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
Full-Array Noise Performance of Deployment-Grade SuperSpec mm-wave On-Chip Spectrometers
Kirit Karkare,Peter S. Barry,Peter S. Barry,Charles M. Bradford,Charles M. Bradford,Scott Chapman,Simon Doyle,Jason Glenn,S. Gordon,S. Hailey-Dunsheath,Reinier M. J. Janssen,Reinier M. J. Janssen,Attila Kovács,Henry G. LeDuc,P. Mauskopf,Ryan McGeehan,J. Redford,Erik Shirokoff,Carole Tucker,Jordan Wheeler,Jonas Zmuidzinas +20 more
TL;DR: SuperSpec as mentioned in this paper is an on-chip filter-bank spectrometer designed for wideband moderate-resolution spectroscopy at millimeter wavelengths, employing TiN kinetic inductance detectors.
Journal ArticleDOI
Full-array noise performance of deployment-grade SuperSpec mm-wave on-chip spectrometers
Kirit Karkare,Peter S. Barry,Peter S. Barry,Charles M. Bradford,Charles M. Bradford,Scott Chapman,Simon Doyle,Jason Glenn,S. Gordon,S. Hailey-Dunsheath,Reinier M. J. Janssen,Reinier M. J. Janssen,Attila Kovács,Henry G. LeDuc,P. Mauskopf,Ryan McGeehan,J. Redford,Erik Shirokoff,Carole Tucker,Jordan Wheeler,Jonas Zmuidzinas +20 more
TL;DR: SuperSpec as discussed by the authors is an on-chip filter bank spectrometer designed for wideband moderate-resolution spectroscopy at millimeter wavelengths, employing TiN kinetic inductance detectors.
Journal ArticleDOI
The central region of spiral galaxies as seen by Herschel. M81, M99 and M100
Marc Sauvage,N. Sacchi,George J. Bendo,A. Boselli,Michael Pohlen,Christine D. Wilson,Robbie Richard Auld,Maarten Baes,M. J. Barlow,J. J. Bock,M. Bradford,V. Buat,N. Castro-Rodriguez,P. Chanial,Stéphane Charlot,Laure Ciesla,David L. Clements,Asantha Cooray,Diane Cormier,Luca Cortese,Jonathan Ivor Davies,E. Dwek,Steve Eales,D. Elbaz,Maud Galametz,Frédéric Galliano,Walter Kieran Gear,Jason Glenn,Haley Louise Gomez,Matthew Joseph Griffin,Sacha Hony,K. G. Isaak,Louis Levenson,Nanyao Y. Lu,S. C. Madden,B. O'Halloran,K. Okumura,S. J. Oliver,M. J. Page,P. Panuzzo,Andreas Papageorgiou,T. J. Parkin,I. Perez-Fournon,N. Rangwala,E. E. Rigby,H. Roussel,A. Rykala,Benjamin L. Schulz,Maximilien R. P. Schirm,Matthew Smith,Luigi Spinoglio,Jamie Stevens,Sundar Srinivasan,M. Symeonidis,M. Trichas,Mattia Vaccari,L. Vigroux,Herve Wozniak,Gillian S. Wright,Werner W. Zeilinger +59 more
TL;DR: In this article, the authors revisited the two-component approach at longer wavelengths, to see if it still provides a working description of the brightness distribution of galaxies, and to determine its implications on the interpretation of global far-infrared properties of galaxies.
Journal ArticleDOI
Follow-up observations of the remarkable double-degenerate binary lb 11146
TL;DR: In this article, a double-degenerate binary system consisting of two white dwarfs of very similar mass and surface temperature, but widely different magnetic field strengths, was studied with a time resolution as high as 11.5 minutes and total baseline of 16 days.
Proceedings ArticleDOI
SWCam: the short wavelength camera for the CCAT Observatory
Gordon J. Stacey,Stephen C. Parshley,Thomas Nikola,German Cortes-Medellin,Justin Schoenwald,Ganesh Rajagopalan,Michael D. Niemack,Tim Jenness,Patricio A. Gallardo,Brian J. Koopman,Charles D. Dowell,Peter K. Day,Matthew I. Hollister,Attila Kovács,Attila Kovács,Henry G. LeDuc,Christopher McKenney,Ryan M. Monroe,Hiroshige Yoshida,Jonas Zmuidzinas,Loren J. Swenson,Simon J. E. Radford,Hien Nguyen,Anthony K. Mroczkowski,Jason Glenn,Jordan Wheeler,Philip R. Maloney,Spencer Brugger,Joseph D. Adams,Frank Bertoldi,Reinhold Schaaf,Mark Halpern,Douglas Scott,G. Marsden,Jack Sayers,Scott Chapman,Joaquin Vieira +36 more
TL;DR: The Short Wavelength Camera (SWCam) as mentioned in this paper was designed for the CCAT observatory to resolve the Cosmic Far-IR Background (CIRB) in our four colors so that we may explore the star and galaxy formation history of the Universe extending to within 500 million years of the Big Bang.