Refueling the Magic Furnace: Kilonova 2017 Rewrites the Story of Element Origins
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IMRE BARTOS Associate Professor of Physics | University of Florida | People.Clas.Ufl.Edu/Imrebartos
IMRE BARTOS Associate Professor of Physics | University of Florida | people.clas.ufl.edu/imrebartos RESEARCH INTEREST Gravitational wave astrophysics, multi-messenger astrophysics, high-energy astroparticle physics, black hole and neutron star evolution and interactions, cosmology. EDUCATION AND TRAINING Columbia University Physics (Szabolcs Marka) PhD 2012 Eotvos University, Hungary Physics Diploma 2006 PROFESSIONAL APPOINTMENTS Associate Professor University of Florida 2021—present Assistant Professor University of Florida 2017—2021 Associate Research Scientist Columbia University 2016—2017 Lecturer in Discipline Columbia University 2012—2016 HONORS AND AWARDS Alfred P. Sloan Foundation Research Fellowship 2020—2022 Excellence Award for Assistant Professors, University of Florida 2020 Columbia Science Fellow, Columbia University 2012—2016 Allan M. Sachs Teaching Award 2011 Columbia Presidential Teaching Award, Finalist 2012 National Science Foundation Highlights 2014 AAS Nova Highlight 2016 5 Favorite Features of the year, Physics World 2018 Brookhaven National Lab Distinguished Lecture 2016 Rising Stars of Science: The Forbes 30 Under 30 (Forbes Magazine) 2012 Summer Undergraduate Research Fellowship, Caltech 2004 As a member of the LIGO Scientific Collaboration: Special Breakthrough Prize in Fundamental Physics 2016 Gruber Cosmology Prize 2016 Princess of Asturias Award for Technical and Scientific Research 2017 Einstein Medal from the Einstein Society in Bern, Switzerland 2017 Bruno Rossi Prize 2017 Science’s Breakthrough of the -
Kyung Ha Lee
Kyung Ha Lee Phone: +82-31-290-7042, Email: [email protected] Academic Activities Sungkyunkwan University, Department of Physics, Suwon, South Korea Assistant Professor Sep. 2020 – Present Relevant Area of Science: Gravitational Wave Research (LIGO) Stanford University, Applied Physics, California, United States Postdoc in Applied Physics Feb. 2019 – Aug. 2020 Research Group: Ginzton Laboratory, Martin Fejer Group Relevant Area of Science: Gravitational Wave Research (LIGO) University of Glasgow, School of Physics and Astronomy, Glasgow, United Kingdom Ph.D. in Physics Oct. 2014 – Jan. 2019 Research Group: Institute for Gravitational Research (IGR) Relevant Area of Science: Gravitational Wave Research (LIGO) Seoul National University, School of Physics and Astronomy, Seoul, South Korea Researcher Jun. 2012 – May. 2013 Research Group: RENO Collaboration Relevant Area of Science: Neutrino Oscillation Experiment California Institute of Technology (Caltech), Department of Physics, Pasadena, CA. USA B.S. in Physics with Honor Oct. 2007 – Jun. 2011 Relevant Area of Science: Gravitational Wave Research (LIGO) Awards and Scholarship - Scottish Universities Physics Alliance (SUPA) Prize Studentship (2014) o This studentship is for 3.5 years and provides annual maintenance allowance, annual RTSG (Research Training Support Grant), and full cost of university tuition fees. - Thomson Experimental Prize (2017) o This prize was founded in 1869 by William Thomson later created 1st Baron Kelvin. It is awarded on the recommendation of the Professor of Natural -
Ira Sprague Bowen Papers, 1940-1973
http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington. -
APS Far West Section 2018 Newsletter
APS Far West Section 2018 Newsletter Letter from the Chairs By Hendrik Ohldag, SLAC National Accelerator Laboratory (chair, picture) Andreas Bill, California State University Long Beach (past chair) Dear Fellow APS Member, The Far West Section (FWS) of the American Physical Society aims at bringing together physicists active in academia, industry and research institutions. We welcome all who have a background in, or a link to physics and wish to share their experience and knowledge, or simply wish to stay in touch with colleagues and the advances in the field. Most of our members live in California, Hawaii or Nevada, but the section is open to all who are APS members. Though all can be member of the FWS for free(!), not all are members. If you are an APS member and read these lines you should also be a section member. If not yet, just send a short email to [email protected] to express your interest in joining the Far West Section, or go online using your APS membership credentials (click on “Membership”). Please do so now, and read the rest of the letter after… Physics has undergone many changes in recent years and those in our Far West Section region have played a major role in shaping the physics landscape. Not only have we advanced knowledge in key areas of fundamental research, teaching and industry, but some of our members have also contributed in important ways to the APS itself. The fact that physics has changed so much also means that many more job opportunities are available to physics students. -
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. -
New Contract Award
