A
A. C. Fabian
Researcher at University of Cambridge
Publications - 820
Citations - 43942
A. C. Fabian is an academic researcher from University of Cambridge. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 103, co-authored 818 publications receiving 41589 citations.
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Radio-loud AGN and the extragalactic gamma-ray background.
TL;DR: In this paper, the contribution of radio-loud active galactic nuclei to the γ-ray background using the recent detections by GRO of BL Lacs and flat-spectrum radio quasars at energies > 100 MeV was estimated.
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XMM-Newton discovery of a sharp spectral feature at ∼ 7 keV in the narrow-line Seyfert 1 galaxy 1H 0707-495
Th. Boller,A. C. Fabian,R. A. Sunyaev,Joachim Trümper,Simon Vaughan,David R. Ballantyne,W. N. Brandt,R. Keil,K. Iwasawa +8 more
TL;DR: In this paper, the first detection of a sharp spectral feature in a narrow-line Seyfert 1 galaxy was reported, which suggests a connection with the neutral iron K photoelectric edge, but the lack of any obvious absorption in the spectrum at lower energies makes the interpretation challenging.
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A volume-limited sample of X-ray galaxy groups and clusters – I. Radial entropy and cooling time profiles
TL;DR: In this paper, the authors studied the properties of the innermost ICM in the cores of 101 X-ray galaxy groups and clusters, which is volume-limited in each of three Xray luminosity bins, and determined the effect of non-gravitational processes, such as active galactic nucleus (AGN) feedback, on the ICM.
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X-Ray Spectral Analysis of Elliptical Galaxies from ASCA: the Fe Abundance in a Multi-Phase Medium
David A. Buote,A. C. Fabian +1 more
TL;DR: In this paper, the authors present spectral analysis of ASCA data of 17 elliptical and 3 lenticular galaxies most of which have high L_x/L_B. The abundances derived from the cooling-flow model are also significantly larger, = 0.6 +/- 0.5 Z_sun.
Journal ArticleDOI
The XMM-Newton serendipitous survey - IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS)
Xavier Barcons,Francisco J. Carrera,María Teresa Ceballos,M. J. Page,Javier Bussons-Gordo,Amalia Corral,Jacobo Ebrero,Silvia Mateos,Silvia Mateos,Jonathan Tedds,M. G. Watson,D. Baskill,Mark Birkinshaw,Th. Boller,N. V. Borisov,M. N. Bremer,G. E. Bromage,Hermann Brunner,Alessandro Caccianiga,C. S. Crawford,Mark Cropper,R. Della Ceca,P. Derry,A. C. Fabian,Patrick Guillout,Yasuhiro Hashimoto,Günther Hasinger,B. J. M. Hassall,Georg Lamer,N. S. Loaring,T. Maccacaro,Keith O. Mason,Richard G. McMahon,L. Mirioni,J. P. D. Mittaz,Christian Motch,Ignacio Negueruela,Ignacio Negueruela,J. P. Osborne,Francesca Panessa,I. Perez-Fournon,John P. Pye,Timothy P.L. Roberts,Timothy P.L. Roberts,Simon Rosen,Simon Rosen,Norbert Schartel,Nicholas J. Schurch,Nicholas J. Schurch,Axel Schwope,Paola Severgnini,Richard Sharp,Richard Sharp,G. C. Stewart,G. P. Szokoly,A. Ullan,Martin Ward,Martin Ward,R. S. Warwick,Peter J. Wheatley,Peter J. Wheatley,N. A. Webb,Diana M Worrall,W. Yuan,H. Ziaeepour +64 more
TL;DR: The XMM-Newton Medium Sensitivity Survey (XMS) as mentioned in this paper provides an unbiased and quantitative description of the X-ray source population at these fluxes and in various Xray energy bands.