Annual Report 2013
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Investigating the Unusual Spectroscopic Time-Evolution in SN 2012Fr∗
Draft version October 4, 2018 Typeset using LATEX default style in AASTeX62 Investigating the Unusual Spectroscopic Time-Evolution in SN 2012fr∗ Christopher Cain,1, 2, 3 E. Baron,2, 4, 5 M. M. Phillips,6 Carlos Contreras,7, 8 Chris Ashall,9 Maximilian D. Stritzinger,8 Christopher R. Burns,10 Anthony L. Piro,10 Eric Y. Hsiao,9, 7, 8 P. Hoeflich,9 Kevin Krisciunas,11 and Nicholas B. Suntzeff11 1Azusa Pacific University 901 E Alosta Ave, Azusa, California, 91702, USA 2University of Oklahoma 440 W. Brooks, Rm 100, Norman, Oklahoma, 73019, USA 3Department of Physics and Astronomy, University of California, Riverside, CA 92521, USA 4Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany 5Visiting Astronomer, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark. 6Las Campanas Observatory, Carnegie Observatories Casilla 601, La Serena, Chile 7Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena, Chile 8Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark. 9Department of Physics, Florida State University, Tallahassee, FL 32306, USA 10Observatories of the Carnegie Institution for Science, 813 Santa Barbara St., Pasadena, CA 91101, USA 11George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA (Received ; Revised ; Accepted ) Submitted to ApJ ABSTRACT The type Ia supernova (SN) 2012fr displayed an unusual combination of its Si II λλ5972, 6355 fea- tures. This includes the ratio of their pseudo equivalent widths, placing it at the border of the Shallow Silicon (SS) and Core Normal (CN) spectral subtype in the Branch diagram, while the Si IIλ6355 expansion velocities places it as a High-Velocity (HV) object in the Wang et al. -
Astro2020 Science White Paper
Astro2020 Science White Paper QUASAR MICROLENSING: REVOLUTIONIZING OUR UNDERSTANDING OF QUASAR STRUCTURE AND DYNAMICS Thematic Area: ☒ Galaxy Evolution Principal Author: Name: Leonidas A Moustakas Institution: Jet Propulsion Laboratory, California Institute of Technology Email: [email protected] Phone: 818-393-5095 Co-authors: Timo Anguita (Universidad Andres Bello), George Chartas (College of Charleston), Matthew Cornachione (US Naval Academy), Xinyu Dai (University of Oklahoma), Carina Fian (Instituto de Astrofísica de Canarias and Departamento de Astrofísica, Universidad de la Laguna), Jorge Jimenez-Vicente (Univ. de Granada), Kathleen Labrie (Gemini Observatory), Chelsea Macleod (Center for Astrophysics, Harvard University), Evencio Mediavilla (Instituto de Astrofísica de Canarias), Christopher W Morgan (US Naval Academy), Matthew O’Dowd (Lehman College, City University of New York), Geraint Lewis (University of Sydney), Chelsea MacLeod (Center for Astrophysics, Harvard-Smithsonian), Evencio Mediavilla, (Instituto de Astrofísica de Canarias), Veronica Motta (Universidad de Valparaiso), Anna Nierenberg (Jet Propulsion Laboratory), David Pooley (Trinity University), Karina Rojas (Ecole Polytechnique Fédérale de Lausanne and LSSTC Data Science Fellow), Dominique Sluse (STAR institute, University of Liège), Georgios Vernardos (University of Groningen), Rachel Webster (University of Melbourne), Suk Yee Yong (University of Melbourne) Abstract: Microlensing by stars within distant galaxies acting as strong gravitational lenses of multiply-imaged quasars, provides a unique and direct measurement of the internal structure of the lensed quasar on nano-arcsecond scales. The measurement relies on the temporal variation of high-magnification caustic crossings which vary on timescales of days to years. Multiwavelength observations provide information from distinct emission regions in the quasar. Through monitoring of these strong gravitational lenses, a full tomographic view can emerge with Astronomical-Unit scale resolution. -
Curriculum Vitae Avishay Gal-Yam
