Annual Performance Report 2010/11 Science with a Mission, Women with Vision … Headscience in Herewith a Mission, Women with Vision

Total Page:16

File Type:pdf, Size:1020Kb

Annual Performance Report 2010/11 Science with a Mission, Women with Vision … Headscience in Herewith a Mission, Women with Vision AnnuAl performAnce report 2010/11 Science with a mission, women with vision … headScience in herewith a miSSion, women with viSion The United Nations has proclaimed 2011 as the International Year of Chemistry. At the same time the world celebrates the Centenary of International Women’s Day. In a remarkable confluence of events, 2011 is also the centennial of the Nobel Prize in Chemistry being awarded to Marie Curie for her work on radioactivity. As such, the National Research Foundation (NRF) feels it fitting to use these joint celebrations as the theme for its 2010/11 Annual Performance Report. The NRF joins in the global celebration of the chemical sciences, and their inspirational women researchers, upon which our lives and our future are based. NRF Annual Performance Report 2010/11 ISBN 978-1-86868-073-3 PO Box 2600 Pretoria 0001 Tel: +27 12 481-4000 Fax: +27 12 349-1179 E-mail: [email protected] www.nrf.ac.za ProducedProduced by by www.words-worth.co.zawww.words-worth.co.za contentS CHAIRMAN’S OVERVIEW . 4 Materiality framework . 20 Policy framework . 20 PRESIDENT AND CEO’S STATEMENT . 6 Sustainability management . 20 HIGHLIGHTS . 8 Corporate Human Resources and Transformation . 21 Performance management . 21 Remuneration . 21 BOARD REPORT . 11 Staff recruitment, turnover and succession planning . 22 Employment equity and organisational transformation . 22 NRF overview . 12 Suitably qualified staff . 23 NRF mandate . 12 Training and development . 23 NRF Vision 2015 . 12 Employee assistance . 24 NRF mission statement . 12 Labour relations climate . 24 NRF values . 12 NRF strategic goals . 13 Corporate Finance . 24 NRF core competencies . 13 Composition of the NRF . 13 NRF divisions . 27 South African Agency for Science and Technology The NRF Board . 13 Advancement (SAASTA) . 27 Governance functions of the NRF Board . 13 Purpose and scope . 28 Term of office of the NRF Board . 13 Human capacity development . 28 The NRF Board Members . 14 NRF Board Committees . 15 NRF divisions . 32 Purpose of Board Committees . 15 Research and Innovation Support and Advancement Composition of Board Committees . 15 (RISA) . 32 Meetings of the Board and its Committees . 15 Purpose and scope . 33 Remuneration of Board members . 16 Services . 33 Sources of funding . 33 . NRF governance structures and support 17 Investment policy . 33 . Advisory boards as at 31 March 2011 17 Investment areas . 34 . Strategic planning and reporting 17 RISA structure . 34 Enterprise risk management . 17 NRF ANNUAL PERFORMANCE REPORT 2010/11 | 1 contentS continued NRF divisions (continued) Biodiversity (SAIAB) . 53 RISA programmes . 34 – South African Environmental Network – Human and Institutional Capacity (SAEON) . .54 Development (HICD) . 34 – National Zoological Gardens of – Knowledge Fields Development (KFD) . 36 South Africa (NZG) . 55 – Applied Research and Innovation (ARI) . 39 – International Relations and Cooperation FINANCIAL REPORT . 63 (IR&C) . 39 Statement of responsibility by the Board of Directors . 64 – Knowledge Management and Evaluation Report of the Audit Committee . 65 (KM&E) . 39 Report of the Auditor-General . 66 – Grant Management and Systems Statement of Financial Position . 68 Administration (GMSA) . 41 Statement of Financial Performance . 69 Statement of changes in Net Assets . 70 National Research Facilities . 46 Cash Flow Statements . 71 Characteristics of National Research Facilities . 47 Accounting Policies . 72 Functions of National Research Facilities . 47 Notes to the Annual Financial Statements . 88 Clustering and structure . 47 Financial Information by Segment . 109 National Research Facilities . 48 KEY PERFORMANCE INDICATOR REPORT . 115 Nuclear Sciences . 48 Introduction . 117 – iThemba Laboratory for Accelerator Based Key performance measurements . 118 Sciences (iThemba LABS) . 48 Performance Report: Stakeholder Perspective . 128 Astro/Space/Geosciences . 49 Performance Report: Financial Perspective . 140 – South African Astronomical Performance Report: Organisational Perspective . 143 Observatory (SAAO) . 49 Performance Report: Organisational Learning and – Hartebeesthoek Radio Astronomy Growth Perspective . 