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Robert Hinde Curriculum Vitae
CURRICULUM VITAE Robert A. Hinde Born 26 October 1923 in Norwich, England Education, Degrees, A wards, and Positions 1935-40 Oundle School 1940-45 RAF Pilot, Coastal Command 1946-48 St. John's College, Cambridge 1948 B.A., University of Cambridge; B.Sc., University of London 1948-50 Research Assistant, Edward Grey Institute, Department of Zoology, Oxford University 1950 D.Phil., Oxford University 1950-64 Curator, Ornithological Field Station, Department of Zoology, University of Cambridge (now Sub-Department of Animal Behaviour) 1951-54 Research Fellow, St. John's College, Cambridge 1956-58 Steward, St. John's College 1958-89, 1994- Fellow, St. John's College 1958-1963 Tutor, St. John's College 1989-94 Master, St. John’s College 1961 Sc.D., University of Cambridge 1961 Zoological Society's Scientific Medal 1963-1989 Royal Society Research Professor 1970-89 Honorary Director, Medical Research Council Unit on the Development & Integration of Behaviour 1974 Fellow of the Royal Society (Council member 1985-1987) 1974 Foreign Honorary Member of the American Academy of Arts and Sciences 1974 Docteur honoris causa, Universire Libre, Bruxelles 1976 Honorary Fellow of the American Ornithologists' Union 1978 Honorary Foreign Associate of the National Academy of Sciences 1 1978 Docteur honoris causa, Universire de Paris (Nanterre) 1979 Hitchcock Professor at University of California 1980 Osman Hill Medal, Primate Society of Great Britain 1980 Leonard Cammer A ward, New York Psychiatric Institute, Columbia University 1981 Honorary Fellow of British -
Ubiquitous Argonium \(Arh+\) in the Diffuse Interstellar Medium: A
A&A 566, A29 (2014) Astronomy DOI: 10.1051/0004-6361/201423727 & c ESO 2014 Astrophysics Ubiquitous argonium (ArH+) in the diffuse interstellar medium: A molecular tracer of almost purely atomic gas P. Schilke1, D. A. Neufeld2, H. S. P. Müller1, C. Comito1, E. A. Bergin3, D. C. Lis4;5, M. Gerin6, J. H. Black7, M. Wolfire8, N. Indriolo2, J. C. Pearson9, K. M. Menten10, B. Winkel10, Á. Sánchez-Monge1, T. Möller1, B. Godard6, and E. Falgarone6 1 I. Physikalisches Institut der Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany e-mail: [email protected] 2 The Johns Hopkins University, Baltimore, MD 21218, USA 3 Department of Astronomy, The University of Michigan, 500 Church Street, Ann Arbor, MI 48109-1042, USA 4 California Institute of Technology, Pasadena, CA 91125, USA 5 Sorbonne Universités, Université Pierre et Marie Curie, Paris 6, CNRS, Observatoire de Paris, UMR 8112 LERMA, Paris, France 6 LERMA, CNRS UMR 8112, Observatoire de Paris & École Normale Supérieure, 24 rue Lhomond, 75005 Paris, France 7 Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 439 92 Onsala, Sweden 8 Astronomy Department, University of Maryland, College Park, MD 20742, USA 9 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA 10 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany Received 28 February 2014 / Accepted 29 March 2014 ABSTRACT Aims. We describe the assignment of a previously unidentified interstellar absorption line to ArH+ and discuss its relevance in the + context of hydride absorption in diffuse gas with a low H2 fraction. -
Human Origins
HUMAN ORIGINS Methodology and History in Anthropology Series Editors: David Parkin, Fellow of All Souls College, University of Oxford David Gellner, Fellow of All Souls College, University of Oxford Volume 1 Volume 17 Marcel Mauss: A Centenary Tribute Learning Religion: Anthropological Approaches Edited by Wendy James and N.J. Allen Edited by David Berliner and Ramon Sarró Volume 2 Volume 18 Franz Baerman Steiner: Selected Writings Ways of Knowing: New Approaches in the Anthropology of Volume I: Taboo, Truth and Religion. Knowledge and Learning Franz B. Steiner Edited by Mark Harris Edited by Jeremy Adler and Richard Fardon Volume 19 Volume 3 Difficult Folk? A Political History of Social Anthropology Franz Baerman Steiner. Selected Writings By David Mills Volume II: Orientpolitik, Value, and Civilisation. Volume 20 Franz B. Steiner Human Nature as Capacity: