2017 Annual Report Vision
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Michael Garcia Hubble Space Telescope Users Committee (STUC)
Hubble Space Telescope Users Committee (STUC) April 16, 2015 Michael Garcia HST Program Scientist [email protected] 1 Hubble Sees Supernova Split into Four Images by Cosmic Lens 2 NASA’s Hubble Observations suggest Underground Ocean on Jupiter’s Largest Moon Ganymede file:///Users/ file:///Users/ mrgarci2/Desktop/mrgarci2/Desktop/ hs-2015-09-a-hs-2015-09-a- web.jpg web.jpg 3 NASA’s Hubble detects Distortion of Circumstellar Disk by a Planet 4 The Exoplanet Travel Bureau 5 TESS Transiting Exoplanet Survey Satellite CURRENT STATUS: • Downselected April 2013. • Major partners: - PI and science lead: MIT - Project management: NASA GSFC - Instrument: Lincoln Laboratory - Spacecraft: Orbital Science Corp • Agency launch readiness date NLT June 2018 (working launch date August 2017). • High-Earth elliptical orbit (17 x 58.7 Earth radii). Standard Explorer (EX) Mission PI: G. Ricker (MIT) • Development progressing on plan. Mission: All-Sky photometric exoplanet - Systems Requirement Review (SRR) mapping mission. successfully completed on February Science goal: Search for transiting 12-13, 2014. exoplanets around the nearby, bright stars. Instruments: Four wide field of view (24x24 - Preliminary Design Review (PDR) degrees) CCD cameras with overlapping successfully completed Sept 9-12, 2014. field of view operating in the Visible-IR - Confirmation Review, for approval to enter spectrum (0.6-1 micron). implementation phase, successfully Operations: 3-year science mission after completed October 31, 2014. launch. - Mission CDR on track for August 2015 6 JWST Hardware Progress JWST remains on track for an October 2018 launch within its replan budget guidelines 7 WFIRST / AFTA Widefield Infrared Survey Telescope with Astrophysics Focused Telescope Assets Coronagraph Technology Milestones Widefield Detector Technology Milestones 1 Shaped Pupil mask fabricated with reflectivity of 7/21/14 1 Produce, test, and analyze 2 candidate 7/31/14 -4 10 and 20 µm pixel size. -
A Search for Lorentz-Boosted Higgs Bosons Decaying to Charm Quarks in the CMS Experiment Using Deep Neural Networks
University of California Santa Barbara A search for Lorentz-boosted Higgs bosons decaying to charm quarks in the CMS experiment using deep neural networks A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in Physics by Huilin Qu CERN-THESIS-2019-165 Committee in charge: Professor Joseph Incandela, Chair Associate Professor Nathaniel Craig Professor Jeffrey Richman September 2019 The Dissertation of Huilin Qu is approved. Associate Professor Nathaniel Craig Professor Jeffrey Richman Professor Joseph Incandela, Committee Chair September 2019 A search for Lorentz-boosted Higgs bosons decaying to charm quarks in the CMS experiment using deep neural networks Copyright © 2019 by Huilin Qu iii Acknowledgements The pursuit of my Ph.D. in particle physics is a long journey with many ups and downs. I am grateful to so many people who showed up along this way, influenced me greatly with their knowledge and character, and provided me with invaluable help and support. I apologize I cannot name every one of them here – the list is too long. But I have my sincere gratitude to all of them deep in my heart. First of all, I would like to express my deepest gratitude to my research advisor, Prof. Joseph Incandela, for being always so supportive and inspiring, for allowing a lot of freedom in my research, and for providing me with countless valuable suggestions not only about my research but also on how to grow as a scientist. Talking with him is like magic – his words are so inspiring, and can always clear up my doubts and leave me motivated. -
Dancing to the Tempo of LEP
INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERN COURIER VOLUME 40 NUMBER 10 DECEMBER 2000 Dancing to the tempo of LEP SPIN SUPERSYMMETRY INTERNET Polarized protons accelerated Striking suggestions for How the Web was Born, a new in new RHIC ring p8 additional physics symmetry pl7 book p43 E RI Hew Gêner CES Creative Electronic Systems 70 route du Hunt-dun*! CH-1213 Petit-Uncy, Switzerland Internet: nttp://www.ces.cft I The Ultimate VME Machine CES Switzeriand The RI03 features a twin bus architecture, a Tel: ^41.22.879.51.00 ifque fnter-processor communication mechanism Fax: +4U2.792.57.4d Email; [email protected] for ultra-high-speed data acquisitions g and user-level load balance control CES.O Germany with dedicated hardware. Tel: +49.60.51.96.97.41 Fax; +49.60,51.96.97.33 Sheer Speed: Êttuiil: [email protected] # • VME - block transfers in 2eSST at CES MSâ 300 MBytes/s, single cycles at 20 MBytes/s Tel:+ 1.518.843.1445 Fax;+1.518.643.1447 * Memory - 400 MBytes/s average, Email: [email protected] 800 MBytes/s peak • Multi-Access - VME + PCM + PCI 2 + CPU without global degradation CPU Power: PowerPC 750 or 7400 at maximum available speed I Flexible: Two Independent 64-bit PCI with simultaneous access to the memory I Scalable: Up to four additional PMC's on a PMC carrier system MFCC 844x PMC PROCESSORS • 130 KGates user-FPGA • Continuous acquisition at 50 MBytes/s In 32 or 64~bit mode • Full 750 / 7400 computing core • Full network services on PCI * Complete multi-processing software with connection oriented high-speed data transfers SOFTWARE SUPPORT VxWorics®, Lynxob®, muecat® and LINUX® development software including support for hard real-time target machines. -
James Webb Space Telescope… Smashingly Cold Pg 8
National Aeronautics and Space Administration view Volume 6 Issue 11 NASA’S Mars Atmosphere Mission Gets Green Light to Proceed to Development Pg 3 James Webb Space Telescope… Smashingly Cold Pg 8 i am goddard: Curtis Johnson goddard Pg 12 www.nasa.gov 02 NASA and OPTIMUS PRIME GoddardView Collaborate to Educate Youth Volume 6 Issue 11 By Rani Gran NASA has developed a contest to raise students’ awareness of technology transfer Table of Contents efforts and how NASA technologies contribute to our everyday lives. Goddard Updates NASA is collaborating with Hasbro using the correlation between the popular NASA and OPTIMUS PRIME Collaborate to Transformers brand, featuring its leader OPTIMUS PRIME, and spinoffs from NASA Educate Youth – 2 Updates technologies created for aeronautics and space missions that are used here on Earth. NASA’S Mars Atmosphere Mission Gets Green The goal is to help students understand that NASA technology ‘transforms’ into things Light to Proceed to Development – 3 that are used daily. These transformed technologies include water purifiers, medical Cluster Helps Disentangle Turbulence in the imaging software, or fabric that protects against UV rays. Solar Wind – 4 Mobile Mars Laboratory Almost Ready for Flight – 5 The Innovative Partnerships Program Office NASA Makes the Invisible Visible in Medical at Goddard, in conjunction with NASA’s Imaging – 6 Office of Education, has designed Two Goddard Fermi Telescope Scientists Win a video contest for students Lindsay Awards – 7 from third to eighth grade. James Webb Space Telescope…Smashingly Cold – 8 Each student, or group of Goddard Goddard Community students, will submit a Paid to Have Fun – 9 three- to five-minute video OutsideGoddard: Bluegrass Camp – 10 on a selected NASA spinoff i am goddard: Curtis Johnson – 12 technology listed in the 2009 Spinoff publica- tion. -
NASA Mission Directorates and Center Alignment Research Areas
Appendix A: NASA Mission Directorates and Center Alignment NASA’s Mission to pioneer the future in space exploration, scientific discovery, and aeronautics research, draws support from four Mission Directorates and nine NASA Centers plus JPL, each with a specific responsibility. A.1 Aeronautics Research Mission Directorate (ARMD) conducts high-quality, cutting-edge research that generates innovative concepts, tools, and technologies to enable revolutionary advances in our Nation’s future aircraft, as well as in the airspace in which they will fly. ARMD programs will facilitate a safer, more environmentally friendly, and more efficient national air transportation system. Using a Strategic Implementation Plan NASA Aeronautics Research Mission Directorate (ARMD) sets forth the vision for aeronautical research aimed at the next 25 years and beyond. It encompasses a broad range of technologies to meet future needs of the aviation community, the nation, and the world for safe, efficient, flexible, and environmentally sustainable air transportation. Additional information on the Aeronautics Research Mission Directorate (ARMD) can