Volume 640, August 2020
LOFAR Surveys: a new window on the Universe
|Number of page(s)||4|
|Published online||13 August 2020|
The origin of radio emission in broad absorption line quasars: Results from the LOFAR Two-metre Sky Survey (Corrigendum)
Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK
2 SUPA, Institute for Astronomy, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
3 CSIRO Astronomy and Space Science, PO Box 1130, Bentley, WA 6102, Australia
4 Department of Physics, University of the Western Cape, Cape Town 7535, South Africa
5 INAF- Istituto di Radioastronomia, Via P. Gobetti 101, 40129 Bologna, Italy
6 Leiden Observatory, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands
7 Centre for Astrophysics Research, School of Physics, Astronomy and Mathematics, University of Hertfordshire, College Lane, Hatfield AL10 9AB, UK
8 Toruń Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, NCU, Grudziacka 5, 87-100 Toruń, Poland
9 School of Physics, University College Dublin, Belfield, Dublin 4, UK
10 ASTRON, The Netherlands Institute for Radio Astronomy, Postbus 2, 7990, AA Dwingeloo, The Netherlands
11 GEPI & USN, Observatoire de Paris, Université PSL, CNRS, 5 Place Jules Janssen, 92190 Meudon, France
12 Department of Physics & Electronics, Rhodes University, PO Box 94, Grahamstown 6140, South Africa
We report an erratum in Morabito et al. (2019, A&A, 622, A15). When calculating radio powers from observed flux densities, the wrong sign convention was used. This resulted in an underestimation of the radio powers by a median value of 0.6 dex and a maximum of 1 dex. The conclusions of the paper are unchanged.
Key words: galaxies: active / galaxies: jets / radio continuum: galaxies / quasars: general / radiation mechanisms: non-thermal / errata, addenda
© ESO 2020
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