Search Results - (Author, Cooperation:J. Zmuidzinas)
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1D. A. Riechers ; C. M. Bradford ; D. L. Clements ; C. D. Dowell ; I. Perez-Fournon ; R. J. Ivison ; C. Bridge ; A. Conley ; H. Fu ; J. D. Vieira ; J. Wardlow ; J. Calanog ; A. Cooray ; P. Hurley ; R. Neri ; J. Kamenetzky ; J. E. Aguirre ; B. Altieri ; V. Arumugam ; D. J. Benford ; M. Bethermin ; J. Bock ; D. Burgarella ; A. Cabrera-Lavers ; S. C. Chapman ; P. Cox ; J. S. Dunlop ; L. Earle ; D. Farrah ; P. Ferrero ; A. Franceschini ; R. Gavazzi ; J. Glenn ; E. A. Solares ; M. A. Gurwell ; M. Halpern ; E. Hatziminaoglou ; A. Hyde ; E. Ibar ; A. Kovacs ; M. Krips ; R. E. Lupu ; P. R. Maloney ; P. Martinez-Navajas ; H. Matsuhara ; E. J. Murphy ; B. J. Naylor ; H. T. Nguyen ; S. J. Oliver ; A. Omont ; M. J. Page ; G. Petitpas ; N. Rangwala ; I. G. Roseboom ; D. Scott ; A. J. Smith ; J. G. Staguhn ; A. Streblyanska ; A. P. Thomson ; I. Valtchanov ; M. Viero ; L. Wang ; M. Zemcov ; J. Zmuidzinas
Nature Publishing Group (NPG)
Published 2013Staff ViewPublication Date: 2013-04-20Publisher: Nature Publishing Group (NPG)Print ISSN: 0028-0836Electronic ISSN: 1476-4687Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Engargiola, G. ; Zmuidzinas, J. ; Lo, K. Y.
[S.l.] : American Institute of Physics (AIP)
Published 1994Staff ViewISSN: 1089-7623Source: AIP Digital ArchiveTopics: PhysicsElectrical Engineering, Measurement and Control TechnologyNotes: A 492 GHz quasioptical superconductor-insulator-superconductor (SIS) heterodyne receiver for submillimeter astronomy has been constructed with a double-sideband noise temperature of 170±25 K, where the system response is an average over a 600 MHz i.f. bandwidth centered at 1.5 GHz. The excellent sensitivity is achieved through use of a planar twin-slot antenna feeding a pair of Nb–Al2O3–Nb junctions linked by an inductance. A main beam of f/15 has been measured. The performance of this receiver is comparable to that of the best 492 GHz waveguide receivers currently in operation.Type of Medium: Electronic ResourceURL: -
3Bin, M. ; Gaidis, M. C. ; Zmuidzinas, J. ; Phillips, T. G. ; LeDuc, H. G.
Woodbury, NY : American Institute of Physics (AIP)
Published 1996Staff ViewISSN: 1077-3118Source: AIP Digital ArchiveTopics: PhysicsNotes: We describe a 1 THz quasioptical SIS mixer which uses a twin-slot antenna, an antireflection-coated silicon hyperhemispherical lens, Nb/Al-oxide/Nb tunnel junctions, and an aluminum normal-metal tuning circuit in a two-junction configuration. Since the mixer operates substantially above the gap frequency of niobium (ν(approximately-greater-than)2Δ/h∼700 GHz), a normal metal is used in the tuning circuit in place of niobium to reduce the Ohmic loss. The frequency response of the device was measured using a Fourier transform spectrometer and agrees reasonably well with the theoretical prediction. At 1042 GHz, the uncorrected double-sideband receiver noise temperature is 840 K when the physical temperature of the mixer is 2.5 K. This is the first SIS mixer which outperforms GaAs Schottky diode mixers by a large margin at 1 THz. © 1996 American Institute of Physics.Type of Medium: Electronic ResourceURL: -
4Staff View
ISSN: 0020-0891Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
5Last, I. ; Baer, M. ; Konopnicki, M. J. ; Drummond, P. D. ; Eberly, J. H. ; Kaplan, A. E. ; Meystre, P. ; Bergou, J. ; Varró, S. ; Hioe, F. T. ; Benjamin, J. ; Levine, R. D. ; Roosmalen, O. S. ; Tachello, F. ; Zmuidzinas, J. S. ; Walls, D. F. ; Strini, G. ; Casagrande, F. ; Lugiato, L. A. ; Milburn, G. J. ; Yuen, H. P.
