A. M. J. Mortier
Imperial College London
43 Papers
518 Citations
A. M. J. Mortier is an academic researcher from Imperial College London. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 27, co-authored 43 publications. Previous affiliations of A. M. J. Mortier include University of Kent & University of Edinburgh.
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Papers
The SCUBA HAlf Degree Extragalactic Survey - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies
Rob Ivison,Rob Ivison,Thomas R. Greve,James Dunlop,John A. Peacock,Eiichi Egami,Ian Smail,Edo Ibar,E. van Kampen,Itziar Aretxaga,Tom Babbedge,A. D. Biggs,Andrew Blain,Scott Chapman,David L. Clements,K. Coppin,K. Coppin,Duncan Farrah,Mark Halpern,David H. Hughes,Matt J. Jarvis,T. Jenness,Jessica Jones,A. M. J. Mortier,Seb Oliver,C. Papovich,Pablo G. Pérez-González,Alexandra Pope,Steve Rawlings,George H. Rieke,Michael Rowan-Robinson,Richard S. Savage,Douglas Scott,Marc S. Seigar,Stephen Serjeant,Chris Simpson,Jamie Stevens,Mattia Vaccari,Mattia Vaccari,Jeff Wagg,Jeff Wagg,Chris J. Willott +41 more
- 01 Sep 2007
TL;DR: In this paper, the authors identify robust radio and/or infrared counterparts, and hence accurate positions, for over two-thirds of the SCUBA HAlf-Degree Extragalactic Survey (SHADES) Source Catalogue, presenting optical, 24-μm and radio images of each SMG.
DISCOVERY OF A GIANT Lyα EMITTER NEAR THE REIONIZATION EPOCH
Masami Ouchi,Masami Ouchi,Yoshiaki Ono,Eiichi Egami,T. Saito,Masamune Oguri,Patrick J. McCarthy,Duncan Farrah,Duncan Farrah,Nobunari Kashikawa,Ivelina Momcheva,Kazuhiro Shimasaku,Kouichiro Nakanishi,Hisanori Furusawa,Masayuki Akiyama,James Dunlop,James Dunlop,A. M. J. Mortier,Sadanori Okamura,Masao Hayashi,Michele Cirasuolo,Alan Dressler,Masanori Iye,Matt J. Jarvis,Tadayuki Kodama,Crystal L. Martin,Ross J. McLure,Kouji Ohta,Toru Yamada,Michitoshi Yoshida +29 more
TL;DR: In this paper, the authors reported the discovery of a giant Lyα emitter with a Spitzer/Infrared Array Camera (IRAC) counterpart near the reionization epoch at z = 6.595.
The Herschel Multi-Tiered Extragalactic Survey: source extraction and cross-identifications in confusion-dominated SPIRE images
Isaac Roseboom,Seb Oliver,Martin Kunz,Bruno Altieri,Alexandre Amblard,V. Arumugam,Robbie Richard Auld,Herve Aussel,T. Babbedge,Matthieu Béthermin,Andrew Blain,James J. Bock,James J. Bock,Alessandro Boselli,Drew Brisbin,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,Antonio Cava,Pierre Chanial,Edward L. Chapin,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Eli Dwek,Simon Dye,Stephen Anthony Eales,David Elbaz,Duncan Farrah,M. Fox,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,E. A. González Solares,Matthew Joseph Griffin,Mark Halpern,Martin Harwit,Evanthia Hatziminaoglou,J.-S. Huang,Edo Ibar,Kate Gudrun Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,L. R. Levenson,L. R. Levenson,N. Lu,Suzanne C. Madden,Bruno Maffei,G. Mainetti,Lucia Marchetti,G. Marsden,A. M. J. Mortier,Hien Nguyen,Hien Nguyen,B. O'Halloran,Alain Omont,Mat Page,Pasquale Panuzzo,Andreas Papageorgiou,H. Patel,C. P. Pearson,C. P. Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Jonathan Rawlings,Gwenifer Raymond,Dimitra Rigopoulou,Dimitra Rigopoulou,D. Rizzo,Michael Rowan-Robinson,M. Sanchez Portal,Benjamin L. Schulz,Douglas Scott,Nick Seymour,D. L. Shupe,A. J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,Joaquin Vieira,L. Vigroux,Lian-Tao Wang,Robyn L. Ward,G. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +97 more
- 21 Nov 2010
TL;DR: In this paper, a combination of linear inversion and model selection techniques is used to produce reliable cross-identification catalogues based on Spitzer MIPS 24-mu m source positions.
