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Analysis and Measurement of Horn Antennas for CMB Experiments
Analysis and Measurement of Horn Antennas for CMB Experiments Ian Mc Auley (M.Sc. B.Sc.) A thesis submitted for the Degree of Doctor of Philosophy Maynooth University Department of Experimental Physics, Maynooth University, National University of Ireland Maynooth, Maynooth, Co. Kildare, Ireland. October 2015 Head of Department Professor J.A. Murphy Research Supervisor Professor J.A. Murphy Abstract In this thesis the author's work on the computational modelling and the experimental measurement of millimetre and sub-millimetre wave horn antennas for Cosmic Microwave Background (CMB) experiments is presented. This computational work particularly concerns the analysis of the multimode channels of the High Frequency Instrument (HFI) of the European Space Agency (ESA) Planck satellite using mode matching techniques to model their farfield beam patterns. To undertake this analysis the existing in-house software was upgraded to address issues associated with the stability of the simulations and to introduce additional functionality through the application of Single Value Decomposition in order to recover the true hybrid eigenfields for complex corrugated waveguide and horn structures. The farfield beam patterns of the two highest frequency channels of HFI (857 GHz and 545 GHz) were computed at a large number of spot frequencies across their operational bands in order to extract the broadband beams. The attributes of the multimode nature of these channels are discussed including the number of propagating modes as a function of frequency. A detailed analysis of the possible effects of manufacturing tolerances of the long corrugated triple horn structures on the farfield beam patterns of the 857 GHz horn antennas is described in the context of the higher than expected sidelobe levels detected in some of the 857 GHz channels during flight. -
Rcosmo: R Package for Analysis of Spherical, Healpix and Cosmological Data Arxiv:1907.05648V1 [Stat.CO] 12 Jul 2019
CONTRIBUTED RESEARCH ARTICLE 1 rcosmo: R Package for Analysis of Spherical, HEALPix and Cosmological Data Daniel Fryer, Ming Li, Andriy Olenko Abstract The analysis of spatial observations on a sphere is important in areas such as geosciences, physics and embryo research, just to name a few. The purpose of the package rcosmo is to conduct efficient information processing, visualisation, manipulation and spatial statistical analysis of Cosmic Microwave Background (CMB) radiation and other spherical data. The package was developed for spherical data stored in the Hierarchical Equal Area isoLatitude Pixelation (Healpix) representation. rcosmo has more than 100 different functions. Most of them initially were developed for CMB, but also can be used for other spherical data as rcosmo contains tools for transforming spherical data in cartesian and geographic coordinates into the HEALPix representation. We give a general description of the package and illustrate some important functionalities and benchmarks. Introduction Directional statistics deals with data observed at a set of spatial directions, which are usually positioned on the surface of the unit sphere or star-shaped random particles. Spherical methods are important research tools in geospatial, biological, palaeomagnetic and astrostatistical analysis, just to name a few. The books (Fisher et al., 1987; Mardia and Jupp, 2009) provide comprehensive overviews of classical practical spherical statistical methods. Various stochastic and statistical inference modelling issues are covered in (Yadrenko, 1983; Marinucci and Peccati, 2011). The CRAN Task View Spatial shows several packages for Earth-referenced data mapping and analysis. All currently available R packages for spherical data can be classified in three broad groups. The first group provides various functions for working with geographic and spherical coordinate systems and their visualizations. -
