B
Bruce Bumble
Researcher at California Institute of Technology
Publications - 113
Citations - 3474
Bruce Bumble is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Detector & Heterodyne. The author has an hindex of 28, co-authored 102 publications receiving 3126 citations. Previous affiliations of Bruce Bumble include Jet Propulsion Laboratory.
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Journal ArticleDOI
The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI)
Th. de Graauw,Th. de Graauw,Frank Helmich,Thomas G. Phillips,J. Stutzki,Emmanuel Caux,Emmanuel Caux,N. Whyborn,Pieter Dieleman,Pieter R. Roelfsema,H. Aarts,R. Assendorp,Rafael Bachiller,W. Baechtold,A. Barcia,D. A. Beintema,Victor Belitsky,Arnold O. Benz,R. Bieber,Adwin Boogert,Colin Borys,Bruce Bumble,P. Cais,P. Cais,M. Caris,Pasquale Cerulli-Irelli,Goutam Chattopadhyay,Serguei Cherednichenko,M. Ciechanowicz,O. Coeur-Joly,O. Coeur-Joly,C. Comito,A. Cros,A. Cros,A. de Jonge,G. de Lange,B. Delforges,B. Delforges,Y. Delorme,T. den Boggende,J. Desbat,J. Desbat,C. Diez-Gonzalez,A. M. di Giorgio,L. Dubbeldam,K. Edwards,K. Edwards,Martin Eggens,Neal R. Erickson,Jaap Evers,Michel Fich,T. Finn,B. Franke,Todd Gaier,C. Gal,Jian-Rong Gao,Juan Daniel Gallego,S. Gauffre,S. Gauffre,John Gill,S. Glenz,H. Golstein,H. Goulooze,T. Gunsing,R. Güsten,Paul Hartogh,W. A. Hatch,R. Higgins,R. Higgins,E. C. Honingh,R. Huisman,Brian Jackson,H. Jacobs,Karl Jacobs,Christopher Jarchow,Hamid Javadi,Willem Jellema,M. Justen,Alexandre Karpov,C. Kasemann,J. Kawamura,Geert Keizer,Dominicus Kester,T. M. Klapwijk,Th. Klein,Erik L. Kollberg,Jacob Kooi,P.-P. Kooiman,B. Kopf,M. Krause,J. M. Krieg,C. Kramer,B. Kruizenga,T. Kuhn,W. M. Laauwen,R. Lai,Bengt Larsson,Henry G. LeDuc,Christian Leinz,R. H. Lin,René Liseau,René Liseau,G. S. Liu,Alexander Loose,I. Lopez-Fernandez,S. D. Lord,W. Luinge,A. Marston,Jesús Martín-Pintado,Alain Maestrini,Frank Maiwald,C. McCoey,Imran Mehdi,A. Megej,M. Melchior,L. Meinsma,Harald Franz Arno Merkel,M. Michalska,Christian Monstein,D. Moratschke,Patrick W. Morris,Holger S. P. Müller,J. A. Murphy,A. Naber,E. Natale,W. Nowosielski,Francesco Nuzzolo,Michael Olberg,Michael Olberg,M. Olbrich,R. Orfei,Piotr Orleanski,Volker Ossenkopf,T. Peacock,J. C. Pearson,I. Peron,S. Phillip-May,Lorenzo Piazzo,P. Planesas,M. Rataj,L. Ravera,L. Ravera,Christophe Risacher,M. Salez,Lorene Samoska,Paolo Saraceno,Rudolf Schieder,Erich Schlecht,F. Schlöder,F. Schmülling,M. Schultz,K. F. Schuster,O. Siebertz,H. Smit,Ryszard Szczerba,R. Shipman,E. Steinmetz,J. A. Stern,M. Stokroos,Rafael Teipen,David Teyssier,T. Tils,Neil Trappe,C. van Baaren,B. J. van Leeuwen,H. van de Stadt,Hubregt J. Visser,K. Wildeman,C. K. Wafelbakker,John Ward,P.R. Wesselius,Wolfgang Wild,S. Wulff,Hans-Joachim Wunsch,X. Tielens,X. Tielens,P. Zaal,Herbert Zirath,Jonas Zmuidzinas,F. Zwart +179 more
TL;DR: The Heterodyne Instrument for the Far-Infrared (HIFI) was launched onboard ESA's Herschel Space Observatory in May 2009 as mentioned in this paper, which is a set of 7 heterodyne receivers that are electronically tuneable, covering 480-1250 GHz with SIS mixers and the 1410-1910 GHz range with hot electron bolometer mixers.