144 Observatory (HartRAO) . .50 Performance Report: Human Resources – Hermanus Magnetic Observatory (HMO) . .51 and Transformation Perspective . 146 – Square Kilometre Array (SKA) South Africa Project . 52 PUBLICATIONS . 149 Biodiversity/Conservation/Environment . 53 – South African Institute for Aquatic ACRONYMS . 157 2 | NRF ANNUAL PERFORMANCE REPORT 2010/11 introduction introduction | ort the national research Foundation (NRF) is proud to present its annual P e Performance report for 2010/11. this report offers an overview of the r activities and performance of the NRF and highlights the impact of a small Board selection of NRF-supported research projects. IsiSwati – National Research Foundation (i-NRF) iyatigcabha IsiZulu – I-National Research Foundation (NRF) iyaziqhenya ngekwetfula Umbiko Wemnyaka wa-2010/11. Lombiko ngokwethula umbiko wayo wonyaka ka-2010/11. Lo mbiko usitfulela imisebenti kanye nekusebenta kwe-NRF kanye unikeza umbono jikelele ngemisebenzi kanye nokusebenza netibonelo temtselela yemiklamo lemincane yekuphenya kwe-NRF futhi ugqamisa umthelela wokhetho oluncane leyesekelwe yi-NRF. lwamaphrojekthi ocwaningo axhaswe yi-NRF. XiTsonga – National Research Foundation (NRF) ya TshiVenda – National Research foundation (NRF) i a ḓihudza tinyungubyisa ku andlala Xiviko xa yona xa Lembe ra 2010/11. kha u vha ṋetshedza Muvhigo waha wa 2010/11. Hoyu Xiviko lexi xi nyika mbalango wa migingiriko na matirhelo ya muvhigo u sumbedza mishumo yothe yo itwaho na kushumele NRF no kombisa ntshikelelo wa nhlayo yitsongo ya tiphurojeke kwa NRF na u tahisa zwe thandela thukhu dzo nanguludzwaho ta vulavisisi lebyi seketeriwaka hi NRF. dzo tikedzwaho nga NRF dza bveledza. Sepedi – National Research Foundation (NRF) ka boikgantšho IsiNdebele – National Research Foundation (NRF) e hlagiša Pego ya yona ya Ngwaga wa 2010/11. Pego ye e fa iyazikhakhazisa ekwethuleni umBiko womNyaka we-2010/11. tebelelokakaretšo ya mešomo le phethagatšo ya NRF gomme Lombiko unikela ngokurhunyeziweko imisebenzi eyenziwa e bontšha khuetšo ya kgetho ye nnyane ya diprotšeke tša yi-NRF begodu uveza imithelela yamaprojekte amancani dinyakišišo tšeo di thekgilwego ka ditšhelete ke NRF. werhubhulululo akhethiweko asekelwe yi-NRF. IsiXhosa – I-National Research Foundation (NRF) inebhongo Setswana – National Research Foundation (NRF) e motlotlo ngokuthi thaca kwayo iNgxelo yayo yoNyaka ka-2010/11. Le go tlhagisa Pegelo ya yona ya Ngwaga wa 2010/11. Pegelo ngxelo inika isishwankathelo semisebenzi kunye nokusebenza e e neelana ka tshekatsheko ya ditiro le go dira ga NRF le go kwe-NRF kwaye iqaqambisa iimpembelelo zemikhankaso supa bokao jwa karolo e nnye ya diporojeke tsa dipatlisiso tse di emincinane yophando ezixhaswa yi- NRF. tshegediwang ke NRF. Sesotho – National Research Foundation (NRF) e motlotlo ho Afrikaans – Die Nasionale Navorsingstigting (NNS) bied met fana ka Pehelo ya yona ya Selemo bakeng sa 2010/11. Pehelo trots sy Jaarverslag vir 2010/11 aan. Hierdie verslag bied ’n ena e nehelana ka kakaretso ya diketsahalo le mosebetsi wa oorsig oor die bedrywighede en werkverrigting van die NNS NRF mme e hlahisa dintlhakholo tsa sephetho sa karolo e en plaas klem op die impak van ’n beperkte keuse uit NNS- nyenyane ya diprojeke tsa diphuputso tse tshehetswang ke ondersteunde navorsingsprojekte. NRF. NRF ANNUAL PERFORMANCE REPORT 2010/11 | 3 chairman’S overview It is a privilege for me to present this NRF Annual Performance the delivery of a broad range of programmes supporting and Report, the last under my chairmanship. In this final reporting year fostering research and research capacity development. In line of the Board it is opportune to reflect on the main achievements with the review it is appropriate to mention as highlights the since 2008 and to consider the challenges that may lie ahead establishment of a smaller Corporate Executive team as part for the incoming Board. of a new governance structure, the goodwill of numerous local and international researchers who participated in the peer Strategic point OF departure review processes of the NRF, and flagship programmes such as The NRF strategic plan Vision 2015 was approved in 2008. the PhD project, the Blue Skies research programme, Centres Apart from being based on the mandate of the NRF as of Excellence (CoE) and the South African Research Chairs outlined in the National Research Foundation Act (Act No. 23 Initiative (SARChI)..