January 27, 2017 Curriculum Vitae Avishay Gal-Yam Personal Name: Avishay Gal-Yam Current address: Department of Particle Physics and Astrophysics, Weizmann Institute of Science, 76100 Rehovot, Israel. Telephones: home: 972-8-9464749, work: 972-8-9342063, Fax: 972-8-9344477 e-mail: [email protected] Born: March 15, 1970, Israel Family status: Married + 3 Citizenship: Israeli Education 1997-2003: Ph.D., School of Physics and Astronomy, Tel-Aviv University, Israel. Advisor: Prof. Dan Maoz 1994-1996: B.Sc., Magna Cum Laude, in Physics and Mathematics, Tel-Aviv University, Israel. (1989-1993: Military service.) Positions 2013- : Head, Physics Core Facilities Unit, Weizmann Institute of Science, Israel. 2012- : Associate Professor, Weizmann Institute of Science, Israel. 2008- : Head, Kraar Observatory Program, Weizmann Institute of Science, Israel. 2007- : Visiting Associate, California Institute of Technology. 2007-2012: Senior Scientist, Weizmann Institute of Science, Israel. 2006-2007: Postdoctoral Scholar, California Institute of Technology. 2003-2006: Hubble Postdoctoral Fellow, California Institute of Technology. 1996-2003: Physics and Mathematics Research and Teaching Assistant, Tel Aviv University. Honors and Awards 2012: Kimmel Award for Innovative Investigation. 2010: Krill Prize for Excellence in Scientific Research. 2010: Isreali Physical Society (IPS) Prize for a Young Physicist (shared with E. Nakar). 2010: German Federal Ministry of Education and Research (BMBF) ARCHES Prize. 2010: Levinson Physics Prize. 2008: The Peter and Patricia Gruber Award. 2007: European Union IRG Fellow. 2006: “Citt`adi Cefal`u"Prize. 2003: Hubble Fellow. 2002: Tel Aviv U. School of Physics and Astronomy award for outstanding achievements. 2000: Colton Fellow. 2000: Tel Aviv U. School of Physics and Astronomy research and teaching excellence award. -
JOHN NOVEMBRE, Phd
JOHN NOVEMBRE, PhD The University of Chicago Department of Human Genetics 920 E 58th Steet CLSC 421 Chicago, IL 60637 Email: [email protected] Webpage: http://jnpopgen.org/ Curriculum Vitae Formatted to Guidelines for UChicago Biological Sciences Division ACADEMIC APPOINTMENTS 2017- Professor, University of Chicago, Department of Human Genetics, Department of Ecology and Evolutionary Biology (secondary appointment) 2013-2017 Associate Professor, University of Chicago, Department of Human Genetics, Department of Ecology and Evolutionary Biology (secondary appointment) 2012-2013 Associate Professor, University of California–Los Angeles, Department of Ecology and Evolutionary Biology, Interdepartmental Program in Bioinformatics 2008-2012 Assistant Professor, University of California–Los Angeles, Department of Ecology and Evolutionary Biology, Interdepartmental Program in Bioinformatics Ph.D.-Granting Committee, Program, Institute, and Center Appointments 2013- Committee on Evolutionary Biology, University of Chicago 2013- Committee on Genetics, Genomics, and Systems Biology, University of Chicago 2008-2013 Indepartmental Program in Bioinformatics, UCLA 2012-2009 Center for Society and Genetics, UCLA ACADEMIC TRAINING 2006-2008 Postdoctoral training, Department of Human Genetics University of Chicago, Chicago, IL. Advisor: Matthew Stephens 2006 PhD, Integrative Biology, designated emphasis in Computational Biology/Genomics University of California-Berkeley, Berkeley, CA. Advisor: Montgomery Slatkin Dissertation title: Statistical methods -
SKA-Athena Synergy White Paper
SKA-Athena Synergy White Paper SKA-Athena Synergy Team July 2018. Edited by: Francisco J. Carrera and Silvia Martínez-Núñez on behalf of the Athena Community Office. Revisions provided by: Judith Croston, Andrew C. Fabian, Robert Laing, Didier Barret, Robert Braun, Kirpal Nandra Authorship Authors Rossella Cassano (INAF-Istituto di Radioastronomia, Italy). • Rob Fender (University of Oxford, United Kingdom). • Chiara Ferrari (Observatoire de la Côte d’Azur, France). • Andrea Merloni (Max-Planck Institute for Extraterrestrial Physics, Germany). • Contributors Takuya Akahori (Kagoshima University, Japan). • Hiroki Akamatsu (SRON Netherlands Institute for Space Research, The Netherlands). • Yago Ascasibar (Universidad Autónoma de Madrid, Spain). • David Ballantyne (Georgia Institute of Technology, United States). • Gianfranco Brunetti (INAF-Istituto di Radioastronomia, Italy) and Maxim Markevitch (NASA-Goddard • Space Flight Center, United States). Judith Croston (The Open University, United Kingdom). • Imma Donnarumma (Agenzia Spaziale Italiana, Italy) and E. M. Rossi (Leiden Observatory, The • Netherlands). Robert Ferdman (University of East Anglia, United Kingdom) on behalf of the SKA Pulsar Science • Working Group. Luigina Feretti (INAF-Istituto