Repository of University of Nova Gorica

Show document
A+ | A- | Help | SLO | ENG

Title:Covering the celestial sphere at ultra-high energies: Full-sky cosmic-ray maps beyond the ankle and the flux suppression
Authors:ID Biteau, J. (Author)
ID Lundquist, Jon Paul, UNG (Author), et al.
Files:.pdf epjconf_uhecr18_01005.pdf (4,92 MB)
MD5: 67353A5FD975192CF5DCDFE93CC9D803
 
Language:English
Work type:Not categorized
Typology:1.08 - Published Scientific Conference Contribution
Organization:UNG - University of Nova Gorica
Abstract: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.
Keywords:UHECR, cosmic rays, anisotropy, Telescope Array, Pierre Auger Observatory
Publication version:Version of Record
Year of publishing:2019
Number of pages:9
Numbering:UHECR2018, 210
PID:20.500.12556/RUNG-5168-1fb4b436-4117-b4d9-56ea-cfed89de2a9b New window
COBISS.SI-ID:12867587 New window
DOI:10.1051/epjconf/201921001005 New window
NUK URN:URN:SI:UNG:REP:TFYDXXHB
Publication date in RUNG:28.04.2020
Views:2554
Downloads:82
Metadata:XML RDF-CHPDL DC-XML DC-RDF
:
Copy citation
  
Average score:(0 votes)
Your score:Voting is allowed only for logged in users.
Share:Bookmark and Share


Hover the mouse pointer over a document title to show the abstract or click on the title to get all document metadata.

Record is a part of a proceedings

Title:Ultra HIgh Energy Cosmic Rays (UHECR) 2018

Record is a part of a journal

Title:EPJ Web of Conferences
Shortened title:EPJ Web Conf.
Year of publishing:2019

Licences

License:CC BY-NC-ND 4.0, Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
Link:http://creativecommons.org/licenses/by-nc-nd/4.0/
Description:The most restrictive Creative Commons license. This only allows people to download and share the work for no commercial gain and for no other purposes.
Licensing start date:28.04.2020

Back