Recommended publications
  • Durham E-Theses
    Durham E-Theses First visibility of the lunar crescent and other problems in historical astronomy. Fatoohi, Louay J. How to cite: Fatoohi, Louay J. (1998) First visibility of the lunar crescent and other problems in historical astronomy., Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/996/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk me91 In the name of Allah, the Gracious, the Merciful >° 9 43'' 0' eji e' e e> igo4 U61 J CO J: lic 6..ý v Lo ý , ý.,, "ý J ýs ýºý. ur ý,r11 Lýi is' ý9r ZU LZJE rju No disaster can befall on the earth or in your souls but it is in a book before We bring it into being; that is easy for Allah. In order that you may not grieve for what has escaped you, nor be exultant at what He has given you; and Allah does not love any prideful boaster.
    [Show full text]
  • Atmob Newsletter
    Sperling received a BA from Michigan State University after graduating from Montgomery Blair High School in Silver Spring, Maryland. He followed that with an MA in History of Science from the University of California, Berkeley. He has taught STAR astronomy and related courses at Sonoma State University, California State University, Hayward, UC Berkeley, and San FIELDS Francisco State University. He has also taught many personal interest adult classes. Sperling currently lives in San Mateo, California. Norm founded the astronomical supplier and publisher blog, Newsletter of the Everything in the Universe, in 1977. He was an assistant editor Amateur Telescope Makers of Boston for Sky & Telescope magazine and, as of 2011, the editor and Including the Bond Astronomical Club publisher of the Journal of Irreproducible Results, a science Established in 1934 humor magazine. He has authored What Your Astronomy In the Interest of Telescope Making & Using Textbook Won’t Tell You and edited and published John Dobson's book How and Why to Make a User-Friendly Sidewalk Vol. 27, No. 7 July 2015 Telescope. He has also been published in Technology Review, Astronomy, Pacific Discovery, Journal of College Science Teaching, Mercury, Popular Astronomy, Telescope Making, This Month’s Meeting . Griffith Observer, and Reflector. Thursday, July 9th, 2015 at 8:00 PM Phillips Auditorium Norm also invented for Spherical Concepts, Inc. an acrylic Harvard-Smithsonian Center for Astrophysics globe named "The Stars Above", which is sold as a personal planetarium. Parking at the CfA is allowed for the duration of the meeting Please join us for a pre-meeting dinner discussion at Changsho, 1712 Mass Ave, Cambridge, MA at 6:00pm before the meeting.
