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Editorial What the Nose Knows, What The
Neuroscience 190 (2011) 1–11 EDITORIAL WHAT THE NOSE KNOWS, WHAT THE EYES SEE, HOW WE FEEL, HOW WE LEARN, HOW WE UNDERSTAND MOTOR ACTS, WHY “YY” IS ESSENTIAL FOR ION TRANSPORT, HOW EPIGENETICS MEET NEUROBIOLOGY IN RETT SYNDROME: SEVEN TOPICS AT THE 2010 KAVLI PRIZE SYMPOSIUM ON NEUROSCIENCE L. H. BERGERSEN,a M. SANDERb AND Symposium included lectures by: Richard Axel of Colum- J. STORM-MATHISENa* bia University, New York, USA; Tobias Bonhoeffer of Max aDepartment of Anatomy, Institute of Basic Medical Sciences and Planck Institute of Neurobiology, Martinsried, Germany; Centre for Molecular Biology and Neuroscience, University of Oslo, Michael E. Goldberg of Columbia University, New York, PO Box 1105 Blindern, 0317 Oslo, Norway USA; Poul Nissen of Aarhus University, Denmark; Gia- b Page One Editorial Services, 685 Poplar Avenue, Boulder, CO como Rizzolatti of the University of Parma, Italy; and Huda 80304, USA Y Zoghbi of Baylor College of Medicine, Houston, Texas, USA. The seven symposium lectures described the most The Kavli Prizes were awarded for the second time in recent advances in understanding emotion, olfaction, vi- Oslo, Norway on 7 September, 2010 to eight of the sual information processing, synaptic plasticity, ion flux in world’s most prominent scientists in astrophysics, nano- neurons, perception of self and other, and the conse- science, and neuroscience. Jerry Nelson, of the Univer- quences of epigenetic dysregulation in the human brain. sity of California, Santa Cruz, USA, Ray Wilson, formerly The Kavli Prize Symposium on Neuroscience was or- of Imperial College London and the European Southern ganized by Linda H. Bergersen, Edvard Moser, May-Britt Observatory, and Roger Angel, of the University of Ari- Moser, and Jon Storm-Mathisen, and was made possible zona, Tucson, USA, shared the astrophysics prize for by the combined support of The Kavli Foundation, the their innovative contributions in the field of telescope Norwegian Academy of Science and Letters, and the Nor- design. -
Cfa in the News ~ Week Ending 3 January 2010
Wolbach Library: CfA in the News ~ Week ending 3 January 2010 1. New social science research from G. Sonnert and co-researchers described, Science Letter, p40, Tuesday, January 5, 2010 2. 2009 in science and medicine, ROGER SCHLUETER, Belleville News Democrat (IL), Sunday, January 3, 2010 3. 'Science, celestial bodies have always inspired humankind', Staff Correspondent, Hindu (India), Tuesday, December 29, 2009 4. Why is Carpenter defending scientists?, The Morning Call, Morning Call (Allentown, PA), FIRST ed, pA25, Sunday, December 27, 2009 5. CORRECTIONS, OPINION BY RYAN FINLEY, ARIZONA DAILY STAR, Arizona Daily Star (AZ), FINAL ed, pA2, Saturday, December 19, 2009 6. We see a 'Super-Earth', TOM BEAL; TOM BEAL, ARIZONA DAILY STAR, Arizona Daily Star, (AZ), FINAL ed, pA1, Thursday, December 17, 2009 Record - 1 DIALOG(R) New social science research from G. Sonnert and co-researchers described, Science Letter, p40, Tuesday, January 5, 2010 TEXT: "In this paper we report on testing the 'rolen model' and 'opportunity-structure' hypotheses about the parents whom scientists mentioned as career influencers. According to the role-model hypothesis, the gender match between scientist and influencer is paramount (for example, women scientists would disproportionately often mention their mothers as career influencers)," scientists writing in the journal Social Studies of Science report (see also ). "According to the opportunity-structure hypothesis, the parent's educational level predicts his/her probability of being mentioned as a career influencer (that ism parents with higher educational levels would be more likely to be named). The examination of a sample of American scientists who had received prestigious postdoctoral fellowships resulted in rejecting the role-model hypothesis and corroborating the opportunity-structure hypothesis. -
Nima Arkani-Hamed, Juan Maldacena, Nathan Both Particle Physicists and Astrophysicists, We Are in an Ideal Seiberg, and Edward Witten
