Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Arjen van Vliet"'
Publikováno v:
The Astrophysical Journal, Vol 953, Iss 2, p 129 (2023)
The Pierre Auger Observatory (PAO) and Telescope Array (TA) collaborations report significant differences in the observed energy spectra of ultra-high-energy cosmic rays (UHECRs) above 30 EeV. In this work we present a joint fit of TA and PAO data us
Externí odkaz:
https://doaj.org/article/5c2d7c5e792041fc833777739a9a9303
Publikováno v:
Monthly notices of the Royal Astronomical Society 517(2), 2534-2545 (2022). doi:10.1093/mnras/stac2778
Monthly notices of the Royal Astronomical Society 517(2), 2534 - 2545 (2022). doi:10.1093/mnras/stac2778
We consider the synchrotron emission from electrons out in the Galactic halo bubble region where the Fermi bubble structures reside. Utilisi
We consider the synchrotron emission from electrons out in the Galactic halo bubble region where the Fermi bubble structures reside. Utilisi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ab1ad86abe3671aab5ad4d737af4a23
Autor:
Rafael Alves Batista, Julia Becker Tjus, Julien Dörner, Andrej Dundovic, Björn Eichmann, Antonius Frie, Christopher Heiter, Mario R. Hoerbe, Karl-Heinz Kampert, Lukas Merten, Gero Müller, Patrick Reichherzer, Andrey Saveliev, Leander Schlegel, Günter Sigl, Arjen van Vliet, Tobias Winchen
Publikováno v:
Journal of Cosmology and Astroparticle Physics, 2022, 1-33
Journal of cosmology and astroparticle physics : JCAP 9, 035 (2022). doi:10.1088/1475-7516/2022/09/035
Journal of Cosmology and Astroparticle Physics, 2022, 9, pp. 1-33
JCAP
JCAP, 2022, 09, pp.035. ⟨10.1088/1475-7516/2022/09/035⟩
Journal of cosmology and astroparticle physics : JCAP 9, 035 (2022). doi:10.1088/1475-7516/2022/09/035
Journal of Cosmology and Astroparticle Physics, 2022, 9, pp. 1-33
JCAP
JCAP, 2022, 09, pp.035. ⟨10.1088/1475-7516/2022/09/035⟩
The landscape of high- and ultra-high-energy astrophysics has changed in the last decade, largely due to the inflow of data collected by large-scale cosmic-ray, gamma-ray, and neutrino observatories. At the dawn of the multimessenger era, the interpr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2534f5bc72f329777291ec4eae5a7ab
http://hdl.handle.net/2066/283217
http://hdl.handle.net/2066/283217
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Publikováno v:
Physical review letters 126(19), 191101 (1-6) (2021). doi:10.1103/PhysRevLett.126.191101
We demonstrate that a population of active galactic nuclei (AGN) can describe the observed spectrum of ultra-high-energy cosmic rays (UHECRs) at and above the ankle, and that the dominant contribution comes from low-luminosity BL Lacertae objects. An
Autor:
Günter Sigl, Julien Dörner, Arjen van Vliet, Rafael Alves Batista, Leander Schlegel, Christopher Heiter, Gero Müller, Mario R. Hoerbe, Björn Eichmann, Andrey Saveliev, Andrej Dundovic, Patrick Reichherzer, Karl-Heinz Kampert, Julia Becker Tjus, Lukas Merten, Tobias Winchen, Antonius Frie
Publikováno v:
PoS
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.978, ⟨10.22323/1.395.0978⟩
Scopus-Elsevier
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.978, ⟨10.22323/1.395.0978⟩
Scopus-Elsevier
The landscape of high- and ultra-high-energy astrophysics has changed in the last decade, in large part owing to the inflow of high-quality data collected by present cosmic-ray, gamma-ray, and neutrino observatories. At the dawn of the multimessenger
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ddca1c0cc1e6de621918f34d2cdaca4
Autor:
