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.
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Journal ArticleDOI
The UKIRT Infrared Deep Sky Survey (UKIDSS)
Andy Lawrence,Stephen J. Warren,Omar Almaini,Alastair C. Edge,Nigel Hambly,Richard F. Jameson,Philip W. Lucas,M. Casali,Andrew J. Adamson,Simon Dye,J. P. Emerson,S. Foucaud,P. C. Hewett,Paul Hirst,Simon Hodgkin,Mike Irwin,N. Lodieu,Richard G. McMahon,Chris Simpson,Chris Simpson,Ian Smail,Daniel J. Mortlock,M. Folger +22 more
TL;DR: The final version published in MNRAS August 2007 included significant revisions including significant revisions to the original version April 2006.
Journal ArticleDOI
A luminous quasar at a redshift of z = 7.085
Daniel J. Mortlock,Stephen J. Warren,Bram Venemans,Mitesh Patel,Paul C. Hewett,Richard G. McMahon,Chris Simpson,Tom Theuns,Tom Theuns,E. Gonzales-Solares,Andy Adamson,Simon Dye,Nigel Hambly,Paul Hirst,Mike Irwin,Ernst Kuiper,Andy Lawrence,Huub Röttgering +17 more
TL;DR: Observations of a quasar at a redshift of 7.3 are reported, suggesting that the neutral fraction of the intergalactic medium in front of ULAS J1120+0641 exceeded 0.1.
Journal ArticleDOI
Nearly 5000 Distant Early-Type Galaxies in COMBO-17: A Red Sequence and Its Evolution since z ~ 1
Eric F. Bell,Christian Wolf,Klaus Meisenheimer,Hans-Walter Rix,Andrea Borch,Simon Dye,M. Kleinheinrich,Lutz Wisotzki,Daniel H. McIntosh +8 more
TL;DR: In this paper, the rest-frame colors and luminosities of 25,000 mR 24 galaxies in the redshift range 0.2 < z ≤ 1.1 drawn from the COMBO-17 survey (Classifying Objects by Medium-Band Observations in 17 Filters).
Journal ArticleDOI
Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release
Simon P. Driver,David T. Hill,Lee S. Kelvin,Aaron S. G. Robotham,Jochen Liske,Peder Norberg,Ivan K. Baldry,Steven P. Bamford,Andrew M. Hopkins,Jon Loveday,John A. Peacock,E. Andrae,Jonathan Bland-Hawthorn,Sarah Brough,Michael J. I. Brown,Ewan Cameron,J. H. Y. Ching,Matthew Colless,Christopher J. Conselice,Scott M. Croom,Nicholas Cross,R. De Propris,Simon Dye,Michael J. Drinkwater,Simon Ellis,Alister W. Graham,Meiert W. Grootes,Madusha Gunawardhana,David Heath Jones,E. van Kampen,Claudia Maraston,Robert C. Nichol,H Parkinson,Steven Phillipps,Kevin A. Pimbblet,Cristina Popescu,Matthew Prescott,Isaac Roseboom,Elaine M. Sadler,Anne E. Sansom,Rob Sharp,Daniel J. Smith,Edward N. Taylor,Edward N. Taylor,Daniel Thomas,Richard J. Tuffs,D. Wijesinghe,Loretta Dunne,Carlos S. Frenk,Matt J. Jarvis,Barry F. Madore,Martin Meyer,Mark Seibert,Lister Staveley-Smith,William J. Sutherland,Stephen J. Warren +55 more
TL;DR: The Galaxy and Mass Assembly (GAMA) survey has been operating since 2008 February on the 3.9m Anglo-Australian Telescope using the AAOmega fibre-fed spectrograph facility to acquire spectra with a resolution of R ≈ 1300 for 120 862 Sloan Digital Sky Survey selected galaxies.
Journal ArticleDOI
The Herschel Multi-tiered Extragalactic Survey: HerMES
Seb Oliver,James J. Bock,James J. Bock,Bruno Altieri,Alexandre Amblard,V. Arumugam,Herve Aussel,Tom Babbedge,Alexandre Beelen,Matthieu Béthermin,Matthieu Béthermin,Andrew Blain,Alessandro Boselli,C. Bridge,Drew Brisbin,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,P. Chanial,Michele Cirasuolo,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Elizabeth Dubois,Eli Dwek,Simon Dye,Stephen Anthony Eales,David Elbaz,Duncan Farrah,A. Feltre,P. Ferrero,P. Ferrero,N. Fiolet,N. Fiolet,M. Fox,Alberto Franceschini,Walter Kieran Gear,E. Giovannoli,Jason Glenn,Yan Gong,E. A. González Solares,Matthew Joseph Griffin,Mark Halpern,Martin Harwit,Evanthia Hatziminaoglou,Sebastien Heinis,Peter Hurley,Ho Seong Hwang,A. Hyde,Edo Ibar,O. Ilbert,K. G. Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,E. Le Floc'h,L. R. Levenson,L. R. Levenson,B. Lo Faro,Nanyao Y. Lu,S. C. Madden,Bruno Maffei,Georgios E. Magdis,G. Mainetti,Lucia Marchetti,G. Marsden,J. Marshall,J. Marshall,A. M. J. Mortier,Hien Nguyen,Hien Nguyen,B. O'Halloran,Alain Omont,Mat Page,P. Panuzzo,Andreas Papageorgiou,H. Patel,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Jonathan Rawlings,Gwenifer Raymond,Dimitra Rigopoulou,Dimitra Rigopoulou,L. Riguccini,D. Rizzo,Giulia Rodighiero,Isaac Roseboom,Isaac Roseboom,Michael Rowan-Robinson,M. Sanchez Portal,Benjamin L. Schulz,Douglas Scott,Nick Seymour,Nick Seymour,D. L. Shupe,A. J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,Joaquin Vieira,Marco P. Viero,L. Vigroux,Lifan Wang,Robyn L. Ward,Julie Wardlow,G. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +120 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ∼380deg^2 as mentioned in this paper.