The origin of radio emission in broad absorption line quasars: Results from the LOFAR Two-metre Sky Survey ( Corrigendum )

L. Morabito , J. Matthews , P. Best , G. Gürkan , M. Jarvis , I. Prandoni , K. Duncan , M. Hardcastle , M. Kunert-Bajraszewska , A. Mechev , S. Mooney , J. Sabater , H. Röttgering , T. Shimwell , D. Smith , C. Tasse (1, 2) , W. Williams

1 USN - Unité Scientifique de la Station de Nançay
2 GEPI - Galaxies, Etoiles, Physique, Instrumentation

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.

Mots clés: galaxies; active -galaxies; jets -radio continuum; galaxies -quasars; general -radiation mechanisms; non-thermalerrata; addenda

Domaines: Physique [physics]; Astrophysique [astro-ph]

L. Morabito, J. Matthews, P. Best, G. Gürkan, M. Jarvis, et al.. The origin of radio emission in broad absorption line quasars: Results from the LOFAR Two-metre Sky Survey ( Corrigendum ). Astronomy and Astrophysics - A&A, 2020, 640, pp.C4. ⟨10.1051/0004-6361/201833821e⟩. ⟨hal-03200618⟩