohse, T., Lypova, I., Mackey, J., Majumdar, J., Malyshev, D., Marandon, V., Marchegiani, P., Marcowith, A., Mares, A., Mart��-Devesa, G., Marx, R., Maurin, G., Meintjes, P. J., Moderski, R., Mohamed, M., Mohrmann, L., Moore, C., Morris, P., Moulin, E., Muller, J., Murach, T., Nakashima, S., Nakashima, K., de Naurois, M., Ndiyavala, H., Niederwanger, F., Niemiec, J., Oakes, L., O'Brien, P., Odaka, H., Ohm, S., Wilhelmi, E. de Ona, Ostrowski, M., Panter, M., Parsons, R. D., Peyaud, B., Piel, Q., Pita, S., Poireau, V., Noel, A. Priyana, Prokhorov, D. A., Prokoph, H., P��hlhofer, G., Punch, M., Quirrenbach, A., Raab, S., Rauth, R., Reimer, A., Reimer, O., Remy, Q., Renaud, M., Rieger, F., Rinchiuso, L., Romoli, C., Rowell, G., Rudak, B., Ruiz-Velasco, E., Sahakian, V., Sailer, S., Saito, S., Sanchez, D. A., Santangelo, A., Sasaki, M., Scalici, M., Schlickeiser, R., Sch��ssler, F., Schulz, A., Schutte, H., Schwanke, U., Schwemmer, S., Seglar-Arroyo, M., Senniappan, M., Seyffert, A. S., Shafi, N., Shiningayamwe, K., Simoni, R., Sinha, A., Sol, H., Specovius, A., Spencer, S., Spir-Jacob, M., Stawarz, ��., Steenkamp, R., Stegmann, C., Steppa, C., Takahashi, T., Tavernier, T., Taylor, A. M., Terrier, R., Tiziani, D., Tluczykont, M., Tomankova, L., Trichard, C., Tsirou, M., Tsuji, N., Tuffs, R., Uchiyama, Y., van der Walt, D. J., van Eldik, C., van Rensburg, C., van Soelen, B., Vasileiadis, G., Veh, J., Venter, C., Vincent, P., Vink, J., V��lk, H. J., Vuillaume, T., Wadiasingh, Z., Wagner, S. J., Watson, J., Werner, F., White, R., Wierzcholska, A., Yang, R., Yoneda, H., Zacharias, M., Zanin, R., Zdziarski, A. A., Zech, A., Zorn, J., Zywucka, N., Rodrigues, X., North-West University [Potchefstroom] (NWU), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Rikkyo University [Tokyo], Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), University of Oxford [Oxford], Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, H.E.S.S., 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), 26598973 - Abdalla, Hassan, 30588766 - Arcaro, Cornelia, 28644743 - Backes, Michael, 20574266 - Barnard, Monica, 24420530 - Böttcher, Markus, 30366755 - Chand, Tej B., 31125417 - Chandra, Sunil, 33379009 - Kreter, Michael, 26403366 - Ndiyavala, Hambeleleni, 22799133 - Schutte, Hester M., 20126999 - Seyffert, Albertus Stefanus, 10060499 - Van der Walt, Diederick Johannes, 21106266 - Van Rensburg, Carlo, 12006653 - Venter, Christo, 26594080 - Wadiasingh, Zorawar, 29092086 - Zacharias, Michael, 34208968 - Zywucka-Hejzner, Natalia, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-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)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), H. E. S. S. Collaboration, Faculty of Science, High Energy Astrophys. & Astropart. Phys (API, FNWI), Gravitation and Astroparticle Physics Amsterdam, Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)
Subjects: emission [X-ray], electron, neutron star: binary, 010504 meteorology & atmospheric sciences, magnetic field, Astrophysics, binary [neutron star], Kilonova, 01 natural sciences, HESS, 010303 astronomy & astrophysics, Stellar evolution, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), radio wave, nucleosynthesis, r-process, Gamma-ray bursts, Astrophysics - High Energy Astrophysical Phenomena, Radio wave, Ejecta, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, burst [gamma ray], Context (language use), Astrophysics::Cosmology and Extragalactic Astrophysics, gamma ray: burst, Gamma-ray transient sources, 0103 physical sciences, Stellar mergers, X-ray: emission, High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, Gamma-ray astronomy, Gravitational wave, gravitational radiation, Astronomy and Astrophysics, Neutron star, electromagnetic, 13. Climate action, Space and Planetary Science, [SDU]Sciences of the Universe [physics], HESS - Abteilung Hinton, ddc:520, Gamma-ray burst, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: The astrophysical journal / 1 894(2), 1-5 (2020). doi:10.3847/2041-8213/ab8b59, The detection of the first electromagnetic counterpart to the binary neutron star (BNS) merger remnant GW170817 established the connection between short $γ$-ray bursts and BNS mergers. It also confirmed the forging of heavy elements in the ejecta (a so-called kilonova) via the r-process nucleosynthesis. The appearance of nonthermal radio and X-ray emission, as well as the brightening, which lasted more than 100 days, were somewhat unexpected. Current theoretical models attempt to explain this temporal behavior as either originating from a relativistic off-axis jet or a kilonova-like outflow. In either scenario, there is some ambiguity regarding how much energy is transported in the nonthermal electrons versus the magnetic field of the emission region. Combining the Very Large Array (radio) and Chandra (X-ray) measurements with observations in the GeV–TeV domain can help break this ambiguity, almost independently of the assumed origin of the emission. Here we report for the first time on deep H.E.S.S. observations of GW170817/GRB 170817A between 124 and 272 days after the BNS merger with the full H.E.S.S. array of telescopes, as well as on an updated analysis of the prompt (, Published by Institute of Physics Publ., London
Published: 2020

13. Unified thermal model for photohadronic neutrino production in astrophysical sources

Author: Arjen van Vliet, Damiano Fiorillo, S. Morisi, and Walter Winter
Subjects: photon hadron, Particle physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, burst [gamma ray], 01 natural sciences, 7. Clean energy, High Energy Physics - Phenomenology (hep-ph), production [neutrino], muon, 0103 physical sciences, Production (economics), ddc:530, neutrino antineutrino, AGN, detector [neutrino], capture, 010303 astronomy & astrophysics, effect [magnetic field], High Energy Astrophysical Phenomena (astro-ph.HE), Physics, flavor, thermal [model], 010308 nuclear & particles physics, cosmic radiation [photon], spectrum [neutrino], temperature, Astronomy and Astrophysics, flux [neutrino], sensitivity, High Energy Physics - Phenomenology, 13. Climate action, black body, High Energy Physics::Experiment, Neutrino, Thermal model, Astrophysics - High Energy Astrophysical Phenomena
Abstract: High-energy astrophysical neutrino fluxes are, for many applications, modeled as simple power laws as a function of energy. While this is reasonable in the case of neutrino production in hadronuclear $pp$ sources, it typically does not capture the behavior in photohadronic $p\gamma$ sources: in that case, the neutrino spectrum depends on the properties of the target photons the cosmic rays collide with and on possible magnetic-field effects on the secondary pions and muons. We show that the neutrino production from known photohadronic sources can be reproduced by a thermal (black-body) target-photon spectrum if one suitably adjusts the temperature, thanks to multi-pion production processes. This allows discussing neutrino production from most known $p\gamma$ sources, such as gamma-ray bursts, active galactic nuclei and tidal disruption events, in terms of a few parameters. We apply this thermal model to study the sensitivity of different classes of neutrino telescopes to photohadronic sources: we classify the model parameter space according to which experiment is most suitable for detection of a specific source class and demonstrate that different experiment classes, such as dense arrays, conventional neutrino telescopes, or radio-detection experiments, cover different parts of the parameter space. Since the model can also reproduce the flavor and neutrino-antineutrino composition, we study the impact on the track-to-shower ratio and the Glashow resonance., Comment: 38 pages, 13 figures; data available at https://github.com/damianofiorillo/Unified-thermal-model
Published: 2021

14. Determining the fraction of cosmic-ray protons at ultra-high energies with cosmogenic neutrinos

Author: Arjen van Vliet, Rafael Alves Batista, and Jörg R. Hörandel
Subjects: Astronomy, Astrophysics::High Energy Astrophysical Phenomena, Hadron, photon pi, Cosmic background radiation, UHE [cosmic radiation], FOS: Physical sciences, burst [gamma ray], Cosmic ray, primary [cosmic radiation], Astrophysics, cosmic background radiation, power spectrum, 7. Clean energy, 01 natural sciences, Luminosity, IceCube, cosmic radiation [p], formation [star], 0103 physical sciences, ddc:530, luminosity, AGN, detector [neutrino], 010303 astronomy & astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, model [interaction], photon, Astrophysics::Instrumentation and Methods for Astrophysics, Spectral density, flux [neutrino], Auger, Neutrino detector, 13. Climate action, current [neutrino], ARIANNA, High Energy Physics::Experiment, Neutrino, Gamma-ray burst, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Cosmogenic neutrinos are produced when ultra-high-energy cosmic rays (UHECRs) interact with cosmological photon fields. Limits on the diffuse flux of these neutrinos can be used to constrain the fraction of protons arriving at Earth with energies $E_{p} \gtrsim 30$ EeV, thereby providing constraints on the composition of UHECRs without fully relying on hadronic interaction models. We show to which extent current neutrino telescopes already constrain this fraction of protons and discuss the prospects for next-generation detectors to further constrain it. Additionally, we discuss the implications of these limits for several popular candidates for UHECR source classes., 5 pages, 2 figures, 1 table; Published in PRD, updated to match published version
Published: 2019
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15. Cosmic ray and neutrino emission from gamma-ray bursts with a nuclear cascade