From Stargazing to Space Travel Our Brief History Into Space
From Stargazing to Space Travel Our brief history into space Science in the News Elaine Garcia Angela She November 4th, 2015 Why do we care? Gives us perspective • What did our forefathers think of the Heavens? • Why did they think that? • How did theories change throughout time? Gives us purpose • Mystery drives inquiry and discovery. Important Lessons were Learned and will Continue to be Discovered! Keywords Astrologyl – The study and interpretation of the movements and positions of celestial bodies in relation to Earth and Earthly affairs. Astronomy – The study of physical objects in space: gas, dust, stars, planets, moons, comets, and other non-Earthly mass and phenomena. • Astrophysics – The study of the physical nature and energy of cosmic mass. • Cosmology – A branch of study that theorizes about the origin and nature of the universe. Outline 1. Star Gazing • Theories about why, where, and how 2. Star Studying • Technology to study the unknown 3. Star Reaching • Demo on space exploration Outline 1. Star Gazing • Theories about why, where, and how 2. Star Studying • Technology to study the unknown 3. Star Reaching • Demo on space exploration What are stars’ purpose? Are they the actions, moods, or warnings of celestial beings? Star Worship Is their existence independent and separated from Earth’s existence and purpose? Star Navigation and Measurement Millennia of Lessons 570 BC 384 BC 276 BC 1600 O 1750+ BC 427 BC 310 BC 90 1700 Millennia of Lessons The earliest records of astronomical observations and mathematics. 1750+ BC Greek Rule Zeus King of Gods Hera Queen of Gods Poseidon God of the Sea Hades God of the Underworld Helios The Sun God Ares God of War Aphrodite Goddess of Love Eros God of Love Athena Goddess of Wisdom Hephaestus God of Fire/Forge Wikicommons.com What season is it? Zodiac surrounds the Earth, noting the Seasons Wikicommons.com Millennia of Lessons The earliest records of astronomical observations and mathematics. -
Astronomy Binder
Astronomy Binder Bloomington High School South 2011 Contents 1 Astronomical Distances 2 1.1 Geometric Methods . 2 1.2 Spectroscopic Methods . 4 1.3 Standard Candle Methods . 4 1.4 Cosmological Redshift . 5 1.5 Distances to Galaxies . 5 2 Age and Size 6 2.1 Measuring Age . 6 2.2 Measuring Size . 7 3 Variable Stars 7 3.1 Pulsating Variable Stars . 7 3.1.1 Cepheid Variables . 7 3.1.2 RR Lyrae Variables . 8 3.1.3 RV Tauri Variables . 8 3.1.4 Long Period/Semiregular Variables . 8 3.2 Binary Variables . 8 3.3 Cataclysmic Variables . 11 3.3.1 Classical Nova . 11 3.3.2 Recurrent Novae . 11 3.3.3 Dwarf Novae (U Geminorum) . 11 3.3.4 X-Ray Binary . 11 3.3.5 Polar (AM Herculis) star . 12 3.3.6 Intermediate Polar (DQ Herculis) star . 12 3.3.7 Super Soft Source (SSS) . 12 3.3.8 VY Sculptoris stars . 12 3.3.9 AM Canum Venaticorum stars . 12 3.3.10 SW Sextantis stars . 13 3.3.11 Symbiotic Stars . 13 3.3.12 Pulsating White Dwarfs . 13 4 Galaxy Classification 14 4.1 Elliptical Galaxies . 14 4.2 Spirals . 15 4.3 Classification . 16 4.4 The Milky Way Galaxy (MWG . 19 4.4.1 Scale Height . 19 4.4.2 Magellanic Clouds . 20 5 Galaxy Interactions 20 6 Interstellar Medium 21 7 Active Galactic Nuclei 22 7.1 AGN Equations . 23 1 8 Spectra 25 8.1 21 cm line . 26 9 Black Holes 26 9.1 Stellar Black Holes . -
Ghost Imaging of Space Objects