THE I NSTITUTE L E T T E R INSTITUTE FOR ADVANCED STUDY PRINCETON, NEW JERSEY · SUMMER 2008 PROBING THE DARK SIDE OF THE UNIVERSE ne of The remarkable dis - erTies of dark maTTer, and a Ocoveries in asTrophysics has more precise accounTing of The been The recogniTion ThaT The composiTion of The universe, maTerial we see and are familiar The Two fields of asTrophysics wiTh, which makes up The earTh, (The physics of The very large) The sun, The sTars, and everyday and parTicle physics (The objecTs, such as a Table, is only a physics of The very small) are small fracTion of all of The maTTer each providing some of The in The universe. The resT is dark mosT imporTanT new experi - maTTer, possibly a new form of menTal daTa and TheoreTical elemenTary parTicle ThaT does concepTs for The oTher. Re- noT emiT or absorb lighT, and can search aT The InsTiTuTe for only be deTecTed from iTs gravi - Advanced STudy has played a These three images created by Member Douglas Rudd show the various matter components in a simulation encompassing a volume 86 TaTional effecTs. Megaparsec on a side (for reference, the distance between the Milky Way and its nearest neighbor is 0.75 Mpc). The three compo - significanT role in This develop - In The lasT decade, asTro - nents are dark matter (blue), gas (green), and stars (orange). The stars form in galaxies which lie at the intersection of filaments as menT. The laTe InsTiTuTe Pro - nomical observaTions of several seen in the dark matter and gas profiles. -
Astronomy and Astrophysics
THE DECADE OF DISCOVERY IN ASTRONOMY AND ASTROPHYSICS Astronomy and Astrophysics Survey Committee Board on Physics and Astronomy Commission on Physical Sciences, Mathematics, and Applications National Research Council NATIONAL ACADEMY PRESS Washington, D.C. 1991 NATIONAL ACADEMY PRESS • 2101 Constitution Avenue, NW • Washington, DC 20418 NOTICE: The project that is the subject of this report was approved by the Governing Board of the National Research Council, whose members are drawn from the councils of the National Academy of Sciences, the National Academy of Engineering, and the Institute of Medicine. The members of the committee responsible for the report were chosen for their special compe_nces and with regard for appropriate balance. This report has been reviewed by a group other than the authors according to procedures approved by a Report Review Committee consisting of members of the National Academy of Sciences, the National Academy of Engineering, and the Institute of Medicine. This project was supported by the Department of Energy under Grant No. DE-FGO5- 89ER40421, the National Aeronautics and Space Administration and the National Science Foundation under Grant No. AST-8901685, the Naval Research Laboratory under Contract No. N00173-90-M-9744, and the Smithsonian Institution under Purchase Order No. SF0022430000. Additional support was provided by the Maurice Ewing Earth and Planetary Sciences Fund of the National Academy of Sciences created through a gift from the Palisades Geophysical Institute, Inc., and an anonymous donor. Library of Congress Cataloging-in-Publication Data National Research Council (U.S.). Astronomy and Astrophysics Survey Committee. The decade of discovery in astronomy and astrophysics / Astronomy and Astrophysics Survey Committee, Board on Physics and Astronomy, Commission on Physical Sciences, Mathematics, and Applications, National Research Council. -
On the Stability of the Gliese 876 System of Planets and the Importance of the Inner Planet
On the Stability of the Gliese 876 System of Planets and the Importance of the Inner Planet By: Ricky Leon Murphy Major Project – HET617 – Computational Astrophysics S2 – 2005 | Supervisor: Professor James Murray Background Image Credits: HIRES Echelleogram: http://exoplanets.org/gl876_web/gl876_tech.html Above: Gliese 876d Artist Rendition: http://exoplanets.org/gl876_web/gl876_graphics.html Abstract: Above: Above: Above: Using the SWIFT simulator code, a 5,000 Changing the mass of the inner body has In addition to mass, the eccentricity of the inner year simulation of the current Gliese 876 resulted in the middle planet to take on a body also severely affects system stability. A third planet with a mass of 0.023 MJ was found orbiting the star Gliese 876. system was performed (Monte Carlo more distant orbit. The eccentricity of this Here the mass of the inner body is the same simulations - to determine the best Cartesian body was very high, so the mass of the inner The initial two body system was found to have a perfect orbital resonance as the stable system (0.023M J ) with a change of 2/1. This paper will demonstrate the orbital stability to maintain this coordinates). The result is a system that is body was not available to ensure system in the orbital eccentricity from 0 to 0.1. None of stable. These parameters will be used for the stability. The mass of the inner body was the planets are able to hold their orbits. ratio is highly dependant on the presence of the small, inner planet. In remaining simulations of Gliese 876. -
Scott Duncan Tremaine
Essay‐Contest 2017/18 Leon Ritterbach, International School Kufstein, 9. Schulstufe, Fremdsprachenerwerb: 5 Jahre Scott Duncan Tremaine Astrophysics is a very interesting field of science. You explore the whole universe, from tiny Asteroids to huge black holes. Every time you solve one of the mind breaking riddles that the universe has to offer, it raises new questions. You can find out how the universe works and how forces like gravity form the universe we know and act on us. Scott Duncan Tremaine is one of the people who were lucky enough to be able to study astrophysics. Today, he is 68 years old and one of the world’s leading astrophysicists. He is a fellow of the Royal Society and a member of the National Academy of Sciences. He made predictions about planetary rings, has written an outstanding book “Galactic Dynamics” and named the Kuiper belt. Scott Tremaine’s research is focused on the dynamics of a wide range of astrophysical systems, including planetary rings, comets, planetary systems, galaxies, and clusters of galaxies (structures that consists of anywhere from hundreds to thousands of galaxies). He is known for his contributions to the theory of Solar Systems, Galactic Dynamics and his prediction of small moons keeping the belts of planets in place. Tremaine is so popular that there is even an asteroid named after him, 3806 Tremaine. (Canada under the stars/ 2007), (Princeton University, Department of astrophysical sciences, 2018), (Perimeter Institute for Theoretical Physics/ 2012), (National Academy of Sciences/ 2002), (The Royal Society/ 1994), (Scott Tremaine ‐ Video Learning ‐ WizScience.com/ 2015), (IAS/ 2018) Tremaine grew up in Toronto. -
Physics Today
Physics Today The Dynamical Evidence for Dark Matter Scott Tremaine Citation: Physics Today 45(2), 28 (1992); doi: 10.1063/1.881329 View online: http://dx.doi.org/10.1063/1.881329 View Table of Contents: http://scitation.aip.org/content/aip/magazine/physicstoday/45/2?ver=pdfcov Published by the AIP Publishing This article is copyrighted as indicated in the article. Reuse of AIP content is subject to the terms at: http://scitation.aip.org/termsconditions. Downloaded to IP: 128.112.203.62 On: Mon, 25 Aug 2014 15:15:09 THE DYNAMICAL EVIDENCE FOR DARK MATTER 'The Starry Night/ by Vincent van Gogh. The 1889 oil painting suggests how the night sky might look if all of the mass in the universe were luminous. Observations of galaxy dynamics and modern theories of galaxy formation imply that the visible components of galaxies, composed mostly of stars, lie at the centers of vast halos of dark matter that may be 30 or more times larger than the visible galaxy. In most models of galaxy formation, the halos are comparable in size to the distance between galaxies. The halos form as a result of the gravitational instability of small density fluctuations in the early universe; the star-forming gas collects at the minima of the halo potential wells. Infall of outlying material into existing halos and mergers of small halos with larger ones continue at the present time. If the halos were visible to the naked eye, there would be well over 1000 nearby galaxies with halo diameters larger than the full Moon. -
The Kavli Prize Laureate Lecture
