Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Iris Gebauer"'
Autor:
J. Casaus, Pier-Giorgio Rancoita, C. Mañá, M. Molero, Massimo Gervasi, Iris Gebauer, Miguel Angel Velasco, Giuseppe Vacca, S. Zeissler, M. Graziani
Publikováno v:
Proceedings of The 39th International Conference on High Energy Physics — PoS(ICHEP2018).
A measurement of the dipole anisotropy in the arrival directions of galactic cosmic positrons, electrons and protons has been performed with the Alpha Magnetic Spectrometer (AMS) onboard the International Space Station (ISS) using the first 6 years o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24730c6a6aa361d3da7bb4cde1d850d9
https://doi.org/10.22323/1.340.0370
https://doi.org/10.22323/1.340.0370
Autor:
Emma Kun, L. Caramete, László Á. Gergely, Peter L. Biermann, Biman B. Nath, Roland Diehl, Philipp P. Kronberg, Todor Stanev, Eberhard Haug, Iris Gebauer, A. Meli, Wim De Boer, Julia Becker Tjus, Alessandro Chieffi
Most cosmic ray particles observed derive from the explosions of massive stars, which commonly produce stellar black holes in their supernova explosions. When two such black holes find themselves in a tight binary system they finally merge in a gigan
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5e339493b2f496ea93801209568cb38
http://arxiv.org/abs/1803.10752
http://arxiv.org/abs/1803.10752
Publikováno v:
Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017).
The so-called "GeV-excess" of the diffuse Galactic gamma-ray emission is studied with a spectral template fit based on energy spectra. The spectral templates can be obtained in a data-driven way from the gamma-ray data, which avoids the use of emissi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::518912a4f461ac6a1ee6c71c52942e7c
https://doi.org/10.22323/1.301.0908
https://doi.org/10.22323/1.301.0908
Publikováno v:
Scopus-Elsevier
The search for anisotropies in cosmic ray arrival directions with space experiments like the Alpha Magnetic Spectrometer (AMS-02) on the International Space Station is subject to a number of time and energy dependent effects originating from the dete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bb30e19940a72f32cb365cee7793718
http://hdl.handle.net/11391/1472214
http://hdl.handle.net/11391/1472214
Autor:
Iris Gebauer
Publikováno v:
Proceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cbc6f823a389919b12564c5a7a6d3bd7
https://doi.org/10.22323/1.236.0404
https://doi.org/10.22323/1.236.0404
Autor:
Iris Gebauer
Publikováno v:
Proceedings of The 34th International Cosmic Ray Conference — PoS(ICRC2015).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::653ebccda7dffa1f6eca17c9744b8bca
https://doi.org/10.22323/1.236.0543
https://doi.org/10.22323/1.236.0543
Autor:
Iris Gebauer
Publikováno v:
Proceedings of Identification of dark matter 2008 — PoS(idm2008).
The ROSAT Galactic wind observations confirm that our Galaxy launches supernova (SN) driven Galactic winds with wind speeds of about 150 km/s in the Galactic plane. Galactic winds of this strength are incompatible with current isotropic models for Co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::38dbc1afd64263af54373de77b849e93
https://doi.org/10.22323/1.064.0030
https://doi.org/10.22323/1.064.0030
The diffuse galactic EGRET gamma ray data show a clear excess for energies above 1 GeV in comparison with the expectations from conventional galactic models. This excess shows all the features expected from Dark Matter WIMP Annihilation: a)it is pres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d569b50de8c1c78cc51aaa53a658b401
Publikováno v:
Scopus-Elsevier
CIÊNCIAVITAE
CIÊNCIAVITAE
The arrival directions of energetic positrons and electrons convey fundamental information on their origin. PAMELA, and more recently AMS, have measured an anomalous population of energetic positrons, which cannot be explained in standard cosmic ray
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::63cdb80d8c44b73b7776721fdc483025
http://www.scopus.com/inward/record.url?eid=2-s2.0-84988703529&partnerID=MN8TOARS
http://www.scopus.com/inward/record.url?eid=2-s2.0-84988703529&partnerID=MN8TOARS