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Curriculum Vitae Brian P
Curriculum Vitae Brian P. Schmidt AC FAA FRS Address: Office of the Vice Chancellor The Australian National University Canberra, ACT 2600, Australia Birthdate: 24 February 1967, Missoula Montana USA Citizenship: United States of America and Australia Telephone: +61 2 6125 2510 email: [email protected] Academic Qualifications: 1993: Ph.D. in Astronomy, Harvard University 1992: A.M. in Astronomy, Harvard University 1989: B.S. in Physics, University of Arizona 1989: B.S. in Astronomy, University of Arizona PhD thesis: Type II Supernovae, Expanding Photospheres, and the Extragalactic Distance Scale – Supervisor: Robert P. Kirshner Research and other Interests: Observational Cosmology, Studies of Supernovae, Gamma Ray Bursts, Large Surveys, Photometry and Calibration, Extremely Metal Poor Stars, Exoplanet Discovery Public Policy in the Areas of Education, Science, and Innovation Vigneron and Grape Grower: Maipenrai Vineyard and Winery Academic Positions Held: 2016- Vice Chancellor and President, The Australian National University 2013-2015 Public Policy Fellow, Crawford School, The Australian National University 2010- Distinguished Professor, The Australian National University 2010-2015 Australian Research Council Laureate Fellow (ANU) 2005-2009 Australian Research Council Federation Fellow (ANU) 2003-2005 Australian Research Council Professorial Fellow, (ANU) 1999-2002 Fellow, The Australian National University (RSAA) 1997-1999 Research Fellow, The Australian National University (MSSSO) 1995-1996 Postdoctoral Fellow, The Australian National University -
Hunting Down Stars with Unusual Infrared Properties Using Supervised Machine Learning
. Magnificent beasts of the Milky Way: Hunting down stars with unusual infrared properties using supervised machine learning Julia Ahlvind1 Supervisor: Erik Zackrisson1 Subject reader: Eric Stempels1 Examiner: Andreas Korn1 Degree project E in Physics { Astronomy, 30 ECTS 1Department of Physics and Astronomy { Uppsala University June 22, 2021 Contents 1 Background 2 1.1 Introduction................................................2 2 Theory: Machine Learning 2 2.1 Supervised machine learning.......................................3 2.2 Classification...............................................3 2.3 Various models..............................................3 2.3.1 k-nearest neighbour (kNN)...................................3 2.3.2 Decision tree...........................................4 2.3.3 Support Vector Machine (SVM)................................4 2.3.4 Discriminant analysis......................................5 2.3.5 Ensemble.............................................6 2.4 Hyperparameter tuning.........................................6 2.5 Evaluation.................................................6 2.5.1 Confusion matrix.........................................6 2.5.2 Precision and classification accuracy..............................7 3 Theory: Astronomy 7 3.1 Dyson spheres...............................................8 3.2 Dust-enshrouded stars..........................................8 3.3 Gray Dust.................................................9 3.4 M-dwarf.................................................. 10 3.5 post-AGB -
Extremely Extended Dust Shells Around Evolved Intermediate Mass Stars: Probing Mass Loss Histories,Thermal Pulses and Stellar Evolution
EXTREMELY EXTENDED DUST SHELLS AROUND EVOLVED INTERMEDIATE MASS STARS: PROBING MASS LOSS HISTORIES,THERMAL PULSES AND STELLAR EVOLUTION A Thesis presented to the Faculty of the Graduate School at the University of Missouri In Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy by BASIL MENZI MCHUNU Dr. Angela K. Speck December 2011 The undersigned, appointed by the Dean of the Graduate School, have examined the dissertation entitled: EXTREMELY EXTENDED DUST SHELLS AROUND EVOLVED INTERMEDIATE MASS STARS PROBING MASS LOSS HISTORIES, THERMAL PULSES AND STELLAR EVOLUTION USING FAR-INFRARED IMAGING PHOTOMETRY presented by Basil Menzi Mchunu, a candidate for the degree of Doctor of Philosophy