Ghost Imaging of Space Objects Dmitry V. Strekalov, Baris I. Erkmen, Igor Kulikov, and Nan Yu Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109-8099 USA NIAC Final Report September 2014 Contents I. The proposed research 1 A. Origins and motivation of this research 1 B. Proposed approach in a nutshell 3 C. Proposed approach in the context of modern astronomy 7 D. Perceived benefits and perspectives 12 II. Phase I goals and accomplishments 18 A. Introducing the theoretical model 19 B. A Gaussian absorber 28 C. Unbalanced arms configuration 32 D. Phase I summary 34 III. Phase II goals and accomplishments 37 A. Advanced theoretical analysis 38 B. On observability of a shadow gradient 47 C. Signal-to-noise ratio 49 D. From detection to imaging 59 E. Experimental demonstration 72 F. On observation of phase objects 86 IV. Dissemination and outreach 90 V. Conclusion 92 References 95 1 I. THE PROPOSED RESEARCH The NIAC Ghost Imaging of Space Objects research program has been carried out at the Jet Propulsion Laboratory, Caltech. The program consisted of Phase I (October 2011 to September 2012) and Phase II (October 2012 to September 2014). The research team consisted of Drs. Dmitry Strekalov (PI), Baris Erkmen, Igor Kulikov and Nan Yu. The team members acknowledge stimulating discussions with Drs. Leonidas Moustakas, Andrew Shapiro-Scharlotta, Victor Vilnrotter, Michael Werner and Paul Goldsmith of JPL; Maria Chekhova and Timur Iskhakov of Max Plank Institute for Physics of Light, Erlangen; Paul Nu˜nez of Coll`ege de France & Observatoire de la Cˆote d’Azur; and technical support from Victor White and Pierre Echternach of JPL. -
Arxiv:2103.07476V1 [Astro-Ph.GA] 12 Mar 2021
FERMILAB-PUB-21-075-AE-LDRD Draft version September 3, 2021 Typeset using LATEX twocolumn style in AASTeX63 The DECam Local Volume Exploration Survey: Overview and First Data Release A. Drlica-Wagner ,1, 2, 3 J. L. Carlin ,4 D. L. Nidever ,5, 6 P. S. Ferguson ,7, 8 N. Kuropatkin ,1 M. Adamow´ ,9, 10 W. Cerny ,2, 3 Y. Choi ,11 J. H. Esteves,12 C. E. Mart´ınez-Vazquez´ ,13 S. Mau ,14, 15 A. E. Miller,16, 17 B. Mutlu-Pakdil ,2, 3 E. H. Neilsen ,1 K. A. G. Olsen ,6 A. B. Pace ,18 A. H. Riley ,7, 8 J. D. Sakowska ,19 D. J. Sand ,20 L. Santana-Silva ,21 E. J. Tollerud ,11 D. L. Tucker ,1 A. K. Vivas ,13 E. Zaborowski,2 A. Zenteno ,13 T. M. C. Abbott ,13 S. Allam ,1 K. Bechtol ,22, 23 C. P. M. Bell ,16 E. F. Bell ,24 P. Bilaji,2, 3 C. R. Bom ,25 J. A. Carballo-Bello ,26 D. Crnojevic´ ,27 M.-R. L. Cioni ,16 A. Diaz-Ocampo,28 T. J. L. de Boer ,29 D. Erkal ,19 R. A. Gruendl ,30, 31 D. Hernandez-Lang,32, 13, 33 A. K. Hughes,20 D. J. James ,34 L. C. Johnson ,35 T. S. Li ,36, 37, 38 Y.-Y. Mao ,39, 38 D. Mart´ınez-Delgado ,40 P. Massana,19, 41 M. McNanna ,22 R. Morgan ,22 E. O. Nadler ,14, 15 N. E. D. Noel¨ ,19 A. Palmese ,1, 2 A. H. G. Peter ,42 E. S. -
Building a Popular Science Library Collection for High School to Adult Learners: ISSUES and RECOMMENDED RESOURCES
Building a Popular Science Library Collection for High School to Adult Learners: ISSUES AND RECOMMENDED RESOURCES Gregg Sapp GREENWOOD PRESS BUILDING A POPULAR SCIENCE LIBRARY COLLECTION FOR HIGH SCHOOL TO ADULT LEARNERS Building a Popular Science Library Collection for High School to Adult Learners ISSUES AND RECOMMENDED RESOURCES Gregg Sapp GREENWOOD PRESS Westport, Connecticut • London Library of Congress Cataloging-in-Publication Data Sapp, Gregg. Building a popular science library collection for high school to adult learners : issues and recommended resources / Gregg Sapp. p. cm. Includes bibliographical references and index. ISBN 0–313–28936–0 1. Libraries—United States—Special collections—Science. I. Title. Z688.S3S27 1995 025.2'75—dc20 94–46939 British Library Cataloguing in Publication Data is available. Copyright ᭧ 1995 by Gregg Sapp All rights reserved. No portion of this book may be reproduced, by any process or technique, without the express written consent of the publisher. Library of Congress Catalog Card Number: 94–46939 ISBN: 0–313–28936–0 First published in 1995 Greenwood Press, 88 Post Road West, Westport, CT 06881 An imprint of Greenwood Publishing Group, Inc. Printed in the United States of America TM The paper used in this book complies with the Permanent Paper Standard issued by the National Information Standards Organization (Z39.48–1984). 10987654321 To Kelsey and Keegan, with love, I hope that you never stop learning. Contents Preface ix Part I: Scientific Information, Popular Science, and Lifelong Learning 1 -
