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
The Herschel-SPIRE instrument and its in-flight performance
Matthew Joseph Griffin,Alain Abergel,A. Abreu,Peter A. R. Ade,Philippe André,J.-L. Augueres,Tom Babbedge,Y. Bae,T. Baillie,Jean-Paul Baluteau,M. J. Barlow,George J. Bendo,Dominique Benielli,James J. Bock,P. Bonhomme,Drew Brisbin,C. Brockley-Blatt,Martin E. Caldwell,C. Cara,N. Castro-Rodriguez,R. Cerulli,Pierre Chanial,Pierre Chanial,Sina Chen,Eric M. Clark,David L. Clements,L. Clerc,J. Coker,D. Communal,Luca Conversi,Peter Timothy Cox,D. Crumb,C. R. Cunningham,F. Daly,Gary R. Davis,P. De Antoni,J. Delderfield,N. Devin,A. M. di Giorgio,Iris Didschuns,Kjetil Dohlen,M. Donati,A. Dowell,C. D. Dowell,L. Duband,Luc Dumaye,R. J. Emery,Marc Ferlet,D. Ferrand,Jean Fontignie,M. Fox,Alberto Franceschini,Margaret A. Frerking,Trevor Fulton,J. Garcia,R. Gastaud,Walter Kieran Gear,Jason Glenn,A-S Goizel,Douglas Griffin,T. Grundy,S. Guest,L. Guillemet,Peter Charles Hargrave,Martin Harwit,P. Hastings,Evanthia Hatziminaoglou,Evanthia Hatziminaoglou,M. Herman,B. Hinde,Viktor Hristov,Maohai Huang,P. Imhof,Kate Gudrun Isaak,Kate Gudrun Isaak,Ulf E. Israelsson,Rob Ivison,D. E. Jennings,Brian John Kiernan,K. J. King,Andrew E. Lange,William B. Latter,Glenn Laurent,Philippe Laurent,S. J. Leeks,Emmanuel Lellouch,Louis Levenson,Bo Li,Jin-Zeng Li,J. Lilienthal,T. L. Lim,S. J. Liu,N. Lu,Suzanne C. Madden,G. Mainetti,P. Marliani,D. J. McKay,K. Mercier,Sergio Molinari,Huw R. Morris,H. Moseley,Jerry Mulder,M. Mur,David A. Naylor,Hien Nguyen,B. O'Halloran,Seb Oliver,G. Olofsson,Hans Olofsson,R. Orfei,Mat Page,I. Pain,P. Panuzzo,Andreas Papageorgiou,G. Parks,P. Parr-Burman,Alan Pearce,C. P. Pearson,C. P. Pearson,Ismael Perez-Fournon,F. Pinsard,Giampaolo Pisano,Giampaolo Pisano,J. Podosek,Michael Pohlen,Edward Polehampton,Edward Polehampton,D. Pouliquen,D. Rigopoulou,D. Rizzo,Isaac Roseboom,Helene Roussel,Michael Rowan-Robinson,B. K. Rownd,P. Saraceno,Marc Sauvage,Richard S. Savage,Giorgio Savini,Giorgio Savini,Eric Sawyer,Carsten Scharmberg,D. Schmitt,D. Schmitt,Nicola Schneider,Benjamin L. Schulz,Arnold A. Schwartz,Rick Shafer,David L. Shupe,B. Sibthorpe,Sunil Sidher,Alan Smith,Anthony J. Smith,David J. Smith,Locke D. Spencer,Locke D. Spencer,Brian Stobie,Rashmikant V. Sudiwala,K. Sukhatme,Christian Surace,Jamie Stevens,B. M. Swinyard,Markos Trichas,T. Tourette,H. Triou,S. Tseng,Carole Tucker,A. D. Turner,Mattia Vaccari,Ivan Valtchanov,L. Vigroux,L. Vigroux,E. Virique,George M. Voellmer,H. J. Walker,Robyn L. Ward,Timothy James Waskett,M. Weilert,Roger Wesson,Glenn J. White,Glenn J. White,Nicola Jane Whitehouse,Christine D. Wilson,Berend Winter,Adam Woodcraft,Gillian S. Wright,C. K. Xu,Annie Zavagno,Michael Zemcov,L. Zhang,E. Zonca +189 more
TL;DR: The Spectral and Photometric Imaging REceiver (SPIRE) is the Herschel Space Observatory's sub-millimetre camera and spectrometer as discussed by the authors, which is used for image and spectroscopic data acquisition.
