DOCSLIB.ORG

19 International Workshop on Low Temperature Detectors

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
19 International Workshop on Low Temperature Detectors 19th International Workshop on Low Temperature Detectors Program version 1.24 - British Summer Time 1 Date Time Session Monday 19 July 14:00 - 14:15 Introduction and Welcome 14:15 - 15:15 Oral O1: Devices 1 15:15 - 15:25 Break 15:25 - 16:55 Oral O1: Devices 1 (continued) 16:55 - 17:05 Break 17:05 - 18:00 Poster P1: MKIDs and TESs 1 Tuesday 20 July 14:00 - 15:15 Oral O2: Cold Readout 15:15 - 15:25 Break 15:25 - 16:55 Oral O2: Cold Readout (continued) 16:55 - 17:05 Break 17:05 - 18:30 Poster P2: Readout, Other Devices, Supporting Science 1 20:00 - 21:00 Virtual Tour of NIST Quantum Sensor Group Labs Wednesday 21 July 14:00 - 15:15 Oral O3: Instruments 15:15 - 15:25 Break 15:25 - 16:55 Oral O3: Instruments (continued) 16:55 - 17:05 Break 17:05 - 18:30 Poster P3: Instruments, Astrophysics and Cosmology 1 18:00 - 19:00 Vendor Exhibitor Hour Thursday 22 July 14:00 - 15:15 Oral O4A: Rare Events 1 Oral O4B: Material Analysis, Metrology, Other 15:15 - 15:25 Break 15:25 - 16:55 Oral O4A: Rare Events 1 (continued) Oral O4B: Material Analysis, Metrology, Other (continued) 16:55 - 17:05 Break 17:05 - 18:30 Poster P4: Rare Events, Materials Analysis, Metrology, Other Applications 20:00 - 21:00 Virtual Tour of NIST Cleanoom Monday 26 July 23:00 - 00:15 Oral O5: Devices 2 00:15 - 00:25 Break 00:25 - 01:55 Oral O5: Devices 2 (continued) 01:55 - 02:05 Break 02:05 - 03:30 Poster P5: MMCs, SNSPDs, more TESs Tuesday 27 July 23:00 - 00:15 Oral O6: Warm Readout and Supporting Science 00:15 - 00:25 Break 00:25 - 01:55 Oral O6: Warm Readout and Supporting Science (continued) 01:55 - 02:05 Break 02:05 - 03:30 Poster P6: Readout, Other Devices, Supporting Science 2 Wednesday 28 July 21:00 - 22:00 Vendor Exhibitor Hour 23:00 - 00:15 Oral O7A: Rare Events 2 Oral O7B: Astrophysics and Cosmology 00:15 - 00:25 Break 00:25 - 01:55 Oral O7A: Rare Events 2 (continued) Oral O7B: Astrophysics and Cosmology (continued) 01:55 - 02:05 Break 02:05 - 03:30 Poster P7: Rare Events, Astrophysics and Cosmology, Instru- ments, more MKIDs Thursday 29 July 23:00 - 00:30 Oral O8: Devices 3 00:30 - 00:40 Break 00:40 - 02:25 Oral O8: Devices 3 (continued) 02:25 - 02:35 Break 02:35 - 03:00 Closing and Introduction of LTD20 Hosts 1Other time zones available here 1 LTD19 Program v1.24 British Summer Time Week 1 Day 1 Monday 19 July 14:00 - Monday 19 July 18:00 (British Summer Time) Introduction and Welcome: 14:00 - 14:15 (Conference webpage) Oral O1: Devices 1 14:15 - 16:55 (Conference webpage) Session chairs: Mark Croce, Los Alamos National Laboratory Ben Mates, National Institute of Standards and Technology 1. 14:15 “Microwave Kinetic Inductance Detectors – detector physics and recent developments” (Invited) Pieter de Visser - SRON 2. 14:45 “Subgap kinetic inductance detector sensitive to 85-GHz radiation” Florence Levy-Bertrand - Institut Néel, Grenoble (France) 3. 15:00 “Strong Generation-Recombination Noise Reduction in Hybrid NbTiN-Al MKIDs” Steven de Rooij - SRON, Netherlands Institute for Space Research Break: 15:15 - 15:25 (10 minutes) 4. 15:25 “Bolometer operating at the threshold for circuit quantum electrodynamics [Nature 586, 47 (2020)]” Mikko Möttönen - Aalto University 5. 15:40 “Modeling of superconductor-ferromagnet thermoelectric detector for X-ray detection” Zhuoran Geng - Nanoscience Center, University of Jyväskylä 6. 15:55 “Transition-Edge Sensors for low-energy electron detection” Mauro Rajteri - INRIM 7. 16:10 “Voltage fluctuations in transition edge sensors and other effects from the 70’s” Luciano Gottardi - NWO-I SRON, Netherlands Institute for Space Research 8. 