Erratum: Non-thermal emission in the lobes of Fornax A (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stz511)

Massimo Persic*, Yoel Rephaeli

*Corresponding author for this work

Research output: Contribution to journalComment/debate

Abstract

In our paper 'Non-thermal emission in the lobes of Fornax A' (Persic & Rephaeli 2019) the dilution factor of the cosmic IR background (CIB) was incorrectly specified to be CCIB = 10-6.724 (section 2.1). The correct value is CCIB = 10-5.629: in the revised Fig. (1)-left shown here the updated Compton/FIR curves are correspondingly higher. Our main conclusion, namely that all the observed Fermi-LAT emission from the lobes of FornaxA can be accounted for by energetic electrons scattering off the ambient optical radiation field, is unaffected by this correction. (Figure Presented).

Original languageEnglish
Pages (from-to)950
Number of pages1
JournalMonthly Notices of the Royal Astronomical Society
Volume486
Issue number1
DOIs
StatePublished - 11 Jun 2019

Fingerprint

Dive into the research topics of 'Erratum: Non-thermal emission in the lobes of Fornax A (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stz511)'. Together they form a unique fingerprint.

Cite this