Journal ArticleDOI
The Herschel-SPIRE instrument and its in-flight performance
Matthew Joseph Griffin,A. Abergel,A. Abreu,Peter A. R. Ade,Pascale Andre,J.-L. Augueres,Tom Babbedge,Y. Bae,T. Baillie,Jean-Paul Baluteau,M. J. Barlow,George J. Bendo,D. Benielli,James J. Bock,P. Bonhomme,D. Brisbin,C. Brockley-Blatt,Martin E. Caldwell,Christophe Cara,N. Castro-Rodriguez,R. Cerulli,P. Chanial,Sina Chen,Eric M. Clark,David L. Clements,L. Clerc,J. Coker,D. Communal,Luca Conversi,Peter Timothy Cox,D. Crumb,Colin Cunningham,F. Daly,Gary R. Davis,P. De Antoni,J. Delderfield,N. Devin,A. M. di Giorgio,Iris Didschuns,Kjetil Dohlen,M. Donati,A. Dowell,C. D. Dowell,L. Duband,Luc Dumaye,R. J. Emery,Marc Ferlet,D. Ferrand,Jean Fontignie,M. Fox,Alberto Franceschini,Margaret A. Frerking,Trevor Fulton,J. Garcia,R. Gastaud,Walter Kieran Gear,Jason Glenn,A-S Goizel,Douglas Griffin,T. Grundy,S. Guest,L. Guillemet,Peter Charles Hargrave,Martin Harwit,P. Hastings,Evanthia Hatziminaoglou,M. Herman,B. Hinde,V. V. Hristov,Maohai Huang,P. Imhof,K. J. Isaak,Ulf E. Israelsson,Rob Ivison,D. E. Jennings,Brian John Kiernan,K. J. King,Andrew E. Lange,William B. Latter,Glenn Laurent,Philippe Laurent,Sarah Leeks,E. Lellouch,Louis Levenson,Bo Li,Jin-Zeng Li,J. Lilienthal,T. L. Lim,J. Liu,N. Lu,S. C. Madden,G. Mainetti,P. Marliani,D. J. McKay,K. Mercier,Sergio Molinari,Huw R. Morris,H. Moseley,Jerry Mulder,M. Mur +99 more
TL;DR: The Spectral and Photometric Imaging Receiver (SPIRE) as discussed by the authors is the Herschel Space Observatory's submillimetre camera and spectrometer, which is used for scan-mapping, whereby the field of view is scanned across the sky to achieve full spatial sampling and to cover large areas.