be found at: http://www.aeronautics.nasa.gov. Areas of Interest - POC: Tony Springer, [email protected] Researchers responding to the ARMD should propose research that is aligned with one or more of the ARMD programs. Proposers are directed to the following: • ARMD Programs: http://www.aeronautics.nasa.gov/programs.htm • The National Aeronautics and Space Administration (NASA), Headquarters, Aeronautics Research Mission Directorate (ARMD) Current Year version of the NASA Research Announcement (NRA) entitled, "Research Opportunities in Aeronautics (ROA)” has been posted on the NSPIRES web site at http://nspires.nasaprs.com (select “Solicitations” and then “Open Solicitations”). -
Language and Materiality Ethnographic and Theoretical Explorations
Language and Materiality Ethnographic and Theoretical Explorations Edited by Jillian R. Cavanaugh CUNY, New York Shalini Shankar Northwestern University University Printing House, Cambridge CB2 8BS, United Kingdom One Liberty Plaza, 20th Floor, New York, NY 10006, USA 477 Williamstown Road, Port Melbourne, VIC 3207, Australia 4843/24, 2nd Floor, Ansari Road, Daryaganj, Delhi - 110002, India 79 Anson Road, #06-04/06, Singapore 079906 Cambridge University Press is part of the University of Cambridge. It furthers the University’s mission by disseminating knowledge in the pursuit of education, learning, and research at the highest international levels of excellence. www.cambridge.org Information on this title: www.cambridge.org/9781107180949 DOI: 10.1017/9781316848418 C Cambridge University Press 2017 This publication is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. First published 2017 Printed in <country> by <printer> A catalogue record for this publication is available from the British Library. Library of Congress Cataloging-in-Publication Data ISBN 978-1-107-18094-9 Hardback Cambridge University Press has no responsibility for the persistence or accuracy of URLs for external or third-party internet websites referred to in this publication and does not guarantee that any content on such websites is, or will remain, accurate or appropriate. 4 Fontroversy! Or, How to Care about the Shape of Language Keith M. Murphy Introduction On July 4, 2012, standing in the well of a packed lecture hall on the cam- pus of the European Organization for Nuclear Research (CERN), just outside Geneva, particle physicist Joseph Incandela looked up at the hall’s projection screen and, with only a hint of nerves in his voice, uttered the following pro- nouncement: “If we combine the ZZ and gamma-gamma, this is what we get. -
HEIC1117: EMBARGOED UNTIL 15:00 CET/09:00 Am EST 10 Nov, 2011
HEIC1117: EMBARGOED UNTIL 15:00 CET/09:00 am EST 10 Nov, 2011 http://www.spacetelescope.org/news/heic1117/ Science release: Hubble Uncovers Tiny Galaxies Bursting with Starbirth in Early Universe 10-Nov 2011 Using its infrared vision to peer nine billion years back in time, the NASA/ESA Hubble Space Telescope has uncovered an extraordinary population of tiny, young galaxies that are brimming with star formation. The galaxies are churning out stars at such a rate that the number of stars in them would double in just ten million years. For comparison, the Milky Way has taken a thousand times longer to double its stellar population. These newly discovered dwarf galaxies are around a hundred times smaller than the Milky Way. Their star formation rates are extremely high, even for the young Universe, when most galaxies were forming stars at higher rates than they are today. They have turned up in the Hubble images because the radiation from young, hot stars has caused the oxygen in the gas surrounding them to light up like a fluorescent sign. Astronomers believe this rapid starbirth represents an important phase in the formation of dwarf galaxies, the most common galaxy type in the cosmos. “The galaxies have been there all along, but up until recently astronomers have been able only to survey tiny patches of sky at the sensitivities necessary to detect them,” says Arjen van der Wel of the Max Planck Institute for Astronomy in Heidelberg, Germany, lead author of a paper that will appear in a forthcoming issue of the Astrophysical Journal. -
Request for Proposals
