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Title: CORRELATIONS BETWEEN ULTRAHIGH ENERGY COSMIC RAYS AND INFRARED-LUMINOUS GALAXIES

Abstract

We confirm the ultrahigh energy cosmic ray (UHECR) horizon established by the Pierre Auger Observatory using the heterogeneous Veron-Cetty-Veron (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 10{sup 10} L{sub sun}. The strongest correlation-for z < 0.016, {psi} = 2.{sup 0}1, and L{sub ir} {>=} 10{sup 10.5} L{sub sun}-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.

Authors:
 [1]; ;  [2]
  1. Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States)
  2. Center for Cosmology and Particle Physics and Department of Physics, New York University, New York, NY 10003 (United States)
Publication Date:
OSTI Identifier:
21452947
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal
Additional Journal Information:
Journal Volume: 716; Journal Issue: 2; Other Information: DOI: 10.1088/0004-637X/716/2/914; Journal ID: ISSN 0004-637X
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; COSMIC RADIATION; GALAXIES; GALAXY NUCLEI; LUMINOSITY; POINT SOURCES; RED SHIFT; IONIZING RADIATIONS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATION SOURCES; RADIATIONS

Citation Formats

Berlind, Andreas A, Farrar, Glennys R, and Zaw, Ingyin. CORRELATIONS BETWEEN ULTRAHIGH ENERGY COSMIC RAYS AND INFRARED-LUMINOUS GALAXIES. United States: N. p., 2010. Web. doi:10.1088/0004-637X/716/2/914.
Berlind, Andreas A, Farrar, Glennys R, & Zaw, Ingyin. CORRELATIONS BETWEEN ULTRAHIGH ENERGY COSMIC RAYS AND INFRARED-LUMINOUS GALAXIES. United States. https://doi.org/10.1088/0004-637X/716/2/914
Berlind, Andreas A, Farrar, Glennys R, and Zaw, Ingyin. 2010. "CORRELATIONS BETWEEN ULTRAHIGH ENERGY COSMIC RAYS AND INFRARED-LUMINOUS GALAXIES". United States. https://doi.org/10.1088/0004-637X/716/2/914.
@article{osti_21452947,
title = {CORRELATIONS BETWEEN ULTRAHIGH ENERGY COSMIC RAYS AND INFRARED-LUMINOUS GALAXIES},
author = {Berlind, Andreas A and Farrar, Glennys R and Zaw, Ingyin},
abstractNote = {We confirm the ultrahigh energy cosmic ray (UHECR) horizon established by the Pierre Auger Observatory using the heterogeneous Veron-Cetty-Veron (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 10{sup 10} L{sub sun}. The strongest correlation-for z < 0.016, {psi} = 2.{sup 0}1, and L{sub ir} {>=} 10{sup 10.5} L{sub sun}-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.},
doi = {10.1088/0004-637X/716/2/914},
url = {https://www.osti.gov/biblio/21452947}, journal = {Astrophysical Journal},
issn = {0004-637X},
number = 2,
volume = 716,
place = {United States},
year = {Sun Jun 20 00:00:00 EDT 2010},
month = {Sun Jun 20 00:00:00 EDT 2010}
}