Author: Biehl, Daniel, Boncioli, D., Fedynitch, A., and Winter, W.
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Cosmic rays, Gamma-ray burst: general, Neutrinos, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, burst [gamma ray], flux [neutrino], tension, IceCube, Auger, injection [nucleus], observatory, stacking, ddc:520, cascade [nucleus], Astrophysics - High Energy Astrophysical Phenomena
Abstract: Astronomy and astrophysics 611, A101 (2018). doi:10.1051/0004-6361/201731337, We discuss neutrino and cosmic-ray emission from Gamma-Ray Bursts (GRBs) with the injection of nuclei, where we take into account that a nuclear cascade from photo-disintegration can fully develop in the source. One of our main objectives is to test if recent results from the IceCube and the Pierre Auger Observatory can be accommodated with the paradigm that GRBs are the sources of Ultra-High Energy Cosmic Rays (UHECRs). While our key results are obtained using an internal shock model, we discuss how the secondary emission from a GRB shell can be interpreted in terms of other astrophysical models. It is demonstrated that the expected neutrino flux from GRBs weakly depends on the injection composition, which implies that prompt neutrinos from GRBs can efficiently test the GRB-UHECR paradigm even if the UHECRs are nuclei. We show that the UHECR spectrum and composition, as measured by the Pierre Auger Observatory, can be self-consistently reproduced in a combined source-propagation model. In an attempt to describe the energy range including the ankle, we find tension with the IceCube bounds from the GRB stacking analyses. In an alternative scenario, where only the UHECRs beyond the ankle originate from GRBs, the requirement for a joint description of cosmic-ray and neutrino observations favors lower luminosities, which does not correspond to the typical expectation from $\gamma$-ray observations., Published by EDP Sciences, Les Ulis
Published: 2018
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16. Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Author: ANTARES, IceCube, Auger, Pierre, Scientific, Ligo, Virgo Collaborations, Albert, A., Andre, M., Anghinolfi, M., Ardid, M., Aubert, J. -J, Aublin, J., Avgitas, T., Baret, B., Barrios-Marti, J., Basa, S., Belhorma, B., Bertin, V., Biagi, S., Bormuth, R., Bourret, S., Bouwhuis, M. C., Branzacs, H., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Cherkaoui El Moursli, R., Chiarusi, T., Circella, M., Coelho, J. A. B., Coleiro, A., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Diaz, A. F., Deschamps, A., Bonis, G., Distefano, C., Di Palma, I., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., El Bojaddaini, I., El Khayati, N., Elsasser, D., Enzenhofer, A., Ettahiri, A., Fassi, F., Felis, I., Fusco, L. A., Gay, P., Giordano, V., Glotin, H., Gregoire, T., Ruiz, R. Gracia, Graf, K., Hallmann, S., Haren, H., Heijboer, A. J., Hello, Y., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., Illuminati, G., James, C. W., Jong, M., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Kiessling, D., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lachaud, C., Lahmann, R., Lef Evre, D., Leonora, E., Lotze, M., Loucatos, S., Marcelin, M., Margiotta, A., Marinelli, A., Martinez-Mora, J. A., Mele, R., Melis, K., Michael, T., Migliozzi, P., Moussa, A., Navas, S., Nezri, E., Organokov, M., Puavualacs, G. E., Pellegrino, C., Perrina, C., Piattelli, P., Popa, V., Pradier, T., Quinn, L., Racca, C., Riccobene, G., Sanchez-Losa, A., Salda Na, M., Salvadori, I., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schussler, F., Sieger, C., Spurio, M., Stolarczyk, Th, Taiuti, M., Tayalati, Y., Trovato, A., Turpin, D., Tonnis, C., Vallage, B., Elewyck, V., Versari, F., Vivolo, D., Vizzoca, A., Wilms, J., Zornoza, J. D., Niga, J. Zu, Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Samarai, I. 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T., Raab, C., Radel, L., Rameez, M., Rawlins, K., Rea, I. C., Reimann, R., Relethford, B., Relich, M., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Salzer, T., Sanchez Herrera, S. E., Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Schlunder, P., Schmidt, T., Schneider, A., Schoenen, S., Schoneberg, S., Schumacher, L., Seckel, D., Seunarine, S., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stasik, A., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stossl, A., Strotjohann, N. L., Stuttard, T., Sullivan, G. W., Sutherland, M., Taboada, I., Tatar, J., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Tevsic, G., Tilav, S., Toale, P. A., Tobin, M. N., Toscano, S., Tosi, D., Tselengidou, M., Tung, C. F., Turcati, A., Turley, C. 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G., Blanco, A., Blazek, J., Bleve, C., Bohavcova, M., Bonifazi, C., Borodai, N., Botti, A. M., Brack, J., Brancus, I., Bretz, T., Bridgeman, A., Briechle, F. L., Buchholz, P., Bueno, A., Buitink, S., Buscemi, M., Caballero-Mora, K. S., Caccianiga, L., Cancio, A., Canfora, F., Caruso, R., Castellina, A., Catalani, F., Cataldi, G., Cazon, L., Chavez, A. G., Chinellato, J. A., Chudoba, J., Clay, R. W., Cobos Cerutti, A. C., Colalillo, R., Coleman, A., Collica, L., Coluccia, M. R., Conceicc Ao, R., Consolati, G., Contreras, F., Cooper, M. J., Coutu, S., Covault, C. E., Croninaltaffiliation Deceased, J., 2016., August, D Amico, S., Daniel, B., Dasso, S., Daumiller, K., Dawson, B. R., Day, J. A., Almeida, R. M., Jong, S. J., Mauro, G., Mello Neto, J. R. T., Mitri, I., Oliveira, J., Souza, V., Debatin, J., Deligny, O., Diaz Castro, M. L., Diogo, F., Dobrigkeit, C., D Olivo, J. C., Dorosti, Q., Dos Anjos, R. C., Dova, M. T., Dundovic, A., Ebr, J., Engel, R., Erdmann, M., Erfani, M., Escobar, C. O., Espadanal, J., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipvcivc, A., Freire, M. M., Fujii, T., Fuster, A., Gaior, R., Garcia, B., Gate, F., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Glas, D., Glaser, C., Golup, G., Gomez Berisso, M., Gomez Vitale, P. F., Gonzalez, N., Gorgi, A., Gottowik, M., Grilloaltaffiliation Deceased, A. F., 2017., February, Grubb, T. D., Guarino, F., Guedes, G. P., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. E., Hojvat, C., Holt, E., Homola, P., Horandel, J. R., Horvath, P., Hrabovsky, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Kaapa, A., Kampert, K. 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S., Radkins, H., Raffai, P., Raja, S., Rajan, C., Rajbhandari, B., Rakhmanov, M., Ramirez, K. E., Ramos-Buades, A., Rapagnani, P., Raymond, V., Razzano, M., Read, J., Regimbau, T., Rei, L., Reid, S., Reitze, D. H., Ren, W., Reyes, S. D., Ricci, F., Ricker, P. M., Rieger, S., Riles, K., Rizzo, M., Robertson, N. A., Robie, R., Robinet, F., Rocchi, A., Rolland, L., Rollins, J. G., Roma, V. J., Romano, R., Romel, C. L., Romie, J. H., Rosinska, D., Ross, M. P., Rowan, S., Rudiger, A., Ruggi, P., Rutins, G., Ryan, K., Sachdev, S., Sadecki, T., Sadeghian, L., Sakellariadou, M., Salconi, L., Saleem, M., Salemi, F., Samajdar, A., Sammut, L., Sampson, L. M., Sanchez, E. J., Sanchez, L. E., Sanchis-Gual, N., Sandberg, V., Sanders, J. R., Sassolas, B., Sathyaprakash, B. S., Saulson, P. R., Sauter, O., Savage, R. L., Sawadsky, A., Schale, P., Scheel, M., Scheuer, J., Schmidt, J., Schmidt, P., Schnabel, R., Schofield, R. M. S., Schonbeck, A., Schreiber, E., Schuette, D., Schulte, B. W., Schutz, B. 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B., Tapai, M., Taracchini, A., Tasson, J. D., Taylor, J. A., Taylor, R., Tewari, S. V., Theeg, T., Thies, F., Thomas, E. G., Thomas, M., Thomas, P., Thorne, K. A., Thrane, E., Tiwari, S., Tiwari, V., Tokmakov, K. V., Toland, K., Tonelli, M., Tornasi, Z., Torres-Forne, A., Torrie, C. I., Toyra, D., Travasso, F., Traylor, G., Trinastic, J., Tringali, M. C., Trozzo, L., Tsang, K. W., Tse, M., Tso, R., Tsukada, L., Tsuna, D., Tuyenbayev, D., Ueno, K., Ugolini, D., Unnikrishnan, C. S., Urban, A. L., Usman, S. A., Vahlbruch, H., Vajente, G., Valdes, G., Bakel, N., Beuzekom, M., Den Brand, J. F. J., Den Broeck, C., Vander-Hyde, D. C., Schaaf, L., Heijningen, J. V., Veggel, A. A., Vardaro, M., Varma, V., Vass, S., Vasuth, M., Vecchio, A., Vedovato, G., Veitch, J., Veitch, P. J., Venkateswara, K., Venugopalan, G., Verkindt, D., Vetrano, F., Vicere, A., Viets, A. D., Vinciguerra, S., Vine, D. J., Vinet, J. -Y, Vitale, S., Vo, T., Vocca, H., Vorvick, C., Vyatchanin, S. P., Wade, A. R., Wade, L. E., Wade, M., Walet, R., Walker, M., Wallace, L., Walsh, S., Wang, G., Wang, H., Wang, J. Z., Wang, W. H., Wang, Y. F., Ward, R. L., Warner, J., Was, M., Watchi, J., Weaver, B., Wei, L. -W, Weinert, M., Weinstein, A. J., Weiss, R., Wen, L., Wessel, E. K., Wessels, P., Westerweck, J., Westphal, T., Wette, K., Whelan, J. T., Whiting, B. F., Whittle, C., Wilken, D., Williams, D., Williams, R. D., Williamson, A. R., Willis, J. L., Willke, B., Wimmer, M. H., Winkler, W., Wipf, C. C., Wittel, H., Woan, G., Woehler, J., Wofford, J., Wong, K. W. K., Worden, J., Wright, J. L., Wu, D. S., Wysocki, D. M., Xiao, S., Yamamoto, H., Yancey, C. C., Yap, M. J., Yazback, M., Yu, Hang, Yu, Haocun, Yvert, M., Zadro Zny, A., Zanolin, M., Zelenova, T., Zendri, J. -P, Zevin, M., Zhang, L., Zhang, M., Zhang, T., Zhang, Y. -H, Zhao, C., Zhou, M., Zhou, Z., Zhu, S. J., Zhu, X. J., Zucker, M. E., Zweizig, J., Centre de Physique des Particules de Marseille ( CPPM ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Aix Marseille Université ( AMU ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), 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'Etudes Spatiales ( CNES ), Géoazur ( GEOAZUR ), Université Nice Sophia Antipolis ( UNS ), Université Côte d'Azur ( UCA ) -Université Côte d'Azur ( UCA ) -Institut national des sciences de l'Univers ( INSU - 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A., Ahlers, M., Ahrens, M., Al Samarai, I., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Argã¼elles, C., Auffenberg, J., Axani, S., Bagherpour, H., Bai, X., Barron, J. P., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Tjus, J. Becker, Becker, K. -. H., Benzvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Bohm, C., Bã¶rner, M., Bos, F., Bose, D., Bã¶ser, S., Botner, O., Bourbeau, E., Bourbeau, J., Bradascio, F., Braun, J., Brayeur, L., Brenzke, M., Bretz, H. -. P., Bron, S., Brostean-Kaiser, J., Burgman, A., Carver, T., Casey, J., Casier, M., Cheung, E., Chirkin, D., Christov, A., Clark, K., Classen, L., Coenders, S., Collin, G. H., Conrad, J. M., Cowen, D. F., Cross, R., Day, M., De AndrÃ©, J. P. A. M., De Clercq, C., Delaunay, J. J., Dembinski, H., De Ridder, S., Desiati, P., De Vries, K. D., De Wasseige, G., De With, M., Deyoung, T., DÃaz-VÃ©lez, J. C., Di Lorenzo, V., Dujmovic, H., Dumm, J. P., Dunkman, M., Dvorak, E., Eberhardt, B., Ehrhardt, T., Eichmann, B., Eller, P., Evenson, P. A., Fahey, S., Fazely, A. R., Felde, J., Filimonov, K., Finley, C., Flis, S., Franckowiak, A., Friedman, E., Fuchs, T., Gaisser, T. K., Gallagher, J., Gerhardt, L., Ghorbani, K., Giang, W., Glauch, T., Glã¼senkamp, T., Goldschmidt, A., Gonzalez, J. G., Grant, D., Griffith, Z., Haack, C., Hallgren, A., Halzen, F., Hanson, K., Hebecker, D., Heereman, D., Helbing, K., Hellauer, R., Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Hokanson-Fasig, B., Hoshina, K., Huang, F., Huber, M., Hultqvist, K., Hã¼nnefeld, M., In, S., Ishihara, A., Jacobi, E., Japaridze, G. S., Jeong, M., Jero, K., Jones, B. J. P., Kalaczynski, P., Kang, W., Kappes, A., Karg, T., Karle, A., Kauer, M., Keivani, A., Kelley, J. L., Kheirandish, A., Kim, J., Kim, M., Kintscher, T., Kiryluk, J., Kittler, T., Klein, S. R., Kohnen, G., Koirala, R., Kolanoski, H., Kã¶pke, L., Kopper, C., Kopper, S., Koschinsky, J. P., Koskinen, D. J., Kowalski, M., Krings, K., Kroll, M., Krã¼ckl, G., Kunnen, J., Kunwar, S., Kurahashi, N., Kuwabara, T., Kyriacou, A., Labare, M., Lanfranchi, J. L., Larson, M. J., Lauber, F., Lesiak-Bzdak, M., Leuermann, M., Liu, Q. R., Lu, L., Lã¼nemann, J., Luszczak, W., Madsen, J., Maggi, G., Mahn, K. B. M., Mancina, S., Maruyama, R., Mase, K., Maunu, R., Mcnally, F., Meagher, K., Medici, M., Meier, M., Menne, T., Merino, G., Meures, T., Miarecki, S., Micallef, J., Momentã©, G., Montaruli, T., Moore, R. W., Moulai, M., Nahnhauer, R., Nakarmi, P., Naumann, U., Neer, G., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Pollmann, A. Obertacke, Olivas, A., O'Murchadha, A., Palczewski, T., Pandya, H., Pankova, D. V., Peiffer, P., Pepper, J. A., De Los Heros, C. PÃ©rez, Pieloth, D., Pinat, E., Plum, M., Pranav, D., Price, P. B., Przybylski, G. T., Raab, C., Rã¤del, L., Rameez, M., Rawlins, K., Rea, I. C., Reimann, R., Relethford, B., Relich, M., Resconi, E., Rhode, W., Richman, M., Robertson, S., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Rysewyk, D., Sã¤lzer, T., Herrera, S. E. Sanchez, Sandrock, A., Sandroos, J., Santander, M., Sarkar, S., Satalecka, K., Schlunder, P., Schmidt, T., Schneider, A., Schoenen, S., Schã¶neberg, S., Schumacher, L., Seckel, D., Seunarine, S., Soedingrekso, J., Soldin, D., Song, M., Spiczak, G. M., Spiering, C., Stachurska, J., Stamatikos, M., Stanev, T., Stasik, A., Stettner, J., Steuer, A., Stezelberger, T., Stokstad, R. G., Stã¶ã l, A., Strotjohann, N. L., Stuttard, T., Sullivan, G. W., Sutherland, M., Taboada, I., Tatar, J., Tenholt, F., Ter-Antonyan, S., Terliuk, A., Teå¡iä , G., Tilav, S., Toale, P. A., Tobin, M. N., Toscano, S., Tosi, D., Tselengidou, M., Tung, C. F., Turcati, A., Turley, C. F., Ty, B., Unger, E., Usner, M., Vandenbroucke, J., Van Driessche, W., Van Eijndhoven, N., Vanheule, S., Van Santen, J., Vehring, M., Vogel, E., Vraeghe, M., Walck, C., Wallace, A., Wallraff, M., Wandler, F. D., Wandkowsky, N., Waza, A., Weaver, C., Weiss, M. J., Wendt, C., Werthebach, J., Westerhoff, S., Whelan, B. J., Wiebe, K., Wiebusch, C. H., Wille, L., Williams, D. R., Wills, L., Wolf, M., Wood, J., Wood, T. R., Woolsey, E., Woschnagg, K., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Yuan, T., Zoll, M., Aab, A., Abreu, P., Aglietta, M., Albuquerque, I. F. M., Albury, J. M., Allekotte, I., Almela, A., Castillo, J. Alvarez, Alvarez-MuÃ±iz, J., Anastasi, G. A., Anchordoqui, L., Andrada, B., Andringa, S., Aramo, C., Arsene, N., Asorey, H., Assis, P., Avila, G., Badescu, A. M., Balaceanu, A., Barbato, F., Luz, R. J. Barreira, Becker, K. H., Bellido, J. A., Berat, C., Bertaina, M. E., Bertou, X., Biermann, P. L., Biteau, J., Blaess, S. 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O., Espadanal, J., Etchegoyen, A., Falcke, H., Farmer, J., Farrar, G., Fauth, A. C., Fazzini, N., Feldbusch, F., Fenu, F., Fick, B., Figueira, J. M., Filipä iä , A., Freire, M. M., Fujii, T., Fuster, A., Gaã¯or, R., Garcãa, B., Gatã©, F., Gemmeke, H., Gherghel-Lascu, A., Ghia, P. L., Giaccari, U., Giammarchi, M., Giller, M., Gå as, D., Glaser, C., Golup, G., Berisso, M. GÃ³mez, Vitale, P. F. GÃ³mez, Gonzã¡lez, N., Gorgi, A., Gottowik, M., Grillo, A. F., Grubb, T. D., Guarino, F., Guedes, G. P., Halliday, R., Hampel, M. R., Hansen, P., Harari, D., Harrison, T. A., Harvey, V. M., Haungs, A., Hebbeker, T., Heck, D., Heimann, P., Herve, A. E., Hojvat, C., Holt, E., Homola, P., Hã¶randel, J. R., Horvath, P., Hrabovskã½, M., Huege, T., Hulsman, J., Insolia, A., Isar, P. G., Jandt, I., Johnsen, J. A., Josebachuili, M., Jurysek, J., Kã¤ã¤pã¤, A., Kampert, K. H., Keilhauer, B., Kemmerich, N., J., Kemp, Kieckhafer, R. M., Klages, H. O., Kleifges, M., Kleinfeller, J., Krause, R., Krohm, N., Kuempel, D., Mezek, G. Kukec, Kunka, N., Awad, A. Kuotb, Lago, B. L., Lahurd, D., Lang, R. G., Lauscher, M., Legumina, R., De Oliveira, M. A. Leigui, Letessier-Selvon, A., Lhenry-Yvon, I., Link, K., Presti, D. Lo, Lopes, L., Lã³pez, R., Casado, A. LÃ³pez, Lorek, R., Luce, Q., Lucero, A., Malacari, M., Mallamaci, M., Mandat, D., Mantsch, P., Mariazzi, A. G., Mariå , I. C., Marsella, G., Martello, D., Martinez, H., MartÃnez Bravo, O., MasÃas Meza, J. J., Mathes, H. J., Mathys, S., Matthews, J., Matthiae, G., Mayotte, E., Mazur, P. O., Medina, C., Medina-Tanco, G., Melo, D., Menshikov, A., Merenda, K. -. D., Michal, S., Micheletti, M. I., Middendorf, L., Miramonti, L., Mitrica, B., Mockler, D., Mollerach, S., Montanet, F., Morello, C., Morlino, G., Mostafã¡, M., Mã¼ller, A. L., Mã¼ller, G., Muller, M. A., Mã¼ller, S., Mussa, R., Naranjo, I., Nellen, L., Nguyen, P. H., Niculescu-Oglinzanu, M., Niechciol, M., Niemietz, L., Niggemann, T., Nitz, D., Nosek, D., Novotny, V., Noå¾ka, L., Nãºã±ez, L. A., Oikonomou, F., Olinto, A., Palatka, M., Pallotta, J., Papenbreer, P., Parente, G., Parra, A., Paul, T., Pech, M., Pedreira, F., Pkala, J., Pelayo, R., PeÃ±a-Rodriguez, J., Pereira, L. A. S., Perlin, M., Perrone, L., Peters, C., Petrera, S., Phuntsok, J., Pierog, T., Pimenta, M., Pirronello, V., Platino, M., Poh, J., Porowski, C., Prado, R. R., Privitera, P., Prouza, M., Quel, E. J., Querchfeld, S., Quinn, S., Ramos-Pollan, R., Rautenberg, J., Ravignani, D., Ridky, J., Riehn, F., Risse, M., Ristori, P., Rizi, V., De Carvalho, W. Rodrigue, Fernandez, G. Rodriguez, Rojo, J. Rodriguez, Roncoroni, M. J., Roth, M., Roulet, E., Rovero, A. C., Ruehl, P., Saffi, S. J., Saftoiu, A., Salamida, F., Salazar, H., Saleh, A., Salina, G., Sã¡nchez, F., Sanchez-Lucas, P., Santos, E. 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E., Zweizig, J., Groupe de Recherche en Physique des Hautes Energies (GRPHE), Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-IUT de Colmar, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), 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), Géoazur (GEOAZUR 7329), 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)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Laboratoire des Sciences de l'Information et des Systèmes (LSIS), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Arts et Métiers Paristech ENSAM Aix-en-Provence-Centre National de la Recherche Scientifique (CNRS), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut méditerranéen d'océanologie (MIO), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), 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, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique subatomique et des technologies associées (SUBATECH), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-Nantes université - UFR des Sciences et des Techniques (Nantes univ - UFR ST), Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ)-Nantes Université - pôle Sciences et technologie, Nantes Université (Nantes Univ)-Nantes Université (Nantes Univ), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire des matériaux avancés (LMA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS), 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), Institut des Fonctions Optiques pour les Technologies de l'informatiON (Institut FOTON), Université de Rennes (UR)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Kastler Brossel (LKB [Collège de France]), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF (institution))-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL), GBR, Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut Universitaire de Technologie de Colmar, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), 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), Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud]), Centre National de la Recherche Scientifique (CNRS)-Arts et Métiers Paristech ENSAM Aix-en-Provence-Université de Toulon (UTLN)-Aix Marseille Université (AMU), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon, Centre National de la Recherche Scientifique (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)-COMUE Université Côte d'Azur (2015-2019) (COMUE 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), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Sorbonne Université (SU)-Collège de France (CdF (institution)), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de Strasbourg (UNISTRA), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Nantes - Faculté des Sciences et des Techniques, Université de Nantes (UN)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), 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), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-Centre National de la Recherche Scientifique (CNRS)-Université Bretagne Loire (UBL)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Collège de France (CdF)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), (Astro)-Particles Physics, Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN)-Aix Marseille Université (AMU)-Institut de Recherche pour le Développement (IRD), Albert, A, Andre, M, Anghinolfi, M, Ardid, M, Aubert, Jj, Aublin, J, Avgitas, T, Baret, B, Barrios-Marti, J, Basa, S, Belhorma, B, Bertin, V, Biagi, S, Bormuth, R, Bourret, S, Bouwhuis, Mc, Branzas, H, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, El Moursli, Rc, Chiarusi, T, Circella, M, Coelho, Jab, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Diaz, Af, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Domi, A, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, El Khayati, N, Elsasser, D, Enzenhofer, A, Ettahiri, A, Fassi, F, Felis, I, Fusco, La, Gay, P, Giordano, V, Glotin, H, Gregoire, T, Ruiz, Rg, Graf, K, Hallmann, S, van Haren, H, Heijboer, Aj, Hello, Y, Hernandez-Rey, Jj, Hossl, J, Hofestadt, J, Illuminati, G, James, Cw, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Kiessling, D, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefevre, D, Leonora, E, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, Ja, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Navas, S, Nezri, E, Organokov, M, Pavalas, Ge, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Quinn, L, Racca, C, Riccobene, G, Sanchez-Losa, A, Saldana, M, Salvadori, I, Samtleben, Dfe, Sanguineti, M, Sapienza, P, Schussler, F, Sieger, C, Spurio, M, Stolarczyk, T, Taiuti, M, Tayalati, Y, Trovato, A, Turpin, D, Tonnis, C, Vallage, B, Van Elewyck, V, Versari, F, Vivolo, D, Vizzoca, A, Wilms, J, Zornoza, Jd, Zuniga, J, Aartsen, Mg, Ackermann, M, Adams, J, Aguilar, Ja, Ahlers, M, Ahrens, M, Al Samarai, I, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Arguelles, C, Auffenberg, J, Axani, S, Bagherpour, H, Bai, X, Barron, Jp, Barwick, Sw, Baum, V, Bay, R, Beatty, Jj, Tjus, Jb, Becker, Kh, Benzvi, S, Berley, D, Bernardini, E, Besson, Dz, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Bohm, C, Borner, M, Bos, F, Bose, D, Boser, S, Botner, O, Bourbeau, E, Bourbeau, J, Bradascio, F, Braun, J, Brayeur, L, Brenzke, M, Bretz, Hp, Bron, S, Brostean-Kaiser, J, Burgman, A, Carver, T, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Clark, K, Classen, L, Coenders, S, Collin, Gh, Conrad, Jm, Cowen, Df, Cross, R, Day, M, de Andre, Jpam, De Clercq, C, Delaunay, Jj, Dembinski, H, De Ridder, S, Desiati, P, de Vries, Kd, de Wasseige, G, de With, M, Deyoung, T, Diaz-Velez, Jc, di Lorenzo, V, Dujmovic, H, Dumm, Jp, Dunkman, M, Dvorak, E, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eller, P, Evenson, Pa, Fahey, S, Fazel, Ar, Felde, J, Filimonov, K, Finley, C, Flis, S, Franckowiak, A, Friedman, E, Fuchs, T, Gaisser, Tk, Gallagher, J, Gerhardt, L, Ghorbani, K, Giang, W, Glauch, T, Glsenkamp, T, Goldschmidt, A, Gonzalez, Jg, Grant, D, Griffith, Z, Haack, C, Hallgren, A, Halzen, F, Hanson, K, Hebecker, D, Heereman, D, Helbing, K, Hellauer, R, Hickford, S, Hignight, J, Hill, Gc, Hoffman, Kd, Hoffmann, R, Hokanson-Fasig, B, Hoshina, K, Huang, F, Huber, M, Hultqvist, 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Yancey, Cc, Yap, Mj, Yazback, M, Yu, H, Yvert, M, Zadrozny, A, Zanolin, M, Zelenova, T, Zendri, Jp, Zevin, M, Zhang, L, Zhang, M, Zhang, T, Zhang, Yh, Zhao, C, Zhou, M, Zhou, Z, Zhu, Sj, Zhu, Xj, Zucker, Me, Zweizig, J, Andre, M., Aubert, J. -J., Barrios-Marti, J., Branzas, H., El Moursli, R. C., Diaz, A. F., Bojaddaini, I. E., Khayati, N. E., Elsasser, D., Enzenhofer, A., Gregoire, T., Ruiz, R. G., Hernandez-Rey, J. J., Hossl, J., Hofestadt, J., Kiessling, D., Lefevre, D., Martinez-Mora, J. A., Pavalas, G. E., Sanchez-Losa, A., Saldana, M., Schussler, F., Stolarczyk, T., Tonnis, C., Zuniga, J., Arguelles, C., Tjus, J. B., Becker, K. -H., Borner, M., Boser, S., Bretz, H. -P., De Andre, J. P. A. M., Diaz-Velez, J. C., Glusenkamp, T., Hunnefeld, M., Kopke, L., Kruckl, G., Lunemann, J., Momente, G., Pollmann, A. O., De Los Heros, C. P., Radel, L., Salzer, T., Herrera, S. E. S., Schoneberg, S., Stossl, A., Tesic, G., Castillo, J. A., Alvarez-Muniz, J., Luz, R. J. B., Bohacova, M., Cerutti, A. C. C., Conceicao, R., Contreras, F., Diaz Castro, M. L., Anjos, R. C. D., Filipcic, A., Gaior, R., Garcia, B., Gate, F., Glas, D., Berisso, M. G., Vitale, P. F. G., Gonzalez, N., Horandel, J. R., Hrabovsky, M., Kaapa, A., Kemp, J., Mezek, G. K., Awad, A. K., De Oliveira, M. A. L., Presti, D. L., Lopez, R., Casado, A. L., Maris, I. C., Martinez Bravo, O., Masias Meza, J. J., Merenda, K. -D., Mostafa, M., Muller, A. L., Muller, G., Muller, S., Nozka, L., Nunez, L. A., Pena-Rodriguez, J., De Carvalho, W. R., Fernandez, G. R., Rojo, J. R., Sanchez, F., Schovanek, P., Schroder, F. G., Schroder, S., Smida, R., Stanic, S., Duran, M. S., Suomijarvi, T., Supik, J., Peixoto, C. J. T., Tome, B., Elipe, G. T., Galicia, J. F. V., Valino, I., Cardenas, B. V., Vazquez, R. A., Veberic, D., Quispe, I. D. V., Villasenor, L., Wiedenski, M., Wilczynski, H., Becsy, B., Bustillo, J. C., Diaz, J. C., Cavaglia, M., Cerda-Duran, P., Cheng, H. -P., Cohadon, P. -F., Cordero-Carrion, I., Coulon, J. -P., Canton, T. D., Dalya, G., Costa, C. F. D. S., De, S., Deleglise, S., Diaz, M. C., Alvarez, M. D., Eggenstein, H. -B., Fournier, J. -D., Ghosh, A., Gonzalez, G., Castro, J. M. G., Haster, C. -J., Isac, J. -M., Jimenez-Forteza, F., Kefelian, F., Kim, C., Kim, Y. -M., Kramer, C., Krolak, A., Luck, H., Hernandez, I. M., Magana-Sandoval, F., Zertuche, L. M., Marka, S., Marka, Z., Marquina, A., Michel, C., Mukherjee, A., Muniz, E. A., Oram, R. J., Pan, H., Pan, H. -W., Purrer, M., Rosinska, D., Rudiger, A., Schonbeck, A., Singh, A., Szczepanczyk, M. J., Tapai, M., Torres-Forne, A., Toyra, D., Vasuth, M., Vicere, A., Vinet, J. -Y., Wade, M., Wei, L. -W., Wessels, P., Yu, H., Zadrozny, A., Zendri, J. -P., Zhang, Y. -H., The LIGO Scientific Collaboration, The Virgo Collaboration, Brã¢nzaåÿ, H., Hã¶ãÿl, J., Kieãÿling, D., Pçžvçžlaåÿ, G. E., Stã¶ãÿl, A., TeÅ¡iÄ‡, G., GÅ‚as, D., Mariåÿ, I. C., WiedeÅ„ski, M., WilczyÅ„ski, H., RosiÅ„ska, D., SzczepaÅ„czyk, M. J., Weãÿels, P., Yu, Hang, Yu, Haocun, André, M., Barrios-Martí, J., Brânzaş, H., Díaz, A. F., Elsässer, D., Enzenhöfer, A., Grégoire, T., Hernández-Rey, J. J., Hößl, J., Hofestädt, J., Kießling, D., Lefèvre, D., Martínez-Mora, J. A., Pǎvǎlaş, G. E., Sánchez-Losa, A., Saldaña, M., Schüssler, F., Tönnis, C., Zúñiga, J., Argüelles, C., Börner, M., Böser, S., De André, J. P. A. M., Díaz-Vélez, J. C., Glüsenkamp, T., Hünnefeld, M., Köpke, L., Krückl, G., Lünemann, J., Momenté, G., Rädel, L., Sälzer, T., Schöneberg, S., Stößl, A., Tešić, G., Alvarez-Muñiz, J., Boháčová, M., Conceição, R., Díaz Castro, M. L., Filipčič, A., Gaïor, R., García, B., Gaté, F., Głas, D., González, N., Guarino, Fausto, Hörandel, J. R., Hrabovský, M., Kääpä, A., López, R., Mariş, I. C., Martínez Bravo, O., Masías Meza, J. J., Mostafá, M., Müller, A. L., Müller, G., Müller, S., Nožka, L., Núñez, L. A., Peña-Rodriguez, J., Sánchez, F., Schovánek, P., Schröder, F. G., Schröder, S., Šmída, R., Stanič, S., Durán, M. S., Suomijärvi, T., Šupík, J., Tomé, B., Valiño, I., Cárdenas, B. V., Vázquez, R. A., Veberič, D., Villaseñor, L., Wiedeński, M., Wilczyński, H., Bécsy, B., Cavaglià, M., Cerdá-Durán, P., Cordero-Carrión, I., Dálya, G., Deléglise, S., DE ROSA, Rosario, Díaz, M. C., Álvarez, M. D., González, G., Jiménez-Forteza, F., Kéfélian, F., Krämer, C., Królak, A., Lück, H., Magaña-Sandoval, F., Márka, S., Márka, Z., Muñiz, E. A., Pan, H. -. W., Pürrer, M., Rosińska, D., Rüdiger, A., Schönbeck, A., Szczepańczyk, M. J., Tápai, M., Torres-Forné, A., Töyrä, D., Vasúth, M., Viceré, A., Weßels, P., Zadrożny, A., Institut Universitaire de Technologie de Colmar-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA)), Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])-Centre National de la Recherche Scientifique (CNRS)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Institut de Recherche pour le Développement (IRD)-Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Toulon (UTLN), École Nationale Supérieure des Sciences Appliquées et de Technologie (ENSSAT)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-Institut National des Sciences Appliquées - Rennes (INSA Rennes), Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Institut National des Sciences Appliquées (INSA)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS)-Université de Rennes 1 (UR1), and Université de Rennes (UNIV-RENNES)
Subjects: neutron star: binary, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], gamma-ray burst: general, EXTENDED EMISSION, binary [neutron star], general [gamma-ray burst], IceCube, particle: acceleration, neutrino, optical, LIGO, gravitational wave, QC, QB, gamma-ray burst: general – gravitational waves – neutrinos, GAMMA-RAY BURSTS, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), energy: high, Physics, Astrophysics::Instrumentation and Methods for Astrophysics, neutrinos, dissipation, Auger, observatory, gravitational waves, high [energy], burst [neutrino], Astrophysics - High Energy Astrophysical Phenomena, GW, Astrophysics::High Energy Astrophysical Phenomena, burst [gamma ray], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, gamma ray: burst, GLAST, GW, Neutrinos, BNS, ddc:530, Neutrinos, capture, Astronomy and Astrophysics, Space and Planetary Science, Astrophysics::Galaxy Astrophysics, ANTARES, gravitational radiation, Astronomy and Astrophysic, VIRGO, Physics and Astronomy, X-RAY, ddc:520, neutrino: burst, BNS, spectrometer, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], acceleration [particle], general, gravitational waves, neutrinos [gamma-ray burst]
Abstract: The Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merger of this binary was also recorded by the Fermi Gamma-ray Burst Monitor (Fermi-GBM), and the Anticoincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory (INTEGRAL), indicating particle acceleration by the source. The precise location of the event was determined by optical detections of emission following the merger. We searched for high-energy neutrinos from the merger in the GeV--EeV energy range using the ANTARES, IceCube, and Pierre Auger Observatories. No neutrinos directionally coincident with the source were detected within $\pm500$ s around the merger time. Additionally, no MeV neutrino burst signal was detected coincident with the merger. We further carried out an extended search in the direction of the source for high-energy neutrinos within the 14-day period following the merger, but found no evidence of emission. We used these results to probe dissipation mechanisms in relativistic outflows driven by the binary neutron star merger. The non-detection is consistent with model predictions of short GRBs observed at a large off-axis angle., Comment: 22 pages, 2 figures
Published: 2017

