G
Gwenifer Raymond
Researcher at Cardiff University
Publications - 40
Citations - 4022
Gwenifer Raymond is an academic researcher from Cardiff University. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 27, co-authored 40 publications receiving 3870 citations.
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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.
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,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,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 +118 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ~380 deg^2 as mentioned in this paper.
Journal ArticleDOI
HerMES: SPIRE galaxy number counts at 250, 350 and 500 microns
Seb Oliver,Lingyu Wang,Andrew Smith,Bruno Altieri,A. Amblard,V. Arumugam,Robbie Richard Auld,H. Aussel,Tom Babbedge,Andrew Blain,J. J. Bock,A. Boselli,V. Buat,Denis Burgarella,N. Castro-Rodriguez,Antonio Cava,P. Chanial,D. L. Clements,Alex Conley,Luca Conversi,Asantha Cooray,C. D. Dowell,E. Dwek,Steve Eales,D. Elbaz,M. Fox,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,Matthew Joseph Griffin,Mark Halpern,Evanthia Hatziminaoglou,E. Ibar,K. G. Isaak,Rob Ivison,G. Lagache,Louis Levenson,Nanyao Y. Lu,S. C. Madden,Bruno Maffei,G. Mainetti,Lucia Marchetti,K. Mitchell-Wynne,Angela M. J. Mortier,H. T. Nguyen,B. O'Halloran,A. Omont,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,I. Perez-Fournon,M. Pohlen,Jonathan Rawlings,Gwenifer Raymond,D. Rigopoulou,D. Rizzo,Isaac Roseboom,Michael Rowan-Robinson,M. Sanchez Portal,Richard S. Savage,Benjamin L. Schulz,Douglas Scott,Nick Seymour,David L. Shupe,Jamie Stevens,M. Symeonidis,M. Trichas,K. E. Tugwell,Mattia Vaccari,Elisabetta Valiante,I. Valtchanov,Joaquin Vieira,L. Vigroux,Robyn L. Ward,G. Wright,C. K. Xu,Michael Zemcov +77 more
TL;DR: In this paper, the authors used the SPIRE instrument on the Herschel Multi-tiered Extra-Galactic Survey (HerMES) to directly resolve 15% of the infrared extra-galactic background at the wavelength near where it peaks.
Journal ArticleDOI
HerMES: SPIRE galaxy number counts at 250, 350, and 500 μm
Seb Oliver,Lin Wang,Anthony J. Smith,Bruno Altieri,Alexandre Amblard,V. Arumugam,Robbie Richard Auld,Herve Aussel,Tom Babbedge,Andrew Blain,James J. Bock,James J. Bock,Alessandro Boselli,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,Antonio Cava,Pierre Chanial,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Eli Dwek,Stephen Anthony Eales,D. Elbaz,M. Fox,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,Matthew Joseph Griffin,Mark Halpern,Evanthia Hatziminaoglou,Edo Ibar,Kate Gudrun Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,Louis Levenson,Louis Levenson,Nanyao Y. Lu,Suzanne C. Madden,Bruno Maffei,G. Mainetti,Lucia Marchetti,K. Mitchell-Wynne,Angela M. J. Mortier,Hien Nguyen,Hien Nguyen,B. O'Halloran,Alain Omont,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Jonathan Rawlings,Gwenifer Raymond,Dimitra Rigopoulou,Dimitra Rigopoulou,D. Rizzo,Isaac Roseboom,Michael Rowan-Robinson,M. Sanchez Portal,Richard S. Savage,Richard S. Savage,Benjamin L. Schulz,Douglas Scott,Nick Seymour,D. L. Shupe,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Elisabetta Valiante,Ivan Valtchanov,Joaquin Vieira,L. Vigroux,Robyn L. Ward,Gillian S. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +90 more
TL;DR: In this paper, the authors used the SPIRE instrument on the Herschel Multi-tiered Extra-Galactic Survey (HerMES) to directly resolve ~15% of the infrared extra-galactic background at the wavelength near where it peaks.
Journal ArticleDOI
The far-infrared/radio correlation as probed by Herschel
Rob Ivison,Rob Ivison,Benjamin Magnelli,Edo Ibar,Paola Andreani,D. Elbaz,Bruno Altieri,Alexandre Amblard,V. Arumugam,Robbie Richard Auld,Herve Aussel,Tom Babbedge,S. Berta,Andrew Blain,James J. Bock,James J. Bock,Ángel Bongiovanni,Alessandro Boselli,V. Buat,Denis Burgarella,N. Castro-Rodriguez,Antonio Cava,J. Cepa,Pierre Chanial,Andrea Cimatti,Michele Cirasuolo,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,Emanuele Daddi,H. Dominguez,Charles D. Dowell,Charles D. Dowell,Eli Dwek,Stephen Anthony Eales,Duncan Farrah,N. M. Förster Schreiber,M. Fox,Alberto Franceschini,Walter Kieran Gear,Reinhard Genzel,Jason Glenn,Matthew Joseph Griffin,Carlotta Gruppioni,Mark Halpern,Evanthia Hatziminaoglou,Kate Gudrun Isaak,Guilaine Lagache,L. R. Levenson,L. R. Levenson,Nanyao Y. Lu,Dieter Lutz,Suzanne C. Madden,Bruno Maffei,Georgios E. Magdis,G. Mainetti,Roberto Maiolino,Lucia Marchetti,G. E. Morrison,Angela M. J. Mortier,Hien Nguyen,Hien Nguyen,Raanan Nordon,B. O'Halloran,S. J. Oliver,Alain Omont,Frazer N. Owen,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,A. M. Pérez García,Albrecht Poglitsch,Michael Pohlen,P. Popesso,Francesca Pozzi,Jonathan Rawlings,Gwenifer Raymond,Dimitra Rigopoulou,Dimitra Rigopoulou,L. Riguccini,D. Rizzo,Giulia Rodighiero,Isaac Roseboom,Michael Rowan-Robinson,Amélie Saintonge,M. Sanchez Portal,P. Santini,Benjamin L. Schulz,Douglas Scott,Nick Seymour,Lijing Shao,D. L. Shupe,A. J. Smith,Jamie Stevens,E. Sturm,M. Symeonidis,Linda J. Tacconi,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,Joaquin Vieira,L. Vigroux,Lian-Tao Wang,Robyn L. Ward,Gillian S. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +113 more
TL;DR: In this article, the authors determined the ratio, q(IR), of rest-frame 8-1000um flux to monochromatic radio flux, S(1.4GHz), for galaxies selected at far-IR and radio wavelengths, to search for signs that the ratio evolves with redshift, luminosity or dust temperature.