P-1 | Parisa Y. Aghdam | Chalmers University of Technology, Sweden | On Specific Capacitance of SIS Junctions |
P-2 | Dominic Benford | NASA/Goddard Space Flight Center | Focal Plane Arrays for HAWC+, SOFIA's upgraded High-resolution Airborne Wideband Camera and polarimeter |
P-3 | Jiajun Chen | University of Cambridge | Modal Optical Modelling of a Test System for Ultra-Low-Noise Transition Edge Sensors for Space Science |
P-4 | Gert de Lange | SRON, the Netherlands | A low-background test facility for spectral response measurements at 70 mK of ultra-sensitive TES detectors. |
P-5 | Fabien Defrance | LERMA, Observatoire de Paris, France | Non-periodic phase gratings |
P-6 | Vladimir Drakinskiy | Chalmers University of Technology | Status and Progress of Schottky Technology Development for SWI and ISMAR |
P-7 | Gregory Gay | LERMA, Observatoire de Paris, France | Development of Membrane Based Quasi-optical HEB Mixers at 1.4 THz |
P-8 | Alvaro Gonzalez | NAOJ, Japan | The need of compact profiled corrugated horns at longer mm-waves (ALMA band 1) and at around 1 THz (band 10) |
P-9 | Paul Grimes | Smithsonian Astrophysical Observatory | Testing an array of 350 GHz drilled smoothwall horns using a vector near-field beam scanner |
P-10 | Quan Guo | National University of Defense Technology, China | Fourfold Azimuthal Dependence of Terahertz Radiation from (100) Silicon |
P-11 | Arvid Hammar | Omnisys Instruments AB, Sweden | Optical Designs for a Multi-Beam 340 and 625/640 GHz Spaceborne Climate Research Instrument |
P-12 | Andre Hector | University of Oxford, UK | Investigating the Origin of Harmonics in a 230 GHz Local Oscillator |
P-13 | Todd Hunter | National Radio Astronomical Observatory | Statistical Topics Concerning Radiometer Theory |
P-14 | Yoshihisa Irimajiri | National Institute of Information and Communications Technology, Japan | Performance evaluation of phase-locking for THz-QCL using a HEB mixer |
P-15 | Ling Jiang | Nanjing Forestry University, China | Terahertz spectra of vitamins studied by terahertz spectroscopy and density functional theory |
P-16 | Glenn Jones | Columbia University | A Cryogenic Millimeter Wavelength Test Facility |
P-17 | Boris Karasik | Jet Propulsion Laboratory | Analysis of a normal metal nano-HEB THz array |
P-18 | Akira Kawakami | National Institute of Information and Communications Technology, Japan | Fabrication of 3 THz superconducting hot electron bolometer mixers |
P-19 | Andrey Khudchenko | SRON, the Netherlands | High Gap Nb-A1N-NbN SIS Junctions for Frequency Band 790-950 GHz |
P-20 | Hyunjoo Kim | University of Bern, Switzerland | Optical design study for Submillimeter Wave Instrument for the Jupiter mission |
P-21 | Takafumi Kojima | National Astronomical Observatory of Japan | Development of a Terahertz HEB Mixer-Amplifier with SiGe HBTs |
P-22 | Takafumi Kojima | National Astronomical Observatory of Japan | Design of Superconducting On-chip Frequency Multiplexers for a Low-noise Multiband Receiver |
P-23 | Y. Kozuki | Osaka Prefecture University, Japan | Development for a wideband 100GHz SIS mixer |
P-24 | Matthias Kroug | National Astronomical Observatory of Japan | High Current Density SIS Junctions Based on Nb/A1,A1N/Nb Tri-layers |
P-25 | Jing Li | Purple Mountain Observatory, China | Development of an 8X8 CPW Microwave Kinetic Inductance Detectors (MKIDs) Array at 0.35 THz |
P-26 | Kuan-Yu Liu | ASIAA, Taiwan | The Performance of an Integrated Dual Polarization SIS Mixer at 350 GHz |
P-27 | Yury Lobanov | Moscow Institute of Physics and Technology, Russia | Antenna-Coupled 30 THz Hot Electron Bolometer Mixers |
P-28 | Sylvain Mahieu | IRAM, France | Dual-Band SIS Receiver Design for Atmospheric Physics Research |
P-29 | Francois Mattiocco | IRAM, France | Electronically Tuned Local Oscillators for the NOEMA Interferometer |
P-30 | Shirin Montazeri | University of Massachusetts Amherst | Direct Integration of an SIS Mixer with a High-Impedance SiGe Low Noise Amplifier |
P-31 | Evgenii Novoselov | Chalmers University of Technology, Sweden | Noise measurements of the low Tc MgB2 HEB mixer at 1.6THz and 2.6THz |
P-32 | Hawal Rashid | Chalmers University of Technology, Sweden | Metamaterial-Like Properties of the Distributed SIS Tunnel Junction |
P-33 | Arne Schroeder | University of Bern, Switzerland | Measurements, Simulations, and Optimization of an ALMA Band 5 Vacuum Window Prototype |
P-34 | Andrei Sergeev | SUNY Buffalo | Engineering of electron and phonon processes in HEB sensors |
P-35 | Wenlei Shan | Purple Mountain Observatory, China | Experimental Study of NbTiN Microstrip Lines |
P-36 | Alexander Shurakov | Moscow State Pedagogical University, Russia | Performance of an HEB Direct Detector Utilizing a Microwave Reflection Readout Scheme |
P-37 | Boon Kok Tan | University of Oxford, UK | A 220 GHz Finline Mixer with Ultra-Wide Instantaneous Bandwidth |
P-38 | Boon Kok Tan | University of Oxford, UK | Investigation of the Dynamic Range of Superconducting Nano-Bridge Switches |
P-39 | Ivan Tretyakov | Moscow State Pedagogical University, Russia | Impact of operating conditions on noise and gain bandwidth of NbN HEB mixers |
P-40 | Andrey Trifonov | Harvard-Smithsonian Center for Astrophysics | An Investigation of the DC and IF Performance of Silicon-membrane HEB Mixer Elements |
P-41 | Jonathan Weintroub | Harvard-Smithsonian Center for Astrophysics | 20 gigasample per second analog-to-digital conversion for ultra-wideband radio astronomy |
P-42 | Jonathan Weintroub | Harvard-Smithsonian Center for Astrophysics | SWARM: A compact high resolution correlator and wideband VLBI phased array upgrade for SMA |
P-43 | Matthaeus Wolak | Temple University | Ultrathin MgB2 Films for Hot Electron Bolometer Mixers Fabricated by HPCVD and Ion Milling |
P-44 | Lingzhen Zeng | Smithsonian Astrophysical Observatory | Experimental Verification of the Fundamental Gaussian Beam Properties of Smooth-walled Feedhorns |
P-45 | Lingzhen Zeng | Smithsonian Astrophysical Observatory | A Wideband Edge-Mode Isolator for Cryogenic Operation |
P-46 | Wen Zhang | Purple Mountain Observatory, China | Characterization of superconducting Ti transition edge sensors with different microbridge length |
P-47 | John Vaillancourt | Universities Space Research Association | The Stratospheric Observatory for Infrared Astronomy (SOFIA) |