17. Expected neutrino fluence from short Gamma-Ray Burst 170817A and off-axis angle constraint

Author: Biehl, D, Heinze, J, and Winter, W
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, photon, gravitational radiation, FOS: Physical sciences, burst [gamma ray], sensitivity, time delay, energy [p], production [neutrino], efficiency, emission [gamma ray], ddc:520, High Energy Physics::Experiment, density [radiation], structure, Astrophysics - High Energy Astrophysical Phenomena, detector [neutrino]
Abstract: We compute the expected neutrino fluence from SGRB 170817A, associated with the gravitational wave event GW 170817, directly based on Fermi observations in two scenarios: structured jet and off-axis (observed) top-hat jet. While the expected neutrino fluence for the structured jet case is very small, large off-axis angles imply high radiation densities in the jet, which can enhance the neutrino production efficiency. In the most optimistic allowed scenario, the neutrino fluence can reach only $10^{-4}$ of the sensitivity of the neutrino telescopes. We furthermore demonstrate that the fact that gamma-rays can escape limits the baryonic loading (energy in protons versus photons) and the off-axis angle for the internal shock scenario. In particular, for a baryonic loading of ten, the off-axis angle is more strongly constrained by the baryonic loading than by the time delay between the gravitational wave event and the onset of the gamma-ray emission., 9 pages, 6 figures
Published: 2017
Full Text: View/download PDF

18. Multi-messenger light curves from gamma-ray bursts in the internal shock model

Author: Bustamante, Mauricio, Murase, Kohta, and Winter, Walter
Subjects: ANTARES, Astrophysics::High Energy Astrophysical Phenomena, UHE [cosmic radiation], pi, burst [gamma ray], shock waves, UHE [gamma ray], sensitivity, IceCube, UHE [neutrino], relativistic [jet], production [neutrino], efficiency, muon, time dependence, structure, acceleration [particle], plasma
Abstract: Gamma-ray bursts (GRBs) are promising as sources of neutrinos and cosmic rays. In the internal shock scenario, blobs of plasma emitted from a central engine collide within a relativistic jet and form shocks, leading to particle acceleration and emission. Motivated by present experimental constraints and sensitivities, we improve the predictions of particle emission by investigating time-dependent effects from multiple shocks. We produce synthetic light curves with different variability timescales that stem from properties of the central engine. For individual GRBs, qualitative conclusions about model parameters, neutrino production efficiency, and delays in high-energy gamma rays can be deduced from inspection of the gamma-ray light curves. GRBs with fast time variability without additional prominent pulse structure tend to be efficient neutrino emitters, whereas GRBs with fast variability modulated by a broad pulse structure tend to be inefficient neutrino emitters and produce delayed high-energy gamma-ray signals. Our results can be applied to quantitative tests of the GRB origin of ultra-high-energy cosmic rays, and have the potential to impact current and future multi-messenger searches.
Published: 2016

19. Participation of DESY-Zeuthen in the IceCube project

Author: Biron, A., Boeser, Sebastian, Desiati, P., Gaug, M., Hauschildt, T., Kowalski, M., Leich, H., Leuthold, M., Ribordy, M., Schmidt, T., Spiering, C., Steffen, P., Sudhoff, P., Sulanke, K. H., Wiebusch, C., Wischnewski, R., and Wissing, H.
Subjects: cosmic radiation: particle source, magnetic monopole: search for, cosmic radiation [neutrino], photomultiplier, search for [WIMP], Cherenkov counter: water, water [Cherenkov counter], particle source [cosmic radiation], oscillation [neutrino], search for [magnetic monopole], burst [gamma ray], bibliography, gamma ray: burst, deep underground detector: water, WIMP: search for, neutrino: cosmic radiation, supernova, water [deep underground detector], proposal, neutrino: oscillation, AGN, water [solids], solids: water
Abstract: 129 pp. (2001).
Published: 2001

20. Bounds on Lorentz Invariance Violation from MAGIC Observation of GRB 190114C

Author: M. Peresano, Lara Nava, K. Noda, L. Maraschi, Lorenzo Bellizzi, Elina Lindfors, Daniel Mazin, Sidika Merve Colak, Pratik Majumdar, M. V. Fonseca, L. Pavletić, B. Banerjee, Shunsuke Sakurai, Yating Chai, Stefan Cikota, Pawel Gliwny, M. Vazquez Acosta, Alessandra Lamastra, L. Di Venere, Victoria Moreno, L. Nogués, C. Nigro, U. Colin, David A. Green, Martin Will, Alice Donini, Julian Sitarek, L. A. Antonelli, M. I. Martínez, Kari Nilsson, Jorge Otero-Santos, Seiya Nozaki, Alexander Hahn, Abelardo Moralejo, D. Hadasch, Dominik Baack, D. Ninci, Matteo Cerruti, M. Minev, E. Do Souto Espiñeira, Tomislav Terzić, A. Rugliancich, E. Moretti, Marina Manganaro, Stefano Covino, J. Becerra González, P. G. Prada Moroni, C. Perennes, U. Barres de Almeida, I. Vovk, Yoshiki Ohtani, Daniel Morcuende, Jose Luis Contreras, Jordi Delgado, Kyoshi Nishijima, Daniel Kerszberg, J. M. Paredes, Juan Cortina, Martin Makariev, Fabrizio Tavecchio, M. Palatiello, Alessio Berti, F. Di Pierro, Ž. Bošnjak, Damir Lelas, Victor A. Acciari, D. Dominis Prester, Oscar Blanch, V. D'Elia, Ll. Font, Y. Kajiwara, Antonio Stamerra, Yusuke Suda, Wlodek Bednarek, Nikola Godinovic, Kai Phillip Schmidt, Tomoki Saito, Giovanni Ceribella, Francesco Dazzi, Carlo Vigorito, I. Snidaric, Mosè Mariotti, G. Busetto, Yuki Iwamura, Dorota Sobczyńska, Satoshi Fukami, Camilla Maggio, D. Zarić, N. Torres-Albà, Ferdinando Giordano, J. van Scherpenberg, Daniela Dorner, Davide Depaoli, Marc Ribó, Takeshi Oka, Manuel Delfino, Toshiaki Inada, Bernd Schleicher, Christian Fruck, V. Fallah Ramazani, D. Strom, Jose Miguel Miranda, Ivica Puljak, Junko Kushida, M. Gaug, G. Vanzo, P. Da Vela, Moritz Hütten, John Hoang, Konstancja Satalecka, Hidetoshi Kubo, Ana Babić, F. Leone, Michele Doro, Jürgen Besenrieder, S. Ventura, Karl Mannheim, Saverio Lombardi, J. Herrera, Sanae Inoue, Giacomo D'Amico, Manuela Mallamaci, Alessia Spolon, Léa Jouvin, P. Munar-Adrover, Alicia Fattorini, D. Miceli, T. Surić, Masahiro Teshima, B. Machado de Oliveira Fraga, Elisa Bernardini, T. Schweizer, Vassil Verguilov, F Longo, G. Ferrara, Serena Loporchio, Marie Karjalainen, E. Molina, E. Colombo, B. De Lotto, Dario Hrupec, Stefano Ansoldi, Riccardo Paoletti, Lab Saha, Luca Foffano, M. A. Lopez, N. Giglietto, Simone Mender, Mitsunari Takahashi, R. J. García López, M. Strzys, Y. Kobayashi, A. Arbet Engels, A. De Angelis, Vitaly Neustroev, Tjark Miener, Massimo Persic, David Paneque, Luca Tosti, G. Maneva, Chiara Righi, Adrian Biland, P. Temnikov, Giacomo Bonnoli, J. Rico, Ciro Bigongiari, M. Garczarczyk, R. López-Coto, Wrijupan Bhattacharyya, D. Elsaesser, Pablo Peñil, Saša Mićanović, V. Vitale, Sargis Gasparyan, Wolfgang Rhode, Juan Abel Barrio, Narek Sahakyan, A. López-Oramas, R. Mirzoyan, Kazuma Ishio, Elisa Prandini, Rodolfo Carosi, Ashot Chilingarian, Acciari, V. A., Ansoldi, S., Antonelli, L. A., Arbet Engels, A., Baack, D., Babic, A., Banerjee, B., Barres De Almeida, U., Barrio, J. A., Becerra Gonzalez, J., Bednarek, W., Bellizzi, L., Bernardini, E., Berti, A., Besenrieder, J., Bhattacharyya, W., Bigongiari, C., Biland, A., Blanch, O., Bonnoli, G., Bosnjak, A., Busetto, G., Carosi, R., Ceribella, G., Cerruti, M., Chai, Y., Chilingarian, A., Cikota, S., Colak, S. M., Colin, U., Colombo, E., Contreras, J. L., Cortina, J., Covino, S., D'Amico, G., D'Elia, V., Da Vela, P., Dazzi, F., De Angelis, A., De Lotto, B., Delfino, M., Delgado, J., Depaoli, D., Di Pierro, F., Di Venere, L., Do Souto Espineira, E., Dominis Prester, D., Donini, A., Dorner, D., Doro, M., Elsaesser, D., Fallah Ramazani, V., Fattorini, A., Ferrara, G., Foffano, L., Fonseca, M. V., Font, L., Fruck, C., Fukami, S., Garcia Lopez, R. J., Garczarczyk, M., Gasparyan, S., Gaug, M., Giglietto, N., Giordano, F., Gliwny, P., Godinovic, N., Green, D., Hadasch, D., Hahn, A., Herrera, J., Hoang, J., Hrupec, D., Hutten, M., Inada, T., Inoue, S., Ishio, K., Iwamura, Y., Jouvin, L., Kajiwara, Y., Karjalainen, M., Kerszberg, D., Kobayashi, Y., Kubo, H., Kushida, J., Lamastra, A., Lelas, D., Leone, F., Lindfors, E., Lombardi, S., Longo, F., Lopez, M., Lopez-Coto, R., Lopez-Oramas, A., Loporchio, S., Machado De Oliveira Fraga, B., Maggio, C., Majumdar, P., Makariev, M., Mallamaci, M., Maneva, G., Manganaro, M., Mannheim, K., Maraschi, L., Mariotti, M., Martinez, M., Mazin, D., Mender, S., Micanovic, S., Miceli, D., Miener, T., Minev, M., Miranda, J. M., Mirzoyan, R., Molina, E., Moralejo, A., Morcuende, D., Moreno, V., Moretti, E., Munar-Adrover, P., Neustroev, V., Nigro, C., Nilsson, K., Ninci, D., Nishijima, K., Noda, K., Nogues, L., Nozaki, S., Ohtani, Y., Oka, T., Otero-Santos, J., Palatiello, M., Paneque, D., Paoletti, R., Paredes, J. M., Pavletic, L., Penil, P., Perennes, C., Peresano, M., Persic, M., Prada Moroni, P. G., Prandini, E., Puljak, I., Rhode, W., Ribo, M., Rico, J., Righi, C., Rugliancich, A., Saha, L., Sahakyan, N., Saito, T., Sakurai, S., Satalecka, K., Schleicher, B., Schmidt, K., Schweizer, T., Sitarek, J., Snidaric, I., Sobczynska, D., Spolon, A., Stamerra, A., Strom, D., Strzys, M., Suda, Y., Suric, T., Takahashi, M., Tavecchio, F., Temnikov, P., Terzic, T., Teshima, M., Torres-Alba, N., Tosti, L., Van Scherpenberg, J., Vanzo, G., Vazquez Acosta, M., Ventura, S., Verguilov, V., Vigorito, C. F., Vitale, V., Vovk, I., Will, M., Zaric, D., and Nava, L.
Subjects: Astrophysics and Astronomy, Photon, Gamma ray burst, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics - High Energy Astrophysical Phenomena, GRB190114C, MAGIC, Lorentz Invariance Violation, FOS: Physical sciences, General Physics and Astronomy, burst [gamma ray], astro-ph.HE, 0 [higher-order], Astrophysics, Lorentz covariance, 01 natural sciences, 7. Clean energy, Gamma ray bursts, energy dependence, Astrophysical studies of gravity, Gamma ray astronomy, Quantum gravity, 0103 physical sciences, ddc:530, MAGIC (telescope), Lorentz [invariance], 010306 general physics, Cherenkov radiation, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, velocity [photon], Lorentz [violation], model [quantum gravity], Gamma-ray astronomy, imaging [Cherenkov counter], Speed of light, spectral, Física nuclear, High Energy Astrophysical Phenomena, Gamma-ray burst
Abstract: On January 14, 2019, the Major Atmospheric Gamma Imaging Cherenkov telescopes detected GRB 190114C above 0.2 TeV, recording the most energetic photons ever observed from a gamma-ray burst. We use this unique observation to probe an energy dependence of the speed of light in vacuo for photons as predicted by several quantum gravity models. Based on a set of assumptions on the possible intrinsic spectral and temporal evolution, we obtain competitive lower limits on the quadratic leading order of speed of light modification., 8 pages, 5 figures, Published in Physical Review Letters, Corresponding authors: Tomislav Terzi\'c (tterzic@phy.uniri.hr), Giacomo D'Amico (damico@mppmu.mpg.de), Daniel Kerszberg (dkerszberg@ifae.es), Cedric Perennes (perennes.cedric@gmail.com)
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21. Science with the Cherenkov Telescope Array