16:25 “Impact of the absorber coupling design for Transition Edge Sensor X-ray Calorimeters” Martin de Wit - Netherlands Institute for Space Research (SRON) 9. 16:40 “Fine optimization of TES microcalorimeter design for the X-IFU instrument on ATHENA” Nicholas Wakeham - University of Maryland Baltimore County / NASA Goddard Space Flight Center Break: 16:55 - 17:05 (10 minutes) Poster P1: MKIDs and TESs 1 17:05 - 18:00 (Conference webpage) 1. “A Far-Infrared TES Bolometer with a Magnetically-Switchable High-Power Mode” Michael Audley - SRON Netherlands Institute for Space Research 2. “A kinetic inductance detectors array design for high background conditions at 150 GHz” Shibo Shu - California Institute of Technology 3. “Characterization of the Superconducting Microwave Properties of Aluminum Manganese” Marharyta Lisovenko - Argonne National Laboratory 4. “Compton spectroscopy measurements at the APS 1-BM beamline using traditional semiconductor and ad- vanced high-energy TES X-ray detectors” Umeshkumar Patel - Argonne National Laboratory 5. “Decoupling of the quasiparticle number and lifetime in titanium nitride resonators” Sunil Golwala - California Institute of Technology 6. “Design and preliminary results of the spectroscopic focal plane for the South Pole Telescope Summertime Line Intensity Mapper” Pete Barry - Argonne National Laboratory 7. “Design of a multi-chroic kinetic inductance detectors array coupled to a hierarchical phased-array antenna” Shibo Shu - California Institute of Technology 8. “Development of a fabrication process for large suspended gold absorbers for TES microcalorimeters” Conjeepuram Ambarish - University of Wisconsin-Madison 9. “Development of a prototype detector for Torio-229 experiment” Mariia Fedkevych - Department of Physics, University of Genoa, Genoa, Italy 10. “Development of high-resolution, large absorber TES microcalorimeters for the soft X-ray range” Felix Jaeckel - University of Wisconsin - Madison 11. “Development of MKIDs for Measurement of the Cosmic Microwave Background with the South Pole Tele- scope” Karia Dibert - The University of Chicago 2 LTD19 Program v1.24 British Summer Time 12. “Energy Calibration of Phonon-Mediated Dark Matter Detectors using MKIDs” Ritoban Basu Thakur - California Institute of Technology 13. “Influence of Width of Ti/Au Transition Edge Sensors” Kenichiro Nagayoshi - NWO-I/SRON Netherlands Institute for Space Research 14. “Investigation of Optical Coupling Performance in LEKIDs Using Superconducting Reflective Plates” Paul Nicaise - GEPI - Observatoire de Paris - CNRS 15. “LiteBIRD Low and Mid-Frequency Detectors: Design and Status” Greg Jaehnig - University of Colorado Boulder 16. “Low stray power cross-coupling between MKIDs, for future focal plane spectrometer arrays” Stephen Yates - SRON, Netherlands Institute for Space Research 17. “Model and measurements of an optical stack for broadband absorption in Optical LEKIDs” Kevin Kouwenhoven - SRON Netherlands Institute for Space Research 18. “Modeling and Optimizing Microwave Kinetic Inductance Detectors for the EXCLAIM Mission” Trevor Oxholm - University of Wisconsin-Madison 19. “Near Infrared and Visible Kinetic Inductance Detectors for SPIAKID” Faouzi Boussaha - GEPI-Observatoire de Paris CNRS UMR8111 20. “On-chip Spectrometers operating at 90GHz” Usasi Chowdhury - Institut Neel, UGA 21. “Optimization of Ti/TiN multilayers for optical to near-IR MKIDs and exploring their commercial foundry potential” Gerhard Ulbricht - Dublin Institute for Advanced Studies 22. “Overcoming the challenges for reproducible fabrication of 15 mK tungsten-based TESs with tunable and predictable Tc” Ahmed Abdelhameed - Max-Planck-Institut für Physik 23. “Phonon-trapping enhanced energy resolution in superconducting single photon detectors” Pieter de Visser - SRON 24. “Progress in the development of