Evidence for variability timescale dependent UV/X-ray delay in Seyfert 1 AGN NGC 7469
arXiv:2004.07901 · doi:10.1093/mnras/staa1055
Abstract
Using a month-long X-ray lightcurve from /PCA and 1.5 month long UV continuum lightcurves from spectra in 12201970 , we performed a detailed time-lag study of the Seyfert 1 galaxy NGC 7469. Our cross-correlation analysis confirms previous results showing that the X-rays are delayed relative to the UV continuum at 1315 by 3.49 0.22 days which is possibly caused by either propagating fluctuation or variable comptonisation. However, if variations slower than 5 days are removed from the X-ray lightcurve, the UV variations then lag behind the X-rays variations by 0.370.14 day, consistent with reprocessing of the X-rays by a surrounding accretion disc. A very similar reverberation delay is observed between /XRT X-ray and /UVOT UVW2, U lightcurves. Continuum lightcurves extracted from the /GRISM spectra show delays with respect to X-rays consistent with reverberation. Separating the UV continuum variations faster and slower than 5 days, the slow variations at 1825 lag those at 1315 by day, while the fast variations are coincident ( day). The UV/optical continuum reverberation lag from , and other optical telescopes at different wavelengths are consistent with the relationship: , predicted for the standard accretion disc theory while the best-fit X-ray delay from and /XRT shows a negative X-ray offset of 0.38 days from the standard disc delay prediction.
13 pages, 9 figures, 1 table, accepted for publication in MNRAS
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- Reverberation Mapping Measurements of Black Hole Masses and Broad-Line Region Kinematics in Mrk 817 and NGC 7469
- Revisiting UV/optical continuum time lags in AGN
- The luminosity-dependent contribution from the broad line region to the wavelength-dependent lags in Mrk 110
- Broadband X-ray/UV/optical time-resolved spectroscopy of NGC 5548: The origin of the UV/optical variability in active galactic nuclei
- Contrasting X-ray/UV time-lags in Seyfert 1 galaxies NGC 4593 and NGC 7469 using AstroSat observations
- AGN Light Echoes and the Accretion Disc Self-Gravity Limit
- The Relation between X-ray and Ultraviolet Variability of Quasars
- The evolution of the UV/optical lag spectrum of NGC 7469 seen by the Liverpool Telescope
- Timescale-dependent X-ray to UV time lags of NGC 4593 using high-intensity XMM-Newton observations with Swift and AstroSat