C
Christopher S. Reynolds
Researcher at University of Cambridge
Publications - 570
Citations - 37823
Christopher S. Reynolds is an academic researcher from University of Cambridge. The author has contributed to research in topics: Active galactic nucleus & Galaxy. The author has an hindex of 95, co-authored 541 publications receiving 34690 citations. Previous affiliations of Christopher S. Reynolds include University of Maryland, College Park & Tohoku Gakuin University.
Papers
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A Chandra HETGS Spectral Study of the Iron K Bandpass in MCG-6-30-15: A Narrow View of the Broad Iron Line
Andrew J. Young,Julia C. Lee,Andrew C. Fabian,Christopher S. Reynolds,R. R. Gibson,Claude R. Canizares +5 more
TL;DR: In this article, the authors present a high-resolution X-ray spectrum of the iron K bandpass in MCG-6-30-15 based on a 522 ks observation with Chandra's High Energy Transmission Grating Spectrometer (HETGS).
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Multi-epoch X-ray observations of the Seyfert 1.2 galaxy Mrk 79: bulk motion of the illuminating X-ray source
Luigi C. Gallo,Giovanni Miniutti,Jon M. Miller,Laura Brenneman,Andrew C. Fabian,Matteo Guainazzi,Christopher S. Reynolds +6 more
TL;DR: In this paper, multi-epoch X-ray spectroscopy (0.3 25keV) of the Seyfert 1.2 galaxy Mrk 79 (UGC 3973) spanning nearly eight years and a factor of three in broadband flux are analysed.
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The remarkable X-ray variability of IRAS 13224-3809 : I. The variability process
William Alston,A. C. Fabian,D. J. K. Buisson,Erin Kara,Michael Parker,Anne M. Lohfink,Phil Uttley,Dan R. Wilkins,Ciro Pinto,B. De Marco,Edward M. Cackett,Matthew J. Middleton,Dom Walton,Christopher S. Reynolds,Jiachen Jiang,Luigi C. Gallo,Abderahmen Zogbhi,G. Miniutti,Michal Dovciak,Andrew J. Young +19 more
TL;DR: In this article, a detailed X-ray timing analysis of the highly variable narrow-line Seyfert 1 (NLS1) galaxy IRAS 13224-3809 is presented.
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Testing the Propagating Fluctuations Model with a Long, Global Accretion Disk Simulation
TL;DR: In this article, the authors present an analysis of propagating fluctuations in a long-duration, high-resolution, global three-dimensional magnetohydrodynamic (MHD) simulation of a geometrically-thin ($h/r\approx 0.1$) accretion disk around a black hole.
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Ultrafast outflows disappear in high-radiation fields
Ciro Pinto,William Alston,Michael Parker,Andrew C. Fabian,Luigi C. Gallo,Douglas J. K. Buisson,Dominic J. Walton,Erin Kara,Jiachen Jiang,Anne M. Lohfink,Anne M. Lohfink,Christopher S. Reynolds +11 more
TL;DR: In this paper, the authors performed flux-resolved X-ray spectroscopy to study the variability of the UFO and found that the ionisation parameter is correlated with the luminosity.