Thermal Kinetic Inductance Detectors for X-ray spectroscopy” Marco Faverzani - University and INFN of Milano-Bicocca 25. “Resolving power of visible/near-infrared hybrid NbTiN/b-Ta LEKIDs” Kevin Kouwenhoven - SRON Netherlands Institute for Space Research 26. “Simulation of radiative transfer within X-ray microcalorimeter absorbers.” Maximilian Lorenz - Dr. Karl Remeis-Observatory & ECAP 27. “Simulation of the Cosmic Ray impact on the TES detectors of SPICA/SAFARI” Thijs Stockmans - leiden University 28. “Stability Analysis of SAFARI FDM Readout System” Micha Heilman - Leiden Univeristy/ SRON 29. “SuperSpec Improvements for Future Far-IR Missions” Ryan McGeehan - University of Chicago 30. “Susceptibility study of transition-edge sensor micro-calorimeters for X-ray spectroscopy under frequency- domain multiplexing readout” Davide Vaccaro - SRON 31. “Temperature and current sensitivities of bare Mo/Au Transition-Edge Sensors: size effects” Lourdes Fàbrega - ICMAB-CSIC 32. “Thermal Conductance of Individual Layers on TES Legs” Angelina Harke-Hosemann - National Institute of Standards and Technology; University of Colorado Boulder 33. “TiNx MKIDs from a 3.5M euro UHV state-of-the-art sputter system” Mario De Lucia - Dublin Institute for Advanced Studies 34. “X-ray transition edge sensors as backup option for X-IFU on ATHENA space telescope” Emanuele Taralli - Netherlands Institute for Space Research 3 LTD19 Program v1.24 British Summer Time Week 1 Day 2 Tuesday 20 July 14:00 - Tuesday 20 July 21:00 (British Summer Time) Oral O2: Cold Readout 14:00 - 16:55 (Conference webpage) Session chairs: Randy Doriese, National Institute of Standards and Technology Kelsey Morgan, University of Colorado, Boulder 1. 14:00 “Advances in time-division SQUID multiplexing for TES X-ray-microcalorimeter arrays” (Invited) Malcolm Durkin - University of Colorado 2. 14:30 “BICEP Array: 150 GHz detector module development” Alessandro Schillaci - California Institute of Technology 3. 14:45 “The Simons Observatory microwave SQUID multiplexing detector module design” Heather McCarrick - Princeton 4. 15:00 “Demonstration of 37-pixel
Load more

Recommended publications
  • William Adams and Tokugawa Ieyasu!
    Realize a NHK drama centered on William Adams and Tokugawa Ieyasu! We request for your support and cooperation with our Petition Campaign! Recognized in Japan by the name, Miura Anjin, this English sailor became the diplomatic advisor to Tokugawa Ieyasu, and greatly contributed to the development of Japan with his profound knowledge of navigation and shipbuilding. Four cities connected to Adams: Usuki of Oita prefecture, Ito of Shizuoka prefecture, Yokosuka of Kanagawa prefecture, and Hirado of Nagasaki prefecture, have formed the “ANJIN Project Committee,” and are working together to honor Adams achievements, and also propose a theme based on William Adams and Tokugawa Ieyasu for Taiga Drama. Taiga Drama is a renowned historical drama series created by NHK, Japan’s sole public broadcasting organization. Themes for this annual drama are selected from Japan’s rich history. To further increase the chances of our Taiga Drama proposal to NHK, we have started a Petition Campaign! To sign the petition, please fill your name and address on the form below: Petition Form I support the creation of a NHK Taiga Drama based around the theme of William Adams and Tokugawa Ieyasu. Address Name Prefecture* Municipality* Land number is e.g. Taro Yokosuka Kanagawa Ogawa-cho, Yokosuka not required. e.g. William Adams U.K. Medway 1 2 按針メモリアルパーク 3 4 5 三浦按針上陸記念公園 6 7 三浦按針之墓 8 9 会社名 10 *Those overseas should write your Country in “Prefecture” (e.g. U.K.) and your City in “Municipality” (e.g. Medway). ・Please submit the completed form to the division below (bring the form directly or send it by mail or FAX).
