A
Anthony J. Smith
Researcher at University of Sussex
Publications - 63
Citations - 7553
Anthony J. Smith is an academic researcher from University of Sussex. The author has contributed to research in topics: Galaxy & Luminous infrared galaxy. The author has an hindex of 36, co-authored 63 publications receiving 7170 citations.
Papers
More filters
Journal ArticleDOI
The Herschel-SPIRE instrument and its in-flight performance
Matthew Joseph Griffin,Alain Abergel,A. Abreu,Peter A. R. Ade,Philippe André,J.-L. Augueres,Tom Babbedge,Y. Bae,T. Baillie,Jean-Paul Baluteau,M. J. Barlow,George J. Bendo,Dominique Benielli,James J. Bock,P. Bonhomme,Drew Brisbin,C. Brockley-Blatt,Martin E. Caldwell,C. Cara,N. Castro-Rodriguez,R. Cerulli,Pierre Chanial,Pierre Chanial,Sina Chen,Eric M. Clark,David L. Clements,L. Clerc,J. Coker,D. Communal,Luca Conversi,Peter Timothy Cox,D. Crumb,C. R. Cunningham,F. Daly,Gary R. Davis,P. De Antoni,J. Delderfield,N. Devin,A. M. di Giorgio,Iris Didschuns,Kjetil Dohlen,M. Donati,A. Dowell,C. D. Dowell,L. Duband,Luc Dumaye,R. J. Emery,Marc Ferlet,D. Ferrand,Jean Fontignie,M. Fox,Alberto Franceschini,Margaret A. Frerking,Trevor Fulton,J. Garcia,R. Gastaud,Walter Kieran Gear,Jason Glenn,A-S Goizel,Douglas Griffin,T. Grundy,S. Guest,L. Guillemet,Peter Charles Hargrave,Martin Harwit,P. Hastings,Evanthia Hatziminaoglou,Evanthia Hatziminaoglou,M. Herman,B. Hinde,Viktor Hristov,Maohai Huang,P. Imhof,Kate Gudrun Isaak,Kate Gudrun Isaak,Ulf E. Israelsson,Rob Ivison,D. E. Jennings,Brian John Kiernan,K. J. King,Andrew E. Lange,William B. Latter,Glenn Laurent,Philippe Laurent,S. J. Leeks,Emmanuel Lellouch,Louis Levenson,Bo Li,Jin-Zeng Li,J. Lilienthal,T. L. Lim,S. J. Liu,N. Lu,Suzanne C. Madden,G. Mainetti,P. Marliani,D. J. McKay,K. Mercier,Sergio Molinari,Huw R. Morris,H. Moseley,Jerry Mulder,M. Mur,David A. Naylor,Hien Nguyen,B. O'Halloran,Seb Oliver,G. Olofsson,Hans Olofsson,R. Orfei,Mat Page,I. Pain,P. Panuzzo,Andreas Papageorgiou,G. Parks,P. Parr-Burman,Alan Pearce,C. P. Pearson,C. P. Pearson,Ismael Perez-Fournon,F. Pinsard,Giampaolo Pisano,Giampaolo Pisano,J. Podosek,Michael Pohlen,Edward Polehampton,Edward Polehampton,D. Pouliquen,D. Rigopoulou,D. Rizzo,Isaac Roseboom,Helene Roussel,Michael Rowan-Robinson,B. K. Rownd,P. Saraceno,Marc Sauvage,Richard S. Savage,Giorgio Savini,Giorgio Savini,Eric Sawyer,Carsten Scharmberg,D. Schmitt,D. Schmitt,Nicola Schneider,Benjamin L. Schulz,Arnold A. Schwartz,Rick Shafer,David L. Shupe,B. Sibthorpe,Sunil Sidher,Alan Smith,Anthony J. Smith,David J. Smith,Locke D. Spencer,Locke D. Spencer,Brian Stobie,Rashmikant V. Sudiwala,K. Sukhatme,Christian Surace,Jamie Stevens,B. M. Swinyard,Markos Trichas,T. Tourette,H. Triou,S. Tseng,Carole Tucker,A. D. Turner,Mattia Vaccari,Ivan Valtchanov,L. Vigroux,L. Vigroux,E. Virique,George M. Voellmer,H. J. Walker,Robyn L. Ward,Timothy James Waskett,M. Weilert,Roger Wesson,Glenn J. White,Glenn J. White,Nicola Jane Whitehouse,Christine D. Wilson,Berend Winter,Adam Woodcraft,Gillian S. Wright,C. K. Xu,Annie Zavagno,Michael Zemcov,L. Zhang,E. Zonca +189 more
TL;DR: The Spectral and Photometric Imaging REceiver (SPIRE) is the Herschel Space Observatory's sub-millimetre camera and spectrometer as discussed by the authors, which is used for image and spectroscopic data acquisition.