di Radioastronomia, Italy) and Federica Govoni (INAF Osservatorio • Astronomico,Italy). Jan Forbrich (University of Hertfordshire, United Kingdom). • Giancarlo Ghirlanda (INAF-Osservatorio Astronomico di Brera and University Milano Bicocca, Italy). • Adriano Ingallinera (INAF-Osservatorio Astrofisico di Catania, Italy). • Andrei Mesinger (Scuola Normale Superiore, Italy). • Vanessa Moss and Elaine Sadler (Sydney Institute for Astronomy/CAASTRO and University of Sydney, • Australia). Fabrizio Nicastro (Osservatorio Astronomico di Roma,Italy), Edvige Corbelli (INAF-Osservatorio As- • trofisico di Arcetri, Italy) and Luigi Piro (INAF, Istituto di Astrofisica e Planetologia Spaziali, Italy). Paolo Padovani (European Southern Observatory, Germany). • Francesca Panessa (INAF/Istituto di Astrofisica e Planetologia Spaziali, Italy). -
See Tony's Slides Here
Climate change the science & the lies Tony Eggleton Outline Some basic climate stuff – what the science says About trust and lies How to misinform 1. Attack the person 2. “It stands to reason” 3. Cherry pick or brush aside 4. Use lots of wrong numbers 5. Use the wrong data 6. Be important, be wrong, and say it anyway The pillars of climate science causes causes Global warming. • What is the evidence? • Land-based thermometers Boulia, Qld Of course one Met station is not enough, but 30,000 is C) 14.8 ° 14.6 14.4 14.2 14.0 13.8 13.6 Temperature rise ( rise Temperature 13.4 1880 1900 1920 1940 1960 1980 2000 2020 NASA Goddard Space Institute Don’t like scientists’ measurements? • What about oenologists? Date of maturity for grapes is getting earlier every year Mar 20 Mar 1 1930 2010 The Greenhouse Warm body radiates heat away and gets cold Add a blanket, reduce heat loss Thicker blanket, more heat trapped, now a hot dog We are warmed by the sun and radiate our warmth out into space sun earth . There is a lot of cold space out there to accept our radiated heat OK, so you can see - 23° C 14° C We have an atmosphere blanket, the moon does not Sun’s heat comes in 29% is reflected back into space That is known as Earth’s albedo. Compare Venus 90%, the moon 7%. Earth warms air, air radiates heat away 1.8 ppm 0.3 ppm Greenhouse gases and their part in keeping us warm 400 ppm = 0.04% 4%± Why has the Earth warmed over the past two centuries? Because we have added a lot of CO2 Are you sure? Perhaps it is just a coincidence! And what does a bit of warming do? Melts ice, mainly in the Arctic. -
Asymmetries in Sn 2014J Near Maximum Light Revealed Through Spectropolarimetry
ASYMMETRIES IN SN 2014J NEAR MAXIMUM LIGHT REVEALED THROUGH SPECTROPOLARIMETRY Item Type Article Authors Porter, Amber; Leising, Mark D.; Williams, G. Grant; Milne, P. A.; Smith, Paul; Smith, Nathan; Bilinski, Christopher; Hoffman, Jennifer L.; Huk, Leah; Leonard, Douglas C. Citation ASYMMETRIES IN SN 2014J NEAR MAXIMUM LIGHT REVEALED THROUGH SPECTROPOLARIMETRY 2016, 828 (1):24 The Astrophysical Journal DOI 10.3847/0004-637X/828/1/24 Publisher IOP PUBLISHING LTD Journal The Astrophysical Journal Rights © 2016. The American Astronomical Society. All rights reserved. Download date 27/09/2021 22:28:24 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/622057 The Astrophysical Journal, 828:24 (12pp), 2016 September 1 doi:10.3847/0004-637X/828/1/24 © 2016. The American Astronomical Society. All rights reserved. ASYMMETRIES IN SN 2014J NEAR MAXIMUM LIGHT REVEALED THROUGH SPECTROPOLARIMETRY Amber L. Porter1, Mark D. Leising1, G. Grant Williams2,3, Peter Milne2, Paul Smith2, Nathan Smith2, Christopher Bilinski2, Jennifer L. Hoffman4, Leah Huk4, and Douglas C. Leonard5 1 Department of Physics and Astronomy, Clemson University, 118 Kinard Laboratory, Clemson, SC 29634, USA; [email protected] 2 Steward Observatory, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA 3 MMT Observatory, P.O. Box 210065, University of Arizona, Tucson, AZ 85721-0065, USA 4 Department of Physics and Astronomy, University of Denver, 2112 East Wesley Avenue, Denver, CO 80208, USA 5 Department of Astronomy, San Diego State University, PA-210, 5500 Campanile Drive, San Diego, CA 92182-1221, USA Received 2016 February 14; revised 2016 May 11; accepted 2016 May 12; published 2016 August 24 ABSTRACT We present spectropolarimetric observations of the nearby Type Ia supernova SN 2014J in M82 over six epochs: +0, +7, +23, +51, +77, +109, and +111 days with respect to B-band maximum. -