Springer
Published 1982Staff ViewISSN: 1432-0649Keywords: 42.50Source: Springer Online Journal Archives 1860-2000Topics: PhysicsType of Medium: Electronic ResourceURL: -
6Kooi, J. W. ; Stern, J. A. ; Chattopadhyay, G. ; LeDuc, H. G. ; Bumble, B. ; Zmuidzinas, J.
Springer
Published 1998Staff ViewISSN: 1572-9559Keywords: NbTiN superconducting films ; SIS junctions ; Niobium bandgapSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract Recent results at 1 THz using normal-metal tuning circuits have shown that SIS mixers can work well up to twice the gap frequency of the junction material (niobium). However, the performance at 1 THz is limited by the substantial loss in the normal metal films. For better performance superconducting films with a higher gap frequency than niobium and with low RF loss are needed. Niobium nitride has long been considered a good candidate material, but typical NbN films suffer from high RF loss. To circumvent this problem we are currently investigating the RF loss in NbTiN films, a 15K Tc compound superconductor, by incorporating them into quasi-optical slot antenna SIS devices.Type of Medium: Electronic ResourceURL: -
7Bin, M. ; Benford, D. J. ; Gaidis, M. C. ; Büttgenbach, T. H. ; Zmuidzinas, J. ; Serabyn, E. ; Phillips, T. G.
Springer
Published 1999Staff ViewISSN: 1572-9559Keywords: Fourier Transform ; spectroscopy ; quasi-optics ; heterodyne ; SIS ; dielectrics ; submillimeterwaves ; material propertiesSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract We have designed and constructed a Fourier Transform Spectrometer (FTS) for the study of submillimeter-wave mixers and optical components. The FTS has a large aperture (up to 25.4 cm) and small focal ratio (as fast as f/2.5) to achieve a large throughput. It operates in the 100-3750 GHz (3.3-125 cm−1) frequency range with a resolution of up to 75 MHz (0.0025 cm−1). Here we discuss the design goals and provide a detailed description of the construction of the FTS. In addition, we highlight the variety of studies which have been conducted with this instrument, which include characterizing SIS mixers through both direct and heterodyne detection and measuring the properties of optical materials.Type of Medium: Electronic ResourceURL: -
8Kooi, J. W. ; Kawamura, J. ; Chen, J. ; Chattopadhyay, G. ; Pardo, J. R. ; Zmuidzinas, J. ; Phillips, T. G. ; Bumble, B. ; Stern, J. ; LeDuc, H. G.
Springer
Published 2000Staff ViewISSN: 1572-9559Keywords: SIS receiver ; twin-slot planar antenna ; NbTiN superconductor ; bandgap energy ; AlN tunnel barrier ; RF loss ; cooled opticsSource: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract We have developed a niobium titanium nitride (NbTiN) based superconductor-insulator-superconductor (SIS) receiver to cover the 350 micron atmospheric window. This frequency band lies entirely above the energy gap of niobium (700 GHz), a commonly used SIS superconductor. The instrument uses an open structure twin-slot SIS mixer that consists of two Nb/AlN/NbTiN tunnel junctions, NbTiN thin-film microstrip tuning elements, and a NbTiN ground plane. The optical configuration is very similar to the 850 GHz waveguide receiver that was installed at the Caltech Submillimeter Observatory (CSO) in 1997. To minimize front-end loss, we employed reflecting optics and a cooled beamsplitter at 4 K. The instrument has an uncorrected receiver noise temperature of 205K DSB at 800 GHz and 410K DSB at 900 GHz. The degradation in receiver sensitivity with frequency is primarily due to an increase in the mixer conversion loss, which is attributed to the mismatch between the SIS junction and the twin-slot antenna impedance. The overall system performance has been confirmed through its use at the telescope to detect a wealth of new spectroscopic lines.Type of Medium: Electronic ResourceURL: