Understanding Reverberation Lags in 1H0707-495
A. Zoghbi, P. Uttley, A. C. Fabian

TL;DR
This paper critically evaluates the origin of reverberation lags in galaxy 1H0707-495, supporting the interpretation that they originate from matter close to the supermassive black hole rather than distant regions, based on spectral and timing analysis.
Contribution
The study defends the inner reflector model for reverberation lags, demonstrating its consistency with spectral and timing data against alternative outer reflector explanations.
Findings
Inner reflector model explains energy spectrum and timing properties.
Large-scale outer reflector requires implausible conditions.
Original interpretation aligns with observed coherence and power spectra.
Abstract
The first reverberation lag from the vicinity of a supermassive black hole was recently detected in the NLS1 galaxy 1H0707-495. We interpreted the lag as being due to reflection from matter close to the black hole, within a few gravitational radii of the event horizon (an inner reflector). It has since been claimed by Miller et al that the lag can be produced by more distant matter, at hundreds of gravitational radii (an outer reflector). Here, we critically explore their interpretation of the lag. The detailed energy dependence of the time lags between soft and hard energy bands is well modelled by an inner reflector using our previously published spectral model. A contrary claim by Miller et al was obtained by neglecting the blackbody component in the soft band. Soft lags can be produced by a large-scale outer reflector if several, implausible, conditions are met. An additional…
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