Journal ArticleDOI
The Herschel Multi-tiered Extragalactic Survey: HerMES
Seb Oliver,James J. Bock,James J. Bock,Bruno Altieri,Alexandre Amblard,V. Arumugam,Herve Aussel,Tom Babbedge,Alexandre Beelen,Matthieu Béthermin,Matthieu Béthermin,Andrew Blain,Alessandro Boselli,C. Bridge,Drew Brisbin,V. Buat,Denis Burgarella,N. Castro-Rodríguez,N. Castro-Rodríguez,Antonio Cava,P. Chanial,Michele Cirasuolo,David L. Clements,A. Conley,L. Conversi,Asantha Cooray,Asantha Cooray,C. D. Dowell,C. D. Dowell,Elizabeth Dubois,Eli Dwek,Simon Dye,Stephen Anthony Eales,David Elbaz,Duncan Farrah,A. Feltre,P. Ferrero,P. Ferrero,N. Fiolet,N. Fiolet,M. Fox,Alberto Franceschini,Walter Kieran Gear,E. Giovannoli,Jason Glenn,Yan Gong,E. A. González Solares,Matthew Joseph Griffin,Mark Halpern,Martin Harwit,Evanthia Hatziminaoglou,Sebastien Heinis,Peter Hurley,Ho Seong Hwang,A. Hyde,Edo Ibar,O. Ilbert,K. G. Isaak,Rob Ivison,Rob Ivison,Guilaine Lagache,E. Le Floc'h,L. R. Levenson,L. R. Levenson,B. Lo Faro,Nanyao Y. Lu,S. C. Madden,Bruno Maffei,Georgios E. Magdis,G. Mainetti,Lucia Marchetti,G. Marsden,J. Marshall,J. Marshall,A. M. J. Mortier,Hien Nguyen,Hien Nguyen,B. O'Halloran,Alain Omont,Mat Page,P. Panuzzo,Andreas Papageorgiou,H. Patel,Chris Pearson,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Michael Pohlen,Jonathan Rawlings,Gwenifer Raymond,Dimitra Rigopoulou,Dimitra Rigopoulou,L. Riguccini,D. Rizzo,Giulia Rodighiero,Isaac Roseboom,Isaac Roseboom,Michael Rowan-Robinson,M. Sanchez Portal,Benjamin L. Schulz,Douglas Scott,Nick Seymour,Nick Seymour,D. L. Shupe,A. J. Smith,Jamie Stevens,M. Symeonidis,Markos Trichas,K. E. Tugwell,Mattia Vaccari,Ivan Valtchanov,Joaquin Vieira,Marco P. Viero,L. Vigroux,Lifan Wang,Robyn L. Ward,Julie Wardlow,G. Wright,C. K. Xu,Michael Zemcov,Michael Zemcov +120 more
TL;DR: The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy program designed to map a set of nested fields totalling ∼380deg^2 as mentioned in this paper.
Journal ArticleDOI
Clouds, filaments, and protostars: The Herschel Hi-GAL Milky Way
Sergio Molinari,B. Swinyard,John Bally,M. J. Barlow,J.-P. Bernard,Paul Martin,Toby J. T. Moore,Alberto Noriega-Crespo,Rene Plume,Leonardo Testi,Leonardo Testi,Annie Zavagno,Alain Abergel,Babar Ali,L. D. Anderson,Ph. André,J.-P. Baluteau,Cara Battersby,M. T. Beltrán,M. Benedettini,N. Billot,J. A. D. L. Blommaert,Sylvain Bontemps,Sylvain Bontemps,F. Boulanger,Jan Brand,Christopher M. Brunt,Michael G. Burton,Luca Calzoletti,Sean Carey,Paola Caselli,Riccardo Cesaroni,José Cernicharo,Sukanya Chakrabarti,Antonio Chrysostomou,Martin Cohen,Mathieu Compiegne,P. de Bernardis,G. de Gasperis,A. M. di Giorgio,Davide Elia,F. Faustini,Nicolas Flagey,Yasuo Fukui,Gary A. Fuller,K. Ganga,Pedro García-Lario,Jason Glenn,Paul F. Goldsmith,Matthew Joseph Griffin,Melvin Hoare,Maohai Huang,D. Ikhenaode,C. Joblin,G. Joncas,Mika Juvela,Jason M. Kirk,Guilaine Lagache,Jin-Zeng Li,T. L. Lim,S. D. Lord,Massimo Marengo,Douglas J. Marshall,Silvia Masi,Fabrizio Massi,Mikako Matsuura,Vincent Minier,Marc-Antoine Miville-Deschenes,L. Montier,L. K. Morgan,Frédérique Motte,Joseph C. Mottram,T. G. Müller,Paolo Natoli,J. Neves,Luca Olmi,Roberta Paladini,Deborah Paradis,Harriet Parsons,Nicolas Peretto,Nicolas Peretto,M. R. Pestalozzi,Stefano Pezzuto,F. Piacentini,Lorenzo Piazzo,D. Polychroni,M. Pomarès,Cristina Popescu,William T. Reach,Isabelle Ristorcelli,Jean-François Robitaille,Thomas P. Robitaille,J. A. Rodón,A. Roy,Pierre Royer,D. Russeil,Paolo Saraceno,Marc Sauvage,Peter Schilke,Eugenio Schisano,Nicola Schneider,Frederic Schuller,Benjamin L. Schulz,B. Sibthorpe,Hazel Smith,Michael D. Smith,L. Spinoglio,Dimitrios Stamatellos,Francesco Strafella,Guy S. Stringfellow,E. Sturm,R. Taylor,Mark Thompson,Alessio Traficante,Richard J. Tuffs,Grazia Umana,Luca Valenziano,R. Vavrek,M. Veneziani,Serena Viti,C. Waelkens,Derek Ward-Thompson,Glenn J. White,L. A. Wilcock,Friedrich Wyrowski,Harold W. Yorke,Qizhou Zhang +126 more
TL;DR: In this paper, the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key program that will map the inner Galactic plane of the Milky Way in 5 bands, were presented.