Author: Cascone, E., Valore, L., Vallania, P., Valentino, M., Vagnetti, F., Vagelli, V., Umana, G., Tsujimoto, S., Pujadas, I., Trifoglio, M., Trichard, C., Travnicek, P., Tovmassian, G., Tothill, N., Tosti, G., Torresi, E., Torres, D., Tornikoski, M., Tonev, D., Tomastik, J., Tokanai, F., Peixoto, C., Tluczykont, M., Tibaldo, L., Tian, W., Thoudam, S., Testa, V., Teshima, M., Terzic, T., Terrier, R., Terada, Y., Temnikov, P., Tejedor, L., Tayabaly, K., Tavernet, J., Tavecchio, F., Tavani, M., Tajima, H., Tagliaferri, G., Supanitsky, A., Suomijarvi, T., Straumann, U., Stratta, G., Stolarczyk, T., Stephan, M., Stefanik, S., Stawarz, Ł., Starling, R., Stanič, S., Stamerra, A., Sol, H., Slowikowska, A., Sliusar, V., Sitarek, J., Sironi, G., Sillanpää, A., Siejkowski, H., Sidoli, L., Shellard, R., Shalchi, A., Servillat, M., Sergijenko, O., Semikoz, D., Seitenzahl, I., Scuderi, S., Sciacca, E., Schwanke, U., Schussler, F., Schulz, A., Schovanek, P., Schoorlemmer, H., Schneider, M., Schlenstedt, S., Schioppa, E., Saturni, F., Satalecka, K., Sarkar, S., Santander, M., Sano, H., Sanguillon, M., Sangiorgi, P., Sandoval, A., Sandaker, H., Sánchez-Conde, M., Salina, G., Sakurai, S., Sakaki, N., Saito, T., Safi-Harb, S., Sadeh, I., Rulten, C., Rugliancich, A., Rudak, B., Rowell, G., Rovero, A., Rosado, J., Romeo, G., Romano, P., Rojas, G., Vázquez, J., Fernandez, G., Rodriguez, J., Rizi, V., Rivoire, S., Riquelme, M., Rieger, F., Rico, J., Richtler, T., Ribó, M., Ribeiro, D., Rhode, W., Rezaeian, A., Renaud, M., Reisenegger, A., Reimer, A., Reimer, O., Razzaque, S., Rainò, S., Quirrenbach, A., Queiroz, F., Pürckhauer, S., Punch, M., Pühlhofer, G., Prouza, M., Prokoph, H., Prokhorov, D., Principe, G., Prast, J., Prandini, E., Pozo, D., Polo, M., Pohl, M., Pita, S., Pisarski, A., Piano, G., Pfeifer, M., Peyaud, B., Petruk, O., Petrucci, P., Petrashyk, A., Persic, M., Perri, M., Pedaletti, G., Pech, M., PeEr, A., Parsons, R., Pareschi, G., Paredes, J., Naito, T., Nagayoshi, T., Nagataki, S., Nagai, A., Murase, K., Muraishi, H., Murach, T., Mundell, C., Mukherjee, R., Moulin, E., Morselli, A., Morris, P., Morlino, G., Mori, K., Morcuende-Parrilla, D., Moralejo, A., Montaruli, T., Mohrmann, L., Mohammed, M., Moderski, R., Mizuno, T., Mitchell, A., Mirzoyan, R., Mirabal, N., Minaya, I., Meyer, M., Mereghetti, S., Melandri, A., Medina, C., Mazin, D., Maxted, N., Maurin, G., Masuda, S., Masetti, N., Martínez, G., Martínez, M., Martin, P., Martí, J., Markoff, S., Marín, J., Marcowith, A., Mangano, S., Manganaro, M., Maneva, G., Mandat, D., Malaguti, G., Majumdar, P., Maier, G., Maccarone, M., Lyard, E., Luque-Escamilla, P., Lucarelli, F., Lu, C., López-Coto, R., López, M., Longo, F., Lombardi, S., Lohse, T., Lindfors, E., Limon, M., Lico, R., Lenain, J., De Oliveira, M., Lefaucheur, J., Lees, J., Leach, S., Blanc, O., Lapington, J., Lang, R., Lamanna, G., La Palombara, N., Kushida, J., Kuroda, H., Mezek, G., Kubo, H., Krauß, F., Krause, M., Kraus, M., Kosack, K., Komin, N., Kohri, K., Koch, B., Knödlseder, J., Knapp, J., Kisaka, S., Kimura, S., Kimeswenger, S., Kieda, D., Khélifi, B., Kazanas, D., Kawanaka, N., Katz, U., Katagiri, H., Karkar, S., Kaaret, P., Jurysek, J., Jung-Richardt, I., Jean, P., Jankowsky, D., Janecek, P., Jamrozy, M., Iwamura, Y., Ishio, K., Iori, M., Ioka, K., Iocco, F., Inoue, Y., Inoue, T., Inoue, S., Inome, Y., Inada, T., Iarlori, M., Hütten, M., Humensky, T., Hrupec, D., Hrabovsky, M., Hovatta, T., Horvath, P., Horns, D., Hörandel, J., Horan, D., Holder, J., Hofmann, W., Hnatyk, B., Hinton, J., Hermann, G., Helo, J., Heller, M., Hayashida, M., Hayashi, K., Hassan, T., Hardcastle, M., Hara, S., Hadasch, D., Gunji, S., Griffiths, S., Greenshaw, T., Green, A., Granot, J., Grandi, P., Graham, J., Götz, D., González, J., González, M., Gómez-Vargas, G., Goldoni, P., Godinovic, N., Gnatyk, R., Glicenstein, J., Giuliani, A., Giroletti, M., Giro, E., Giordano, F., Giommi, P., Giglietto, N., Giavitto, G., Gerard, L., Gaug, M., Gasparetto, T., Gaskins, J., Garczarczyk, M., López, R., Garcia, B., Gallant, Y., Gadola, A., Gabici, S., Füßling, M., Funk, S., Fukazawa, Y., Fujita, Y., Fruck, C., Coromina, L., Fortson, L., Fornasa, M., Fontaine, G., Fioretti, V., Filipovic, M., Fesquet, M., Ferrand, G., Fernández-Barral, A., Fernandez-Alonso, M., Fegan, S., Fedorova, E., Fasola, G., Farnier, C., Falcone, A., Falceta-Goncalves, D., Fairbairn, M., Evoli, C., Espinoza, C., Ernenwein, J., Elsässer, D., Ekoume, T., Einecke, S., Egberts, K., Eckner, C., Ebr, J., Dwarkadas, V., Dubus, G., Dravins, D., Drass, H., Doro, M., Dorner, D., Prester, D., Domínguez, A., Djannati-Ataï, A., Diebold, S., Dib, C., Díaz, C., Di Venere, L., Di Pierro, F., Di Girolamo, T., Della Volpe, D., Delgado, C., Del Santo, M., Deil, C., Covino, S., Cotter, G., Costantini, H., Costa, A., Cortina, J., Contreras, J., Conrad, J., Connaughton, V., Conforti, V., Colin, P., Colafrancesco, S., Coco, V., Cieślar, M., Chudoba, J., 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J., Orito, R., Orienti, M., Ong, R., Okumura, A., Okazaki, N., Ohm, S., Ohishi, M., Ohira, Y., Oakes, L., OBrien, P., Nozaki, S., Novosyadlyj, B., Nosek, D., Noda, K., Nishijima, K., Nikołajuk, M., Nieto, D., Niemiec, J., Nakamura, Y., Nakamori, T., Asano, K., Arrabito, L., Arqueros, F., Armstrong, T., Araya, M., Aramo, C., Antolini, E., Ambrosi, G., Amato, E., Alispach, C., Alfaro, J., Alfaro, R., Agudo, I., Zhdanov, V.I., Zdziarski, A.A., Williams, D.A., Watson, J.J., Ward, J.E., Wagner, S.J., Vettolani, G.P., Varner, G.S., Torres, D.F., Todero Peixoto, C.J., Tejedor, L.A., Tavernet, J.-P., Supanitsky, A.D., Shellard, R.C., Rovero, A.C., Vázquez, J.J., Rezaeian, A.H., Parsons, R.D., Paredes, J.M., Osborne, J.P., Ong, R.A., De Souza, V., De Persio, F., De Palma, F., Wilhelmi, E., De Naurois, M., De Lucia, M., De Luca, A., De Lotto, B., Lopez, R., De La Calle, I., Pino, E., De Franco, A., De Cesare, G., Anjos, R., De Angelis, A., Dazzi, F., Dawson, B., Davids, I., Daniel, M., DUrso, D., DAvanzo, P., DAmmando, F., DAì, A., Cumani, P., Cuevas, O., Cuadra, J., Crocker, R., Minaya, I.A., Maccarone, M.C., Luque-Escamilla, P.L., Lenain, J.-P., De Oliveira M.A., Leigui, Lees, J.-P., Lang, R.G., Kukec Mezek, G., Kieda, D.B., Humensky, T.B., De Los Reyes Lopez, R., De Gouveia Dal Pino, E.M., Contreras, J.L., Chaves, R.C., Brown, A.M., Schioppa, E.J., Saturni, F.G., Bernardini, M.G., Barrio, J.A., Barres De Almeida, U., Antonelli, L.A., Amans, J.-P., Alves Batista, R., Al Samarai, I., Acharya, B.S., Helo, J.C., Hardcastle, M.J., Green, A.J., González, J.M., González, M.M., Glicenstein, J.-F., Ernenwein, J.-P., Ekoume, T.R., Dwarkadas, V.V., Dominis Prester, D., Chaves, R., Brown, A., Bernardini, M., Barrio, J., De Almeida, U., Antonelli, L., Amans, J., Batista, R., Samarai, I., Acharya, B., Consortium, The Cherenkov, Zorn, J., Ziegler, A., Zhdanov, V., Zechlin, H., Zech, A., Zdziarski, A., Zavrtanik, D., Zavrtanik, M., Zanin, R., Zandanel, F., Zampieri, L., Zaharijas, G., Zacharias, M., Yoshikoshi, T., Yoshiike, S., Yoshida, T., Yang, L., Yanagita, S., Yamazaki, R., Yamamoto, T., Wood, M., Wischnewski, R., Williams, D., Will, M., Wilcox, P., Wierzcholska, A., White, R., White, M., Werner, F., Watson, J., Warren, D., Ward, J., Walter, R., Wagner, R., Wagner, S., Vuillaume, T., Vrastil, M., Vorobiov, S., Vollhardt, A., Voelk, H., Villanueva, J., Vigorito, C., Viana, A., Vettolani, G., Verzi, V., Vergani, S., Veres, P., Vercellone, S., Vega, A., Vecchi, M., Acosta, M., Vassiliev, V., Vasileiadis, G., Varner, G., Vandenbroucke, J., Van Eldik, C., Cherenkov Telescope Array Consortium, The, Acharya, B. S., Agudo, I., Al Samarai, I., Alfaro, R., Alfaro, J., Alispach, C., Alves Batista, R., Amans, J. -P., Amato, E., Ambrosi, G., Antolini, E., Antonelli, L. A., Aramo, C., Araya, M., Armstrong, T., Arqueros, F., Arrabito, L., Asano, K., Ashley, M., Backes, M., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Bamba, A., Barkov, M., Barres de Almeida, U., Barrio, J. A., Bastieri, D., Becherini, Y., Belfiore, A., Benbow, W., Berge, D., Bernardini, E., Bernardini, M. G., Bernardos, M., Bernlöhr, K., Bertucci, B., Biasuzzi, B., Bigongiari, C., Biland, A., Bissaldi, E., Biteau, J., Blanch, O., Blazek, J., Boisson, C., Bolmont, J., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonnoli, G., Bosnjak, Z., Böttcher, M., Braiding, C., Bregeon, J., Brill, A., Brown, A. M., Brun, P., Brunetti, G., Buanes, T., Buckley, J., Bugaev, V., Bühler, R., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Canestrari, R., Capalbi, M., Capitanio, F., Caproni, A., Caraveo, P., Cárdenas, V., Carlile, C., Carosi, R., Carquín, E., Carr, J., Casanova, S., Cascone, E., Catalani, F., Catalano, O., Cauz, D., Cerruti, M., Chadwick, P., Chaty, S., Chaves, R. C. G., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Christov, A., Chudoba, J., Cieślar, M., Coco, V., Colafrancesco, S., Colin, P., Conforti, V., Connaughton, V., Conrad, J., Contreras, J. L., Cortina, J., Costa, A., Costantini, H., Cotter, G., Covino, S., Crocker, R., Cuadra, J., Cuevas, O., Cumani, P., D'Aì, A., D'Ammando, F., D'Avanzo, P., D'Urso, D., Daniel, M., Davids, I., Dawson, B., Dazzi, F., De Angelis, A., de Cássia dos Anjos, R., De Cesare, G., De Franco, A., de Gouveia Dal Pino, E. M., de la Calle, I., de los Reyes Lopez, R., De Lotto, B., De Luca, A., De Lucia, M., de Naurois, M., de Oña Wilhelmi, E., De Palma, F., De Persio, F., de Souza, V., Deil, C., Del Santo, M., Delgado, C., della Volpe, D., Di Girolamo, T., Di Pierro, F., Di Venere, L., Díaz, C., Dib, C., Diebold, S., Djannati-Ataï, A., Domínguez, A., Dominis Prester, D., Dorner, D., Doro, M., Drass, H., Dravins, D., Dubus, G., Dwarkadas, V. V., Ebr, J., Eckner, C., Egberts, K., Einecke, S., Ekoume, T. R. 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C., Hermann, G., Hinton, J., Hnatyk, B., Hofmann, W., Holder, J., Horan, D., Hörandel, J., Horns, D., Horvath, P., Hovatta, T., Hrabovsky, M., Hrupec, D., Humensky, T. B., Hütten, M., Iarlori, M., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Iocco, F., Ioka, K., Iori, M., Ishio, K., Iwamura, Y., Jamrozy, M., Janecek, P., Jankowsky, D., Jean, P., Jung-Richardt, I., Jurysek, J., Kaaret, P., Karkar, S., Katagiri, H., Katz, U., Kawanaka, N., Kazanas, D., Khélifi, B., Kieda, D. B., Kimeswenger, S., Kimura, S., Kisaka, S., Knapp, J., Knödlseder, J., Koch, B., Kohri, K., Komin, N., Kosack, K., Kraus, M., Krause, M., Krauß, F., Kubo, H., Kukec Mezek, G., Kuroda, H., Kushida, J., La Palombara, N., Lamanna, G., Lang, R. G., Lapington, J., Le Blanc, O., Leach, S., Lees, J. -P., Lefaucheur, J., Leigui de Oliveira, M. A., Lenain, J. -P., Lico, R., Limon, M., Lindfors, E., Lohse, T., Lombardi, S., Longo, F., López, M., López-Coto, R., Lu, C. -C., Lucarelli, F., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maier, G., Majumdar, P., Malaguti, G., Mandat, D., Maneva, G., Manganaro, M., Mangano, S., Marcowith, A., Marín, J., Markoff, S., Martí, J., Martin, P., Martínez, M., Martínez, G., Masetti, N., Masuda, S., Maurin, G., Maxted, N., Mazin, D., Medina, C., Melandri, A., Mereghetti, S., Meyer, M., Minaya, I. A., Mirabal, N., Mirzoyan, R., Mitchell, A., Mizuno, T., Moderski, R., Mohammed, M., Mohrmann, L., Montaruli, T., Moralejo, A., Morcuende-Parrilla, D., Mori, K., Morlino, G., Morris, P., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Murach, T., Muraishi, H., Murase, K., Nagai, A., Nagataki, S., Nagayoshi, T., Naito, T., Nakamori, T., Nakamura, Y., Niemiec, J., Nieto, D., Nikołajuk, M., Nishijima, K., Noda, K., Nosek, D., Novosyadlyj, B., Nozaki, S., O'Brien, P., Oakes, L., Ohira, Y., Ohishi, M., Ohm, S., Okazaki, N., Okumura, A., Ong, R. A., Orienti, M., Orito, R., Osborne, J. P., Ostrowski, M., Otte, N., Oya, I., Padovani, M., Paizis, A., Palatiello, M., Palatka, M., Paoletti, R., Paredes, J. M., Pareschi, G., Parsons, R. D., Pe'Er, A., Pech, M., Pedaletti, G., Perri, M., Persic, M., Petrashyk, A., Petrucci, P., Petruk, O., Peyaud, B., Pfeifer, M., Piano, G., Pisarski, A., Pita, S., Pohl, M., Polo, M., Pozo, D., Prandini, E., Prast, J., Principe, G., Prokhorov, D., Prokoph, H., Prouza, M., Pühlhofer, G., Punch, M., Pürckhauer, S., Queiroz, F., Quirrenbach, A., Rainò, S., Razzaque, S., Reimer, O., Reimer, A., Reisenegger, A., Renaud, M., Rezaeian, A. H., Rhode, W., Ribeiro, D., Ribó, M., Richtler, T., Rico, J., Rieger, F., Riquelme, M., Rivoire, S., Rizi, V., Rodriguez, J., Rodriguez Fernandez, G., Rodríguez Vázquez, J. J., Rojas, G., Romano, P., Romeo, G., Rosado, J., Rovero, A. C., Rowell, G., Rudak, B., Rugliancich, A., Rulten, C., Sadeh, I., Safi-Harb, S., Saito, T., Sakaki, N., Sakurai, S., Salina, G., Sánchez-Conde, M., Sandaker, H., Sandoval, A., Sangiorgi, P., Sanguillon, M., Sano, H., Santander, M., Sarkar, S., Satalecka, K., Saturni, F. G., Schioppa, E. J., Schlenstedt, S., Schneider, M., Schoorlemmer, H., Schovanek, P., Schulz, A., Schussler, F., Schwanke, U., Sciacca, E., Scuderi, S., Seitenzahl, I., Semikoz, D., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Sidoli, L., Siejkowski, H., Sillanpää, A., Sironi, G., Sitarek, J., Sliusar, V., Slowikowska, A., Sol, H., Stamerra, A., Stanič, S., Starling, R., Stawarz, Ł., Stefanik, S., Stephan, M., Stolarczyk, T., Stratta, G., Straumann, U., Suomijarvi, T., Supanitsky, A. D., Tagliaferri, G., Tajima, H., Tavani, M., Tavecchio, F., Tavernet, J. -P., Tayabaly, K., Tejedor, L. A., Temnikov, P., Terada, Y., Terrier, R., Terzic, T., Teshima, M., Testa, V., Thoudam, S., Tian, W., Tibaldo, L., Tluczykont, M., Todero Peixoto, C. J., Tokanai, F., Tomastik, J., Tonev, D., Tornikoski, M., Torres, D. F., Torresi, E., Tosti, G., Tothill, N., Tovmassian, G., Travnicek, P., Trichard, C., Trifoglio, M., Troyano