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.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.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.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 |