    [Show full text]
  • POSTERS SESSION I: Atmospheres of Massive Stars
    Abstracts of Posters 25 POSTERS (Grouped by sessions in alphabetical order by first author) SESSION I: Atmospheres of Massive Stars I-1. Pulsational Seeding of Structure in a Line-Driven Stellar Wind Nurdan Anilmis & Stan Owocki, University of Delaware Massive stars often exhibit signatures of radial or non-radial pulsation, and in principal these can play a key role in seeding structure in their radiatively driven stellar wind. We have been carrying out time-dependent hydrodynamical simulations of such winds with time-variable surface brightness and lower boundary condi- tions that are intended to mimic the forms expected from stellar pulsation. We present sample results for a strong radial pulsation, using also an SEI (Sobolev with Exact Integration) line-transfer code to derive characteristic line-profile signatures of the resulting wind structure. Future work will compare these with observed signatures in a variety of specific stars known to be radial and non-radial pulsators. I-2. Wind and Photospheric Variability in Late-B Supergiants Matt Austin, University College London (UCL); Nevyana Markova, National Astronomical Observatory, Bulgaria; Raman Prinja, UCL There is currently a growing realisation that the time-variable properties of massive stars can have a funda- mental influence in the determination of key parameters. Specifically, the fact that the winds may be highly clumped and structured can lead to significant downward revision in the mass-loss rates of OB stars. While wind clumping is generally well studied in O-type stars, it is by contrast poorly understood in B stars. In this study we present the analysis of optical data of the B8 Iae star HD 199478.
    [Show full text]
  • Educator's Guide: Orion
    Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations.
    [Show full text]
  • Fy10 Budget by Program
    AURA/NOAO FISCAL YEAR ANNUAL REPORT FY 2010 Revised Submitted to the National Science Foundation March 16, 2011 This image, aimed toward the southern celestial pole atop the CTIO Blanco 4-m telescope, shows the Large and Small Magellanic Clouds, the Milky Way (Carinae Region) and the Coal Sack (dark area, close to the Southern Crux). The 33 “written” on the Schmidt Telescope dome using a green laser pointer during the two-minute exposure commemorates the rescue effort of 33 miners trapped for 69 days almost 700 m underground in the San Jose mine in northern Chile. The image was taken while the rescue was in progress on 13 October 2010, at 3:30 am Chilean Daylight Saving time. Image Credit: Arturo Gomez/CTIO/NOAO/AURA/NSF National Optical Astronomy Observatory Fiscal Year Annual Report for FY 2010 Revised (October 1, 2009 – September 30, 2010) Submitted to the National Science Foundation Pursuant to Cooperative Support Agreement No. AST-0950945 March 16, 2011 Table of Contents MISSION SYNOPSIS ............................................................................................................ IV 1 EXECUTIVE SUMMARY ................................................................................................ 1 2 NOAO ACCOMPLISHMENTS ....................................................................................... 2 2.1 Achievements ..................................................................................................... 2 2.2 Status of Vision and Goals ................................................................................
    [Show full text]
  • The Orbital Motion of the Quintuplet Cluster—A Common Origin for the Arches and Quintuplet Clusters?∗
    The Astrophysical Journal, 789:115 (20pp), 2014 July 10 doi:10.1088/0004-637X/789/2/115 C 2014. The American Astronomical Society. All rights reserved. Printed in the U.S.A. THE ORBITAL MOTION OF THE QUINTUPLET CLUSTER—A COMMON ORIGIN FOR THE ARCHES AND QUINTUPLET CLUSTERS?∗ A. Stolte1,B.Hußmann1, M. R. Morris2,A.M.Ghez2, W. Brandner3,J.R.Lu4, W. I. Clarkson5, M. Habibi1, and K. Matthews6 1 Argelander Institut fur¨ Astronomie, Auf dem Hugel¨ 71, D-53121 Bonn, Germany; [email protected] 2 Division of Astronomy and Astrophysics, UCLA, Los Angeles, CA 90095-1547, USA; [email protected], [email protected] 3 Max-Planck-Institut fur¨ Astronomie, Konigstuhl¨ 17, D-69117 Heidelberg, Germany; [email protected] 4 Institute for Astronomy, University of Hawai’i, 2680 Woodlawn Drive, Honolulu, HI 96822, USA; [email protected] 5 Department of Natural Sciences, University of Michigan-Dearborn, 125 Science Building, 4901 Evergreen Road, Dearborn, MI 48128, USA; [email protected] 6 Caltech Optical Observatories, California Institute of Technology, MS 320-47, Pasadena, CA 91225, USA; [email protected] Received 2014 January 16; accepted 2014 May 14; published 2014 June 20 ABSTRACT We investigate the orbital motion of the Quintuplet cluster near the Galactic center with the aim of constraining formation scenarios of young, massive star clusters in nuclear environments. Three epochs of adaptive optics high-angular resolution imaging with the Keck/NIRC2 and Very Large Telescope/NAOS-CONICA systems were obtained over a time baseline of 5.8 yr, delivering an astrometric accuracy of 0.5–1 mas yr−1.
