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J. R. Allison, E. M. Sadler, V. A. Moss, M. T. Whiting, R. W. Hunstead, M. B. Pracy, S. J. Curran, S. M. Croom, M. Glowacki, R. Morganti, S. S. Shabala, M. A. Zwaan, G. Allen, S. W. Amy, P. Axtens, L. Ball, K. W. Bannister, S. Barker, M. E. Bell, D. C.-J. Bock, R. Bolton, M. Bowen, B. Boyle, R. Braun, S. Broadhurst, D. Brodrick, M. Brothers, A. Brown, J. D. Bunton, C. Cantrall, J. Chapman, W. Cheng, A. P. Chippendale, Y. Chung, F. Cooray, T. Cornwell, D. DeBoer, P. Diamond, P. G. Edwards, R. Ekers, I. Feain, R. H. Ferris, R. Forsyth, R. Gough, A. Grancea, N. Gupta, J. C. Guzman, G. Hampson, L. Harvey-Smith, C. Haskins, S. Hay, D. B. Hayman, I. Heywood, A. W. Hotan, S. Hoyle, B. Humphreys, B. T. Indermuehle, C. Jacka, C. Jackson, S. Jackson, K. Jeganathan, S. Johnston, J. Joseph, R. Kendall, M. Kesteven, D. Kiraly, B. S. Koribalski, M. Leach, E. Lenc, E. Lensson, S. Mackay, A. Macleod, M. Marquarding, J. Marvil, N. McClure-Griffiths, D. McConnell, P. Mirtschin, R. P. Norris, S. Neuhold, A. Ng, J. O'Sullivan, J. Pathikulangara, S. Pearce, C. Phillips, A. Popping, R. Y. Qiao, J. E. Reynolds, P. Roberts, R. J. Sault, A. Schinckel, P. Serra, R. Shaw, M. Shields, T. Shimwell, M. Storey, T. Sweetnam, E. Troup, B. Turner, J. Tuthill, A. Tzioumis, M. A. Voronkov, T. Westmeier, C. D. Wilson, Erratum: Discovery of H i gas in a young radio galaxy at z = 0.44 using the Australian Square Kilometre Array Pathfinder, Monthly Notices of the Royal Astronomical Society, Volume 456, Issue 3, 01 March 2016, Pages 3030–3031, https://doi.org/10.1093/mnras/stv2908
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The paper ‘Discovery of H i gas in a young radio galaxy at z = 0.44 using the Australian Square Kilometre Array Pathfinder’ was first published in MNRAS, 453, 1249 (2015). In this erratum, we correct the X-ray luminosity given for PKS B1740−517 in Section 4.2.1. The luminosity was incorrectly calculated as 4.3 × 1043 erg s−1 from a simple absorbed power-law model fitted to the XMM–Newton data. The correct value for this model is L2–10 keV ≈ 6.2 × 1044 erg s−1.
This erratum does not change the conclusions reached by Allison et al. (2015) and is still consistent with the distribution of X-ray luminosities measured for other GHz-peaked spectrum (GPS) radio sources (e.g. Tengstrand et al. 2009).
We thank Roberto Soria and Ryan Urquhart for bringing this error to our attention.
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