dc.contributor.author | Read, Shaun C | |
dc.contributor.author | Smith, Daniel James B | |
dc.contributor.author | Jarvis, Matt J | |
dc.date.accessioned | 2020-11-10T09:05:58Z | |
dc.date.available | 2020-11-10T09:05:58Z | |
dc.date.issued | 2020 | |
dc.identifier.citation | Read, S.C. et al. (2020). The performance of photometric reverberation mapping at high redshift and the reliability of damped random walk models.Monthly Notices of the Royal Astronomical Society, 492 (3), 3940-3959 | en_US |
dc.identifier.issn | 1365-2966 | |
dc.identifier.uri | http://hdl.handle.net/10566/5403 | |
dc.description.abstract | Accurate methods for reverberation mapping using photometry are highly sought after since
they are inherently less resource intensive than spectroscopic techniques. However, the effectiveness
of photometric reverberation mapping for estimating black hole masses is sparsely
investigated at redshifts higher than z ≈ 0.04. Furthermore, photometric methods frequently
assume a damped random walk (DRW) model, which may not be universally applicable. | en_US |
dc.language.iso | en | en_US |
dc.publisher | Oxford University Press | en_US |
dc.subject | Techniques | en_US |
dc.subject | Photometric | en_US |
dc.subject | Quasars | en_US |
dc.subject | Emission lines | en_US |
dc.subject | General | en_US |
dc.title | The performance of photometric reverberation mapping at high redshift and the reliability of damped random walk models | en_US |
dc.type | Article | en_US |