2010ApJ...716..914B


Query : 2010ApJ...716..914B

2010ApJ...716..914B - Astrophys. J., 716, 914-917 (2010/June-3)

Correlations between ultrahigh energy cosmic rays and infrared-luminous galaxies.

BERLIND A.A., FARRAR G.R. and ZAW I.

Abstract (from CDS):

We confirm the ultrahigh energy cosmic ray (UHECR) horizon established by the Pierre Auger Observatory using the heterogeneous Véron-Cetty-Véron (VCV) catalog of active galactic nuclei by performing a redshift-angle-IR luminosity scan using point-source catalog with redshift (PSCz) galaxies having infrared luminosity greater than 1010 L☉. The strongest correlation–for z < 0.016, ψ = 2{fdg}1, and Lir≥ 1010.5 L☉–arises in fewer than 0.3% of scans with isotropic source directions. When we apply a penalty for using the UHECR energy threshold that was tuned to maximize the correlation with VCV, the significance degrades to 1.1%. Since the PSCz catalog is complete and volume-limited for these parameters, this suggests that the UHECR horizon discovered by the Pierre Auger Observatory is not an artifact of the incompleteness and other idiosyncrasies of the VCV catalog. The strength of the correlation between UHECRs and the nearby highest-IR-luminosity PSCz galaxies is stronger than in about 90% of trials with scrambled luminosity assignments for the PSCz galaxies. If confirmed by future data, this result would indicate that the sources of UHECRs are more strongly associated with luminous IR galaxies than with ordinary, lower IR luminosity galaxies.

Abstract Copyright: ∼

Journal keyword(s): acceleration of particles - astroparticle physics - infrared: galaxies

Simbad objects: 13

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Number of rows : 13
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 424 Sy1 01 11 27.6385025496 -38 05 00.421096524   13.76 14.12 12.38 12.8 ~ 346 1
2 NGC 1204 Sy2 03 04 39.8863185024 -12 20 28.999064652   15   13.11   ~ 67 0
3 NGC 1346 Sy1 03 30 13.2634890840 -05 32 35.991525660   17.06 16.39 12.58   ~ 63 1
4 MCG-03-24-009 GiG 09 27 13.876 -19 31 57.14   14.25   12.68   ~ 31 0
5 NGC 4945 Sy2 13 05 27.279 -49 28 04.44   9.31 14.40 7.55   ~ 1582 2
6 ESO 270-7 EmG 13 23 15.7277924448 -43 32 38.349125412   14.38   12.97   ~ 30 0
7 NAME Centaurus A BLL 13 25 27.61521044 -43 01 08.8050291   8.18 6.84 6.66   ~ 4774 3
8 IC 4523 Sy1 15 05 10.5321975384 -43 30 34.383602196   13.2   12.47 13.1 ~ 34 0
9 LEDA 165747 AG? 17 54 41.2141961088 -60 54 40.257078624           ~ 14 0
10 NGC 7130 Sy2 21 48 19.5412287192 -34 57 04.492024884   12.86 13.87 11.57   ~ 483 1
11 IC 5179 Sy1 22 16 09.1191653256 -36 50 37.117603752   12.29 11.89 11.38   ~ 214 1
12 IC 5186 Sy2 22 18 46.531 -36 48 05.86   13.25 11.80 12.29   ~ 45 1
13 NGC 7648 GiG 23 23 54.031 +09 40 02.85   13.5       ~ 87 1

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