Transcending Discourse and Edited by Jeremy Adler and Richard Fardon Classification Volume 4 Edited by Nigel Rapport The Problem of Context Volume 21 Edited by Roy Dilley The Life of Property: House, Family and Inheritance in Volume 5 Béarn, South-West France Religion in English Everyday Life By Timothy Jenkins By Timothy Jenkins Volume 22 Volume 6 Out of the Study and Into the Field: Ethnographic Theory Hunting the Gatherers: Ethnographic Collectors, Agents and Practice in French Anthropology and Agency in Melanesia, 1870s–1930s Edited by Robert Parkin and Anna de Sales Edited by Michael O’Hanlon and Robert L. Welsh Volume 23 Volume 7 The Scope of Anthropology: Maurice Godelier’s Work in Anthropologists in a Wider World: Essays on Field Context Research Edited by Laurent Dousset and Serge Tcherkézoff Edited by Paul Dresch, Wendy James, and David Parkin Volume 24 Volume 8 Anyone: The Cosmopolitan Subject of Anthropology Categories and Classifications: Maussian Reflections on By Nigel Rapport the Social Volume 25 By N.J. -
Ubiquitous Argonium, Arh+, in the Diffuse Interstellar Medium
Ubiquitous Argonium, ArH+, in the Interstellar Medium P. Schilke, Holger S. P. Müller, C. Comito, Á. Sánchez-Monge, D. A. Neufeld, N. Indriolo, E. A. Bergin, D. C. Lis, M. Gerin, J. H. Black, M. G. Wolfire, J. C. Pearson, K. M. Menten, B. Winkel V.6, 13th International HITRAN Conference, CfA, Cambridge, MA, USA, June 23–25, 2014 What is Argonium? ArH+, 1Σ+, isoelectronic to HCl + + Formation: Ar + H2 → ArH + H + + Destruction (e.g.): ArH + H2 → Ar + H3 Isotopic ratio: 36Ar : 38Ar : 40Ar terrestrial: 84.2 : 15.8 : 25018.8 (from decay of 40K) solar/ISM: ~84.6 : ~15.4 : 0.025 36ArH+ toward Crab Nebula SNR: J = 1 – 0 & 2 – 1 in emission (w. OH+ N = 1 – 0); SPIRE/Herschel M. J. Barlow et al., Science 342 (2013) 1343 On the Spectroscopy of ArH+ 40ArH+; rotational spectroscopy: K. B. Laughlin et al., PRL 58 (1987) 996: J" = 0 J. M. Brown et al., JMSp 128 (1988) 587: J" = 1 – 6 D. J. Liu et al., JCP 87 (1987) 2442: J" = 20 – 24; v ≤ 4 (MIR) 40ArD+; rotational spectroscopy: W. C. Bowman et al., JCP 79 (1983) 2093: J" = 0 (+ 36ArD+ & 38ArD+ H. Odashima et al., JMSp 195 (1999) 356: J" = 2 – 14 rovibrational spectroscopy: J. W. Brault & S. P. Davis, Phys. Sript. 25 (1982) 268: 40ArH+ J. W. C. Johns, JMSp 106 (1984) 124: 40ArH+, 40ArD+ R. R. Filueira & C. E. Blom, JMSp 127 (1988) 279: 36ArH+, 38ArH+ M. Cueto et al., ApJ 783 (2014) L5: 36ArH+, 38ArH+ ArH+ toward Sagittarius B2(M) – HIFI Line Survey Absorption toward Sgr B2(M) massive star-forming regions as background sources with approximate origins Sagittarius B2(M) Interstellar Chemistry of ArH+ I + + + + Ar + H2 → ArH + H exothermic (endo. -
Book of Abstracts
THE PHYSICS AND CHEMISTRY OF THE INTERSTELLAR MEDIUM Celebrating the first 40 years of Alexander Tielens' contribution to Science Book of Abstracts Palais des Papes - Avignon - France 2-6 September 2019 CONFERENCE PROGRAM Monday 2 September 2019 Time Speaker 10:00 Registration 13:00 Registration & Welcome Coffee 13:30 Welcome Speech C. Ceccarelli Opening Talks 13:40 PhD years H. Habing 13:55 Xander Tielens and his contributions to understanding the D. Hollenbach ISM The Dust Life Cycle 14:20 Review: The dust cycle in galaxies: from stardust to planets R. Waters and back 14:55 The properties of silicates in the interstellar medium S. Zeegers 15:10 3D map of the dust distribution towards the Orion-Eridanus S. Kh. Rezaei superbubble with Gaia DR2 15:25 Invited Talk: Understanding interstellar dust from polariza- F. Boulanger tion observations 15:50 Coffee break 16:20 Review: The life cycle of dust in galaxies M. Meixner 16:55 Dust grain size distribution across the disc of spiral galaxies M. Relano 17:10 Investigating interstellar dust in local group galaxies with G. Clayton new UV extinction curves 17:25 Invited Talk: The PROduction of Dust In GalaxIES C. Kemper (PRODIGIES) 17:50 Unravelling dust nucleation in astrophysical media using a L. Decin self-consistent, non steady-state, non-equilibrium polymer nucleation model for AGB stellar winds 19:00 Dining Cocktail Tuesday 3 September 2019 08:15 Registration PDRs 09:00 Review: The atomic to molecular hydrogen transition: a E. Roueff major step in the understanding of PDRs 09:35 Invited Talk: The Orion Bar: from ALMA images to new J. -