and hereby certify that, in their opinion, it is worthy of acceptance. Dr. Angela K. Speck Dr. Sergei Kopeikin Dr. Adam Helfer Dr. Bahram Mashhoon Dr. Haskell Taub DEDICATION This thesis is dedicated to my family, who raised me to be the man I am today under challenging conditions: my grandfather Baba (Samuel Mpala Mchunu), my grandmother (Ma Magasa, Nonhlekiso Mchunu), my aunt Thembeni, and my mother, Nombso Betty Mchunu. I would especially like to thank my mother for all the courage she gave me, bringing me chocolate during my undergraduate days to show her love when she had little else to give, and giving her unending support when I was so far away from home in graduate school. She passed away, when I was so close to graduation. To her, I say, ′′Ulale kahle Macingwane.′′ I have done it with the help from your spirit and courage. I would also like to thank my wife, Heather Shawver, and our beautiful children, Rosemary and Brianna , for making me see life with a new meaning of hope and prosperity. -
Jpc-Final-Program.Pdf
49th AIAA/ASME/SAE/ASEE Joint Propulsion Conference and Exhibit (JPC) Advancing Propulsion Capabilities in a New Fiscal Reality 14–17 July 2013 San Jose Convention Center 11th International Energy Conversion San Jose, California Engineering Conference (IECEC) FINAL PROGRAM www.aiaa.org/jpc2013 www.iecec.org #aiaaPropEnergy www.aiaa.org/jpc2013 • www.iecec.org 1 #aiaaPropEnergy GET YOUR CONFERENCE INFO ON THE GO! Download the FREE Conference Mobile App FEATURES • Browse Program – View the program at your fingertips • My Itinerary – Create your own conference schedule • Conference Info – Including special events • Take Notes – Take notes during sessions • Venue Map – San Jose Convention Center • City Map – See the surrounding area • Connect to Twitter – Tweet about what you’re doing and who you’re meeting with #aiaaPropEnergy HOW TO DOWNLOAD Any version can be run without an active Internet connection! You can also sync an Compatible with itinerary you created online with the app by entering your unique itinerary name. iPhone/iPad, MyItinerary Mobile App MyItinerary Web App Android, and • For optimal use, we recommend • For optimal use, we recommend: rd BlackBerry! iPhone 3GS, iPod Touch (3 s iPhone 3GS, iPod Touch (3rd generation), iPad iOS 4.0, or later generation), iPad iOS 4.0, • Download the MyItinerary app by or later searching for “ScholarOne” in the s Most mobile devices using Android App Store directly from your mobile 2.2 or later with the default browser device. Or, access the link below or scan the QR code to access the iTunes s BlackBerry Torch or later device Sponsored by: page for the app. -
Monash Physics and Astronomy
MONASH PHYSICS AND ASTRONOMY study.monash PHYSICS AND ASTRONOMY Have you ever wondered if absolute zero temperature can be reached, how a black hole forms, or what the Universe is made of? Have you ever had a CT, an ultrasound or an MRI scan? Do you use a smart phone, the internet or a computer? Almost everything that makes your life more comfortable, The skills you gain through studying physics and astrophysics or allows you to work efficiently in the 21st century, is due to at Monash can be used in many areas, such as: developing engineered solutions based on physical principles. For example, medical instrumentation, radiotherapy treatment of cancer, the discovery of electricity, magnetism, relativity and quantum modelling climate and weather, analysing big data and financial mechanics came about through human curiosity; however, systems, developing innovative ways to address sustainability, technologies based on these discoveries did not eventuate until exploring emergent behaviour in complex biological systems, much later. and understanding the function of the brain. Physicists and Astrophysicists explore the Universe at all scales of Physics and astronomy at Monash is going through an exciting length, time and energy – from sub-atomic particles (such as the period of growth – investing significantly in people and facilities. Higgs boson) to the large scale structure of the Universe; from We are working across a broad range of creative, curiosity-driven ultra cold gases (close to absolute zero temperature), to what research areas that will impact on future generations – including happened at the Big Bang. Physics seeks to understand the biomedical imaging, quantum computing, atomtronics, and nature of space, time and matter, and in doing so it addresses novel materials for next generation photonics, optoelectronics profound philosophical questions about the nature of reality and and spintronics. -
