M
Michael Rowan-Robinson
Researcher at Imperial College London
Publications - 70
Citations - 2483
Michael Rowan-Robinson is an academic researcher from Imperial College London. The author has contributed to research in topics: Luminous infrared galaxy & Galaxy. The author has an hindex of 26, co-authored 70 publications receiving 2457 citations. Previous affiliations of Michael Rowan-Robinson include Queen Mary University of London.
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Journal ArticleDOI
A high-redshift IRAS galaxy with huge luminosity―hidden quasar or protogalaxy?
Michael Rowan-Robinson,Tom Broadhurst,Andy Lawrence,Richard G. McMahon,Carol J. Lonsdale,S. J. Oliver,A. N. Taylor,Perry B. Hacking,Perry B. Hacking,Tim Conrow,Tim Conrow,Will Saunders,Rowan Ellis,George Efstathiou,James J. Condon +14 more
TL;DR: In this article, the authors found an emission-line galaxy at a redshift of 2.286, and with the enormous far-infrared luminosity of 3 × 10^(14) times that of the Sun.
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The density field of the local universe
Will Saunders,Will Saunders,Carlos S. Frenk,Michael Rowan-Robinson,George Efstathiou,Andy Lawrence,Nick Kaiser,Richard S. Ellis,John W. Crawford,Xiao-Yang Xia,Ian Parry +10 more
TL;DR: An all-sky redshift survey of galaxies detected by IRAS (the Infrared Astronomical Satellite) has been used to map the Universe out to 140h−1 Mpc as mentioned in this paper.
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An Alternative to the cosmological 'concordance model'
TL;DR: In this article, it was shown that an Einstein-de Sitter universe with zero cosmological constant can fit the data as well as the best concordance model, and unlike a Λ-dominated universe, such an universe has no strong integrated Sachs-Wolfe effect.
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The spatial correlation function of IRAS galaxies on small and intermediate scales
TL;DR: In this article, the spatial correlation function of IRAS galaxies is determined on scales 0.1-30 h -1 Mpc using a cross-correlation technique between the QDOT survey and the QMW IRAS galaxy catalogue.
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An alternative to the cosmological 'concordance model'
TL;DR: In this article, the authors relax the hypothesis that the fluctuation spectrum can be described by a single power law, and demonstrate that an Einstein-de Sitter universe with zero cosmological constant can fit the data as well as the best concordance model.