Journal ArticleDOI
A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34
Dominik Riechers,Dominik Riechers,Charles M. Bradford,Charles M. Bradford,David L. Clements,C. D. Dowell,C. D. Dowell,Ismael Perez-Fournon,Ismael Perez-Fournon,Rob Ivison,Rob Ivison,Carrie Bridge,A. Conley,Hai Fu,Joaquin Vieira,Julie Wardlow,J. A. Calanog,Asantha Cooray,Asantha Cooray,Peter Hurley,R. Neri,Julia Kamenetzky,James E. Aguirre,Bruno Altieri,V. Arumugam,Dominic J. Benford,Matthieu Béthermin,Matthieu Béthermin,James J. Bock,James J. Bock,Denis Burgarella,A. Cabrera-Lavers,A. Cabrera-Lavers,Scott Chapman,Peter Timothy Cox,James Dunlop,L. Earle,Duncan Farrah,P. Ferrero,P. Ferrero,Alberto Franceschini,Raphael Gavazzi,Jason Glenn,E. A. González Solares,Mark Gurwell,Mark Halpern,Evanthia Hatziminaoglou,A. Hyde,Edo Ibar,Attila Kovács,Attila Kovács,M. Krips,Roxana Lupu,P. R. Maloney,P. Martinez-Navajas,P. Martinez-Navajas,Hideo Matsuhara,Eric J. Murphy,B. J. Naylor,H. T. Nguyen,H. T. Nguyen,Seb Oliver,Alain Omont,M. J. Page,Glen Petitpas,Naseem Rangwala,Isaac Roseboom,Isaac Roseboom,Douglas Scott,Anthony J. Smith,Johannes Staguhn,Johannes Staguhn,Alina Streblyanska,Alina Streblyanska,Alasdair Thomson,Ivan Valtchanov,Marco P. Viero,Lin Wang,Michael Zemcov,Michael Zemcov,Jonas Zmuidzinas,Jonas Zmuidzinas +81 more
TL;DR: Despite the overall downturn in cosmic star formation towards the highest redshifts, it seems that environments mature enough to form the most massive, intense starbursts existed at least as early as 880 million years after the Big Bang.
Journal ArticleDOI
The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4
Carlotta Gruppioni,Francesca Pozzi,Giulia Rodighiero,Ivan Delvecchio,S. Berta,Lucia Pozzetti,G. Zamorani,P. Andreani,Alessandro Cimatti,O. Ilbert,E. Le Floc'h,Dieter Lutz,Benjamin Magnelli,Lucia Marchetti,Lucia Marchetti,Pierluigi Monaco,Raanan Nordon,Seb Oliver,P. Popesso,L. Riguccini,Isaac Roseboom,Isaac Roseboom,David J. Rosario,Mark Sargent,Mattia Vaccari,Mattia Vaccari,Bruno Altieri,H. Aussel,Ángel Bongiovanni,J. Cepa,Emanuele Daddi,H. Dominguez-Sanchez,H. Dominguez-Sanchez,D. Elbaz,N. M. Foerster Schreiber,R. Genzel,Alvaro Iribarrem,M. Magliocchetti,Roberto Maiolino,Albrecht Poglitsch,A. M. Pérez García,M. Sánchez-Portal,Eckhard Sturm,Linda J. Tacconi,Ivan Valtchanov,Alexandre Amblard,V. Arumugam,M. Bethermin,James J. Bock,James J. Bock,A. Boselli,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,P. Chanial,David L. Clements,A. Conley,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Eli Dwek,Stephen Anthony Eales,Alberto Franceschini,Jason Glenn,Matthew Joseph Griffin,Evanthia Hatziminaoglou,Edo Ibar,K. G. Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,Louis Levenson,Louis Levenson,Nanyao Y. Lu,S. C. Madden,Bruno Maffei,G. Mainetti,H. T. Nguyen,H. T. Nguyen,B. O'Halloran,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Dimitra Rigopoulou,Dimitra Rigopoulou,Michael Rowan-Robinson,Benjamin L. Schulz,Douglas Scott,Nick Seymour,Nick Seymour,D. L. Shupe,Anthony J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,L. Vigroux,Lian-Tao Wang,G. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov,S. Bardelli,M. Carollo,Thierry Contini,O. Le Fevre,Simon J. Lilly,Vincenzo Mainieri,Alvio Renzini,Marco Scodeggio,E. Zucca +118 more
TL;DR: In this article, the authors exploit the deep and extended far-IR data sets (at 70, 100 and 160 μm) of the GPS PACS Evolutionary Probe (PEP) Survey, in combination with the Herschel Multi-tiered Extragalactic Survey data at 250, 350 and 500 μm, to derive the evolution of the rest-frame 35-, 60-, 90- and total infrared luminosity functions (LFs) up to z ∼ 4.
Journal ArticleDOI
In-flight calibration of the Herschel-SPIRE instrument
B. M. Swinyard,Peter A. R. Ade,Jean-Paul Baluteau,Herve Aussel,M. J. Barlow,George J. Bendo,Dominique Benielli,James J. Bock,Drew Brisbin,A. Conley,L. Conversi,A. Dowell,Darren Dowell,Marc Ferlet,T. Fulton,Jason Glenn,Adrian M. Glauser,Adrian M. Glauser,Douglas Griffin,Matthew Joseph Griffin,S. Guest,P. Imhof,Kate Gudrun Isaak,S. C. Jones,K. J. King,S. J. Leeks,L. R. Levenson,T. L. Lim,Nanyao Y. Lu,Gibion Makiwa,David A. Naylor,Hien Nguyen,Seb Oliver,Pasquale Panuzzo,Andreas Papageorgiou,C. P. Pearson,C. P. Pearson,Michael Pohlen,Edward Polehampton,Edward Polehampton,D. Pouliquen,Dimitra Rigopoulou,Dimitra Rigopoulou,S. Ronayette,Helene Roussel,A. Rykala,Giorgio Savini,Bernhard Schulz,Arnold A. Schwartz,David L. Shupe,Bruce Sibthorpe,S. D. Sidher,Anthony J. Smith,Locke D. Spencer,Markos Trichas,H. Triou,Ivan Valtchanov,Roger Wesson,Adam Woodcraft,C. K. Xu,Michael Zemcov,L. Zhang +61 more
TL;DR: In this article, the authors present the photometric, spectroscopic and spatial accuracy of the SPIRE system using a combination of the emission from the Herschel telescope itself and the modelled continuum emission from solar system objects and other astronomical targets.
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.