Professor Robert Mccredie May
Professor Robert McCredie May The degree of Doctor of Science (honoris causa) was conferred upon Professor Robert McCredie May at the Science ceremony held in the Great Hall at 9.30am on 19 May 1995. Professor Robert May, photo, Tracey Schramm, 'The University of Sydney News', 12 July 1995. Citation Presented by the Vice-Chancellor and Principal Professor D McNicol Chancellor I have the honour to present Professor Robert McCredie May for admission to the degree of Doctor of Science (honoris causa). Professor May has a record of outstanding achievement in two very different fields of science - theoretical physics and population biology. Born and educated in Sydney, Professor May graduated BSc at this University with the University Medal in Physics in 1956, and PhD in Theoretical Physics in 1959, supervised by Dr M.R. Schafroth. After a brief interlude at Harvard University, he returned to join the academic staff of the School of Physics in 1962. For his distinguished theoretical contributions to the physics of ionized gases, he was awarded the Pawsey Medal by the Australian Academy of Science in 1967. In 1969 he was the first to be appointed to a Personal Chair in this University. The metamorphosis from physics to biology began with Professor May's investigation of the problem of the relation between stability and complexity in natural communities. His elegant mathematical solution to the predator-prey problem later led to him being regarded as one of the fathers of the modem theory of chaos. The transition to biology was completed in 1973 with his appointment to Princeton University to take up the Class of 1877 Professorship of Zoology. -
Quantum Measurement and Control Howard M
Cambridge University Press 978-0-521-80442-4 - Quantum Measurement and Control Howard M. Wiseman and Gerard J. Milburn Frontmatter More information QUANTUM MEASUREMENT AND CONTROL The control of individual quantum systems promises a new technology for the twenty-first century – quantum technology. This book is the first comprehensive treatment of modern quantum measurement and measurement-based quantum control, which are vital elements for realizing quantum technology. Readers are introduced to key experiments and technologies through dozens of recent experiments in cavity QED, quantum optics, mesoscopic electronics and trapped particles, several of which are analysed in detail. Nearly 300 exercises help build understanding, and prepare readers for research in these exciting areas. This important book will interest graduate students and researchers in quantum informa- tion, quantum metrology, quantum control and related fields. Novel topics covered include adaptive measurement; realistic detector models; mesoscopic current detection; Markovian, state-based and optimal feedback; and applications to quantum information processing. howard m. wiseman is Director of the Centre for Quantum Dynamics at Griffith University, Australia. He has worked in quantum measurement and control theory since 1992, and is a Fellow of the Australian Academy of Science (AAS). He has received the Bragg Medal of the Australian Institute of Physics, the Pawsey Medal of the AAS and the Malcolm Macintosh Medal of the Federal Science Ministry. gerard j. milburn is an Australian Research Council Federation Fellow at the Uni- versity of Queensland, Australia. He has written three previous books, on quantum optics, quantum technology and quantum computing. He has been awarded the Boas Medal of the Australian Institute of Physics and is a Fellow of the Australian Academy of Science and the American Physical Society. -