    [Show full text]
  • Passion for Cycling Tourism
    TUSCANY if not HERE, where? PASSION FOR CYCLING TOURISM Tuscany offers you • Unique landscapes and climate • A journey into history and art: from Etruscans to Renaissance down to the present day • An extensive network of cycle paths, unpaved and paved roads with hardly any traffic • Unforgettable cuisine, superb wines and much more ... if not HERE, where? Tuscany is the ideal place for a relaxing cycling holiday: the routes are endless, from the paved roads of Chianti to trails through the forests of the Apennines and the Apuan Alps, from the coast to the historic routes and the eco-paths in nature photo: Enrico Borgogni reserves and through the Val d’Orcia. This guide has been designed to be an excellent travel companion as you ride from one valley, bike trail or cultural site to another, sometimes using the train, all according to the experiences reported by other cyclists. But that’s not all: in the guide you will find tips on where to eat and suggestions for exploring the various areas without overlooking small gems or important sites, with the added benefit of taking advantage of special conditions reserved for the owners of this guide. Therefore, this book is suitable not only for families and those who like easy routes, but can also be helpful to those who want to plan multiple-day excursions with higher levels of difficulty or across uscanyT for longer tours The suggested itineraries are only a part of the rich cycling opportunities that make Tuscany one of the paradises for this kind of activity, and have been selected giving priority to low-traffic roads, white roads or paths always in close contact with nature, trying to reach and show some of our region’s most interesting destinations.
    [Show full text]
  • A Biomolecular Anthropological Investigation of William Adams, The
    www.nature.com/scientificreports OPEN A biomolecular anthropological investigation of William Adams, the frst SAMURAI from England Fuzuki Mizuno1*, Koji Ishiya2,3, Masami Matsushita4, Takayuki Matsushita4, Katherine Hampson5, Michiko Hayashi1, Fuyuki Tokanai6, Kunihiko Kurosaki1* & Shintaroh Ueda1,5 William Adams (Miura Anjin) was an English navigator who sailed with a Dutch trading feet to the far East and landed in Japan in 1600. He became a vassal under the Shogun, Tokugawa Ieyasu, was bestowed with a title, lands and swords, and became the frst SAMURAI from England. "Miura" comes from the name of the territory given to him and "Anjin" means "pilot". He lived out the rest of his life in Japan and died in Hirado, Nagasaki Prefecture, in 1620, where he was reportedly laid to rest. Shortly after his death, graveyards designated for foreigners were destroyed during a period of Christian repression, but Miura Anjin’s bones were supposedly taken, protected, and reburied. Archaeological investigations in 1931 uncovered human skeletal remains and it was proposed that they were those of Miura Anjin. However, this could not be confrmed from the evidence at the time and the remains were reburied. In 2017, excavations found skeletal remains matching the description of those reinterred in 1931. We analyzed these remains from various aspects, including genetic background, dietary habits, and burial style, utilizing modern scientifc techniques to investigate whether they do indeed belong to the frst English SAMURAI. William Adams was born in Gillingham, England in 1564. He worked in a shipyard from the age of 12, and later studied shipbuilding techniques, astronomy and navigation.