Detection of Extragalactic Argonium, Arh+, Toward PKS 1830−211⋆
A&A 582, L4 (2015) Astronomy DOI: 10.1051/0004-6361/201527254 & c ESO 2015 Astrophysics Letter to the Editor Detection of extragalactic argonium, ArH+, toward PKS 1830−211 Holger S. P. Müller1, Sébastien Muller2, Peter Schilke1, Edwin A. Bergin3, John H. Black2, Maryvonne Gerin4, Dariusz C. Lis5,6, David A. Neufeld7, and Sümeyye Suri1 1 I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany e-mail: [email protected] 2 Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, 43992 Onsala, Sweden 3 Department of Astronomy, The University of Michigan, 500 Church Street, Ann Arbor, MI 48109-1042, USA 4 LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, École normale supérieure, 75005 Paris, France 5 LERMA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Univ. Paris 06, 75014 Paris, France 6 Cahill Center for Astronomy and Astrophysics 301-17, California Institute of Technology, Pasadena, CA 91125, USA 7 Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA Received 26 August 2015 / Accepted 22 September 2015 ABSTRACT Context. Argonium has recently been detected as a ubiquitous molecule in our Galaxy. Model calculations indicate that its abundance peaks at molecular fractions in the range of 10−4 to 10−3 and that the observed column densities require high values of the cosmic ray ionization rate. Therefore, this molecular cation may serve as an excellent tracer of the very diffuse interstellar medium (ISM), as well as an indicator of the cosmic ray ionization rate. -
A Visual Motion Detection Circuit Suggested by Drosophila Connectomics
ARTICLE doi:10.1038/nature12450 A visual motion detection circuit suggested by Drosophila connectomics Shin-ya Takemura1, Arjun Bharioke1, Zhiyuan Lu1,2, Aljoscha Nern1, Shiv Vitaladevuni1, Patricia K. Rivlin1, William T. Katz1, Donald J. Olbris1, Stephen M. Plaza1, Philip Winston1, Ting Zhao1, Jane Anne Horne2, Richard D. Fetter1, Satoko Takemura1, Katerina Blazek1, Lei-Ann Chang1, Omotara Ogundeyi1, Mathew A. Saunders1, Victor Shapiro1, Christopher Sigmund1, Gerald M. Rubin1, Louis K. Scheffer1, Ian A. Meinertzhagen1,2 & Dmitri B. Chklovskii1 Animal behaviour arises from computations in neuronal circuits, but our understanding of these computations has been frustrated by the lack of detailed synaptic connection maps, or connectomes. For example, despite intensive investigations over half a century, the neuronal implementation of local motion detection in the insect visual system remains elusive. Here we develop a semi-automated pipeline using electron microscopy to reconstruct a connectome, containing 379 neurons and 8,637 chemical synaptic contacts, within the Drosophila optic medulla. By matching reconstructed neurons to examples from light microscopy, we assigned neurons to cell types and assembled a connectome of the repeating module of the medulla. Within this module, we identified cell types constituting a motion detection circuit, and showed that the connections onto individual motion-sensitive neurons in this circuit were consistent with their direction selectivity. Our results identify cellular targets for future functional investigations, and demonstrate that connectomes can provide key insights into neuronal computations. Vision in insects has been subject to intense behavioural1,physiological2 neuroanatomy14. Given the time-consuming nature of such recon- and anatomical3 investigations, yet our understanding of its underlying structions, we wanted to determine the smallest medulla volume, neural computations is still far from complete. -
Framing Youth Suicide in a Multi-Mediated World: the Construction of the Bridgend Problem in the British National Press