    [Show full text]
  • Instrumental Methods for Professional and Amateur
    Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, Francois Colas, Alain Klotz, Christophe Pellier, Jean-Marc Petit, Philippe Rousselot, et al. To cite this version: Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, et al.. Instru- mental Methods for Professional and Amateur Collaborations in Planetary Astronomy. Experimental Astronomy, Springer Link, 2014, 38 (1-2), pp.91-191. 10.1007/s10686-014-9379-0. hal-00833466 HAL Id: hal-00833466 https://hal.archives-ouvertes.fr/hal-00833466 Submitted on 3 Jun 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy O. Mousis, R. Hueso, J.-P. Beaulieu, S. Bouley, B. Carry, F. Colas, A. Klotz, C. Pellier, J.-M. Petit, P. Rousselot, M. Ali-Dib, W. Beisker, M. Birlan, C. Buil, A. Delsanti, E. Frappa, H. B. Hammel, A.-C. Levasseur-Regourd, G. S. Orton, A. Sanchez-Lavega,´ A. Santerne, P. Tanga, J. Vaubaillon, B. Zanda, D. Baratoux, T. Bohm,¨ V. Boudon, A. Bouquet, L. Buzzi, J.-L. Dauvergne, A.
    [Show full text]
  • Variable Star Classification and Light Curves Manual
    Variable Star Classification and Light Curves An AAVSO course for the Carolyn Hurless Online Institute for Continuing Education in Astronomy (CHOICE) This is copyrighted material meant only for official enrollees in this online course. Do not share this document with others. Please do not quote from it without prior permission from the AAVSO. Table of Contents Course Description and Requirements for Completion Chapter One- 1. Introduction . What are variable stars? . The first known variable stars 2. Variable Star Names . Constellation names . Greek letters (Bayer letters) . GCVS naming scheme . Other naming conventions . Naming variable star types 3. The Main Types of variability Extrinsic . Eclipsing . Rotating . Microlensing Intrinsic . Pulsating . Eruptive . Cataclysmic . X-Ray 4. The Variability Tree Chapter Two- 1. Rotating Variables . The Sun . BY Dra stars . RS CVn stars . Rotating ellipsoidal variables 2. Eclipsing Variables . EA . EB . EW . EP . Roche Lobes 1 Chapter Three- 1. Pulsating Variables . Classical Cepheids . Type II Cepheids . RV Tau stars . Delta Sct stars . RR Lyr stars . Miras . Semi-regular stars 2. Eruptive Variables . Young Stellar Objects . T Tau stars . FUOrs . EXOrs . UXOrs . UV Cet stars . Gamma Cas stars . S Dor stars . R CrB stars Chapter Four- 1. Cataclysmic Variables . Dwarf Novae . Novae . Recurrent Novae . Magnetic CVs . Symbiotic Variables . Supernovae 2. Other Variables . Gamma-Ray Bursters . Active Galactic Nuclei 2 Course Description and Requirements for Completion This course is an overview of the types of variable stars most commonly observed by AAVSO observers. We discuss the physical processes behind what makes each type variable and how this is demonstrated in their light curves. Variable star names and nomenclature are placed in a historical context to aid in understanding today’s classification scheme.