Request for Proposals Kansas NASA EPSCoR Program Partnership Development Grant (PDG) NASA in Kansas Proposal Due: Noon, October 31, 2019 Anticipated Grant End Date: June 30, 2020 With support from NASA and the Kansas Board of Regents - the Kansas NASA EPSCoR Program (KNEP) is preparing to award Partnership Development Grants (PDG) to Kansas investigators, under the KNEP Research Infrastructure Development (RID) program. These grants are intended to facilitate the development of beneficial and promising NASA collaborations. The PDG recipient is expected to initiate, develop, and formalize a meaningful professional relationship with a NASA researcher. Given this expectation, it is vital investigators and students travel to a NASA center if selected for an award. Ideally the faculty member, student, and research host become co-participants in a promising research effort. Indeed, the PDG award should lead to sustained collaborations, joint publications, and, most importantly, future grant proposals. Award Criteria PDG awards are competitive, with a strong emphasis on: § Addressing NASA Mission Directorate and Kansas interests (required) § Developing new, sustained, and meaningful NASA contacts (required) § Involving US-students, especially underrepresented and underserved Kansas undergraduate and graduate students, in the research (required) § Strengthening collaboration among academia, government agencies, business, and industry § Exploring new and unique R&D opportunities § Shared publications and future EPSCoR and non-EPSCoR grant submissions -
Connecting Scientists with NASA Astrophysics
219th AAS Meeting – Austin, TX “Connecting Scientists with NASA Astrophysics Education and Public Outreach” Splinter Meeting January 12, 2012, 9:30AM-11:00AM Facilitators: NASA Astrophysics Science E/PO Forum Text of Presentation Slides Slide 1: Splinter Meeting Plan • Introduction, Who we are, Why we are here • Showcase of NASA Astrophysics E/PO resources and opportunities • Explore resources and opportunities, one-on-one Slide 2: Who We Are: NASA Science E/PO Forums Presenter: Mangala Sharma (msharma[at]stsci.edu) URL: Smdepo.org The 4 SMD E/PO Forums connect scientists with E/PO information, resources, opportunities, potential partners related to NASA SMD E/PO. Slide 3: Who We Are (2): NASA SMD E/PO • Part of NASA’s education effort, supports Agency education goals • SMD’s vision for E/PO: To share the story, the science, and the adventure of NASA’s scientific explorations… through stimulating and informative activities and experiences… • Scientists + educators working together! Slide 4: Why We Are Here Presenter: Mangala Sharma URL: Smdepo.org • To connect scientists, NASA Astrophysics E/PO teams and SMD E/PO program officers • Explore and collect NASA Astrophysics E/PO resources you can use in your own E/PO • Discover how to participate in current and future SMD E/PO opportunities • Connect with other scientists interested in E/PO Slide 5: NASA SMD E/PO Grant Opportunities Presenter: James Lochner (James.C.Lochner[at]nasa.gov) URL: http://tinyurl.com/smd-epo-guides EPOESS: 1 to 4 year grants for projects in Formal and Informal Education, Higher Education, and Outreach. • No funding limit, but previous awards ~ $100K-$200K in first year. -
2016 Faculty Research Lecture Flyer
THE 61ST ANNUAL FACULTY RESEARCH LECTURE Joseph Incandela Searching for the Genetic Code of our Universe Monday, October 17, 2016 / FREE 4:00 PM Reception/ 5:00 PM Lecture Corwin Pavilion University Center The 2012 discovery of the Higgs boson at the CERN LHC accelerator complex completes a powerful and comprehensive description of nature known as the standard model of particle physics. The next step is to find the new physics that underpins this model, which many physicists believe could solve mysteries first seen in astrophysical and cosmological data, such as dark matter and neutrino mixing. Professor Incandela will give a general overview of where things stand and what's being planned, including his own research plans to address these very fundamental questions about the universe. Joseph Incandela received his PhD from the University of Chicago under Professor Henry Frisch in 1986 for a search for magnetic monopoles using superconducting coils whose currents were measured by Superconducting Quantum Interference Devices. Awarded a CERN Fellowship in 1987, he joined the UA2 experiment at CERN and was a leading contributor to the first precision measurement of the mass of the Z boson. He then proposed and led the first search at a hadron collider for a Higgs boson using hadronic tau decay final states. He joined the CDF experiment as a Wilson Fellow at Fermilab in 1991 where he led silicon detector projects and also led the search for top quarks that provided the most significant contribution to the discovery of the top quark in 1995. With regard to the LHC, he created the US CMS Silicon tracker project in 1997 that eventually constructed and tested ~60% (by area) of the silicon strip tracking system. -
