Matthew Joseph Griffin
Cardiff University
535 Papers
11.8K Citations
Matthew Joseph Griffin is an academic researcher from Cardiff University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 92, co-authored 513 publications. Previous affiliations of Matthew Joseph Griffin include University of London & Max Planck Society.
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Papers
Bolometers for far-infrared and submillimetre astronomy
TL;DR: In this article, a review of the development of a wide range of sensor arrays for ground-based and space-borne far-infrared and sub-millimetre observations is presented, including spider-web NTD bolometers, transition-edge superconducting sensors and micromachined planar arrays of ion-implanted silicon bolometers.
Evidence for Environmental Changes in the Submillimeter Dust Opacity
Peter G. Martin,A. Roy,Sylvain Bontemps,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,Peter A. R. Ade,James J. Bock,Edward L. Chapin,Mark J. Devlin,Simon Dicker,Matthew Joseph Griffin,Joshua O. Gundersen,Mark Halpern,Peter Charles Hargrave,David H. Hughes,Jeff Klein,Gaelen Marsden,Philip Daniel Mauskopf,Calvin B. Netterfield,Luca Olmi,Guillaume Patanchon,Marie Rex,Douglas Scott,Christopher Semisch,Matthew D. P. Truch,Carole Tucker,Gregory S. Tucker,Marco P. Viero,Donald Wiebe +28 more
TL;DR: In this article, a pixel-by-pixel correlation of images of continuum emission with a proxy for column density was used to quantify the submillimeter opacity of dust in the diffuse interstellar medium (ISM) in the Galactic plane.
Probing the molecular interstellar medium of M82 with Herschel-SPIRE spectroscopy ?
Pasquale Panuzzo,Naseem Rangwala,A. Rykala,Kate Gudrun Isaak,Kate Gudrun Isaak,Jason Glenn,Christine D. Wilson,Robbie Richard Auld,Maarten Baes,M. J. Barlow,George J. Bendo,James J. Bock,Alessandro Boselli,M. Bradford,V. Buat,N. Castro-Rodriguez,Pierre Chanial,Stephane Charlot,Laure Ciesla,David L. Clements,A. Cooray,Diane Cormier,Luca Cortese,Jonathan Ivor Davies,Eli Dwek,Stephen Anthony Eales,D. Elbaz,T. Fulton,Maud Galametz,Frédéric Galliano,Walter Kieran Gear,Haley Louise Gomez,Matthew Joseph Griffin,Sacha Hony,L. R. Levenson,N. Lu,Suzanne C. Madden,B. O'Halloran,Koryo Okumura,Seb Oliver,Mat Page,Andreas Papageorgiou,T. J. Parkin,Ismael Perez-Fournon,Michael Pohlen,Edward Polehampton,Edward Polehampton,E. E. Rigby,Helene Roussel,N. Sacchi,Marc Sauvage,Benjamin L. Schulz,Maximilien R. P. Schirm,Matthew Smith,L. Spinoglio,Jamie Stevens,Sundar Srinivasan,M. Symeonidis,B. Swinyard,Markos Trichas,Mattia Vaccari,L. Vigroux,Herve Wozniak,Gillian S. Wright,Werner W. Zeilinger +64 more
TL;DR: In this paper, the Herschel SPIRE Fourier transform spectrometer was used to detect the CO rotational ladder from 4 − 3 to 13 − 12 emitted by the central region of the starburst galaxy M82.
SPIRE instrument for FIRST
TL;DR: SPIRE, the Spectral and Photometric Imaging Receiver, will be a bolometer instrument for ESA's FIRST satellite as mentioned in this paper, whose main scientific goals are deep extragalactic and galactic imaging surveys and spectroscopy of star-forming regions in own and nearby galaxies.
The Herschel census of infrared SEDs through cosmic time
M. Symeonidis,Mattia Vaccari,Mattia Vaccari,S. Berta,Mat Page,Dieter Lutz,V. Arumugam,Herve Aussel,James J. Bock,James J. Bock,A. Boselli,V. Buat,Peter Capak,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Duncan Farrah,Alberto Franceschini,E. Giovannoli,Jason Glenn,Matthew Joseph Griffin,Evanthia Hatziminaoglou,Ho Seong Hwang,Edo Ibar,O. Ilbert,Rob Ivison,E. Le Floc'h,S. J. Lilly,J. Kartaltepe,Benjamin Magnelli,Georgios E. Magdis,Lucia Marchetti,H. T. Nguyen,H. T. Nguyen,Raanan Nordon,B. O'Halloran,Seb Oliver,Alain Omont,Andreas Papageorgiou,H. Patel,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,P. Popesso,Francesca Pozzi,D. Rigopoulou,D. Rigopoulou,L. Riguccini,David J. Rosario,Isaac Roseboom,Michael Rowan-Robinson,Mara Salvato,Benjamin L. Schulz,Douglas Scott,Nick Seymour,D. L. Shupe,Anthony J. Smith,Ivan Valtchanov,Lian-Tao Wang,C. K. Xu,Michael Zemcov,Michael Zemcov,Stijn Wuyts +68 more
TL;DR: In this paper, the authors examined the dust properties of infrared (IR)-luminous (LIR > 1010 L⊙) galaxies at 0.1 45 K.