I. E. Papadakis

University of Crete — Greece

Physics and Astronomy · Physical Sciences

53h-index14.2kcitations333works2.32yr avg
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Research Topics

Astrophysical Phenomena and Observations(178), Astrophysics and Cosmic Phenomena(102), Galaxies: Formation, Evolution, Phenomena(93), Gamma-ray bursts and supernovae(54), Astronomical Observations and Instrumentation(40)

Publications320 total

The X-ray/UV connection in NGC 5548: A rapidly varying corona
Astronomy and Astrophysics·2025Open Access
Characterising the X-ray variability of QSOs to the highest Eddington ratios and black hole masses with eROSITA light curves
arXiv (Cornell University)·2025Open Access
The ensemble broad-frequency power spectrum of Stripe-82 quasars from multiple surveys
Astronomy and Astrophysics·2025Open Access
The X-ray/UV Connection in NGC 5548: A Rapidly Varying Corona
ArXiv.org·2025Open Access
Characterizing the X-ray variability of QSOs to the highest Eddington ratios and black hole masses with eROSITA light curves
Monthly Notices of the Royal Astronomical Society·2025Open Access
The ensemble broad-frequency power spectrum of Stripe-82 quasars from multiple surveys
arXiv (Cornell University)·2025Open Access
X-ray reverberation modelling of the observed UV/optical power spectra of quasars
arXiv (Cornell University)·2025Open Access
X-ray reverberation modelling of the observed UV/optical power spectra of quasars
Astronomy and Astrophysics·2025· 2 citedOpen Access
BASS. LIII. The Eddington Ratio as the Primary Regulator of the Fraction of X-Ray Emission in Active Galactic Nuclei
The Astrophysical Journal·2025Open Access
Exploring the Accretion Disk/Corona Connection in NGC 6814: Insights from UV and X-Ray Spectral-timing Studies
The Astrophysical Journal·2025· 1 citedOpen Access
Continuum optical-UV and X-ray variability of AGN: current results and future challenges
Rivista Del Nuovo Cimento·2025· 4 citedOpen Access
BASS LIII: The Eddington Ratio as the Primary Regulator of the Fraction of X-ray Emission in Active Galactic Nuclei
arXiv (Cornell University)·2025Open Access
Measuring monster black hole masses: Maybe mighty, maybe merely massive
Astronomy and Astrophysics·2025Open Access
Exploring the Accretion disc/Corona Connection in NGC 6814: Insights from UV and X-ray spectral-timing studies
arXiv (Cornell University)·2025Open Access
Frequency-resolved Time Lags due to X-Ray Disk Reprocessing in AGN
The Astrophysical Journal·2025· 4 citedOpen Access
Explaining the UV to X-ray correlation in active galactic nuclei within the framework of X-ray illumination of accretion discs
Astronomy and Astrophysics·2025· 2 citedOpen Access
Explaining the UV to X-ray correlation in AGN within the framework of X-ray illumination of accretion discs
arXiv (Cornell University)·2025Open Access
Frequency-resolved time lags due to X-ray disk reprocessing in AGN
arXiv (Cornell University)·2025Open Access
High-frequency Power Spectrum of Active Galactic Nucleus NGC 4051 Revealed by NICER
The Astrophysical Journal Letters·2025· 1 citedOpen Access
Multi-epoch UV–X-Ray Spectral Study of NGC 4151 with AstroSat
The Astrophysical Journal·2024· 2 citedOpen Access
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Frequent Co-authors

J. Papamastorakis(13), I. M. McHardy(12), P. Uttley(12), P. Reig(11), C. M. Raiteri(10), M. Villata(10), O. M. Kurtanidze(10), M. G. Nikolashvili(10), E. Angelakis(10), T. Hovatta(10), N. D. Kylafis(10), M. Ibrahimov(9), V. M. Larionov(9), D. Blinov(9), V. Pavlidou(9), G. V. Panopoulou(9), A. J. Kus(9), I. Myserlis(9), T. J. Pearson(9), A. N. Ramaprakash(9)