The Kavli Prize Laureate Lecture 24 April 2013, 17:00 – 20:00 The Nordic Embassies in Berlin, Rauchstraße 1, 10787 Berlin-Tiergarten In co-operation with: Berlinffff The Kavli Prize is a partnership between The Norwegian Academy of Science and Letters, The Kavli Foundation and The Norwegian Ministry of Education and Research Programme: 16:30 Registration Please be seated by 16:55 17:00 Welcome Sven E. Svedman, Norwegian Ambassador to Germany 17:05 ”The Kavli Prize: fostering scientific excellence and international cooperation” Ms Kristin Halvorsen, Norwegian Minister of Education and Research 17:20 „Internationale Herausforderungen – internationale Kooperationen: Der Auftrag der Wissenschaft“ Prof. Dr. Johanna Wanka, Federal Minister of Education and Research 17:35 Short remarks Prof. Dr. Herbert Jäckle, Vice President of the Max Planck Society 17:40 Short remarks Professor Kirsti Strøm Bull President of The Norwegian Academy of Science and Letters 17:45 Lecture: “Following the Brain’s Wires” Kavli Prize Laureate Prof. Dr. Winfried Denk Max Planck Institute for Medical Research, Heidelberg 18:10 Lecture: “Towards an Understanding of Neural Codes” Prof. Dr. Gilles Laurent Director of the Max Planck Institute for Brain Research, Frankfurt 18:35 Reception Exhibition Hall of the Nordic Embassies in Berlin “Following the Brain’s Wires” Kavli Prize Laureate Prof. Dr. Winfried Denk To understand neural circuits we need to know how neurons are connected. Over the past decade we have developed methods that allow the reconstruction of neural wiring diagrams via the acquisition and analysis of high-resolution three-dimensional electron microscopic data. We have applied these methods to the retina in order to explore, for example, how direction-selective signals are computed. -
Acknowledgment of Reviewers, 2015
Acknowledgment of Reviewers, 2015 The PNAS editors would like to thank all the individuals who dedicated their considerable time and expertise to the journal by serving as reviewers in 2015. Their generous contribution is deeply appreciated. A Peter B. Adler Colin J. Akerman Eric E. Allen James Ammerman Duur K. Aanen Ralph Adolphs Joshua M. Akey Heather C. Allen David M. Amodio Adam R. Abate Ruedi Aebersold Anna Akhmanova Jim Allen Valentin Amrhein John T. Abatzoglou Hugo Aerts Hajime Akimoto Karen N. Allen Esther Amstad Jonathan Abbatt Hagit P. Affek Akin Akinc Michael F. Allen Ronald Amundson Allison Abbott Arash Afraz Shizuo Akira Paul M. Allen Weihua An Jeffrey Abbott Theodor Agapie Ozan Akkus Rosalind J. Allen Zhiqiang An Larry F. Abbott David A. Agard Ivona Aksentijevich Morten Erik Allentoft Laura Diaz Anadon Nicholas L. Abbott Sapan Agarwal Serap Aksoy Stefano Allesina Ganesh Srinivasan Anand Chaouki T. Abdallah Joel W. Ager III Yousef Al-Abed David B. Allison Cort Anastasio Omar Abdel-Wahab Ingi Agnarsson Ashraf Al-Amoudi Steven D. Allison Lefteris Jason Ikuro Abe Anurag A. Agrawal Eric E. Alani Julian M. Allwood Anastasopoulos Stephen Tobias Abedon Ashutosh Agrawal Balbino Alarcón Eric J. Alm Hossain Anawar Moshe Abeles Rakesh Agrawal Qais Al-Awqati Benjamin A. Alman Elissar Andari Asa Abeliovich Jon Ågren Joseph Albanesi Ingvild Almas William R. L. Anderegg John Aber Alan Agresti Francis Albarede Steven C. Almo John M. Anderies Clara Abraham Jeremy J. Agresti Umberto Albarella Douglas Almond Mark L. Andermann John Abraham Jay J. Ague Silas D. Alben Uri Alon Bogi Andersen Daniel A. Abrams Fernan Agüero Frank Alber José M. -
Astro2010: the Astronomy and Astrophysics Decadal Survey
Astro2010: The Astronomy and Astrophysics Decadal Survey Notices of Interest 1. 4 m space telescope for terrestrial planet imaging and wide field astrophysics Point of Contact: Roger Angel, University of Arizona Summary Description: The proposed 4 m telescope combines capabilities for imaging terrestrial exoplanets and for general astrophysics without compromising either. Extremely high contrast imaging at very close inner working angle, as needed for terrestrial planet imaging, is accomplished by the powerful phase induced amplitude apodization method (PIAA) developed by Olivier Guyon. This method promises 10-10 contrast at 2.0 l/D angular separation, i.e. 50 mas for a 4 m telescope at 500 nm wavelength. The telescope primary mirror is unobscured with off-axis figure, as