April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86. -
FY13 High-Level Deliverables
National Optical Astronomy Observatory Fiscal Year Annual Report for FY 2013 (1 October 2012 – 30 September 2013) Submitted to the National Science Foundation Pursuant to Cooperative Support Agreement No. AST-0950945 13 December 2013 Revised 18 September 2014 Contents NOAO MISSION PROFILE .................................................................................................... 1 1 EXECUTIVE SUMMARY ................................................................................................ 2 2 NOAO ACCOMPLISHMENTS ....................................................................................... 4 2.1 Achievements ..................................................................................................... 4 2.2 Status of Vision and Goals ................................................................................. 5 2.2.1 Status of FY13 High-Level Deliverables ............................................ 5 2.2.2 FY13 Planned vs. Actual Spending and Revenues .............................. 8 2.3 Challenges and Their Impacts ............................................................................ 9 3 SCIENTIFIC ACTIVITIES AND FINDINGS .............................................................. 11 3.1 Cerro Tololo Inter-American Observatory ....................................................... 11 3.2 Kitt Peak National Observatory ....................................................................... 14 3.3 Gemini Observatory ........................................................................................ -
Measuring Inflation with CLASS
Measuring Inflation with CLASS by Dominik Gothe A dissertation submitted to Johns Hopkins University in conformity with the requirements for the degree of Doctor of Philosophy. July 2015 Baltimore, Maryland c Dominik Gothe All rights reserved Abstract Using the Cosmology Large Angular Scale Surveyor (CLASS), we will measure the po- larization of the Cosmic Microwave Background (CMB) to constrain inflationary theory. The gravitational waves generated during the inflationary epoch imprinted specific polar- ization patterns – quantifiable by tensor-to-scalar ratio r – onto the CMB, which CLASS is designed to detect. Furthermore, we will be able to make assertions about the energy scale during inflation by discovering the features of the polarization power spectrum, providing a probe into physics of energy scales not conceivable in particle-accelerator physics. CLASS is a unique ground based experiment with extensive consideration given to mitigating sys- tematic uncertainties. A brief introduction into inflationary cosmology and review of current scientific results will be presented in the light of the upcoming measurements with the newly built CLASS de- tector. I will detail some of my technical contribution to the construction of this telescope. I have conducted my research under the advise of Prof. Bennett. Additionally the thesis was reviewed by Prof. Marriage, Prof. Kamionkowski, Prof. Chuss, and Prof. Strobel. ii Acknowledgments I would like to thank my wife, friends, members of the Johns Hopkins community, my mentors, teachers, supervisors, and dissertation committee. The CLASS project receives support from the National Science Foundation Division of Astronomical Sciences under Grant Numbers 0959349 and 1429236. iii Contents I Physics of the Origin of the Universe 1 1 Introduction to the Big Bang Framework . -