    [Show full text]
  • Evidence from Covid-19 Pandemic
    RISK PERCEPTIONS AND PROTECTIVE BEHAVIORS: EVIDENCE FROM COVID-19 PANDEMIC Maria Polyakova M. Kate Bundorf Duke University Stanford University & NBER & NBER Jill DeMatteis Jialu L. Streeter Westat Stanford University Grant Miller Jonathan Wivagg Stanford University Westat & NBER April, 2021 Working Paper No. 21-022 Risk Perceptions and Protective Behaviors: Evidence from COVID-19 Pandemic.∗ M. Kate Bundorf Jill DeMatteis Grant Miller Maria Polyakova Duke University Westat Stanford University Stanford University and NBER and NBER and NBER Jialu L. Streeter Jonathan Wivagg Stanford University Westat April 28, 2021 Abstract We analyze data from a survey we administered during the COVID-19 pandemic to investigate the relationship between people's subjective risk beliefs and their protective behaviors. We report three main findings. First, on average, people substantially overestimate the absolute level of risk associated with economic activity, but have correct signals about their relative risk. Second, people who believe that they face a higher risk of infection are more likely to report avoiding economic activities. Third, government mandates restricting economic behavior attenuate the relationship between subjective risk beliefs and protective behaviors. ∗Corresponding author: Maria Polyakova ([email protected]). We are grateful to Sarah B¨ogland Aava Farhadi for excellent research assistance. We have made the de-identified survey dataset used in this manuscript available at the following link. We gratefully acknowledge in-kind survey support from Westat. 1 1 Introduction Subjective perceptions of risk guide decision making in nearly all economic domains (Hurd, 2009). While a rich theoretical literature highlights the importance of subjective beliefs for individual ac- tions, fewer studies provide empirical evidence of the link between risk perceptions and behaviors, particularly in non-laboratory settings and in high-income countries (Peltzman, 1975; Delavande, 2014; Delavande and Kohler, 2015; Mueller et al., 2021).
    [Show full text]
  • CMB Telescopes and Optical Systems to Appear In: Planets, Stars and Stellar Systems (PSSS) Volume 1: Telescopes and Instrumentation
    CMB Telescopes and Optical Systems To appear in: Planets, Stars and Stellar Systems (PSSS) Volume 1: Telescopes and Instrumentation Shaul Hanany ([email protected]) University of Minnesota, School of Physics and Astronomy, Minneapolis, MN, USA, Michael Niemack ([email protected]) National Institute of Standards and Technology and University of Colorado, Boulder, CO, USA, and Lyman Page ([email protected]) Princeton University, Department of Physics, Princeton NJ, USA. March 26, 2012 Abstract The cosmic microwave background radiation (CMB) is now firmly established as a funda- mental and essential probe of the geometry, constituents, and birth of the Universe. The CMB is a potent observable because it can be measured with precision and accuracy. Just as importantly, theoretical models of the Universe can predict the characteristics of the CMB to high accuracy, and those predictions can be directly compared to observations. There are multiple aspects associated with making a precise measurement. In this review, we focus on optical components for the instrumentation used to measure the CMB polarization and temperature anisotropy. We begin with an overview of general considerations for CMB ob- servations and discuss common concepts used in the community. We next consider a variety of alternatives available for a designer of a CMB telescope. Our discussion is guided by arXiv:1206.2402v1 [astro-ph.IM] 11 Jun 2012 the ground and balloon-based instruments that have been implemented over the years. In the same vein, we compare the arc-minute resolution Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT). CMB interferometers are presented briefly. We con- clude with a comparison of the four CMB satellites, Relikt, COBE, WMAP, and Planck, to demonstrate a remarkable evolution in design, sensitivity, resolution, and complexity over the past thirty years.
