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

dc.contributor.author	Morabito, Leah K.
dc.contributor.author	Matthews, James H.
dc.contributor.author	Best, Phillip N.
dc.date.accessioned	2020-11-06T12:51:59Z
dc.date.available	2020-11-06T12:51:59Z
dc.date.issued	2020
dc.identifier.citation	Morabito, L. K. et al. (2020). The origin of radio emission in broad absorption line quasars: Results from the Lofar Two-metre Sky Survey (Corrigendum).Astronomy and Astrophysics, 640,201833821e. Doi: https://doi.org/10.1051/0004-6361/201833821e	en_US
dc.identifier.issn	1432-0746
dc.identifier.uri	http://hdl.handle.net/10566/5390
dc.description.abstract	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.	en_US
dc.language.iso	en	en_US
dc.publisher	EDP Sciences	en_US
dc.subject	Galaxies: active	en_US
dc.subject	Radio continuum: galaxies	en_US
dc.subject	Quasars: genera	en_US
dc.subject	Radiation mechanisms: non-thermal	en_US
dc.subject	Addenda	en_US
dc.title	The origin of radio emission in broad absorption line quasars: Results from the Lofar Two-metre Sky Survey (Corrigendum)	en_US
dc.type	Article	en_US