Augmented Reality in Teaching Descriptive Geometry, Engineering and Computer Graphics – Systematic Review and Results of the Russian Teachers’ Experience
EURASIA Journal of Mathematics, Science and Technology Education, 2019, 15(12), em1816 ISSN:1305-8223 (online) OPEN ACCESS Research Paper https://doi.org/10.29333/ejmste/113503 Augmented Reality in Teaching Descriptive Geometry, Engineering and Computer Graphics – Systematic Review and Results of the Russian Teachers’ Experience Marianna V. Voronina 1, Zlata O. Tretyakova 1*, Ekaterina G. Krivonozhkina 2, Stanislav I. Buslaev 3, 3 Grigory G. Sidorenko 1 Saint-Petersburg Mining University, Saint Petersburg, RUSSIA 2 Kazan (Volga region) Federal University, Kazan, RUSSIA 3 Financial University under the Government of the Russian Federation, Moscow, RUSSIA Received 10 June 2019 ▪ Revised 25 September 2019 ▪ Accepted 14 October 2019 ABSTRACT The relevance and feasibility of this study are determined by the absence of serious, scientific research, as well as teaching materials, when it comes to the use of Augmented Reality (AR) in teaching students and future teachers Descriptive Geometry, Engineering and Computer Graphics (DGECG). The purpose of the study is to examine the current state of knowledge and practice of existing courses, which use the AR concept; to conduct a pedagogical experiment by teaching students how to create an information model of a building structure using the AR concept; to study the impact of the AR technology on students, lecturers, on the quality of students’ design works and project presentation. The research methods used were a set of various, complementing each other methods, which can be divided into two groups: 1) theoretical: analysis of the teachers’ and psychologists’ works on the point of the research, analysis of methodological and educational literature; empirical: observation, statement, pedagogical experiment. -
07037 Melbuni MUM AUG07 ART.Indd
Melbouru ne University Magazine AUGUST EDITION 2007 Noise: A loud and clear cinematic success story for Matthew Saville Medical tourism: First world medicine at third world prices? Climate change: Can we get it right? Analysis: David Hicks’ guilty plea, what it really means Review Noise: An Australian Medical tourism film of striking 04 06 power 08 Melbourne University Magazine 2 0 07, Editorial Board August Edition Sean Cubitt – Director Media and Melbourne University Magazine is a publication Communications Program for alumni and friends of the University of Faculty of Arts (Chair) Melbourne. All correspondence relating to Silvia Dropulich – Writer & Editor, Marketing the editorial content of the magazine should & Communications (Editor/Managing Editor) be addressed to: Campbell Bairstow – General Manager, The Editor: Silvia Dropulich Alumni Relations, Advancement Melbourne University Magazine, Marketing and Communications, Dr Elizabeth Presa – Head and Academic The University of Melbourne, Coordinator, Centre for Ideas, VCA Victoria 3010 Dr Philip Batterham – Associate Professor Phone: +61 3 8344 7999 and Reader, Bio21 Institute of Molecular Fax: +61 3 8344 4921 Science and Biotechnology Email: [email protected] Dr Douglas Parbery – Committee of Cover: From the movie Noise, image supplied Convocation courtesy of Madman Cinema Change of address: Yee Fui Ng – International Law Alumna If you would like to be added to the Views expressed by contributors are not Melbourne University Magazine mailing list, or necessarily endorsed by -
The Center for Nanotechnology in Society at Arizona State University