    [Show full text]
  • The Design of the Ali CMB Polarization Telescope Receiver
    The design of the Ali CMB Polarization Telescope receiver M. Salatinoa,b, J.E. Austermannc, K.L. Thompsona,b, P.A.R. Aded, X. Baia,b, J.A. Beallc, D.T. Beckerc, Y. Caie, Z. Changf, D. Cheng, P. Chenh, J. Connorsc,i, J. Delabrouillej,k,e, B. Doberc, S.M. Duffc, G. Gaof, S. Ghoshe, R.C. Givhana,b, G.C. Hiltonc, B. Hul, J. Hubmayrc, E.D. Karpela,b, C.-L. Kuoa,b, H. Lif, M. Lie, S.-Y. Lif, X. Lif, Y. Lif, M. Linkc, H. Liuf,m, L. Liug, Y. Liuf, F. Luf, X. Luf, T. Lukasc, J.A.B. Matesc, J. Mathewsonn, P. Mauskopfn, J. Meinken, J.A. Montana-Lopeza,b, J. Mooren, J. Shif, A.K. Sinclairn, R. Stephensonn, W. Sunh, Y.-H. Tsengh, C. Tuckerd, J.N. Ullomc, L.R. Valec, J. van Lanenc, M.R. Vissersc, S. Walkerc,i, B. Wange, G. Wangf, J. Wango, E. Weeksn, D. Wuf, Y.-H. Wua,b, J. Xial, H. Xuf, J. Yaoo, Y. Yaog, K.W. Yoona,b, B. Yueg, H. Zhaif, A. Zhangf, Laiyu Zhangf, Le Zhango,p, P. Zhango, T. Zhangf, Xinmin Zhangf, Yifei Zhangf, Yongjie Zhangf, G.-B. Zhaog, and W. Zhaoe aStanford University, Stanford, CA 94305, USA bKavli Institute for Particle Astrophysics and Cosmology, Stanford, CA 94305, USA cNational Institute of Standards and Technology, Boulder, CO 80305, USA dCardiff University, Cardiff CF24 3AA, United Kingdom eUniversity of Science and Technology of China, Hefei 230026 fInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049 gNational Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 hNational Taiwan University, Taipei 10617 iUniversity of Colorado Boulder, Boulder, CO 80309, USA jIN2P3, CNRS, Laboratoire APC, Universit´ede Paris, 75013 Paris, France kIRFU, CEA, Universit´eParis-Saclay, 91191 Gif-sur-Yvette, France lBeijing Normal University, Beijing 100875 mAnhui University, Hefei 230039 nArizona State University, Tempe, AZ 85004, USA oShanghai Jiao Tong University, Shanghai 200240 pSun Yat-Sen University, Zhuhai 519082 ABSTRACT Ali CMB Polarization Telescope (AliCPT-1) is the first CMB degree-scale polarimeter to be deployed on the Tibetan plateau at 5,250 m above sea level.
    [Show full text]
  • Estimating the Overdispersion in COVID
    Wellcome Open Research 2020, 5:67 Last updated: 13 JUL 2020 RESEARCH ARTICLE Estimating the overdispersion in COVID-19 transmission using outbreak sizes outside China [version 3; peer review: 2 approved] Akira Endo 1,2, Centre for the Mathematical Modelling of Infectious Diseases COVID-19 Working Group, Sam Abbott 1,3, Adam J. Kucharski1,3, Sebastian Funk 1,3 1Department of Infectious Disease Epidemiology, London School of Hygiene & Tropical Medicine, London, WC1E 7HT, UK 2The Alan Turing Institute, London, NW1 2DB, UK 3Centre for the Mathematical Modelling of Infectious Diseases, London School of Hygiene & Tropical Medicine, London, WC1E 7HT, UK First published: 09 Apr 2020, 5:67 Open Peer Review v3 https://doi.org/10.12688/wellcomeopenres.15842.1 Second version: 03 Jul 2020, 5:67 https://doi.org/10.12688/wellcomeopenres.15842.2 Reviewer Status Latest published: 10 Jul 2020, 5:67 https://doi.org/10.12688/wellcomeopenres.15842.3 Invited Reviewers 1 2 Abstract Background: A novel coronavirus disease (COVID-19) outbreak has now version 3 spread to a number of countries worldwide. While sustained transmission (revision) report chains of human-to-human transmission suggest high basic reproduction 10 Jul 2020 number R0, variation in the number of secondary transmissions (often characterised by so-called superspreading events) may be large as some countries have observed fewer local transmissions than others. version 2 Methods: We quantified individual-level variation in COVID-19 (revision) report report transmission by applying a mathematical model to observed outbreak sizes 03 Jul 2020 in affected countries. We extracted the number of imported and local cases in the affected countries from the World Health Organization situation report and applied a branching process model where the number of secondary version 1 transmissions was assumed to follow a negative-binomial distribution.
