Repozitorij Univerze v Novi Gorici

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Naslov:Arrival directions of the highest-energy cosmic rays detected with the Pierre Auger Observatory
Avtorji:ID Aublin, Julien (Avtor)
ID Filipčič, Andrej (Avtor)
ID Kukec Mezek, Gašper (Avtor)
ID Saleh, Ahmed (Avtor)
ID Stanič, Samo (Avtor)
ID Trini, Marta (Avtor)
ID Veberič, Darko (Avtor)
ID Vorobiov, Serguei (Avtor)
ID Yang, Lili (Avtor)
ID Zavrtanik, Danilo (Avtor)
ID Zavrtanik, Marko (Avtor), et al.
Datoteke:.pdf ICRC2015_310.pdf (1,32 MB)
MD5: 95D64819DD9B0789BE955125A587B319
 
Jezik:Angleški jezik
Vrsta gradiva:Delo ni kategorizirano
Tipologija:1.08 - Objavljeni znanstveni prispevek na konferenci
Organizacija:UNG - Univerza v Novi Gorici
Opis:We present the results of a search for small to intermediate scale anisotropies in the distribution of arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory. The data set, gathered in ten years of operation, includes arrival directions with zenith angles up to 80◦, and is about three times larger than that used in earlier studies. We update the test based on correlations with active galactic nuclei (AGNs) from the Véron-Cetty and Véron catalog, which does not yield a significant indication of anisotropy with the present data set. We perform a blind search for localized excess fluxes and for self-clustering of arrival directions at angular scales up to 30◦ and for different energy thresholds between 40 EeV and 80 EeV. We also examine the correlation of arrival directions with relatively nearby galaxies in the 2MRS catalog, AGNs detected by Swift-BAT, and a sample of radio galaxies with jets and with the Centaurus A galaxy. None of the searches shows a statistically significant evidence of anisotropy. The two largest departures from isotropy that were found have a post-trial probability ≈ 1.4%. One is for cosmic rays with energy above 58 EeV that arrive within 15◦ of the direction toward Centaurus A. The other is for arrival directions within 18◦ of Swift-BAT AGNs closer than 130 Mpc and brighter than 10[sup]44 erg/s, with the same energy threshold.
Ključne besede:ultra-high energy cosmic rays anisotropy studies active galactic nuclei Pierre Auger Observatory
Status publikacije:Objavljeno
Leto izida:2015
PID:20.500.12556/RUNG-2132 Novo okno
COBISS.SI-ID:4150267 Novo okno
NUK URN:URN:SI:UNG:REP:QTEATD9S
Datum objave v RUNG:02.03.2016
Število ogledov:5107
Število prenosov:231
Metapodatki:XML RDF-CHPDL DC-XML DC-RDF
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Gradivo je del monografije

Naslov:The 34th International Cosmic Ray Conference : ICRC 2015 (The Hague, Netherlands)
Založnik:PoS, http://pos.sissa.it/
Leto izida:2015
Prireditelj konference:Union of Pure and Applied Physics (IUPAP)
Naslov zbirke:Proceedings of ICRC 2015

Licence

Licenca:CC BY-NC-SA 4.0, Creative Commons Priznanje avtorstva-Nekomercialno-Deljenje pod enakimi pogoji 4.0 Mednarodna
Povezava:http://creativecommons.org/licenses/by-nc-sa/4.0/deed.sl
Opis:Licenca Creative Commons, ki prepoveduje komercialno uporabo in zahteva, da uporabnik predelana dela objavi z enako licenco.
Začetek licenciranja:02.03.2016

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