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.
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Journal ArticleDOI
HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-Forming Galaxies
Marco P. Viero,Lingyu Wang,Michael Zemcov,Graeme E. Addison,Alexandre Amblard,V. Arumugam,H. Aussel,Matthieu Béthermin,J. J. Bock,A. Boselli,V. Buat,Denis Burgarella,Caitlin M. Casey,D. L. Clements,Alex Conley,Luca Conversi,Asantha Cooray,G. de Zotti,C. D. Dowell,Duncan Farrah,Alberto Franceschini,Jason Glenn,Matthew Joseph Griffin,Evanthia Hatziminaoglou,Sebastien Heinis,E. Ibar,R. J. Ivision,G. Lagache,Louis Levenson,Lucia Marchetti,G. Marsden,H. T. Nguyen,B. O'Halloran,S. J. Oliver,A. Omont,M. J. Page,Andreas Papageorgiou,C. P. Peason,I. Perez-Fournon,Michael Pohlen,D. Rigopoulou,Isaac Roseboom,Michael Rowan-Robinson,Douglas Scott,Nick Seymour,Benjamin L. Schulz,D. L. Shupe,Andrew Smith,M. Symeonidis,Mattia Vaccari,I. Valtchanov,Joaquin Vieira,Julie Wardlow,C. K. Xu +53 more
TL;DR: In this article, the authors measured the auto-and cross-frequency power spectra of the cosmic infrared background (CIB) at 250, 350, and 500um (1200, 860, and 600 GHz) from observations totaling ~ 70 deg 2 made with the SPIRE instrument aboard the Herschel Space Observatory.
Journal ArticleDOI
HerMES: THE CONTRIBUTION TO THE COSMIC INFRARED BACKGROUND FROM GALAXIES SELECTED BY MASS AND REDSHIFT*
Marco P. Viero,Lorenzo Moncelsi,Ryan Quadri,V. Arumugam,Roberto J. Assef,Roberto J. Assef,Matthieu Béthermin,Matthieu Béthermin,J. J. Bock,J. J. Bock,Carrie Bridge,Caitlin M. Casey,A. Conley,Asantha Cooray,Asantha Cooray,Duncan Farrah,Jason Glenn,Sebastien Heinis,Edo Ibar,Edo Ibar,Soh Ikarashi,Rob Ivison,Rob Ivison,Kotaro Kohno,G. Marsden,S. J. Oliver,Isaac Roseboom,Benjamin L. Schulz,Douglas Scott,Paolo Serra,Mattia Vaccari,Joaquin Vieira,Lingyu Wang,Julie Wardlow,Grant W. Wilson,M. S. Yun,Michael Zemcov,Michael Zemcov +37 more
TL;DR: In this paper, the authors quantify the fraction of the cosmic infrared background (CIB) that originates from galaxies identified in the UV/optical/near-infrared by stacking 81,250 (~35.7 arcmin^(2)) K-selected sources (K_(AB) 350 μm).
Journal ArticleDOI
Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10 11 solar masses
Alexandre Amblard,Asantha Cooray,Asantha Cooray,Paolo Serra,Bruno Altieri,V. Arumugam,Herve Aussel,Andrew Blain,J. J. Bock,J. J. Bock,Alessandro Boselli,V. Buat,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,Antonio Cava,Pierre Chanial,E. L. Chapin,David L. Clements,A. Conley,L. Conversi,C. D. Dowell,C. D. Dowell,Eli Dwek,Stephen Anthony Eales,D. Elbaz,Duncan Farrah,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,Matthew Joseph Griffin,Mark Halpern,Evanthia Hatziminaoglou,Edo Ibar,Kate Gudrun Isaak,Rob Ivison,Rob Ivison,Ali Ahmad Khostovan,Guilaine Lagache,Louis Levenson,Louis Levenson,Nanyao Y. Lu,Suzanne C. Madden,Bruno Maffei,G. Mainetti,Lucia Marchetti,G. Marsden,K. Mitchell-Wynne,H. T. Nguyen,H. T. Nguyen,B. O'Halloran,S. J. Oliver,Alain Omont,M. J. Page,P. Panuzzo,Andreas Papageorgiou,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Naseem Rangwala,Isaac Roseboom,Michael Rowan-Robinson,M. Sanchez Portal,Benjamin L. Schulz,Douglas Scott,N. Seymour,D. L. Shupe,Anthony J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Elisabetta Valiante,Ivan Valtchanov,Joaquin Vieira,L. Vigroux,Lian-Tao Wang,Robyn L. Ward,Gillian S. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +84 more
TL;DR: Excess clustering over the linear prediction at arcminute angular scales in the power spectrum of brightness fluctuations at 250, 350 and 500 μm is reported, and it is found that submillimetre galaxies are located in dark matter haloes with a minimum mass, Mmin, which corresponds to the most efficient mass scale for star formation in the Universe.