    [Show full text]
  • Clover: Measuring Gravitational-Waves from Inflation
    ClOVER: Measuring gravitational-waves from Inflation Executive Summary The existence of primordial gravitational waves in the Universe is a fundamental prediction of the inflationary cosmological paradigm, and determination of the level of this tensor contribution to primordial fluctuations is a uniquely powerful test of inflationary models. We propose an experiment called ClOVER (ClObserVER) to measure this tensor contribution via its effect on the geometric properties (the so-called B-mode) of the polarization of the Cosmic Microwave Background (CMB) down to a sensitivity limited by the foreground contamination due to lensing. In order to achieve this sensitivity ClOVER is designed with an unprecedented degree of systematic control, and will be deployed in Antarctica. The experiment will consist of three independent telescopes, operating at 90, 150 or 220 GHz respectively, and each of which consists of four separate optical assemblies feeding feedhorn arrays arrays of superconducting detectors with phase as well as intensity modulation allowing the measurement of all three Stokes parameters I, Q and U in every pixel. This project is a combination of the extensive technical expertise and experience of CMB measurements in the Cardiff Instrumentation Group (Gear) and Cavendish Astrophysics Group (Lasenby) in UK, the Rome “La Sapienza” (de Bernardis and Masi) and Milan “Bicocca” (Sironi) CMB groups in Italy, and the Paris College de France Cosmology group (Giraud-Heraud) in France. This document is based on the proposal submitted to PPARC by the UK groups (and funded with 4.6ML), integrated with additional information on the Dome-C site selected for the operations. This document has been prepared to obtain an endorsement from the INAF (Istituto Nazionale di Astrofisica) on the scientific quality of the proposed experiment to be operated in the Italian-French base of Dome-C, and to be submitted to the Commissione Scientifica Nazionale Antartica and to the French INSU and IPEV.
    [Show full text]
  • The Japanese Samurai Code: Classic Strategies for Success Kindle
    THE JAPANESE SAMURAI CODE: CLASSIC STRATEGIES FOR SUCCESS PDF, EPUB, EBOOK Boye Lafayette De Mente | 192 pages | 01 Jun 2005 | Tuttle Publishing | 9780804836524 | English | Boston, United States The Japanese Samurai Code: Classic Strategies for Success PDF Book Patrick Mehr on May 4, pm. The culture and tradition of Japan, so different from that of Europe, never ceases to enchant and intrigue people from the West. Hideyoshi was made daimyo of part of Omi Province now Shiga Prefecture after he helped take the region from the Azai Clan, and in , Nobunaga sent him to Himeji Castle to face the Mori Clan and conquer western Japan. It is an idea taken from Confucianism. Ieyasu was too late to take revenge on Akechi Mitsuhide for his betrayal of Nobunaga—Hideyoshi beat him to it. Son of a common foot soldier in Owari Province now western Aichi Prefecture , he joined the Oda Clan as a foot soldier himself in After Imagawa leader Yoshimoto was killed in a surprise attack by Nobunaga, Ieyasu decided to switch sides and joined the Oda. See our price match guarantee. He built up his capital at Edo now Tokyo in the lands he had won from the Hojo, thus beginning the Edo Period of Japanese history. It emphasised loyalty, modesty, war skills and honour. About this item. Installing Yoshiaki as the new shogun, Nobunaga hoped to use him as a puppet leader. Whether this was out of disrespect for a "beast," as Mitsuhide put it, or cover for an act of mercy remains a matter of debate. While Miyamoto Musashi may be the best-known "samurai" internationally, Oda Nobunaga claims the most respect within Japan.
    [Show full text]
  • Transience10
    a publication of ADVENTURE CYCLING ASSOCIATION AN EPIC ACT OF TRANSIENCE10 $6.95 OCT/NOV 2019 Vol.46 No.8 STACK LONG DAYS. CLIMB LIKE A MOUNTAIN GOAT. Saddle, back, neck and wrist pain no longer get a say in your plans. Our patented drive system brings together the best of traditional and recumbent touring bikes so you don’t have to sacrifice performance for comfort. But we should warn you, your cheeks may hurt from smiling. Adventure Cyclist readers get $100 off the Cruzbike of their choice Use code: ADVENTURE at C ruzbike.com Letter from the Editor online WHAT YEAR IS IT AGAIN? Revolution, evolution, and the march of progress PHOTO CONTEST OPEN NOW ➺I recently found myself standing on a quiet main ’Tis the season for submitting street in front of a small-town Montana theater. I’d your best images to the 11th been on the road for a while and small towns can start Annual Bicycle Travel Photo to look the same, but when I looked up at the marquee Contest. Winning images are published in the May 2020 and saw “Lion King,” for a moment I was sure of EDGERTONADAM neither where I was nor when. Adventure Cyclist, plus these Depending on the level of charity you’re inclined shots appear in our annual to employ, there are either no more ideas left, or we calendar. Send us your best simply evolve the same core idea over and over to at adventurecycling.org/ reintroduce it to new generations. I was certainly thinking about the photcontest now through spectrum of “invention” as I read Bob Marr’s story on page 20 about turn- November 30.
