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20012025
most citedThe WEBT BL Lacertae Campaign 2001 and its extension

143 citations · 1.3k across the 30 of their papers we have counts for

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Showing astro-ph.HEShow all

7 papers · 1 filter

astro-ph.HE2025

Measuring monster MBHs: maybe mighty, maybe merely massive

M. Gliozzi, A. Akylas, J. K. Williams +1

Accurate black hole mass (MBH) measurements in high-z galaxies are difficult yet crucial to constrain the growth of supermassive BHs, and to discriminate between competing BH seed…

astro-ph.HE2024★ 14 cited

Broadband X-ray/UV/optical time-resolved spectroscopy of NGC 5548: The origin of the UV/optical variability in active galactic nuclei

E. Kammoun, I. E. Papadakis, M. Dovčiak +1

Recently, nearby active galactic nuclei (AGN) have been subject to long X-rays/UV/optical monitoring campaigns. These campaigns reveal a strong correlation between the various UV a…

astro-ph.HE2023

Comparing indirect methods for black hole masses in AGN: the good, the bad, and the ugly

M. Gliozzi, J. K. Williams, A. Akylas +4

The black hole mass MBH is crucial in constraining the growth of supermassive BHs within their host galaxies. Since direct measurements of MBH with dynamical methods are restricted…

astro-ph.HE2023★ 8 cited

Detection of X-ray/UV delay in NGC 4051 using AstroSat observations

Kavita Kumari, G. C. Dewangan, I. E. Papadakis +1

We study the connection between the variations in the far ultra-violet (FUV), near ultra-violet (NUV) and X-ray band emission from NGC 4051 using 4-days long AstroSat observations…

astro-ph.HE2017★ 100 cited

RoboPol: Connection between optical polarization plane rotations and gamma-ray flares in blazars

D. Blinov, V. Pavlidou, I. Papadakis +21

We use results of our 3 year polarimetric monitoring program to investigate the previously suggested connection between rotations of the polarization plane in the optical emission…

astro-ph.HE2017★ 8 cited

The nature of X-ray spectral variability in MCG-6-30-15

E. S. Kammoun, I. E. Papadakis

The flux-flux plot (FFP) method can provide model-independent clues regarding the X-ray variability of active galactic nuclei. To use it properly, the bin size of the light curves…