Journal ArticleDOI
The Bolocam Galactic Plane Survey: λ = 1.1 and 0.35 mm dust continuum emission in the Galactic center region
John Bally,James E. Aguirre,Cara Battersby,Eric Todd Bradley,Claudia Cyganowski,Darren Dowell,Meredith Drosback,Miranda K. Dunham,Neal J. Evans,Adam Ginsburg,Jason Glenn,Paul Harvey,Elisabeth A. C. Mills,Manuel Merello,Erik Rosolowsky,Wayne M. Schlingman,Yancy L. Shirley,Guy S. Stringfellow,Josh Walawender,Jonathan Williams +19 more
Abstract: The Bolocam Galactic Plane Survey (BGPS) data for a 6 deg2 region of the Galactic plane containing the Galactic center are analyzed and compared to infrared and radio continuum data. The BGPS 1.1 mm emission consists of clumps interconnected by a network of fainter filaments surrounding cavities, a few of which are filled with diffuse near-IR emission indicating the presence of warm dust or with radio continuum characteristic of H II regions or supernova remnants. New 350 μm images of the environments of the two brightest regions, Sgr A and B, are presented. Sgr B2 is the brightest millimeter-emitting clump in the Central Molecular Zone (CMZ) and may be forming the closest analog to a super star cluster in the Galaxy. The CMZ contains the highest concentration of millimeter- and submillimeter-emitting dense clumps in the Galaxy. Most 1.1 mm features at positive longitudes are seen in silhouette against the 3.6-24 μm background observed by the Spitzer Space Telescope. However, only a few clumps at negative longitudes are seen in absorption, confirming the hypothesis that positive longitude clumps in the CMZ tend to be on the near side of the Galactic center, consistent with the suspected orientation of the central bar in our Galaxy. Some 1.1 mm cloud surfaces are seen in emission at 8 μm, presumably due to polycyclic aromatic hydrocarbons. A ~02 (~30 pc) diameter cavity and infrared bubble between l 00 and 02 surround the Arches and Quintuplet clusters and Sgr A. The bubble contains several clumpy dust filaments that point toward Sgr A*; its potential role in their formation is explored. Bania's Clump 2, a feature near l = 3°-35 which exhibits extremely broad molecular emission lines (ΔV> 150 km s–1), contains dozens of 1.1 mm clumps. These clumps are deficient in near- and mid-infrared emission in the Spitzer images when compared to both the inner Galactic plane and the CMZ. Thus, Bania's Clump 2 is either inefficient in forming stars or is in a pre-stellar phase of clump evolution. The Bolocat catalog of 1.1 mm clumps contains 1428 entries in the Galactic center between l = 3585 and l = 45 of which about 80% are likely to be within about 500 pc of the center. The mass spectrum above about 80 M ☉ can be described by a power-law ΔN/ΔM = N 0 M –2.14(+0.1,–0.4). The power-law index is somewhat sensitive to systematic grain temperature variations, may be highly biased by source confusion, and is very sensitive to the spatial filtering inherent in the data acquisition and reduction.
Journal ArticleDOI
HerMES: Candidate High-redshift Galaxies Discovered with Herschel/SPIRE
C. Darren Dowell,C. Darren Dowell,A. Conley,Jason Glenn,V. Arumugam,V. Asboth,Herve Aussel,Frank Bertoldi,Matthieu Béthermin,James J. Bock,James J. Bock,Alessandro Boselli,Carrie Bridge,V. Buat,Denis Burgarella,Antonio Cabrera-Lavers,Antonio Cabrera-Lavers,Caitlin M. Casey,Scott Chapman,Scott Chapman,David L. Clements,L. Conversi,A. Cooray,A. Cooray,Helmut Dannerbauer,F. De Bernardis,Timothy P. Ellsworth-Bowers,Duncan Farrah,Alberto Franceschini,M. Griffin,Mark Gurwell,Mark Halpern,Evanthia Hatziminaoglou,Sebastien Heinis,Edo Ibar,Edo Ibar,Rob Ivison,Rob Ivison,Nicolas Laporte,Nicolas Laporte,Lucia Marchetti,Lucia Marchetti,P. Martinez-Navajas,P. Martinez-Navajas,G. Marsden,Glenn Morrison,Hien Nguyen,Hien Nguyen,B. O'Halloran,S. J. Oliver,Alain Omont,Mat Page,Andreas Papageorgiou,C. P. Pearson,C. P. Pearson,Glen Petitpas,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Dominik A. Riechers,Dominik A. Riechers,Dimitra Rigopoulou,Dimitra Rigopoulou,Isaac Roseboom,Isaac Roseboom,M. Rowan-Robinson,Jack Sayers,Bernhard Schulz,Douglas Scott,Nick Seymour,David L. Shupe,Anthony J. Smith,Alina Streblyanska,Alina Streblyanska,M. Symeonidis,Mattia Vaccari,Mattia Vaccari,Ivan Valtchanov,Joaquin Vieira,Marco P. Viero,Lian-Tao Wang,Julie Wardlow,C. K. Xu,Michael Zemcov +83 more
TL;DR: In this article, a method for selecting z > 4 dusty, star-forming galaxies (DSFGs) using Herschel/Spectral and Photometric Imaging Receiver 250/350/500 μm flux densities to search for red sources was presented.