Issue 9 Jul09
Issue 9, July 2009 SCHOOL OF PHYSICS ALUMNI & FRIENDS NEWSLETTER MESSAGE FROM THE HEAD Also in 2009 we have seen Dean’s awards This year and hopefully reveal the Higgs boson. to our staff for research and outreach. is a year of With regard to the second, the Square These went to Andrew Melatos for his work remarkable physics Kilometre Array will look back in time to on sources of gravitational waves and to anniversaries! the early universe and reveal the first stars Roger Rassool for his science shows for Here in the School and answer some of the most profound primary and secondary students. A further of Physics we are questions about the origin and evolution raft of Dean’s awards went to our research celebrating the of the universe. We have high hopes that students Dougal Maclaurin, Paul Fraser, 400th anniversary Australia will be chosen for the site for the Michelle Strack, Andrew McCulloch and of Galileo’s first SKA. Rebecca Ryan. We are very grateful to astronomical People in Physics here in Melbourne are the sponsors of these awards that make it discoveries. We deeply involved in these two big projects. possible to recognise the accomplishments are also celebrating We have been very pleased to see of our students. the 100th our people working on these and other anniversary of the year Ernest Rutherford projects recognised for their excellence by It is also worth noting that the new and his students “reverse engineered” the a flood of medals and awards. Melbourne Model curriculum has atom and discovered the nucleus. -
Astrometrically Registered Maps of H2O and Sio Masers Toward VX Sagittarii
ARTICLE DOI: 10.1038/s41467-018-04767-8 OPEN Astrometrically registered maps of H2O and SiO masers toward VX Sagittarii Dong-Hwan Yoon1,2, Se-Hyung Cho2,3, Youngjoo Yun2, Yoon Kyung Choi2, Richard Dodson4, María Rioja4,5, Jaeheon Kim6, Hiroshi Imai7, Dongjin Kim3, Haneul Yang1,2 & Do-Young Byun2 The supergiant VX Sagittarii is a strong emitter of both H2O and SiO masers. However, previous VLBI observations have been performed separately, which makes it difficult to 1234567890():,; spatially trace the outward transfer of the material consecutively. Here we present the astrometrically registered, simultaneous maps of 22.2 GHz H2O and 43.1/42.8/86.2/129.3 GHz SiO masers toward VX Sagittarii. The H2O masers detected above the dust-forming layers have an asymmetric distribution. The multi-transition SiO masers are nearly circular ring, suggesting spherically symmetric wind within a few stellar radii. These results provide the clear evidence that the asymmetry in the outflow is enhanced after the smaller molecular gas clump transform into the inhomogeneous dust layers. The 129.3 GHz maser arises from the outermost region compared to that of 43.1/42.8/86.2 GHz SiO masers. The ring size of the 129.3 GHz maser is maximized around the optical maximum, suggesting that radiative pumping is dominant. 1 Astronomy Program, Department of Physics and Astronomy, Seoul National University, 1 Gwanak-ro, Gwanak-gu, Seoul 08826, Korea. 2 Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Korea. 3 Department of Astronomy, Yonsei University, 50 Yonsei-ro, Seodaemun-gu, Seoul 03722, Korea. -
CURRICULUM VITAE: PROF. BRYAN M. GAENSLER (He/Him)
CURRICULUM VITAE: PROF. BRYAN M. GAENSLER (he/him) Dunlap Institute for Astronomy and Astrophysics Phone: +1 416 978 6223 The University of Toronto Email: [email protected] 50 St. George Street, Toronto, ON M5S 3H4, Canada WWW: http://dunlap.utoronto.ca/∼bgaensler/ EDUCATION 1995 – 1999 Doctor of Philosophy, School of Physics, The University of Sydney 1994 First Class Honours, School of Physics, The University of Sydney 1991 – 1993 Bachelor of Science, The University of Sydney (Majors: Physics, Applied Mathematics) EMPLOYMENT 2015 – Director, Dunlap Institute for Astronomy and Astrophysics, The University of Toronto 2015 – Professor of Astronomy, The University of Toronto 2011 – 2014 Director, ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) 2006 – 2014 Professor of Physics, The University of Sydney 2006 Associate Professor of