    [Show full text]
  • 121012-AAS-221 Program-14-ALL, Page 253 @ Preflight
    221ST MEETING OF THE AMERICAN ASTRONOMICAL SOCIETY 6-10 January 2013 LONG BEACH, CALIFORNIA Scientific sessions will be held at the: Long Beach Convention Center 300 E. Ocean Blvd. COUNCIL.......................... 2 Long Beach, CA 90802 AAS Paper Sorters EXHIBITORS..................... 4 Aubra Anthony ATTENDEE Alan Boss SERVICES.......................... 9 Blaise Canzian Joanna Corby SCHEDULE.....................12 Rupert Croft Shantanu Desai SATURDAY.....................28 Rick Fienberg Bernhard Fleck SUNDAY..........................30 Erika Grundstrom Nimish P. Hathi MONDAY........................37 Ann Hornschemeier Suzanne H. Jacoby TUESDAY........................98 Bethany Johns Sebastien Lepine WEDNESDAY.............. 158 Katharina Lodders Kevin Marvel THURSDAY.................. 213 Karen Masters Bryan Miller AUTHOR INDEX ........ 245 Nancy Morrison Judit Ries Michael Rutkowski Allyn Smith Joe Tenn Session Numbering Key 100’s Monday 200’s Tuesday 300’s Wednesday 400’s Thursday Sessions are numbered in the Program Book by day and time. Changes after 27 November 2012 are included only in the online program materials. 1 AAS Officers & Councilors Officers Councilors President (2012-2014) (2009-2012) David J. Helfand Quest Univ. Canada Edward F. Guinan Villanova Univ. [email protected] [email protected] PAST President (2012-2013) Patricia Knezek NOAO/WIYN Observatory Debra Elmegreen Vassar College [email protected] [email protected] Robert Mathieu Univ. of Wisconsin Vice President (2009-2015) [email protected] Paula Szkody University of Washington [email protected] (2011-2014) Bruce Balick Univ. of Washington Vice-President (2010-2013) [email protected] Nicholas B. Suntzeff Texas A&M Univ. suntzeff@aas.org Eileen D. Friel Boston Univ. [email protected] Vice President (2011-2014) Edward B. Churchwell Univ. of Wisconsin Angela Speck Univ. of Missouri [email protected] [email protected] Treasurer (2011-2014) (2012-2015) Hervey (Peter) Stockman STScI Nancy S.
    [Show full text]
  • 2012 Annual Progress Report and 2013 Program Plan of the Gemini Observatory
    2012 Annual Progress Report and 2013 Program Plan of the Gemini Observatory Association of Universities for Research in Astronomy, Inc. Table of Contents 0 Executive Summary ....................................................................................... 1 1 Introduction and Overview .............................................................................. 5 2 Science Highlights ........................................................................................... 6 2.1 Highest Resolution Optical Images of Pluto from the Ground ...................... 6 2.2 Dynamical Measurements of Extremely Massive Black Holes ...................... 6 2.3 The Best Standard Candle for Cosmology ...................................................... 7 2.4 Beginning to Solve the Cooling Flow Problem ............................................... 8 2.5 A Disappearing Dusty Disk .............................................................................. 9 2.6 Gas Morphology and Kinematics of Sub-Millimeter Galaxies........................ 9 2.7 No Intermediate-Mass Black Hole at the Center of M71 ............................... 10 3 Operations ...................................................................................................... 11 3.1 Gemini Publications and User Relationships ............................................... 11 3.2 Science Operations ........................................................................................ 12 3.2.1 ITAC Software and Queue Filling Results ..................................................
    [Show full text]
  • Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
    Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis,
    [Show full text]
  • 1910Ap J 31 8B on a GREAT NEBULOUS REGION
    8B 31 J 1910Ap ON A GREAT NEBULOUS REGION AND ON THE QUES- TION OF ABSORBING MATTER IN SPACE AND THE TRANSPARENCY OF THE NEBULAE By E. E. BARNARD While photographing the region of the great nebula of p Ophiuchi (which I had found with the Willard lens) at the Lick Observatory in 1893, the plates with the small lantern lens (ii inches diameter, also attached to the Willard mounting) showed a remarkable nebula involving the 4.5 magnitude star v Scorpii (Plate I). It had not been noticed on the Willard lens photograph, where it was very faint and near the edge of the plate. The discovery of this object therefore is due to the small lantern lens. Roughly this nebula is bounded by the figure formed by the follow- ing places (for 1855.0) : a S f j i5h 59m —180 2o/ 16 4 —18 o and 16 10 —21 00 16 16 —18 50 In its fainter portions it involves to the southeast the stars B. D. i9?4357, —19?4359, and — i9?436i. The last two are in a dense nebulous mass in which on the north following side close to the stars are a thin dark lane and a narrow strip of brighter nebulosity. These two stars are joined to —19?4357, which is itself nebulous, by a thin thread of nebulosity which is well shown in Plate II A. North and following these objects are dark regions where there are apparently very few stars. The extensions of this great nebula reach to, and in a feeble manner connect with, the great nebula of p Ophiuchi.
    [Show full text]