HerMES: Far infrared properties of known AGN in the HerMES fields
Evanthia Hatziminaoglou,Alain Omont,Jamie Stevens,Alexandre Amblard,V. Arumugam,Robbie Richard Auld,Herve Aussel,T. Babbedge,Andrew Blain,James J. Bock,James J. Bock,Alessandro Boselli,V. Buat,Denis Burgarella,N. Castro-Rodriguez,Antonio Cava,Pierre Chanial,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,Charles D. Dowell,Charles D. Dowell,Eli Dwek,Simon Dye,Stephen Anthony Eales,David Elbaz,Duncan Farrah,M. Fox,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,E. A. González Solares,Matthew Joseph Griffin,Mark Halpern,Edo Ibar,Kate Gudrun Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,L. R. Levenson,L. R. Levenson,N. Lu,Suzanne C. Madden,Bruno Maffei,G. Mainetti,Lucia Marchetti,A. M. J. Mortier,Hien Nguyen,Hien Nguyen,B. O'Halloran,Seb Oliver,M. J. Page,P. Panuzzo,Andreas Papageorgiou,C. P. Pearson,C. P. Pearson,Ismael Perez-Fournon,Michael Pohlen,J. I. Rawlings,Dimitra Rigopoulou,Dimitra Rigopoulou,D. Rizzo,Isaac Roseboom,Michael Rowan-Robinson,M. Sanchez Portal,Benjamin L. Schulz,Douglas Scott,Nick Seymour,D. L. Shupe,A. J. Smith,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,L. Vigroux,Lifan Wang,Robyn L. Ward,Gillian S. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +83 more
TL;DR: In this paper, the authors study large samples of spectroscopically confirmed type 1 and type 2 AGN lying within the Herschel Multi-tiered Extragalactic Survey (HerMES) fields observed during the science demonstration phase, aiming to understand their FIR colour distributions and constrain their starburst contributions.
Evolution of dust temperature of galaxies through cosmic time as seen by Herschel
Ho Seong Hwang,David Elbaz,Georgios E. Magdis,Emanuele Daddi,M. Symeonidis,Bruno Altieri,Alexandre Amblard,Paola Andreani,V. Arumugam,Robbie Richard Auld,Herve Aussel,T. Babbedge,S. Berta,Andrew Blain,James J. Bock,James J. Bock,Ángel Bongiovanni,Ángel Bongiovanni,Alessandro Boselli,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,Antonio Cava,J. Cepa,J. Cepa,Pierre Chanial,Edward L. Chapin,Ranga-Ram Chary,Andrea Cimatti,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,Helmut Dannerbauer,Mark Dickinson,H. Dominguez,Charles D. Dowell,Charles D. Dowell,James Dunlop,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,Edo Ibar,Kate Gudrun Isaak,Rob Ivison,Rob Ivison,Woong-Seob Jeong,Guilaine Lagache,D. Le Borgne,E. Le Floc'h,H. M. Lee,Jounghun Lee,Myung Gyoon Lee,L. R. Levenson,L. R. Levenson,N. Lu,Dieter Lutz,Suzanne C. Madden,Bruno Maffei,Benjamin Magnelli,G. Mainetti,Roberto Maiolino,Lucia Marchetti,A. M. J. Mortier,Hien Nguyen,Hien Nguyen,Raanan Nordon,B. O'Halloran,Koryo Okumura,S. J. Oliver,Alain Omont,Mat Page,P. Panuzzo,Andreas Papageorgiou,C. P. Pearson,C. P. Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,A. M. Pérez García,A. M. Pérez García,Albrecht Poglitsch,Michael Pohlen,Paola Popesso,Francesca Pozzi,Jonathan Rawlings,Dimitra Rigopoulou,Dimitra Rigopoulou,L. Riguccini,D. Rizzo,Giulia Rodighiero,Isaac Roseboom,Michael Rowan-Robinson,Amélie Saintonge,M. Sanchez Portal,Paola Santini,Marc Sauvage,Benjamin L. Schulz,Douglas Scott,Nick Seymour,Lijing Shao,D. L. Shupe,A. J. Smith,Jamie Stevens,E. Sturm,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 +129 more
- 21 Nov 2010
TL;DR: In this paper, the spectral energy distribution fit of the far-IR (FIR) flux densities obtained with the PACS and SPIRE instruments onboard Herschel was analyzed for galaxies in the redshift range 0.1 to 0.5.