Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Crete
Univ. of Crete
University of Crete, Heraklion, Crete, Greece
University of Crete, Greece
U.of Crete / FORTH
University of Crete;
U. of Crete
Physics Department, Southampton University, University Road, Southampton SO9 5NH
Department of Physics, The University, Southampton SO17 1BJ
IESL, FORTH, 711 10 Heraklion, Crete, Greece; Physics Department, University of Crete, PO Box 2208, 710 03 Heraklion, Crete, Greece
University of Crete, Physics Department
U. Crete and IESL, Greece
CEA / Saclay, Gif-Sur-Yvette, 91191, Saclay, France
Physics Department, University of Crete, Heraklion, 71003, Crete, Greece; IESL, Foundation for Research and Technology-Hellas, 711 10 Heraklion, Crete, Greece
Queen Mary and Westfield College, London, United Kingdom
University of Southampton, Southampton SO17 1BJ, United Kingdom
Department of Physics and Astronomy, University of Southampton, University Road, Southampton, SO17 1BJ, UK
IESL, FORTH, 711 10 Heraklion, Crete, Greece; Physics Department, University of Crete, 710 03 Heraklion, Crete, Greece
Physics Department, University of Crete, PO Box 2208, 710 03 Heraklion, Crete, Greece ; IESL, Foundation for Research and Technology, 711 10, Heraklion, Crete, Greece Department, University of Crete, 710 03 Heraklion, Crete, Greece Department, Southampton University, University Road, Southampton SO17 1BJ, UK
Physics Department, University of Crete, 71 003 Heraklion, Crete, Greece; IESL, FORTH-Hellas, 71 110, Heraklion, Crete, Greece
University of Crete and IESL FORTH-Hellas
University of Crete, Crete, Greece
Physics Department, University of Crete, Greece; IESL, Foundation for Research and Technology, 71110 Heraklion, Greece
1ES 1927+654: Persistent and rapid X-ray variability in an AGN with low intrinsic neutral X-ray absorption and narrow optical emission lines
A break in the power spectrum of MRK 421
A correlation between the spectral and timing properties of AGN
A detailed X-ray variability study of the Seyfert galaxy NGC 4051
A jet model for black-hole X-ray sources
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Profile ID: LFWR-SCP-P-60654