    [Show full text]
  • The Future of NATO and European Defence
    House of Commons Defence Committee The future of NATO and European defence Ninth Report of Session 2007–08 Report, together with formal minutes, oral and written evidence Ordered by The House of Commons to be printed 4 March 2008 HC 111 [Incorporating HC 707-i & ii] Published on 20 March 2008 by authority of the House of Commons London: The Stationery Office Limited £0.00 The Defence Committee The Defence Committee is appointed by the House of Commons to examine the expenditure, administration, and policy of the Ministry of Defence and its associated public bodies. Current membership Rt Hon James Arbuthnot MP (Conservative, North East Hampshire) (Chairman) Mr David S Borrow MP (Labour, South Ribble) Mr David Crausby MP (Labour, Bolton North East) Linda Gilroy MP (Labour, Plymouth Sutton) Mr David Hamilton MP (Labour, Midlothian) Mr Mike Hancock MP (Liberal Democrat, Portsmouth South) Mr Dai Havard MP (Labour, Merthyr Tydfil and Rhymney) Mr Adam Holloway MP (Conservative, Gravesham) Mr Bernard Jenkin MP (Conservative, North Essex) Mr Brian Jenkins MP (Labour, Tamworth) Mr Kevan Jones MP (Labour, Durham North) Robert Key MP (Conservative, Salisbury) John Smith MP (Labour, Vale of Glamorgan) Richard Younger-Ross MP (Liberal Democrat, Teignbridge) The following Members were also Members of the Committee during the Parliament. Mr Colin Breed MP (Liberal Democrat, South East Cornwall) Derek Conway MP (Conservative, Old Bexley and Sidcup) Mr Mark Lancaster MP (Conservative, North East Milton Keynes) Willie Rennie MP (Liberal Democrat, Dunfermline and West Fife) Mr Desmond Swayne MP (Conservative, New Forest West) Powers The Committee is one of the departmental select committees, the powers of which are set out in House of Commons Standing Orders, principally in SO No 152.
    [Show full text]
  • The Cℓover Experiment
    Invited Paper The CℓOVER Experiment L. Piccirillo1, P. Ade2, M. D. Audley3, C. Baines1, R. Battye1, M. Brown3, P. Calisse2, A. Challinor5,6, W. D. Duncan7, P. Ferreira4, W. Gear2, D. M. Glowacka3, D. Goldie3, P.K. Grimes4, M. Halpern8, V. Haynes1, G. C. Hilton7, K. D. Irwin7, B. Johnson4, M. Jones4, A. Lasenby3, P. Leahy1, J. Leech4, S. Lewis1, B. Maffei1, L. Martinis1, P. D. Mauskopf2, S. J. Melhuish1, C. E. North4, D. O'Dea3, S. Parsley2, G. Pisano1, C. D. Reintsema7, G. Savini2, R.V. Sudiwala2, D. Sutton4, A. Taylor4, G. Teleberg2, D. Titterington3, V. N. Tsaneva3, C. Tucker2, R. Watson1, S. Withington3, G. Yassin4, J. Zhang2 1 School of Physics and Astronomy, University of Manchester, UK 2 School of Physics and Astronomy, Cardiff University, UK 3 Cavendish Laboratory, University of Cambridge, Cambridge, UK 4 Astrophysics, University of Oxford, Oxford, UK 5 Institute of Astronomy, University of Cambridge, Cambridge, UK 6 DAMTP, University of Cambridge, Cambridge, UK 7 National Institute of Standards and Technology, USA 8 University of British Columbia, Canada CℓOVER is a multi-frequency experiment optimised to measure the Cosmic Microwave Background (CMB) polarization, in particular the B- mode component. CℓOVER comprises two instruments observing respectively at 97 GHz and 150/225 GHz. The focal plane of both instruments consists of an array of corrugated feed-horns coupled to TES detectors cooled at 100 mK. The primary science goal of CℓOVER is to be sensitive to gravitational waves down to r ~ 0.03 (at 3σ) in two years of operations. 1 Introduction The Cosmic Microwave Background (CMB) Radiation is a very powerful tool to study the origin and evolution of the Universe.
    [Show full text]