M
Manfred W. Pakull
Researcher at University of Strasbourg
Publications - 58
Citations - 2220
Manfred W. Pakull is an academic researcher from University of Strasbourg. The author has contributed to research in topics: Galaxy & Luminosity. The author has an hindex of 23, co-authored 57 publications receiving 2087 citations.
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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.
Journal ArticleDOI
A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source
Christian Motch,Manfred W. Pakull,Roberto Soria,Fabien Grisé,Grzegorz Pietrzyński,Grzegorz Pietrzyński +5 more
TL;DR: The results demonstrate that in P13, soft thermal emission and spectral curvature are indeed signatures of supercritical accretion, and by analogy, ultraluminousX-ray sources with similar X-ray spectra and luminosities can be explained by super critical accretion onto massive stellar-mass black holes.
Journal ArticleDOI
A 300-parsec-long jet-inflated bubble around a powerful microquasar in the galaxy NGC 7793
TL;DR: It is reported that the large nebula S26 in the nearby galaxy NGC 7793 is powered by a black hole with a pair of collimated jets, similar to the famous Galactic source SS433, but twice as large and a few times more powerful.
Journal ArticleDOI
The XMM-Newton Serendipitous Survey I. The role of XMM-Newton Survey Science Centre
M. G. Watson,J.-L. Auguères,J. Ballet,Xavier Barcons,Didier Barret,M. Boer,Th. Boller,G. E. Bromage,Hermann Brunner,Francisco J. Carrera,Francisco J. Carrera,Mark Cropper,M. Denby,M. Ehle,Martin Elvis,A. C. Fabian,Michael Freyberg,P. Guillout,Jean-Marie Hameury,Günther Hasinger,D. Hinshaw,D. Hinshaw,Tommaso Maccacaro,Keith O. Mason,Richard G. McMahon,Laurent Michel,L. Mirioni,J. P. D. Mittaz,C. Motch,J-F. Olive,J. P. Osborne,Clive G. Page,Manfred W. Pakull,B. H. Perry,B. H. Perry,Marguerite Pierre,Wolfgang Pietsch,John P. Pye,A. M. Read,Timothy P.L. Roberts,Simon Rosen,J. L. Sauvageot,Axel Schwope,Kazuhiro Sekiguchi,G. C. Stewart,Ian M. Stewart,I. Valtchanov,Martin Ward,R. S. Warwick,Richard G. West,Nicholas E. White,Diana M Worrall +51 more
TL;DR: The role of the Survey Science Centre (SSC) in the XMM-Newton serendipitous survey is outlined in this article, together with the presentation of some of the first results.
Journal ArticleDOI
Probable intermediate-mass black holes in NGC 4559: XMM–Newton spectral and timing constraints
Mark Cropper,Roberto Soria,Richard Mushotzky,Kinwah Wu,Craig B. Markwardt,Craig B. Markwardt,Manfred W. Pakull +6 more
TL;DR: In this article, the authors examined X-ray and optical observations of two ultraluminous X-rays sources, X7 and X10 in NGC 4559, using XMM-Newton, Chandra and the Hubble Space Telescope (HST).