Corrected Table for the Parametric Coefficients for the Optical Depth of the Universe to Gamma-rays at Various Redshifts

Simple item page
dc.creatorStecker, F. W.
dc.creatorMalkan, M. A.
dc.creatorScully, S. T.
dc.date2006-12-01
dc.date2007-02-02
dc.date.accessioned2026-07-07T10:21:08Z
dc.date.available2026-07-07T10:21:08Z
dc.descriptionTable 1 in our paper, ApJ 648, 774 (2006) entitled "Intergalactic Photon Spectra from the Far IR to the UV Lyman Limit for 0 < z < 6 and the Optical Depth of the Universe to High Energy Gamma-Rays" had erroneous numbers for the coefficients fitting the parametric form for the optical depth of the universe to gamma-rays. The correct values for these parameters as described in the original text are given here in a corrected table for various redshifts for the baseline model (upper row) and fast evolution (lower row) for each individual redshift. The parametric approximation is good for optical depths between 0.01 and 100 and for gamma-ray energies up to ~2 TeV for all redshifts but also for energies up to ~10 TeV for redshifts less than 1.
dc.descriptionTable 1 corrected and new gamma-ray energy range of validity given
dc.identifierhttps://arxiv.org/abs/astro-ph/0612048
dc.identifierhttp://arxiv.org/abs/astro-ph/0612048
dc.identifierAstrophys.J.658:1392,2007
dc.identifierdoi:10.1086/511738
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175073
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCorrected Table for the Parametric Coefficients for the Optical Depth of the Universe to Gamma-rays at Various Redshifts
dc.typetext

Files

Collections

arXiv