The EBEX Balloon Borne Experiment-Optics, Receiver, and Polarimetry
The EBEX Balloon Borne Experiment - Optics, Receiver, and Polarimetry The EBEX Collaboration: Asad M. Aboobaker1, Peter Ade2, Derek Araujo3, Fran¸cois Aubin4, Carlo Baccigalupi5;6, Chaoyun Bao4, Daniel Chapman3, Joy Didier3, Matt Dobbs7;8, Christopher Geach4, Will Grainger9, Shaul Hanany4;∗, Kyle Helson10, Seth Hillbrand3, Johannes Hubmayr11, Andrew Jaffe12, Bradley Johnson3, Terry Jones4, Jeff Klein4, Andrei Korotkov10, Adrian Lee13, Lorne Levinson14, Michele Limon3, Kevin MacDermid7, Tomotake Matsumura4;15, Amber D. Miller3, Michael Milligan4, Kate Raach4, Britt Reichborn-Kjennerud3, Ilan Sagiv14, Giorgio Savini16, Locke Spencer2;17, Carole Tucker2, Gregory S. Tucker10, Benjamin Westbrook11, Karl Young4, Kyle Zilic4 ABSTRACT The E and B Experiment (EBEX) was a long-duration balloon-borne cosmic mi- crowave background polarimeter that flew over Antarctica in 2013. We describe the experiment's optical system, receiver, and polarimetric approach, and report on their in-flight performance. EBEX had three frequency bands centered on 150, 250, and 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 2School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom 3Physics Department, Columbia University, New York, NY 10027 4University of Minnesota School of Physics and Astronomy, Minneapolis, MN 55455 5Astrophysics Sector, SISSA, Trieste, 34014, Italy 6INFN, Sezione di Trieste, Via Valerio 2, I-34127 Trieste, Italy 7McGill University, Montreal, Quebec, H3A 2T8, Canada 8Canadian Institute for -
How Slaves Used Northern Seaports' Maritime Industry to Escape And
Eastern Illinois University The Keep Faculty Research & Creative Activity History May 2008 Ports of Slavery, Ports of Freedom: How Slaves Used Northern Seaports’ Maritime Industry To Escape and Create Trans-Atlantic Identities, 1713-1783 Charles Foy Eastern Illinois University, [email protected] Follow this and additional works at: http://thekeep.eiu.edu/history_fac Part of the United States History Commons Recommended Citation Foy, Charles, "Ports of Slavery, Ports of Freedom: How Slaves Used Northern Seaports’ Maritime Industry To Escape and Create Trans-Atlantic Identities, 1713-1783" (2008). Faculty Research & Creative Activity. 7. http://thekeep.eiu.edu/history_fac/7 This Article is brought to you for free and open access by the History at The Keep. It has been accepted for inclusion in Faculty Research & Creative Activity by an authorized administrator of The Keep. For more information, please contact [email protected]. © Charles R. Foy 2008 All rights reserved PORTS OF SLAVERY, PORTS OF FREEDOM: HOW SLAVES USED NORTHERN SEAPORTS’ MARITIME INDUSTRY TO ESCAPE AND CREATE TRANS-ATLANTIC IDENTITIES, 1713-1783 By Charles R. Foy A dissertation submitted to the Graduate School-New Brunswick Rutgers, The State University of New Jersey in partial fulfillment of the requirements for the Degree of Doctor of Philosophy Graduate Program in History written under the direction of Dr. Jan Ellen Lewis and approved by ______________________ ______________________ ______________________ ______________________ ______________________ New Brunswick, New Jersey May, 2008 ABSTRACT OF THE DISSERTATION PORTS OF SLAVERY, PORTS OF FREEDOM: HOW SLAVES USED NORTHERN SEAPORTS’ MARITIME INDUSTRY TO ESCAPE AND CREATE TRANS-ATLANTIC IDENTIES, 1713-1783 By Charles R. Foy This dissertAtion exAmines and reconstructs the lives of fugitive slAves who used the mAritime industries in New York, PhilAdelphiA and Newport to achieve freedom.