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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Proceedings ArticleDOI
Current status of Bolocam: a large-format millimeter-wave bolometer camera
Jason Glenn,Peter A. R. Ade,Mihail Amarie,James J. Bock,S. F. Edgington,A. Goldin,Sunil Golwala,D. Haig,Andrew E. Lange,Glenn Laurent,Philip Daniel Mauskopf,Minhee Yun,Hien Nguyen +12 more
TL;DR: Bolocam as discussed by the authors, a 144-element, bolometric, millimeter-wave camera, is currently in its commissioning stage at the Caltech Submillimeter Observatory, where it is being used for a series of experiments.
Journal ArticleDOI
Herschel-spire fourier transform spectrometer observations of excited co and [c i] in the antennae (ngc 4038/39): warm and cold molecular gas*
Maximilien R. P. Schirm,Christine D. Wilson,T. J. Parkin,Julia Kamenetzky,Jason Glenn,Naseem Rangwala,Luigi Spinoglio,M. Pereira-Santaella,Maarten Baes,M. J. Barlow,David L. Clements,Asantha Cooray,Ilse De Looze,O. Ł. Karczewski,Suzanne C. Madden,Aurélie Rémy-Ruyer,Ronin Wu +16 more
TL;DR: In this article, the SPIRE-FTS was used to detect five CO transitions (J = 4-3 to J = 8-7), both [C I] transitions, and the [N II] 205 μm transition across the entire system, which was supplemented with ground-based observations of the CO J = 1-0, J = 2-1, and J = 3-2 transitions and [C II] and [O I] 63 μm.
Journal ArticleDOI
Herschel SPIRE-FTS Observations of Excited CO and [CI] in the Antennae (NGC 4038/39): Warm and Cold Molecular Gas
Maximilien R. P. Schirm,Christine D. Wilson,T. J. Parkin,Julia Kamenetzky,Jason Glenn,Naseem Rangwala,Luigi Spinoglio,Miguel Pereira-Santaella,Maarten Baes,M. J. Barlow,David L. Clements,Asantha Cooray,Ilse De Looze,O. Ł. Karczewski,Suzanne C. Madden,Aurélie Rémy-Ruyer,Ronin Wu +16 more
TL;DR: In this paper, the authors used the Herschel SPIRE-FTS observations of the Antennae (NGC 4038/39) to detect CO and [CI] transitions and the [NII]$205\mu m$ transition across the entire system.
Journal ArticleDOI
Herschel photometric observations of the low metallicity dwarf galaxy NGC 1705
B. O'Halloran,Maud Galametz,Suzanne C. Madden,Robbie Richard Auld,Maarten Baes,M. J. Barlow,George J. Bendo,J. J. Bock,Alessandro Boselli,M. Bradford,V. Buat,N. Castro-Rodriguez,Pierre Chanial,Stéphane Charlot,Laure Ciesla,David L. Clements,Diane Cormier,Asantha Cooray,Luca Cortese,Jonathan Ivor Davies,Eli Dwek,Stephen Anthony Eales,D. Elbaz,Frédéric Galliano,Walter Kieran Gear,Jason Glenn,Haley Louise Gomez,Sacha Hony,Kate Gudrun Isaak,Louis Levenson,Nanyao Y. Lu,K. Okumura,Seb Oliver,Mat Page,P. Panuzzo,Andreas Papageorgiou,T. J. Parkin,Ismael Perez-Fournon,Michael Pohlen,Naseem Rangwala,E. E. Rigby,Helene Roussel,A. Rykala,N. Sacchi,Marc Sauvage,Benjamin L. Schulz,Maximilien R. P. Schirm,Matthew Smith,L. Spinoglio,Sundar Srinivasan,Jamie Stevens,M. Symeonidis,Markos Trichas,Mattia Vaccari,L. Vigroux,Christine D. Wilson,Herve Wozniak,Gillian S. Wright,Werner W. Zeilinger +58 more
TL;DR: In this article, the presence of two dominant circumnuclear IR-bright regions surrounding the central super star cluster in NGC 1705 was confirmed using SPIRE and PACS photometry.
Proceedings ArticleDOI
MUSIC for sub/millimeter astrophysics
Philip R. Maloney,Nicole G. Czakon,Peter K. Day,T. P. Downes,Ran Duan,Jiansong Gao,Jason Glenn,Sunil Golwala,Matt I. Hollister,Henry G. LeDuc,Benjamin A. Mazin,Sean McHugh,Omid Noroozian,Hien Nguyen,J. Sayers,James A. Schlaerth,Seth Siegel,John E. Vaillancourt,Anastasios Vayonakis,P. Wilson,Jonas Zmuidzinas +20 more
TL;DR: The Multiwavelength Submillimeter kinetic Inductance Camera (MUSIC) as discussed by the authors uses microwave kinetic inductance detectors (MKIDs) as photon detectors and has 576 spatial pixels in four bands at 850, 1100, 1300 and 2000 microns.