needed to achieve such high contrast. Despite the off-axis primary, the telescope nevertheless provides also a very wide field for general astrophysics. A 3 mirror anastigmat design by Jim Burge delivers a 6 by 24 arcminute field whose mean wavefront error of 12 nm rms, i.e.diffraction limited at 360 nm wavelength. Over the best 10 square arcminutes the rms error is 7 nm, for diffraction limited imaging at 200 nm wavelength. Any of the instruments can be fed by part or all of the field, by means of a flat steering mirror at the exit pupil. To allow for this, the field is curved with a radius equal to the distance from the exit pupil. The entire optical system fits in a 4 m diameter cylinder, 8 m long. Many have considered that only by using two spacecraft, a conventional on-axis telescope and a remote occulter, could high contrast and wide field imaging goals be reconciled. -
Carnegie Astronomical Telescopes in the 21St Century
YEAR BOOK02/03 2002–2003 CARNEGIEINSTITUTIONOFWASHINGTON tel 202.387.6400 CARNEGIE INSTITUTION 1530 P Street, NW CARNEGIE INSTITUTION fax 202.387.8092 OF WASHINGTON OF WASHINGTON Washington, DC 20005 web site www.CarnegieInstitution.org New Horizons for Science YEAR BOOK 02/03 2002-2003 Year Book 02/03 THE PRESIDENT’ S REPORT July 1, — June 30, CARNEGIE INSTITUTION OF WASHINGTON ABOUT CARNEGIE Department of Embryology 115 West University Parkway Baltimore, MD 21210-3301 410.554.1200 . TO ENCOURAGE, IN THE BROADEST AND MOST LIBERAL MANNER, INVESTIGATION, Geophysical Laboratory 5251 Broad Branch Rd., N.W. RESEARCH, AND DISCOVERY, AND THE Washington, DC 20015-1305 202.478.8900 APPLICATION OF KNOWLEDGE TO THE IMPROVEMENT OF MANKIND . Department of Global Ecology 260 Panama St. Stanford, CA 94305-4101 The Carnegie Institution of Washington 650.325.1521 The Carnegie Observatories was incorporated with these words in 1902 813 Santa Barbara St. by its founder, Andrew Carnegie. Since Pasadena, CA 91101-1292 626.577.1122 then, the institution has remained true to Las Campanas Observatory its mission. At six research departments Casilla 601 La Serena, Chile across the country, the scientific staff and Department of Plant Biology a constantly changing roster of students, 260 Panama St. Stanford, CA 94305-4101 postdoctoral fellows, and visiting investiga- 650.325.1521 tors tackle fundamental questions on the Department of Terrestrial Magnetism frontiers of biology, earth sciences, and 5241 Broad Branch Rd., N.W. Washington, DC 20015-1305 astronomy. -
Astrophysics and Cosmology
Copyright of the works in this eBook is vested with World Scientific Publishing. The following eBook is allowed for Solvay Institutes website use only and may not be resold, copied, further disseminated, or hosted on any other third party website or repository without the copyright holders' written permission. http://www.worldscientific.com/worldscibooks/10.1142/9953 For any queries, please contact [email protected]. ASTROPHYSICS AND COSMOLOGY - PROCEEDINGS OF THE 26TH SOLVAY CONFERENCE ON PHYSICS http://www.worldscientific.com/worldscibooks/10.1142/9953 ©World Scientific Publishing Company. For post on Solvay Institutes website only. No further distribution is allowed. 9953_9789814759175_tp.indd 1 8/3/16 4:58 PM December 12, 2014 15:40 BC: 9334 { Bose, Spin and Fermi Systems 9334-book9x6 page 2 This page intentionally left blank ASTROPHYSICS AND COSMOLOGY - PROCEEDINGS OF THE 26TH SOLVAY CONFERENCE ON PHYSICS http://www.worldscientific.com/worldscibooks/10.1142/9953 ©World Scientific Publishing Company. For post on Solvay Institutes website only. No further distribution is allowed. ASTROPHYSICS AND COSMOLOGY - PROCEEDINGS OF THE 26TH SOLVAY CONFERENCE ON PHYSICS http://www.worldscientific.com/worldscibooks/10.1142/9953 ©World Scientific Publishing Company. For post on Solvay Institutes website only. No further distribution is allowed. 9953_9789814759175_tp.indd 2 8/3/16 4:58 PM Published by World Scientific Publishing Co. Pte. Ltd. 5 Toh Tuck Link, Singapore 596224 USA office: 27 Warren Street, Suite 401-402, Hackensack, NJ 07601 UK office: 57 Shelton Street, Covent Garden, London WC2H 9HE British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library.