Pujadas, I., Tsujimoto, S., Umana, G., Vagelli, V., Vagnetti, F., Valentino, M., Vallania, P., Valore, L., van Eldik, C., Vandenbroucke, J., Varner, G. S., Vasileiadis, G., Vassiliev, V., Vázquez Acosta, M., Vecchi, M., Vega, A., Vercellone, S., Veres, P., Vergani, S., Verzi, V., Vettolani, G. P., Viana, A., Vigorito, C., Villanueva, J., Voelk, H., Vollhardt, A., Vorobiov, S., Vrastil, M., Vuillaume, T., Wagner, S. J., Wagner, R., Walter, R., Ward, J. E., Warren, D., Watson, J. J., Werner, F., White, M., White, R., Wierzcholska, A., Wilcox, P., Will, M., Williams, D. A., Wischnewski, R., Wood, M., Yamamoto, T., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zaharijas, G., Zampieri, L., Zandanel, F., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A. A., Zech, A., Zechlin, H., Zhdanov, V. I., Ziegler, A., Zorn, J., Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), 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), 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, Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Département de Physique des Particules (ex SPP) (DPP), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), CTA Consortium, Galaxies, Etoiles, Physique, Instrumentation (GEPI), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Arcetri (OAA), Istituto Nazionale di Astrofisica (INAF), Istituto Nazionale di Fisica Nucleare, Sezione di Perugia (INFN, Sezione di Perugia), Istituto Nazionale di Fisica Nucleare (INFN), Departamento de Física Atómica, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), College of Science and Engineering, Aoyama Gakuin University (AGU), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Instituto de Fisica Corpuscular (IFIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Universitat de València (UV), 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), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Istituto di Radioastronomia [Bologna] (IRA), University of Naples Federico II = Università degli studi di Napoli Federico II, Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, INAF - Osservatorio Astronomico di Padova (OAPD), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ISDC Data Centre for Astrophysics, Université de Genève = University of Geneva (UNIGE), Département de Physique Nucléaire et Corpusculaire [Genève] (DPNC), Universities Space Research Association (USRA), Universidad Complutense de Madrid = Complutense University of Madrid [Madrid] (UCM), INAF - Osservatorio Astronomico di Brera (OAB), Istituto di Astrofisica Spaziale e Fisica cosmica - Roma (IASF-Roma), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Dipartimento di Fı'sica Generale dell'Università, Istituto Nazionale di Fisica Nucleare, sezione di Bari (INFN, sezione di Bari), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Institut für Theoretische Physik und Astrophysik [Würzburg], Julius-Maximilians-Universität Würzburg (JMU), Jodrell Bank Centre for Astrophysics (JBCA), University of Manchester [Manchester], Institut des sciences du végétal (ISV), Centre National de la Recherche Scientifique (CNRS), Institut de Física d’Altes Energies [Barcelone] (IFAE), Universitat Autònoma de Barcelona (UAB), Agenzia Spaziale Italiana (ASI), APC - Astrophysique des Hautes Energies (APC - AHE), 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)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-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)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Texas A&M University System, Istituto di Astrofisica Spaziale e Fisica cosmica - Bologna (IASF-Bo), Department of Natural Sciences [Ra'anana}, Open University of Israël, University of Hertfordshire [Hatfield] (UH), Deutsches Elektronen-Synchrotron [Zeuthen] (DESY), Helmholtz-Gemeinschaft = Helmholtz Association, Solar-Terrestrial Environment Laboratory [Nagoya] (STEL), Nagoya University, Laboratoire de l'Accélérateur Linéaire (LAL), Radboud University [Nijmegen], Metsähovi Radio Observatory, Aalto University, Humboldt University Of Berlin, The University of Tokyo (UTokyo), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), 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), Department of Physics and Astronomy [Iowa City], University of Iowa [Iowa City], Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Max-Planck-Institut für Extraterrestrische Physik (MPE), INAF- Milano, Università degli Studi di Udine - University of Udine [Italie], Dipartimento di Fisica [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Astronomical Institute Anton Pannekoek (AI PANNEKOEK), University of Amsterdam [Amsterdam] (UvA), Istituto di Astrofisica Spaziale e Fisica Cosmica - Milano (IASF-MI), NASA Goddard Space Flight Center (GSFC), Institute for Physical Research (IPR), National Academy of Sciences of the Republic of Armenia [Yerevan] (NAS RA), Dept. of Physics, University of Wisconsin-Madison, Infrared Processing and Analysis Center (IPAC), California Institute of Technology (CALTECH), KEK (High energy accelerator research organization), Department of Physics [Tokyo], Tokyo Institure of Technology, Istituto di Radioastronomia INAF, Department of Physics and Astronomy [Leicester], University of Leicester, Departament d'Astronomia i Meteorologia [Barcelona] (DAM), Universitat de Barcelona (UB), IEEC-CSIC, INAF - Osservatorio Astronomico di Trieste (OAT), DLR Institut für Physik der Atmosphäre (IPA), Deutsches Zentrum für Luft- und Raumfahrt [Oberpfaffenhofen-Wessling] (DLR), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Centro de Ciencias de la Atmosfera [Mexico], Universidad Nacional Autónoma de México = National Autonomous University of Mexico (UNAM), Technische Universität Dortmund [Dortmund] (TU), Institut de Ciencies del Cosmos (ICCUB), International Agency for Cancer Research (IACR), School of Chemistry and Physics, University of Adelaide, Copernicus Astronomical Center of the Polish Academy of Sciences (CAMK), Polish Academy of Sciences (PAN), Centro de Ciencias Aplicadas y Desarrollo Tecnológico, University of Oxford, AGH University of Science and Technology [Krakow, PL] (AGH UST), Dipartimento di Fisica 'Giuseppe Occhialini' = Department of Physics 'Giuseppe Occhialini' [Milano-Bicocca], Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Department of Plant Sciences [Univ California Davis] (Plant - UC Davis), University of California [Davis] (UC Davis), University of California (UC)-University of California (UC), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institute for Climate and Atmospheric Science [Leeds] (ICAS), School of Earth and Environment [Leeds] (SEE), University of Leeds-University of Leeds, Antarctic Research a European Network for Astrophysics (ARENA), Institute of Atmospheric Physics [Prague] (IAP), Czech Academy of Sciences [Prague] (CAS), University of California (UC), Laboratoire d'études en Géophysique et océanographie spatiales (LEGOS), Instituto Nacional de Técnica Aeroespacial (INTA), Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Istituto Nazionale di Fisica Nucleare, Sezione di Trieste (INFN, Sezione di Trieste), Jozef Stefan Institute [Ljubljana] (IJS), Istituto di Astrofisica Spaziale e Fisica cosmica - Palermo (IASF-Pa), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), National Institute for Nuclear Physics (INFN), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Consejo Superior de Investigaciones Científicas [Spain] (CSIC)-Universitat de València (UV), University of Naples Federico II, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), University of Geneva [Switzerland], Université de Genève (UNIGE), Complutense University of Madrid (UCM), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Bureau d'Économie Théorique et Appliquée (BETA), Institut National de la Recherche Agronomique (INRA)-Université de Strasbourg (UNISTRA)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut für Theoretische Physik und Astrophysik [Wurzburg], Julius-Maximilians-Universität Würzburg [Wurtzbourg, Allemagne] (JMU), Jodrell Bank Centre for Astrophysics, Universitat Autònoma de Barcelona [Barcelona] (UAB), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Helmholtz-Gemeinschaft, Radboud university [Nijmegen], Humboldt Universität zu Berlin, The University of Tokyo, Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Roma La Sapienza], Università degli Studi di Roma 'La Sapienza' [Rome], National Academy of Sciences of Armenia, CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA, CALTECH, Ctr Infrared Proc & Anal, Pasadena, High Energy Accelerator Research Organization (KEK), University of Tsukuba, Universidad Nacional Autónoma de México (UNAM), University of Oxford [Oxford], Dip. di Fisica 'Occhialini' - Università degli Studi di Milano-Bicocca Piazza della Scienza, Department of Plant Sciences [Davis, CA], University of California-University of California, INAF-OAB, Czech Academy of Sciences [Prague] (ASCR), University of California, Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire Midi-Pyrénées (OMP), Observatoire de Paris - Site de Meudon (OBSPM), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Département de Physique des Particules (ex SPP) (DPhP), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Humboldt-Universität zu Berlin, Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome], Università degli Studi di Milano-Bicocca [Milano] (UNIMIB), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, 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, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)
Subjects: propagation [photon], photon: propagation, Cherenkov Telescope Array, magnetic field, 01 natural sciences, thermal, Observatory, formation [star], HESS, site, cluster, ddc:522.6862, media_common, pulsar, High Energy Astrophysical Phenomena (astro-ph.HE), [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::Instrumentation and Methods for Astrophysics, star: formation, relativistic [jet], CERN LHC Coll, binary [gamma ray], cosmic radiation [electron], axion-like particles, violation, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, performance, Astrophysics and Astronomy, bepress|Physical Sciences and Mathematics|Physics, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, burst [gamma ray], Higgs particle, invariance: Lorentz, X-ray, ionization, supernova, cosmic radiation: UHE, Lorentz [invariance], AGN, Instrumentation and Methods for Astrophysics (astro-ph.IM), CTA, 010308 nuclear & particles physics, Astronomy, sensitivity, Universe, angular resolution, gamma ray: VHE, quantum gravity, galaxy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], HAWC, Computer science, VHE [gamma ray], feedback, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), ultraviolet, black hole, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], cloud, acceleration [hadron], neutron star, 010303 astronomy & astrophysics, astro-ph.HE, radio wave, COSMIC cancer database, imaging, observatory, Supernova, annihilation, bepress|Physical Sciences and Mathematics|Physics|Elementary Particles and Fields and String Theory, infrared, Particle Physics - Experiment, accelerator, WIMP, Ground-based gamma-ray astronomy, Dark matter, UHE [cosmic radiation], FOS: Physical sciences, gamma ray: burst, GLAST, dark matter, jet: relativistic, blazar, target, hadron: acceleration, 0103 physical sciences, 522.6862, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], TeV gamma-ray astronomy, hep-ex, Gravitational wave, background, gravitational radiation, electron: cosmic radiation, gamma ray: binary, redshift, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], monitoring, Sky, bepress|Physical Sciences and Mathematics|Astrophysics and Astronomy, astro-ph.IM
Abstract: Singapur : WORLD SCIENTIFIC, Cherenkov Telescope Array (CTA) 211 pp. (2017). doi:10.1142/10986, The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. The scientific potential of CTA is extremely broad: from understanding the role of relativistic cosmic particles to the search for dark matter. CTA is an explorer of the extreme universe, probing environments from the immediate neighbourhood of black holes to cosmic voids on the largest scales. Covering a huge range in photon energy from 20 GeV to 300 TeV, CTA will improve on all aspects of performance with respect to current instruments. The observatory will operate arrays on sites in both hemispheres to provide full sky coverage and will hence maximize the potential for the rarest phenomena such as very nearby supernovae, gamma-ray bursts or gravitational wave transients. With 99 telescopes on the southern site and 19 telescopes on the northern site, flexible operation will be possible, with sub-arrays available for specific tasks. CTA will have important synergies with many of the new generation of major astronomical and astroparticle observatories. Multi-wavelength and multi-messenger approaches combining CTA data with those from other instruments will lead to a deeper understanding of the broad-band non-thermal properties of target sources. The CTA Observatory will be operated as an open, proposal-driven observatory, with all data available on a public archive after a pre-defined proprietary period. Scientists from institutions worldwide have combined together to form the CTA Consortium. This Consortium has prepared a proposal for a Core Programme of highly motivated observations. The programme, encompassing approximately 40% of the available observing time over the first ten years of CTA operation, is made up of individual Key Science Projects (KSPs), which are presented in this document., Published by WORLD SCIENTIFIC, Singapur

