activity
19992014
most citedA TiO study of the black-hole binary GRO J0422+32 in a very low state

56 citations · 172 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2014★ 5 cited

MAGIC search for VHE -ray emission from AE Aquarii in a multiwavelength context

J. Aleksić, S. Ansoldi, L. A. Antonelli +152

It has been claimed that the nova-like cataclysmic variable (CV) AE Aquarii (AE Aqr) is a very-high-energy (VHE, 100 GeV) source both on observational and theoretical grounds.…

astro-ph.HE2013★ 1 cited

Search for TeV -ray emission from AE Aqr coincident with high optical and X-ray states with the MAGIC telescopes

R. Lopez-Coto, O. Blanch Bigas, J. Cortina +9

We report on observations of the nova-like cataclysmic variable AE Aqr performed by MAGIC. The observations were part of a quasi-simultaneous multi-wavelength campaign carried out…

astro-ph.HE2011

Multiwavelength Campaign of Observations of AE Aqr

C. W. Mauche, M. Abada-Simon, J. -F. Desmurs +8

We provide a summary of results, obtained from a multiwavelength (TeV gamma-ray, X-ray, UV, optical, and radio) campaign of observations of AE Aqr conducted in 2005 August 28-Septe…

astro-ph2008★ 15 cited

The X-ray variability and the near-IR to X-ray spectral energy distribution of four low luminosity Seyfert 1 galaxies

I. E. Papadakis, Z. Ioannou, W. Brinkmann +1

We present the results from a study of the X-ray variability and the near-IR to X-ray spectral energy distribution of four low-luminosity, Seyfert 1 galaxies. We compared their var…

astro-ph2007★ 12 cited

Fourier-Resolved Spectroscopy of AGN using XMM-Newton data: I. The 3-10 keV band results

I. E. Papadakis, Z. Ioannou, D. Kazanas

We present the results from the Fourier Resolved Spectroscopy of archival XMM-Newton data of five AGN, namely, Mrk 766, NGC 3516, NGC 3783, NGC 4051 and Ark 564. This work suppleme…

astro-ph2004★ 3 cited

A new mass-ratio for the X-ray Binary X2127+119 in M15?

L. van Zyl, Z. Ioannou, P. A. Charles +1

The luminous low-mass X-ray binary X2127+119 in the core of the globular cluster M15 (NGC 7078), which has an orbital period of 17 hours, has long been assumed to contain a donor s…