Women of Goddard: Careers in Science, Technology, Engineering, and Mathematics
Women of Goddard: Careers in Science, Technology, Engineering, and Mathematics Engineering, Technology, Careers in Science, of Goddard: Women National Aeronautics and Space Administration Goddard of Parkinson, Millar, Thaller Millar, Parkinson, Careers in Science Technology Engineering & Mathematics Women www.nasa.gov Women of Goddard NASA’s Goddard Space Flight Center IV&V, WV Goddard Institute for Space Studies, Greenbelt, Maryland, Main Campus Wallops Flight Facility, Virginia New York City Testing and Integration Facility, Greenbelt Home of Super Computing and Data Storage, Greenbelt GSFC’s new Sciences and Exploration Building, Greenbelt Women of Goddard: Careers in Science, Technology, Engineering, and Mathematics Editors: Claire L. Parkinson, Pamela S. Millar, and Michelle Thaller Graphics and Layout: Jay S. Friedlander In Association with: The Maryland Women’s Heritage Center (MWHC) NASA Goddard Space Flight Center, Greenbelt, Maryland, July 2011 Women of Goddard Careers in Foreword Science A century ago women in the United States could be schoolteachers and nurses but were largely excluded from the vast majority of other jobs that could Technology be classified as Science, Technology, Engineering, or Mathematics (STEM careers). Some inroads were fortuitously made during World Wars I and II, when because of Engineering the number of men engaged in fighting overseas it became essential that women fill in on jobs of all types on the home front. However, many of these inroads Mathematics were lost after the wars ended and the men -
HIGH ENERGY PHYSICS ADVISORY PANEL to the U.S. DEPARTMENT of ENERGY and NATIONAL SCIENCE FOUNDATION
HIGH ENERGY PHYSICS ADVISORY PANEL to the U.S. DEPARTMENT OF ENERGY and NATIONAL SCIENCE FOUNDATION PUBLIC MEETING MINUTES Hilton Washington DC North/Gaithersburg 620 Perry Parkway Gaithersburg, MD 20877 May 14-15, 2018 HIGH ENERGY PHYSICS ADVISORY PANEL 2 SUMMARY OF MEETING The U.S. Department of Energy (DOE) and National Science Foundation (NSF) High Energy Physics Advisory Panel (HEPAP) was convened at 8:48 a.m. ET on May14-15, 2018, at the Hilton Washington DC North/Gaithersburg, Gaithersburg, MD, by Panel Chair Andrew Lankford. The meeting was open to the public and conducted in accordance with Federal Advisory Committee Act (FACA) requirements. Attendees can visit http://science.energy.gov/hep/hepap for more information about HEPAP. Panel members present: JoAnne Hewett, Chair Kent Irwin Christopher Stubbs Janet Conrad Kay Kinoshita Michael Syphers Kyle Cranmer David Larbalestier Mark Trodden Rohini Godbole Donatella Lucchesi James Wells Jordan Goodman Fulvia Pilat Geralyn Zeller Salman Habib Thomas Roser Joseph Incandela Maria Spiropulu HEPAP Designated Federal Officer: John Boger, DOE, Office of Science (SC), Office of High Energy Physics (HEP), Research Technology, Detector Research & Development (R&D), Director Others present for all or part of the meeting: David Asner, Brookhaven National Michael Cooke, DOE Laboratory (BNL) Jean Cottam, NSF Tali Bar-Shalom, Office of Management and Glen Crawford, DOE Budget Patricia Crumley, DOE Rich Barvainis, NSF Paul Dabbar, DOE Lothar Bauerdick, Fermi National Kyle Dawson, University of Utah Accelerator Laboratory (Fermilab) Marcel Demarteau, Argonne National Doug Benjamin, Duke University Laboratory (ANL) Steve Binkley, DOE Richard Dubois, National Aeronautics and Kevin Black, Boston University Space Administration (NASA) Ken Bloom, University of Nebraska Allison Eckhardt, DOE Greg Bock, Fermilab James Fast, PNNL Joel Butler, Fermilab Laura Fields, Fermilab C.