The Center for Nanotechnology in Society at Arizona State University NSF #0937591 September 1, 2012 – August 31, 2013 PI: David H. Guston, Arizona State University Co-PIs: Elizabeth Corley, Arizona State University Deirdre Meldrum, Arizona State University Clark Miller, Arizona State University Dietram Scheufele, University of Wisconsin, Madison Jan Youtie, Georgia Institute of Technology Annual Report for the Period September 1, 2012 to August 31, 2013 This report includes work conducted at three collaborating universities of NSEC/CNS-ASU: Arizona State University, Georgia Institute of Technology, and the University of Wisconsin-Madison. Annual Report for Award #0937591 September 1, 2012 – August 31, 2013 2. Table of Contents Project Summary 3 List of Center Participants, Advisory Boards, and Participating Institutions 4 Quantifiable Outputs – Table 1 44 Mission, Significant Advances, and Broader Impacts 45 Highlights 61 Strategic Research Plan 70 Research Program, Accomplishments, and Plans 73 a. RTTA 1 73 b. RTTA 2 78 c. RTTA 3 83 d. RTTA 4 92 e. TRC 1 98 f. TRC 2 101 Center Diversity – Progress and Plans 109 Education 113 Outreach and Knowledge Transfer 128 Shared and Other Experimental Facilities 138 Personnel 141 Publications and Patents 146 Biographical Information 263 Honors and Awards 272 Fiscal Sections 274 Cost-Sharing Section 295 Leverage 307 Current and Pending Support 317 1 Annual Report for Award #0937591 September 1, 2012 – August 31, 2013 (2. Table of Contents continued) Tables Table 1 44 Table 2 108 Table 3A 127 Table 3B 127 Table 4A 144 Table 4B 145 Table 5 310 Table 6 311 2 Annual Report for Award #0937591 September 1, 2012 – August 31, 2013 3. -
Cviewoftherestlesssn2009ip Reveals the Explosive Ejection of a Massive Star Envelope Margutti, R., Et Al
1 Peter J. Brown Office Address Contact Information M311 Mitchell Institute for Fundamental Physics and Astronomy E-mail: [email protected] Department of Physics & Astronomy, Texas A&M University Cell: (979) 402-4523 Skype: grbpeter 4242 TAMU, College Station, TX 77843 www.linkedin.com/in/peter-brown-supernova Highlights Observational Astrophysicist with experience in ground and space-based Ultraviolet and• Optical Photometry and Spectroscopy of Supernovae and other Transients Leader of Swift supernova team since 2005 and Swift Cycle 14 Key Project • PI of 5 Hubble Space Telescope Programs • Principal Investigator of External Grants Totaling over $2,600,000 • 18 Refereed, First Author Journal Articles, 140+ Coauthored Journal Articles • 2017 Texas A&M College of Science Undergraduate Research Mentoring Award • Education Ph.D. in Astronomy & Astrophysics – Pennsylvania State University August 2009 Thesis Title: “The Ultraviolet Properties of Supernovae” Thesis Advisor: Dr. P. W. A. Roming B.S. in Physics and Astronomy – Brigham Young University August 2004 Senior Thesis Title: “Observing Gamma Ray Burst Afterglows from BYU’s Orson Pratt Observatory” Thesis Advisor: Professor J. W. Moody Academic Research Scientist – Mitchell Institute, Texas A&M University 2016 – present Positions Visiting Associate Professor Spring 2020 Visiting Assistant Professor Spring 2018 Mitchell Fellow, Postdoctoral Research Associate 2012 – 2016 Supervisor: Professor Lifan Wang Postdoctoral Research Associate – University of Utah 2009 – 2012 Supervisor: Professor -
Mita Brierley Project Officer, AAL
Astronomy Australia Ltd Member update Mita Brierley Project Officer, AAL September 2013 AAL’s context NCA’s 2006 Decadal Plan called for: “A peak body to coordinate Australia’s astronomical activities and to represent it in international partnerships.” AAL Vision: Astronomers in Australia will have access to the best astronomical research infrastructure. AAL Mission: – Engage with Australian astronomers to advance the national research infrastructure priorities of the decadal plan. – Advise the Australian Government on future investments. – Manage investments. www.astronomyaustralia.org.au 2 October 2013 2 What is AAL? Vision: Astronomers in Australia will have access to the best astronomical research infrastructure. www.astronomyaustralia.org.au 2 October 2013 3 Member Representatives AAO A/Prof Andrew Hopkins Australian National University Prof Matthew Colless CSIRO Dr Simon Johnston Curtin University Prof Steven Tingay Macquarie University Prof Quentin Parker Monash University Prof Alexander Heger Swinburne University Prof Karl Glazebrook University of Adelaide Dr Gavin Rowell University of Melbourne Prof Rachel Webster University of New South Wales Prof John Storey University of Queensland Prof Halina Rubinsztein-Dunlop University of Sydney Prof Peter Tuthill University of Tasmania Prof John Dickey University of Western Australia Prof Peter Quinn 4 2 October 2013 Community Representation AAL members elect the Board AAL Committees appointed by the Board Vacancies advertised Aug-Sept each year www.astronomyaustralia.org.au 2 October