TRI-Supported Trial Named Science Magazine’s 2011 “Breakthrough of the Year” Bethesda, Maryland (May 18, 2012): Technical Resources International, Inc. (TRI) is proud to have provided regulatory, safety, and technical support to the Division of AIDS (DAIDS), National Institute of Allergy and Infectious Diseases (NIAID), NIH for the HIV clinical trial that was chosen as the 2011 Breakthrough of the Year by Science Magazine. The NIAID-sponsored HPTN 052 study was an international HIV prevention trial conducted in nine countries. Investigators conducting the study reported that HIV-infected heterosexual individuals who began taking antiretroviral medicines when their immune systems were relatively healthy were 96 percent less likely to transmit the virus to their uninfected partners. Federal officials and the medical community are advocating a ‘treatment-as-prevention’ approach be included as a key component of public health policies due in large part to the results of HPTN 052. They also indicate these findings will have positive implications in domestic and public health in the coming years and even suggest that achieving an end to the HIV/AIDS pandemic is now feasible. About NIAID: NIAID is working to end the HIV/AIDS epidemic by advancing basic knowledge of the pathogenesis and transmission of HIV, supporting the improvement of therapies for HIV infection and its complications, and supporting the development of HIV/AIDS vaccines and other prevention measures. NIAID sponsors Phase I, II, III and IV clinical trials to assess the safety and efficacy of therapeutics, vaccines, and other preventive modalities. Currently, NIAID funds more than 300 HIV/AIDS clinical trials in more than 50 countries at more than 1,000 domestic and international clinical research sites. -
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. -
Page 1 of 6 Science/AAAS | Table of Contents: 18 December 2009; 326
Science/AAAS | Table of Contents: 18 December 2009; 326 (5960) Page 1 of 6 Enter Search Term ADVANCED AAAS.ORG FEEDBACK HELP LIBRARIANS Science Magazine NATIONAL SCIENCE AND TECHNOLOGY DEVELOPMENT AGENCY ALERTS | ACCESS RIGHTS | MY ACCOUNT | SIGN IN Science Home Current Issue Previous Issues Science Express Science Products My Science About the Journal Home > Science Magazine > Issue Archive > 2009 > 18 December 2009 ADVERTISEMENT 18 DECEMBER 2009 VOL 326, ISSUE 5960, PAGES 1577-1744 Special Issue Letters Brevia This Week in Science Books et al. Research Articles Editorial Education Forum Reports Editors' Choice Perspectives News of the Week Association Affairs News Focus Front and Back Matter from the Print Issue [PDF] About the Cover ADVERTISEMENT Author Index Subject Index Set E-Mail Alerts Order an Issue/Article RSS Feeds Search the Journal Issue Highlights Enter Keyword 2009 Breakthrough of the Year Silent Hate This issue only Universal Few-Body Binding Home is Where the Hearth Is Special Issue For all checked items Breakthrough of the Year Video: Ardipithecus ramidus Science 18 December 2009: 1598. A video introduction to the year's top science story, featuring scientists C. Owen Lovejoy, Tim White, Giday WoldeGabriel, Yohannes Haile-Selassie, Science contributing correspondent Ann Gibbons, and commentary by paleoanthropologist Andrew Hill. Summary » Full Text » News BREAKTHROUGH OF THE YEAR Ardipithecus ramidus Ann Gibbons Science 18 December 2009: 1598-1599. A rare 4.4-million-year-old skeleton has drawn back the curtain of time to reveal the surprising body plan and ecology of our earliest ancestors. Summary » Full Text » PDF » BREAKTHROUGH OF THE YEAR The Runners-Up The News Staff Science 18 December 2009: 1600-1607. -
Professor Margaret Burbidge Obituary Trailblazing Astronomer Hailed As ‘Lady Stardust’ Who Became the First Woman Director of the Royal Greenwich Observatory
OBITUARY Professor Margaret Burbidge obituary Trailblazing astronomer hailed as ‘Lady Stardust’ who became the first woman director of the Royal Greenwich Observatory Wednesday April 08 2020, 12.01am, The Times Margaret Burbidge showed how heavier elements are produced from lighter ones in stars AMERICAN INSTITUTE OF PHYSICS/SCIENCE PHOTO LIBRARY In August 1944 Margaret Burbidge, then a young astronomer driven by a thirst for knowledge that would later define her, was studying for her PhD thesis. Her subject was a star called Gamma Cassiopeiae and she was not going to allow the Second World War to stand in her way. Each evening she would travel from the family home close to Hampstead Heath to the University of London Observatory at Mill Hill Park and open up the telescope named after its donor, JG Wilson. She would then spend hours sitting in the cramped and cold space below it, alone with her view of the stars. At that time the Luftwaffe was sending doodlebug flying bombs across the Channel to terrorise the capital but Burbidge ignored the danger. On the night of August 3, her log notes that shortly before 10pm, just after she had opened up the telescope, a flying bomb exploded so close to the observatory that the reverberations from the impact shifted the star out of the telescope’s field of vision. Undeterred she started her observations again a few minutes later only for another doodlebug to explode, this time farther away. Although the star was temporarily lost again she quickly recovered it and completed her observations. “Those nights, standing or sitting on the ladder in the dome of the Wilson reflector . -