Journal ArticleDOI
Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way
Sergio Molinari,B. Swinyard,John Bally,M. J. Barlow,J.-P. Bernard,Paul Martin,Toby J. T. Moore,Alberto Noriega-Crespo,Rene Plume,Leonardo Testi,Annie Zavagno,A. Abergel,Babar Ali,L. D. Anderson,Pascal André,Jean-Paul Baluteau,Cara Battersby,M. T. Beltrán,M. Benedettini,N. Billot,J. A. D. L. Blommaert,Sylvain Bontemps,F. Boulanger,Jan Brand,Christopher M. Brunt,Michael G. Burton,Luca Calzoletti,Sean Carey,Paola Caselli,Riccardo Cesaroni,José Cernicharo,Sukanya Chakrabarti,Antonio Chrysostomou,Martin Cohen,Mathieu Compiegne,P. de Bernardis,G. de Gasperis,A. M. di Giorgio,Davide Elia,F. Faustini,Nicolas Flagey,Yasuo Fukui,Gary A. Fuller,K. Ganga,Pedro García-Lario,Jason Glenn,Paul F. Goldsmith,Matthew Joseph Griffin,Melvin Hoare,Maohai Huang,D. Ikhenaode,C. Joblin,G. Joncas,Mika Juvela,Jason M. Kirk,Guilaine Lagache,Jin-Zeng Li,T. L. Lim,S. D. Lord,Massimo Marengo,D. J. Marshall,Silvia Masi,Fabrizio Massi,Mikako Matsuura,Vincent Minier,Marc-Antoine Miville-Deschenes,L. Montier,L. K. Morgan,Frédérique Motte,Joseph C. Mottram,T. Mueller,Paolo Natoli,J. Neves,Luca Olmi,R. Paladini,D. Paradis,Harriet Parsons,Nicolas Peretto,M. R. Pestalozzi,Stefano Pezzuto,F. Piacentini,Lorenzo Piazzo,D. Polychroni,M. Pomarès,Cristina Popescu,William T. Reach,Isabelle Ristorcelli,Jean-François Robitaille,Thomas P. Robitaille,J. A. Rodón,A. Roy,Pierre Royer,D. Russeil,P. Saraceno,Marc Sauvage,Peter Schilke,Eugenio Schisano,Nicola Schneider,Frederic Schuller,Benjamin L. Schulz,B. Sibthorpe,Howard A. Smith,Michael D. Smith,L. Spinoglio,Dimitrios Stamatellos,Francesco Strafella,Guy S. Stringfellow,E. Sturm,Russell H. Taylor,Maggie A. Thompson,Alessio Traficante,Richard J. Tuffs,Grazia Umana,Luca Valenziano,R. Vavrek,M. Veneziani,Serena Viti,C. Waelkens,Derek Ward-Thompson,Glenn J. White,L. A. Wilcock,Friedrich Wyrowski,H. W. Yorke,Qizhou Zhang +123 more
TL;DR: In this paper, the first results from the science demonstration phase for the Hi-GAL survey, the Herschel key-project that will map the inner Galactic Plane of the Milky Way in 5 bands are presented.