Astronomy, Harvard University 2002 – 2006 Assistant Professor of Astronomy, Harvard University 2001 – 2002 Clay Fellow, Smithsonian Astrophysical Observatory 1998 – 2001 Hubble Fellow, Center for Space Research, Massachusetts Institute of Technology SELECTED PROFESSIONAL AFFILIATIONS AND RESPONSIBILITIES 2019 – 2021 Co-Chair, Canadian Astronomy Long Range Plan 2020–2030 2015 – 2019 Canadian Science Director, Square Kilometre Array Organisation 2009 – 2014 Editor-in-Chief, Publications of the Astronomical Society of Australia 2006 – 2007 International Project Scientist, Square Kilometre Array 2005 – Fellow, Astronomical Society of Australia 2003 – Member, International Astronomical Union 1999 -
AU25: 2, 3, 4.. 50 Estrellas
ars universalis 2, 3, 4… 50 ESTRELLAS Vexilología (II): arte y ciencia de las banderas, pendones y estandartes. De arriba a abajo y de izquierda a derecha, banderas de Australia, Bosnia y Herzegovina, Burundi, Cabo Verde, China (primera columna), Dominica, Guinea Ecuatorial, Granada, Honduras, Micronesia (segunda columna), Nueva Zelanda, Panamá, Papúa Nueva Guinea, San Cristóbal y Nieves, Samoa (tercera columna), Santo Tomé y Príncipe, Eslovenia, Islas Salomón, Siria, Tayikistán (cuarta columna), Tuvalu, Estados Unidos de América y Venezuela (quinta columna). (Cortesía del autor) ste segundo artículo de Nueva Guinea, Samoa y las Islas tralia, Nueva Zelanda, Papúa la serie astrovexilológi- Salomón. Seis las de Australia y Nueva Guinea y Samoa. Las cua- ca está dedicado a veinti- Guinea Ecuatorial (en el escudo tro estrellas en la bandera de trés banderas con dos o de armas). Siete las de Grana- Nueva Zelanda son rojas y file- E 01+02 más estrellas. Dos mullets tienen da y Tayikistán (una estrella so- teadas en blanco: Ácrux ( las banderas de Panamá, San bre cada una de las siete monta- Crucis, B0.5 IV+B1 V, V = 0,76 Cristóbal y Nieves (Saint Kitts ñas con jardines de orquídeas). mag.), Mimosa ( Crucis, 훼B1 IV, and Nevis), Santo Tomé y Prín- Ocho las de Bosnia y Herzego- V = 1,25 mag.), Gacrux ( Cru- cipe y Siria, que representan los vina (en realidad, siete estrellas cis, M3.5 III, V = 훽1,64 mag.) e partidos conservadores y los li- enteras y dos medias, en una su- Imai ( Crucis, B2 IV, V =훾 2,79 berales, dos parejas de islas y la cesión supuestamente infinita; mag.). -
Taking the Measure of the Universe: Precision Astrometry with SIM
Accepted for publication in PASP, January 2008 issue A Preprint typeset using LTEX style emulateapj v. 08/22/09 TAKING THE MEASURE OF THE UNIVERSE: PRECISION ASTROMETRY WITH SIM PLANETQUEST Stephen C. Unwin1, Michael Shao2, Angelle M. Tanner2, Ronald J. Allen3, Charles A. Beichman4, David Boboltz5, Joseph H. Catanzarite2, Brian C. Chaboyer6, David R. Ciardi4, Stephen J. Edberg2, Alan L. Fey5, Debra A. Fischer7, Christopher R. Gelino8, Andrew P. Gould9, Carl Grillmair8, Todd J. Henry10, Kathryn V. Johnston11,12, Kenneth J. Johnston5, Dayton L. Jones2, Shrinivas R. Kulkarni4, Nicholas M. Law4, Steven R. Majewski13, Valeri V. Makarov2, Geoffrey W. Marcy14, David L. Meier2, Rob P. Olling15, Xiaopei Pan2, Richard J. Patterson13, Jo Eliza Pitesky2, Andreas Quirrenbach16, Stuart B. Shaklan2, Edward J. Shaya15, Louis E. Strigari17, John A. Tomsick18,19, Ann E. Wehrle20, and Guy Worthey21 Accepted for publication in PASP, January 2008 issue ABSTRACT Precision astrometry at microarcsecond accuracy has application to a wide range of astrophysical problems. This paper is a study of the science questions that can be addressed using an instrument with flexible scheduling that delivers parallaxes at about 4 microarcsec (µas) on targets as faint as V = 20, and differential accuracy of 0.6 µas on bright targets. The science topics are drawn primarily from the Team Key Projects, selected in 2000, for the Space Interferometry Mission PlanetQuest (SIM PlanetQuest). We use the capabilities of this mission to illustrate the importance of the next level of astrometric precision in modern astrophysics. SIM PlanetQuest is currently in the detailed design phase, having completed in 2005 all of the enabling technologies needed for the flight instrument.