City Research Online City, University of London Institutional Repository Citation: Akrivos, Dimitrios (2015). Framing youth suicide in a multi-mediated world: the construction of the Bridgend problem in the British national press. (Unpublished Doctoral thesis, City University London) This is the accepted version of the paper. This version of the publication may differ from the final published version. Permanent repository link: https://openaccess.city.ac.uk/id/eprint/13648/ Link to published version: Copyright: City Research Online aims to make research outputs of City, University of London available to a wider audience. Copyright and Moral Rights remain with the author(s) and/or copyright holders. URLs from City Research Online may be freely distributed and linked to. Reuse: Copies of full items can be used for personal research or study, educational, or not-for-profit purposes without prior permission or charge. Provided that the authors, title and full bibliographic details are credited, a hyperlink and/or URL is given for the original metadata page and the content is not changed in any way. City Research Online: http://openaccess.city.ac.uk/ [email protected] FRAMING YOUTH SUICIDE IN A MULTI-MEDIATED WORLD THE CONSTRUCTION OF THE BRIDGEND PROBLEM IN THE BRITISH NATIONAL PRESS DIMITRIOS AKRIVOS PhD Thesis CITY UNIVERSITY LONDON DEPARTMENT OF SOCIOLOGY SCHOOL OF ARTS AND SOCIAL SCIENCES 2015 THE FOLLOWING PARTS OF THIS THESIS HAVE BEEN REDACTED FOR COPYRIGHT REASONS: p15, Fig 1.1 p214, Fig 8.8 p16, Fig 1.2 p216, Fig 8.9 p17, Fig -
Ijmp.Jor.Br V
INDEPENDENT JOURNAL OF MANAGEMENT & PRODUCTION (IJM&P) http://www.ijmp.jor.br v. 10, n. 8, Special Edition Seng 2019 ISSN: 2236-269X DOI: 10.14807/ijmp.v10i8.1046 A NEW HYPOTHESIS ABOUT THE NUCLEAR HYDROGEN STRUCTURE Relly Victoria Virgil Petrescu IFToMM, Romania E-mail: [email protected] Raffaella Aversa University of Naples, Italy E-mail: [email protected] Antonio Apicella University of Naples, Italy E-mail: [email protected] Taher M. Abu-Lebdeh North Carolina A and T State Univesity, United States E-mail: [email protected] Florian Ion Tiberiu Petrescu IFToMM, Romania E-mail: [email protected] Submission: 5/3/2019 Accept: 5/20/2019 ABSTRACT In other papers already presented on the structure and dimensions of elemental hydrogen, the elementary particle dynamics was taken into account in order to be able to determine the size of the hydrogen. This new work, one comes back with a new dynamic hypothesis designed to fundamentally change again the dynamic particle size due to the impulse influence of the particle. Until now it has been assumed that the impulse of an elementary particle is equal to the mass of the particle multiplied by its velocity, but in reality, the impulse definition is different, which is derived from the translational kinetic energy in a rapport of its velocity. This produces an additional condensation of matter in its elemental form. Keywords: Particle structure; Impulse; Condensed matter. [http://creativecommons.org/licenses/by/3.0/us/] Licensed under a Creative Commons Attribution 3.0 United States License 1749 INDEPENDENT JOURNAL OF MANAGEMENT & PRODUCTION (IJM&P) http://www.ijmp.jor.br v. -
Primordially Hydridic Earth Viacheslav Zgonnik, Hervé Toulhoat, Vladimir Larin, Nikolay Larin
Primordially hydridic Earth Viacheslav Zgonnik, Hervé Toulhoat, Vladimir Larin, Nikolay Larin Abundances of elements on Earth’s crust relative to Sun’s photosphere and Si plotted versus first ionization potential (IP) • Clearly shows separation of elements by their IP • Outliers are due to use of only Earth’s crust composition • Tested with success for other planets, Moon and asteroids • Described by a Boltzmann distribution depending on the distance to the protosun • Predicts high initial content of hydrogen • Earth currently has about 4% by weight of hydrogen. • It is mainly combined as hydrides and partly dissolved into other phases http://arxiv.org/abs/1208.2909v2 Non-Ionizing UV (< 7 eV) Photochemistry of Cosmic Ice Analogs of Ammonia Radiolysis involves electron Photochemistry involves electron excitation due to particle radiation excitation without ionization in addition to all ionization – reactions initiated by cations – production of low-energy electron cascade – non-uniform distribution of reaction intermediates, non-selective chemistry leading to multiple reaction