902 citations · 1.3k across the 7 of their papers we have counts for
7 papers
Distinct accretion modes of Cygnus X-1 revealed from hard X-rays
Piotr Lubiński, Alexandros Filothodoros, Andrzej A. Zdziarski +1
Thanks to recurrent observations of the black hole binary Cyg X-1 carried out over 15 years the INTEGRAL satellite has collected the largest data set in the hard X-ray band for thi…
Performance of the Cherenkov Telescope Array at energies above 10 TeV
Anna Barnacka, Leszek Bogacz, Mira Grudzińska +4
The Cherenkov Telescope Array (CTA) is the next generation observatory for very high energy gamma rays. The capability of the array to detect gamma-rays above 10 TeV is going to be…
4 m Davies-Cotton telescope for the Cherenkov Telescope Array
R. Moderski, J. A. Aguilar, A. Barnacka +39
The Cherenkov Telescope Array (CTA) is the next generation very high energy gamma-ray observatory. It will consist of three classes of telescopes, of large, medium and small sizes.…
Multiwavelength campaign on Mrk 509: Reverberation of the Fe Kalpha line
G. Ponti, M. Cappi, E. Costantini +17
We report on a detailed study of the Fe K emission/absorption complex in the nearby, bright Seyfert 1 galaxy Mrk 509. The study is part of an extensive XMM-Newton monitoring consis…
The Hard X-ray Emission of Cen A
V. Beckmann, P. Jean, P. Lubinski +2
The radio galaxy Cen A has been detected all the way up to the TeV energy range. This raises the question about the dominant emission mechanisms in the high-energy domain. Spectral…
Design Concepts for the Cherenkov Telescope Array
The CTA Consortium
Ground-based gamma-ray astronomy has had a major breakthrough with the impressive results obtained using systems of imaging atmospheric Cherenkov telescopes. Ground-based gamma-ray…
Correlation between Compton reflection and X-ray slope in Seyferts and X-ray binaries
A. A. Zdziarski, P. Lubiski, D. A. Smith
We find a very strong correlation between the intrinsic spectral slope in X-rays and the amount of Compton reflection from a cold medium in Seyfert AGNs and in hard state of X-ray…