Journal ArticleDOI
Titanium Nitride Films for Ultrasensitive Microresonator Detectors
Henry G. LeDuc,Bruce Bumble,Peter K. Day,Byeong Ho Eom,Jiansong Gao,Sunil Golwala,Benjamin A. Mazin,Sean McHugh,Andrew Merrill,David Moore,Omid Noroozian,Anthony D. Turner,Jonas Zmuidzinas +12 more
TL;DR: Titanium nitride (TiNx) films are ideal for use in superconducting microresonator detectors for the following reasons: (a) the critical temperature varies with composition (0 107) and have noise properties similar to resonators made using other materials, while the quasiparticle lifetimes are reasonably long, 10−200μs as discussed by the authors.
Journal ArticleDOI
Titanium Nitride Films for Ultrasensitive Microresonator Detectors
Henry G. LeDuc,Bruce Bumble,Peter K. Day,Anthony D. Turner,Byeong Ho Eom,Sunil Golwala,David Moore,Omid Noroozian,Jonas Zmuidzinas,Jiansong Gao,Benjamin A. Mazin,Sean McHugh,Andrew Merrill +12 more
TL;DR: Titanium nitride (TiNx) films are ideal for use in superconducting microresonator detectors because: a) the critical temperature varies with composition (0 10^7) and have noise properties similar to resonators made using other materials, while the quasiparticle lifetimes are reasonably long, 10-200 $\mu$s as mentioned in this paper.
Journal ArticleDOI
Herschel observations of EXtra-Ordinary Sources: the present and future of spectral surveys with Herschel/HIFI
E. A. Bergin,Thomas G. Phillips,C. Comito,Nathan R. Crockett,D. C. Lis,Peter Schilke,S. Wang,T. A. Bell,G. A. Blake,Bruce Bumble,Emmanuel Caux,S. Cabrit,Cecilia Ceccarelli,José Cernicharo,Fabien Daniel,Th. de Graauw,Marie-Lise Dubernet,Martin Emprechtinger,P. J. Encrenaz,E. Falgarone,Maryvonne Gerin,Thomas F. Giesen,J. R. Goicoechea,P. F. Goldsmith,H. Gupta,Paul Hartogh,Frank Helmich,Eric Herbst,C. Joblin,D. Johnstone,J. Kawamura,W. D. Langer,William B. Latter,S. D. Lord,Sébastien Maret,Pierrick Martin,Gary J. Melnick,Karl M. Menten,Patrick W. Morris,Holger S. P. Müller,J. A. Murphy,David A. Neufeld,Volker Ossenkopf,Laurent Pagani,J. C. Pearson,M. Perault,Rene Plume,Pieter R. Roelfsema,S.-L. Qin,M. Salez,Stephan Schlemmer,J. Stutzki,Aggm Tielens,Neil Trappe,F. F. S. van der Tak,Charlotte Vastel,H. W. Yorke,Shanshan Yu,Jonas Zmuidzinas +58 more
TL;DR: In this paper, the spectral properties of the Orion hot core were investigated using the Herschel GT key program and the HIFI spectra of Orion KL between 480 and 560 GHz and from 1.06 to 1.115 THz.
Journal ArticleDOI
Herschel observations of EXtra-Ordinary Sources (HEXOS): the present and future of spectral surveys with Herschel/HIFI.
Edwin A. Bergin,Thomas G. Phillips,Claudia Comito,Nathan R. Crockett,Dariusz C. Lis,Peter Schilke,Peter Schilke,S. Wang,Tom Bell,Geoffrey A. Blake,Bruce Bumble,Emmanuel Caux,Emmanuel Caux,Sylvie Cabrit,Cecilia Ceccarelli,José Cernicharo,F. Daniel,F. Daniel,Th. de Graauw,M.-L. Dubernet,Martin Emprechtinger,P. J. Encrenaz,Edith Falgarone,Maryvonne Gerin,Thomas F. Giesen,Javier R. Goicoechea,Paul F. Goldsmith,Harshal Gupta,Paul Hartogh,Frank Helmich,Eric Herbst,Christine Joblin,Christine Joblin,Doug Johnstone,J. Kawamura,W. D. Langer,William B. Latter,S. D. Lord,Sébastien Maret,Peter G. Martin,Gary J. Melnick,Karl M. Menten,Patrick W. Morris,Holger S. P. Müller,J. A. Murphy,David A. Neufeld,Volker Ossenkopf,Volker Ossenkopf,Laurent Pagani,J. C. Pearson,Michel Perault,Rene Plume,Pieter R. Roelfsema,S.-L. Qin,M. Salez,Stephan Schlemmer,J. Stutzki,Alexander G. G. M. Tielens,Neil Trappe,F. F. S. van der Tak,Charlotte Vastel,Charlotte Vastel,Harold W. Yorke,Shanshan Yu,Jonas Zmuidzinas +64 more
TL;DR: In this article, the spectral properties of the Orion hot core were investigated using the Herschel GT key program and the HIFI instrument was used to measure the dust continuum and spectrally resolve emission lines in Orion KL.