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Using a month-long X-ray lightcurve from ${it RXTE}$/PCA and 1.5 month long UV continuum lightcurves from ${it IUE}$ spectra in 1220$-$1970 $r{A}$, 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 $r{A}$ by 3.49 $pm$ 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 0.37$pm$0.14 day, consistent with reprocessing of the X-rays by a surrounding accretion disc. A very similar reverberation delay is observed between ${it Swift}$/XRT X-ray and ${it Swift}$/UVOT UVW2, U lightcurves. Continuum lightcurves extracted from the ${it Swift}$/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 $r{A}$ lag those at 1315 $r{A}$ by $0.29pm0.06$ day, while the fast variations are coincident ($0.04pm0.12$ day). The UV/optical continuum reverberation lag from ${it IUE}$, ${it Swift}$ and other optical telescopes at different wavelengths are consistent with the relationship: $tau propto lambda^{4/3}$, predicted for the standard accretion disc theory while the best-fit X-ray delay from ${it RXTE}$ and ${it Swift}$/XRT shows a negative X-ray offset of $sim$0.38 days from the standard disc delay prediction.
We present intensive quasi-simultaneous X-ray and radio monitoring of the narrow line Seyfert 1 galaxy NGC 4051, over a 16 month period in 2000-2001. Observations were made with the Rossi Timing X-ray Explorer (RXTE) and the Very Large Array (VLA) at
We present a flux-resolved X-ray analysis of the dwarf Seyfert 1.8 galaxy NGC 4395, based on three archival $XMM-Newton$ and one archival $NuSTAR$ observations. The source is known to harbor a low mass black hole ($sim 10^4- {rm a~ few~}times 10^{5}~
We report on daily monitoring of the Seyfert galaxy NGC 7469, around 95 GHz and 143 GHz, with the IRAM 30 m radio telescope, and with the Swift X-Ray and UV/Optical telescopes, over an overlapping period of 45 days. The source was observed on 36 days
We analyse eight XMM-Newton observations of the bright Narrow-Line Seyfert 1 galaxy Arakelian 564 (Ark 564). These observations, separated by ~6 days, allow us to look for correlations between the simultaneous UV emission (from the Optical Monitor) w
We present our analysis of X-ray spectral properties observed from the Seyfrert 1 galactic nucleus NGC~7469 using the RXTE and ASCA observations. We demonstrate strong observational evidence that NGC~7469 undergoes spectral transitions from the low h