Jaroslaw Stasielak, Ana Martina Botti, Marcus Niechciol, Alberto Daniel Supanitsky, Alexey Yushkov, Petr Schovánek, Pavel Horváth, Pedro Assis, Nataliia Borodai, Luis Lopes, Luis Nunez, Carla Bleve, Alberto Blanco, Katharine Mulrey, Antonella Castellina, Francesca Zuccarello, Felicia Carla Tiziana Barbato, Emanuele De Vito, Jose Alfredo Bellido Caceres, Fausto Guarino, Jeffrey Brack, Kai Daumiller, Dariusz Gora, Christian Sarmiento-Cano, Alessio Gorgi, Peter Biermann, Teresa Bister, LORENZO CACCIANIGA, Beatriz Garcia, Bruce Dawson, Alena Bakalova, MASSIMO MASTRODICASA, Edivaldo Moura Santos, Stijn Buitink, Bernardo Tomé, Ana Laura Müller, Mario BUSCEMI, Francesco Salamida, Johannes Hulsman, Henryk Wilczyński, Michael Unger, Ronald Cintra Shellard, Miguel Mostafa, Achille Nucita, Frederic Sarazin, Paul Mantsch, Ruben Conceição, Roger Clay, Lukáš Václavek, Giovanni Marsella, Markus Roth, Jakub Jurysek, Lorenzo Cazon, Eva Dos Santos, Corbin Covault, Francesco Fenu, Dalibor Nosek, Rossella Caruso, Alexandra Saftoiu, Tim Huege, Antonio CONDORELLI, Orazio Zapparrata, Jaime Alvarez-Muniz, Denise Boncioli, Guillermo Torralba Elipe, Martin Erdmann, Bruno Lazarotto Lago, Carlos José Todero Peixoto, Geraldina Golup, Jan Pękala, Maximilian Stadelmaier, Raul Sarmento, Enrique Varela, Antoine Letessier selvon, Vincenzo Rizi, Eleonora Guido, Pedro T. Abreu, Rafael Alves Batista, Arjen Van Vliet, Jan Ebr
Publikováno v:
Physical Review D. 102
We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×1018 eV based on 215,030 events recorded with zenith angles below 60°. A key feature of the work is that the estimates of the energies are independent of assumptio
Autor:
Jaroslaw Stasielak, Ana Martina Botti, Marcus Niechciol, Alberto Daniel Supanitsky, Alexey Yushkov, Petr Schovánek, Toshihiro Fujii, Pavel Horváth, Pedro Assis, Nataliia Borodai, Luis Lopes, Luis Nunez, Carla Bleve, Alberto Blanco, Katharine Mulrey, Antonella Castellina, Francesca Zuccarello, Felicia Carla Tiziana Barbato, Emanuele De Vito, Jose Alfredo Bellido Caceres, Fausto Guarino, Jeffrey Brack, Kai Daumiller, Dariusz Gora, Christian Sarmiento-Cano, Carola Dobrigkeit Chinellato, Alessio Gorgi, Peter Biermann, Teresa Bister, LORENZO CACCIANIGA, Beatriz Garcia, Bruce Dawson, Alena Bakalova, MASSIMO MASTRODICASA, Edivaldo Moura Santos, Stijn Buitink, Bernardo Tomé, Ana Laura Müller, Mario BUSCEMI, Francesco Salamida, Johannes Hulsman, Henryk Wilczyński, Michael Unger, Ronald Cintra Shellard, Miguel Mostafa, Achille Nucita, Frederic Sarazin, Paul Mantsch, Ruben Conceição, Roger Clay, Lukáš Václavek, Giovanni Marsella, Markus Roth, Jakub Jurysek, Lorenzo Cazon, Eva Dos Santos, Corbin Covault, Francesco Fenu, Dalibor Nosek, Rossella Caruso, Alexandra Saftoiu, Tim Huege, Antonio CONDORELLI, Orazio Zapparrata, Jaime Alvarez-Muniz, Denise Boncioli, Guillermo Torralba Elipe, Martin Erdmann, Bruno Lazarotto Lago, Carlos José Todero Peixoto, Geraldina Golup, Jan Pękala, Maximilian Stadelmaier, Raul Sarmento, Enrique Varela, Antoine Letessier selvon, Vincenzo Rizi, Eleonora Guido, Pedro T. Abreu, Rafael Alves Batista, Arjen Van Vliet, Jan Ebr
Publikováno v:
Physical Review Letters. 125
Publikováno v:
Journal of cosmology and astroparticle physics 2021(07), 028 (1-38) (2021). doi:10.1088/1475-7516/2021/07/028
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 be
Publikováno v:
Physical Review D
Physical review / D 100(2), 021302 (2019). doi:10.1103/PhysRevD.100.021302
Physical Review D, 100, 2, pp. 1-5
Physical Review D, 100, 1-5
Physical review / D 100(2), 021302 (2019). doi:10.1103/PhysRevD.100.021302
Physical Review D, 100, 2, pp. 1-5
Physical Review D, 100, 1-5
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_
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0e30a58f79bf0e7315d03ef0688f287
http://arxiv.org/abs/1901.01899
http://arxiv.org/abs/1901.01899