Evaluating the Efficiency of Grnas in CRISPR/Cas9 Mediated Genome
International Journal of Molecular Sciences Article Evaluating the Efficiency of gRNAs in CRISPR/Cas9 Mediated Genome Editing in Poplars Tobias Bruegmann * , Khira Deecke and Matthias Fladung * Thuenen Institute of Forest Genetics, Sieker Landstrasse 2, D-22927 Grosshansdorf, Germany * Correspondence: [email protected] (T.B.); matthias.fl[email protected] (M.F.) Received: 21 June 2019; Accepted: 21 July 2019; Published: 24 July 2019 Abstract: CRISPR/Cas9 has become one of the most promising techniques for genome editing in plants and works very well in poplars with an Agrobacterium-mediated transformation system. We selected twelve genes, including SOC1, FUL, and their paralogous genes, four NFP-like genes and TOZ19 for three different research topics. The gRNAs were designed for editing, and, together with a constitutively expressed Cas9 nuclease, transferred either into the poplar hybrid Populus canescens × or into P. tremula. The regenerated lines showed different types of editing and revealed several homozygous editing events which are of special interest in perennial species because of limited back-cross ability. Through a time series, we could show that despite the constitutive expression of the Cas9 nuclease, no secondary editing of the target region occurred. Thus, constitutive Cas9 expression does not seem to pose any risk to additional editing events. Based on various criteria, we obtained evidence for a relationship between the structure of gRNA and the efficiency of gene editing. In particular, the GC content, purine residues in the gRNA end, and the free accessibility of the seed region seemed to be highly important for genome editing in poplars. Based on our findings on nine different poplar genes, efficient gRNAs can be designed for future efficient editing applications in poplars. -
Nucleosynthesis
Nucleosynthesis Nucleosynthesis is the process that creates new atomic nuclei from pre-existing nucleons, primarily protons and neutrons. The first nuclei were formed about three minutes after the Big Bang, through the process called Big Bang nucleosynthesis. Seventeen minutes later the universe had cooled to a point at which these processes ended, so only the fastest and simplest reactions occurred, leaving our universe containing about 75% hydrogen, 24% helium, and traces of other elements such aslithium and the hydrogen isotope deuterium. The universe still has approximately the same composition today. Heavier nuclei were created from these, by several processes. Stars formed, and began to fuse light elements to heavier ones in their cores, giving off energy in the process, known as stellar nucleosynthesis. Fusion processes create many of the lighter elements up to and including iron and nickel, and these elements are ejected into space (the interstellar medium) when smaller stars shed their outer envelopes and become smaller stars known as white dwarfs. The remains of their ejected mass form theplanetary nebulae observable throughout our galaxy. Supernova nucleosynthesis within exploding stars by fusing carbon and oxygen is responsible for the abundances of elements between magnesium (atomic number 12) and nickel (atomic number 28).[1] Supernova nucleosynthesis is also thought to be responsible for the creation of rarer elements heavier than iron and nickel, in the last few seconds of a type II supernova event. The synthesis of these heavier elements absorbs energy (endothermic process) as they are created, from the energy produced during the supernova explosion. Some of those elements are created from the absorption of multiple neutrons (the r-process) in the period of a few seconds during the explosion. -
Rhodri Evans
Rhodri Evans The Cosmic Microwave Background How It Changed Our Understanding of the Universe Astronomers’ Universe More information about this series at http://www.springer.com/series/6960 Rhodri Evans The Cosmic Microwave Background How It Changed Our Understanding of the Universe 123 Rhodri Evans School of Physics & Astronomy Cardiff University Cardiff United Kingdom ISSN 1614-659X ISSN 2197-6651 (electronic) ISBN 978-3-319-09927-9 ISBN 978-3-319-09928-6 (eBook) DOI 10.1007/978-3-319-09928-6 Springer Cham Heidelberg New York Dordrecht London Library of Congress Control Number: : 2014957530 © Springer International Publishing Switzerland 2015 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. Exempted from this legal reservation are brief excerpts in connection with reviews or scholarly analysis or material supplied specifically for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work. Duplication of this publication or parts thereof is permitted only under the provisions of the Copyright Law of the Publisher’s location, in its current version, and permission for use must always be obtained from Springer. Permissions for use may be obtained through RightsLink at the Copyright Clearance Center. Violations are liable to prosecution under the respective Copyright Law.