S
Simon Dye
Researcher at University of Nottingham
Publications - 338
Citations - 31873
Simon Dye is an academic researcher from University of Nottingham. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 88, co-authored 328 publications receiving 30111 citations. Previous affiliations of Simon Dye include Cardiff University & Universities UK.
Papers
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Journal ArticleDOI
The shear power spectrum from the COMBO-17 survey
Michael L. Brown,A. N. Taylor,D. J. Bacon,Meghan E. Gray,Simon Dye,Klaus Meisenheimer,Christian Wolf +6 more
TL;DR: In this article, the authors performed a statistical weak lensing analysis of the COMBO-17 survey data set and measured the cosmological parameters, including the normalization of the matter power spectrum.
Journal ArticleDOI
Semi-linear gravitational lens inversion
Steve Warren,Simon Dye +1 more
TL;DR: In this paper, a method for analyzing gravitational lens images, where the source light distribution is pixelized, was proposed and shown to be suitable for high resolution, high S/N data of a multiply-imaged extended source.
Journal ArticleDOI
The formation and assembly of a typical star-forming galaxy at redshift z ≈ 3
TL;DR: In this paper, the authors observed a typical star-forming galaxy at z = 3.07, with a linear resolution of ~100 parsecs, and they found a well-ordered compact source in which molecular gas was being converted efficiently into stars, likely to be assembling a spheroidal bulge similar to those seen in spiral galaxies at the present day.
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The evolution of the near-IR galaxy Luminosity Function and colour bimodality up to z ~ 2 from the UKIDSS Ultra Deep Survey Early Data Release
M. Cirasuolo,Ross J. McLure,James Dunlop,Omar Almaini,Sylvie Foucaud,Ian Smail,K. Sekiguchi,Chris Simpson,Steve Eales,Simon Dye,M. G. Watson,M. J. Page,Paul Hirst +12 more
TL;DR: In this paper, the cosmological evolution of the near-infrared galaxy luminosity function was analyzed using a new sample of 22,000 K(AB) < 22.5 galaxies selected over an area of 0.6 square degrees from the Early Data Release of the UKIDSS Ultra Deep Survey (UDS).
Journal ArticleDOI
Gas and dust in a submillimeter galaxy at z = 4.24 from the Herschel ATLAS
Pierre Cox,M. Krips,R. Neri,A. Omont,R. Güsten,Karl M. Menten,Friedrich Wyrowski,Axel Weiss,Alexandre Beelen,Mark Gurwell,Helmut Dannerbauer,Rob Ivison,M. Negrello,Itziar Aretxaga,David H. Hughes,Robbie Richard Auld,Maarten Baes,R. Blundell,S. Buttiglione,Antonio Cava,Asantha Cooray,A. Dariush,Loretta Dunne,Simon Dye,Stephen Anthony Eales,Dave Frayer,Jacopo Fritz,R. Gavazzi,R. Hopwood,E. Ibar,Matt J. Jarvis,Steve Maddox,Michał J. Michałowski,Enzo Pascale,Michael Pohlen,E. E. Rigby,D. J. B. Smith,A. M. Swinbank,Pasquale Temi,I. Valtchanov,P. van der Werf,G. de Zotti +41 more
TL;DR: In this article, ground-based follow-up observations of the exceptional source, ID141, one of the brightest sources detected so far in the H-ATLAS cosmological survey are reported.