J
Jason Glenn
Researcher at University of Colorado Boulder
Publications - 339
Citations - 28559
Jason Glenn is an academic researcher from University of Colorado Boulder. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 81, co-authored 333 publications receiving 27203 citations. Previous affiliations of Jason Glenn include University of Arizona & Goddard Space Flight Center.
Papers
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Journal ArticleDOI
The far-infrared/radio correlation as probed by Herschel
Rob Ivison,Benjamin Magnelli,Edo Ibar,P. Andreani,D. Elbaz,Bruno Altieri,Alexandre Amblard,V. Arumugam,Robbie Richard Auld,H. Aussel,Tom Babbedge,S. Berta,Andrew Blain,James J. Bock,Ángel Bongiovanni,A. Boselli,V. Buat,Denis Burgarella,N. Castro,Antonio Cava,J. Cepa,P. Chanial,A. Cimatti,M. Cirasuolo,David L. Clements,A. Conley,Luca Conversi,Asantha Cooray,Emanuele Daddi,H. Dominguez,C. D. Dowell,E. Dwek,Stephen Anthony Eales,Duncan Farrah,M. Fox,Alberto Franceschini,Walter Kieran Gear,Reinhard Genzel,Jason Glenn,Matthew Joseph Griffin,Carlotta Gruppioni,Mark Halpern,Evanthia Hatziminaoglou,K. G. Isaak,Guilaine Lagache,L. R. Levenson,Nanyao Y. Lu,Dieter Lutz,S. C. Madden,Bruno Maffei,Georgios E. Magdis,G. Mainetti,Roberto Maiolino,Lucia Marchetti,G. E. Morrison,Angela M. J. Mortier,Hien Nguyen,Raanan Nordon,B. O'Halloran,S. J. Oliver,A. Omont,Frazer N. Owen,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,Albrecht Poglitsch,Michael Pohlen,P. Popesso,Francesca Pozzi,Jonathan Rawlings,Gwenifer Raymond,D. Rigopoulou,L. Riguccini,D. Rizzo,Giulia Rodighiero,Isaac Roseboom,Michael Rowan-Robinson,Amelie 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,Lingyu Wang,Robyn L. Ward,Gillian S. Wright,C. K. Xu,Michael Zemcov +101 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.
Journal ArticleDOI
Herschel and SCUBA-2 imaging and spectroscopy of a bright, lensed submillimetre galaxy at z = 2.3
Rob Ivison,A. M. Swinbank,B. Swinyard,Ian Smail,Chris Pearson,D. Rigopoulou,Edward Polehampton,Jean-Paul Baluteau,M. J. Barlow,Andrew Blain,J. J. Bock,David L. Clements,K. Coppin,Asantha Cooray,A. L. R. Danielson,E. Dwek,Alastair C. Edge,Alberto Franceschini,Trevor Fulton,Jason Glenn,Matthew Joseph Griffin,K. G. Isaak,Sarah Leeks,T. L. Lim,David A. Naylor,S. J. Oliver,Mat Page,Ismael Perez-Fournon,Michael Rowan-Robinson,Giorgio Savini,Douglas Scott,Locke D. Spencer,Ivan Valtchanov,L. Vigroux,Gillian S. Wright +34 more
TL;DR: In this paper, a detailed analysis of the far-IR properties of the bright, lensed, z = 2.3, SMG, SMM J2135-0102, using new observations with Herschel, SCUBA-2 and the VLA, is presented.
Journal ArticleDOI
The Bolocam Galactic Plane Survey: Survey Description and Data Reduction
James E. Aguirre,Adam Ginsburg,Miranda K. Dunham,Meredith M. Drosback,John Bally,Cara Battersby,Eric Todd Bradley,Claudia Cyganowski,Darren Dowell,Neal J. Evans,Jason Glenn,Paul Harvey,Paul Harvey,Erik Rosolowsky,Guy S. Stringfellow,Josh Walawender,Jonathan Williams +16 more
TL;DR: The Bolocam Galactic Plane Survey (BGPS) as mentioned in this paper is a 1.1 mm continuum survey at 33" effective resolution of 170 square degrees of the Galactic Plane visible from the northern hemisphere.
Journal ArticleDOI
Comparing Star Formation on Large Scales in the c2d Legacy Clouds: Bolocam 1.1 mm Dust Continuum Surveys of Serpens, Perseus, and Ophiuchus
Melissa L. Enoch,Jason Glenn,Neal J. Evans,Anneila I. Sargent,Kaisa E. Young,Kaisa E. Young,Tracy L. Huard +6 more
TL;DR: In this paper, a 1.1 mm continuum survey of three nearby star-forming clouds using Bolocam at the Caltech Submillimeter Observatory was conducted, detecting 122, 44, and 35 cores, respectively.
Journal ArticleDOI
HerMES: deep number counts at 250, 350, and 500 microns in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background
M. Bethermin,E. Le Floc'h,O. Ilbert,Alex Conley,G. Lagache,A. Amblard,V. Arumugam,H. Aussel,S. Berta,J. J. Bock,A. Boselli,V. Buat,Caitlin M. Casey,N. Castro-Rodriguez,Antonio Cava,D. L. Clements,Asantha Cooray,C. D. Dowell,Steve Eales,Duncan Farrah,Alberto Franceschini,Jason Glenn,Matthew Joseph Griffin,Evanthia Hatziminaoglou,Sebastien Heinis,E. Ibar,Rob Ivison,J. Kartaltepe,Louis Levenson,Georgios E. Magdis,Lucia Marchetti,G. Marsden,H. T. Nguyen,B. O'Halloran,S. J. Oliver,A. Omont,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,I. Perez-Fournon,M. Pohlen,D. Rigopoulou,Isaac Roseboom,Michael Rowan-Robinson,Mara Salvato,Benjamin L. Schulz,Douglas Scott,Nick Seymour,David L. Shupe,Andrew Smith,M. Symeonidis,M. Trichas,K. E. Tugwell,Mattia Vaccari,I. Valtchanov,Joaquin Vieira,Marco Viero,Lingyu Wang,C. K. Xu,Michael Zemcov +60 more
TL;DR: In this article, the authors extracted the bright SPIRE with a method using the positions, the flux densities, and the redshifts of the 24um sources as a prior, and derived the number counts and redshift distributions of the SPIRE sources.