products We see production of N2 and N3 species with high- energy electrons and < 8 eV photons, but not with < 6 eV photons Islem Bouhali Soumaya Bezzaouia Mourad Telmini Theoretical study of Rydberg states of HeH+ ion using the Halfium model Christian Jungen Presented by: Islem Bouhali 2 HeH+ molecular ion in Born-Oppenheimer approximation e2 r12 Max(extern region e1 r2a GMQDT r r 1a 2b r1b Max(reaction surface R MATCHING ++ + He H Max( : reaction volume R-MATRIX Combination of the Variational R-matrix method and of the Generalized Multichannel Quantum Defect Theory Telmini and Jungen, Phys. Rev. A 68 062704 (2003). -
Fossil Corals As an Archive of Secular Variations in Seawater Chemistry Since the Mesozoic
Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 160 (2015) 188–208 www.elsevier.com/locate/gca Fossil corals as an archive of secular variations in seawater chemistry since the Mesozoic Anne M. Gothmann a,⇑, Jarosław Stolarski b, Jess F. Adkins c, Blair Schoene a, Kate J. Dennis a, Daniel P. Schrag d, Maciej Mazur e, Michael L. Bender a a Princeton University, Geosciences, Princeton, NJ, United States b Institute of Paleobiology, Polish Academy of Sciences, Warsaw, Poland c California Institute of Technology, Geological and Planetary Sciences, Pasadena, CA, United States d Harvard University, Earth and Planetary Sciences, Cambridge, MA, United States e University of Warsaw, Department of Chemistry, Warsaw, Poland Received 17 July 2014; accepted in revised form 16 March 2015; available online 25 March 2015 Abstract Numerous archives suggest that the major ion and isotopic composition of seawater have changed in parallel with large variations in geologic processes and Earth’s climate. However, our understanding of the mechanisms driving secular changes in seawater chemistry on geologic timescales is limited by the resolution of data in time, large uncertainties in seawater chem- istry reconstructions, and ambiguities introduced by sample diagenesis. We validated the preservation of a suite of 60 unrecrystallized aragonitic fossil scleractinian corals, ranging in age from Triassic through Recent, for use as new archives of past seawater chemistry. Optical and secondary electron microscopy (SEM) studies reveal that fossil coral crystal fabrics are similar to those of modern coralline aragonite. X-ray diffractometry (XRD), cathodoluminescence microscopy (CL), and Raman studies confirm that these specimens contain little to no secondary calcite. -
A Pilot Trap Survey of Artificial Reefs in New Jersey for Monitoring of Black Sea Bass, Tautog, and Lobster
Final Report Submitted to the New Jersey Department of Environmental Protection, Division of Fish and Wildlife for the following project: Project Title: A Pilot Trap Survey of Artificial Reefs in New Jersey for Monitoring of Black Sea Bass, Tautog, and Lobster Organization Name: Rutgers, the State University of New Jersey Principal Investigator: Dr. Olaf P. Jensen, Associate Professor, Rutgers University ([email protected], 410-812-4842) Project Co-Investigator: Dr. Douglas Zemeckis, Postdoctoral Researcher, Rutgers University ([email protected], 848-932-3450) NJDEP Project Manager: Peter Clarke, Fisheries Biologist, NJDEP Division of Fish and Wildlife ([email protected]) Performance Period: January 1, 2016 through April 1, 2019 Total Budget: $201,905.00 Table of Contents Introduction……………………………………………………………………………………...1 Project Objectives……………………………………………………………………………….6 Methods………………………………………………………………………………………......8 Study Design: Locations and Times……………………………………………………....8 Protocol: Field and Laboratory Methods…………………………………………………10 2016 Spring Seasonal Monitoring of Artificial Reefs…………………………………….11 2016 Summer Seasonal Monitoring of Artificial Reefs…………………………………..12 2016 Fall Seasonal Monitoring of Artificial Reefs………………………………………13 2017 Spring Seasonal Monitoring of Artificial Reefs…………………………………….14 2017 Summer Seasonal Monitoring of Artificial Reefs……………………………..……15 2017 Fall Seasonal Monitoring of Artificial Reefs………………………………………17 2018 Spring Seasonal Monitoring of Artificial Reefs……………………………………18 2018 Summer Seasonal