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The paper ‘HESS J1640−465 – an exceptionally luminous TeV γ-ray supernova remnant’ was published in MNRAS, 439, 2828 (2014). Due to an error in the integration of the differential energy spectrum, the luminosities stated in Sections 2.2 and 4.3 are incorrect. The luminosity of HESS J1640−465 above 1 TeV at 10 kpc distance is L>1 TeV ≃ 7.8 × 1034 (d/10 kpc)2 erg s−1. The calculation of the points in the spectral energy distributions shown in Figs 3 and 5 are not affected by this error. Therefore, our conclusions in the discussion section are unaltered, especially what concerns the energy in interacting cosmic rays Wpn¯H.
|Keywords:||Errata, addenda, Radiation mechanisms: non-thermal, ISM: individual objects: G338.3−0.0– ISM: supernova remnants.|
|Full text:||(VoR) Version of Record|
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|Publisher Web site:||http://dx.doi.org/10.1093/mnras/stu826|
|Publisher statement:||This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.|
|Date accepted:||No date available|
|Date deposited:||22 April 2015|
|Date of first online publication:||July 2014|
|Date first made open access:||No date available|
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