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21 results on '"burst [gamma ray]"'

1. Multicollision Internal Shock Lepto-hadronic Models for Energetic Gamma-Ray Bursts (GRBs)

2. Multi-messenger Model for the Prompt Emission from GRB 221009A

3. Limits on Neutrino Emission from GRB 221009A from MeV to PeV Using the IceCube Neutrino Observatory

4. Systematic parameter space study for the UHECR origin from GRBs in models with multiple internal shocks

5. External Inverse-Compton and Proton Synchrotron Emission from the Reverse Shock as the Origin of VHE Gamma-Rays from the Hyper-Bright GRB 221009A

6. Deep Learning Transient Detection with VERITAS

7. The H.E.S.S. Gravitational Wave Rapid Follow-up Program during O2 and O3

8. VTSCat: The VERITAS Catalog of Gamma-Ray Observations

9. Observation of burst activity from SGR1935+2154 associated to first galactic FRB with H.E.S.S

10. Realtime follow-up of astrophysical transients with the IceCube Neutrino Observatory

11. Ultra-high-energy cosmic-ray nuclei and neutrinos in models of gamma-ray bursts and extragalactic propagation

12. Probing the Magnetic Field in the GW170817 Outflow Using H.E.S.S. Observations

13. Unified thermal model for photohadronic neutrino production in astrophysical sources

14. Determining the fraction of cosmic-ray protons at ultra-high energies with cosmogenic neutrinos

15. Cosmic ray and neutrino emission from gamma-ray bursts with a nuclear cascade

16. Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

17. Expected neutrino fluence from short Gamma-Ray Burst 170817A and off-axis angle constraint

18. Multi-messenger light curves from gamma-ray bursts in the internal shock model

19. Participation of DESY-Zeuthen in the IceCube project

20. Bounds on Lorentz Invariance Violation from MAGIC Observation of GRB 190114C

21. Science with the Cherenkov Telescope Array

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