M
Mickael Coriat
Researcher at University of Toulouse
Publications - 52
Citations - 2560
Mickael Coriat is an academic researcher from University of Toulouse. The author has contributed to research in topics: Accretion (astrophysics) & Black hole. The author has an hindex of 20, co-authored 46 publications receiving 2032 citations. Previous affiliations of Mickael Coriat include Paris Diderot University & University of Cape Town.
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Journal ArticleDOI
The XMM-Newton serendipitous survey - VII. The third XMM-Newton serendipitous source catalogue
Simon Rosen,Natalie A. Webb,Natalie A. Webb,M. G. Watson,Jean Ballet,Didier Barret,Didier Barret,Valentina Braito,Valentina Braito,Francisco J. Carrera,María Teresa Ceballos,Mickael Coriat,Mickael Coriat,R. Della Ceca,G. Denkinson,P. Esquej,Sean Farrell,Michael Freyberg,Fabien Grisé,Patrick Guillout,L. Heil,Filippos Koliopanos,Filippos Koliopanos,D. Law-Green,Georg Lamer,Dacheng Lin,Dacheng Lin,Dacheng Lin,R. Martino,Laurent Michel,Christian Motch,A. Nebot Gomez-Moran,Clive G. Page,K. L. Page,M. J. Page,Manfred W. Pakull,John P. Pye,A. M. Read,P. Rodriguez,Masaaki Sakano,R. D. Saxton,Axel Schwope,A. E. Scott,Richard Sturm,I. Traulsen,Vladimir Yershov,Ivan Zolotukhin,Ivan Zolotukhin +47 more
TL;DR: The 3XMM-DR5 dataset as mentioned in this paper contains 565,962 X-ray detections from the European Space Agency X-Ray observatory XMM-Newton.
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Ubiquitous equatorial accretion disc winds in black hole soft states
Gabriele Ponti,Rob Fender,Mitchell C. Begelman,Mitchell C. Begelman,Robert Dunn,Joseph Neilsen,Mickael Coriat +6 more
TL;DR: In this article, the authors show that a powerful accretion disc wind is observed to be present in softer X-ray states and it has been suggested that it can carry away enough mass and energy to quench the radio jet.
Journal ArticleDOI
Radiatively efficient accreting black holes in the hard state: the case study of H1743-322
Mickael Coriat,Stephane Corbel,Stephane Corbel,L. Prat,James Miller-Jones,D. Cseh,Anastasios Tzioumis,Catherine Brocksopp,Jerome Rodriguez,Rob Fender,Gregory R. Sivakoff +10 more
TL;DR: In this article, the radio and X-ray emission of H1743−322 were investigated and it was shown that the inner accretion flow is radiatively efficient during the hard state, in contrast to what is usually assumed for black hole Xray binaries in this spectral state.
Journal ArticleDOI
Disc-jet coupling in the 2009 outburst of the black hole candidate H1743-322
James Miller-Jones,Gregory R. Sivakoff,Gregory R. Sivakoff,Diego Altamirano,Mickael Coriat,Mickael Coriat,Stephane Corbel,Vivek Dhawan,H. A. Krimm,Ronald A. Remillard,Michael P. Rupen,David M. Russell,Rob Fender,Rob Fender,Sebastian Heinz,Elmar Körding,Elmar Körding,Dipankar Maitra,Sera Markoff,Simone Migliari,Craig L. Sarazin,Valeriu Tudose +21 more
TL;DR: In this article, the authors present an intensive radio and X-ray monitoring campaign on the 2009 outburst of the Galactic black hole candidate Xray binary H1743−322, and measure the proper motions of the jet ejecta relative to the position of the compact core jets detected at the beginning of the outburst.
Journal ArticleDOI
A close-pair binary in a distant triple supermassive black hole system.
Roger Deane,Zsolt Paragi,Matt J. Jarvis,Mickael Coriat,Gianni Bernardi,Rob Fender,Sándor Frey,Ian Heywood,Hans-Rainer Klöckner,K. J. B. Grainge,Clare Rumsey +10 more
TL;DR: Observations of a triple black hole system at redshift z = 0.39 conclude that tight pairs are more common than hitherto believed, which is an important observational constraint for low-frequency gravitational wave experiments.