The performance of photometric reverberation mapping at high redshift and the reliability of damped random walk models

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