Repozitorij Univerze v Novi Gorici

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Naslov:Covering the celestial sphere at ultra-high energies: Full-sky cosmic-ray maps beyond the ankle and the flux suppression
Avtorji:ID Biteau, J. (Avtor)
ID Lundquist, Jon Paul, UNG (Avtor), et al.
Datoteke:.pdf epjconf_uhecr18_01005.pdf (4,92 MB)
MD5: 67353A5FD975192CF5DCDFE93CC9D803
 
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija:UNG - Univerza v Novi Gorici
Opis:Despite deflections by Galactic and extragalactic magnetic fields, the distribution of ultra-high energy cosmic rays (UHECRs) over the celestial sphere remains a most promising observable for the identification of their sources. Thanks to a large number of detected events over the past years, a large-scale anisotropy at energies above 8 EeV has been identified, and there are also indications from the Telescope Array and Pierre Auger Collaborations of deviations from isotropy at intermediate angular scales (about 20 degrees) at the highest energies. In this contribution, we map the flux of UHECRs over the full sky at energies beyond each of two major features in the UHECR spectrum – the ankle and the flux suppression, and we derive limits for anisotropy on different angular scales in the two energy regimes. In particular, full-sky coverage enables constraints on low-order multipole moments without assumptions about the strength of higher-order multipoles. Following previous efforts from the two Collaborations, we build full-sky maps accounting for the relative exposure of the arrays and differences in the energy normalizations. The procedure relies on cross-calibrating the UHECR fluxes reconstructed in the declination band around the celestial equator covered by both observatories. We present full-sky maps at energies above ~10 EeV and ~50 EeV, using the largest datasets shared across UHECR collaborations to date. We report on anisotropy searches exploiting full-sky coverage and discuss possible constraints on the distribution of UHECR sources.
Ključne besede:UHECR, cosmic rays, anisotropy, Telescope Array, Pierre Auger Observatory
Verzija publikacije:Objavljena publikacija
Leto izida:2019
Št. strani:9
Številčenje:UHECR2018, 210
PID:20.500.12556/RUNG-5168-1fb4b436-4117-b4d9-56ea-cfed89de2a9b Novo okno
COBISS.SI-ID:12867587 Novo okno
DOI:10.1051/epjconf/201921001005 Novo okno
NUK URN:URN:SI:UNG:REP:TFYDXXHB
Datum objave v RUNG:28.04.2020
Število ogledov:2563
Število prenosov:82
Metapodatki:XML RDF-CHPDL DC-XML DC-RDF
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Gradivo je del zbornika

Naslov:Ultra HIgh Energy Cosmic Rays (UHECR) 2018

Gradivo je del revije

Naslov:EPJ Web of Conferences
Skrajšan naslov:EPJ Web Conf.
Leto izida:2019

Licence

Licenca:CC BY-NC-ND 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Brez predelav 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by-nc-nd/4.0/deed.sl
Opis:Najbolj omejujoča licenca Creative Commons. Uporabniki lahko prenesejo in delijo delo v nekomercialne namene in ga ne smejo uporabiti za nobene druge namene.
Začetek licenciranja:28.04.2020

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