TY - JOUR
T1 - Erratum
T2 - Non-thermal emission in the lobes of Fornax A (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stz511)
AU - Persic, Massimo
AU - Rephaeli, Yoel
N1 - Publisher Copyright:
© 2019 The Author(s).
PY - 2019/6/11
Y1 - 2019/6/11
N2 - 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).
AB - 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).
UR - http://www.scopus.com/inward/record.url?scp=85073193030&partnerID=8YFLogxK
U2 - 10.1093/mnras/stz828
DO - 10.1093/mnras/stz828
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AN - SCOPUS:85073193030
SN - 0035-8711
VL - 486
SP - 950
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 1
ER -