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I. E. Papadakis

Researcher at University of Crete

Publications -  236
Citations -  16293

I. E. Papadakis is an academic researcher from University of Crete. The author has contributed to research in topics: Active galactic nucleus & Galaxy. The author has an hindex of 57, co-authored 227 publications receiving 14867 citations. Previous affiliations of I. E. Papadakis include Foundation for Research & Technology – Hellas & University of Southampton.

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The CMS experiment at the CERN LHC

S. Chatrchyan, +3175 more
TL;DR: The Compact Muon Solenoid (CMS) detector at the Large Hadron Collider (LHC) at CERN as mentioned in this paper was designed to study proton-proton (and lead-lead) collisions at a centre-of-mass energy of 14 TeV (5.5 TeV nucleon-nucleon) and at luminosities up to 10(34)cm(-2)s(-1)
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The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

Kirpal Nandra, +239 more
TL;DR: The Advanced Telescope for High Energy Astrophysics (Athena+) mission as discussed by the authors provides the necessary performance (e.g., angular resolution, spectral resolution, survey grasp) to address these questions and revolutionize our understanding of the Hot and Energetic Universe.
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Measuring the broad-band power spectra of active galactic nuclei with RXTE

TL;DR: In this paper, a Monte Carlo technique was developed to test models for the true power spectrum of intermittently sampled light curves against the noisy, observed power spectra, and produce a reliable estimate of the goodness of fit of the given model.
Journal ArticleDOI

Measuring the broadband power spectra of active galactic nuclei with RXTE

TL;DR: In this paper, a Monte Carlo technique was developed to test models for the true power spectra of intermittently sampled lightcurves against the noisy, observed power spectrum, and produce a reliable estimate of the goodness of fit of the given model.
Journal ArticleDOI

Combined long and short time-scale X-ray variability of NGC 4051 with RXTE and XMM-Newton

TL;DR: In this article, the authors present a comprehensive analysis of the X-ray variability of the narrow-line Seyfert 1 galaxy NGC 405 1, one of the most variable active galactic nuclei (AGN) in the sky.