DOCSLIB.ORG

88481 Txtmvpr3

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
88481 Txtmvpr3 YEAR BOOK 00/01 2000–2001 CARNEGIE INSTITUTION OF WASHINGTON 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 Opening New Horizons for Scientific Research YEAR BOOK 00/01 2000-2001 GIVING TO THE CARNEGIE INSTITUTION OF WASHINGTON IN 2002 Opening New Horizons for Scientific Research Friends can help the institution financially in many ways, including making a simple pledge of a bequest, an outright gift of cash or securities, or more complex forms of planned giving. The Carnegie Institution is a tax-exempt 501(C)(3) organization under the Internal Revenue Code. Contributions to the institution are eligible for a charitable deduction on your income tax as provided by law. We recommend that you consult your attorney or tax adviser about your individual circumstances when considering a substantial gift. The following are general guidelines: Outright gifts of cash or securities enable you, if you itemize, to take a charitable deduction on your income tax. Gifts of cash are deductible up to 30% of the donor’s adjusted income in the year of the gift. A gift in excess of this 30% limitation may be carried forward for up to five additional years within the same limitations of the law. Gifts of securities are deductible up to 20% of the donor’s adjusted income in the year of the gift. A gift in excess of this 20% limitation may be carried forward for up to five additional years within the same limitations of the law. Donors to private foundations may deduct the fair market value, not just the cost, of publicly traded securities that have risen in value over a period of years. This may allow the donor to avoid paying capital gains tax on these appreciated securities. If you are interested in making a gift of securities, you may contact the institution for assistance. Because the needs of the institution are long term, bequests are a thoughtful way to make a substantial contribution. You can use the following simple statement in your will: “I hereby give, and bequeath the sum of $_______ (or % of my residuary estate) to the Carnegie Institution of Washington, 1530 P Street, N.W., Washington, DC 20005-1910.” OnOn the the cover: cover: Above: This is a simulation of what happens to magnetic metal ions in iron oxide and cobalt oxide as pressure increases. (Courtesy Ronald Cohen, Geophysical Laboratory.) For additional information, please see the Carnegie website at www.CarnegieInstitution.org or call Linda Feinberg in the Office of External Below: Chen-Ming Fan uses the mouse in his research on the genetics of development. This is an image of a Affairs, 202.939.1141, or write: developing cerebellum in that model organism. (See page 49.) Linda Feinberg Office of External Affairs CARNEGIE INSTITUTION OF WASHINGTON 1530 P Street, N.W. Washington, DC 20005 THE PRESIDENT’ S REPORT Year Book 00/01 July 1, — June 30, CARNEGIE INSTITUTION OF WASHINGTON Department of Embryology ABOUT CARNEGIE 115 West University Parkway Baltimore, MD 21210-3301 410.554.1200 . TO ENCOURAGE, IN THE BROADEST AND Department of Plant Biology MOST LIBERAL MANNER, INVESTIGATION, 260 Panama St. RESEARCH, AND DISCOVERY, AND THE Stanford, CA 94305-4101 650.325.1521 APPLICATION OF KNOWLEDGE TO THE Geophysical Laboratory IMPROVEMENT OF MANKIND . 5251 Broad Branch Rd., N.W. Washington, DC 20015-1305 202.478.8900 The Carnegie Institution of Washington Department of Terrestrial Magnetism was incorporated with these words in 1902 5241 Broad Branch Rd., N.W. Washington, DC 20015-1305 by its founder, Andrew Carnegie. Since 202.478.8820 then, the institution has remained true to The Carnegie Observatories 813 Santa Barbara St. its mission. At five research departments Pasadena, CA 91101-1292 across the country, the scientific staff and 626.577.1122 a constantly changing roster of students, Las Campanas Observatory Casilla 601 postdoctoral fellows, and visiting investiga- La Serena, Chile tors tackle fundamental questions on the Office of Administration 1530 P St., N.W. frontiers of biology, earth sciences, and Washington, DC 20005-1910 202.387.6400 astronomy. http://www.CarnegieInstitution.org ISSN 0069-066X Design by Hasten Design, Washington, DC Printing by Mount Vernon Printing, Landover, MD February 2002 CONTENTS The President’s Commentary Losses, Gains, Honors Contributions, Grants, and Private Gifts First Light and CASE Geophysical Laboratory Department of Plant Biology Department of Embryology The Observatories Department of Terrestrial Magnetism Extradepartmental and Administrative Financial Statements Index of Names A supplemental electronic version of the Year Book is accessible via the Internet at www.CarnegieInstitution.org/yearbook.html. The electronic version includes individual essays by Carnegie scientists in addition to the material in this print publication. Former Presidents &Trustees PRESIDENTS Walter S. Gifford, 1931–1966 Franklin D. Murphy, 1978–1985 Carl J. Gilbert, 1962–1983 William I. Myers, 1948–1976 Daniel Coit Gilman, 1902–1904 Cass Gilbert, 1924–1934 Garrison Norton, 1960–1974 Robert S. Woodward, 1904-1920 Frederick H. Gillett, 1924–1935 Paul F. Oreffice, 1988–1993 John C. Merriam, 1921-1938 Daniel C. Gilman, 1902–1908 William Church Osborn, 1927–1934 Vannevar Bush, 1939–1955 Hanna H. Gray, 1974–1978 Walter H. Page, 1971–1979 Caryl P. Haskins, 1956–1971 Crawford H. Greenewalt, 1952–1984 James Parmelee, 1917–1931 Philip H. Abelson, 1971–1978 William C. Greenough, 1975–1989 William Barclay Parsons, 1907–1932 James D. Ebert, 1978–1987 Patrick E. Haggerty, 1974–1975 Stewart Paton, 1916–1942 Edward E. David, Jr. (Acting President, John Hay, 1902–1905 Robert N. Pennoyer, 1968–1989 1987–1988) Barklie McKee Henry, 1949–1966 George W. Pepper, 1914–1919 Myron T. Herrick, 1915–1929 John J. Pershing, 1930–1943 TRUSTEES Abram S. Hewitt, 1902–1903 Henning W. Prentis, Jr., 1942–1959 William R. Hewlett, 1971–2001 Henry S. Pritchett, 1906–1936 Alexander Agassiz, 1904–1905 Henry L. Higginson, 1902–1919 Gordon S. Rentschler, 1946–1948 Robert O. Anderson, 1976–1983 Ethan A. Hitchcock, 1902–1909 Sally K. Ride, 1989–1994 Lord Ashby of Brandon, 1967–1974 Henry Hitchcock, 1902 David Rockefeller, 1952–1956 J. Paul Austin, 1976–1978 Herbert Hoover, 1920–1949 Elihu Root, 1902–1937 George G. Baldwin, 1925–1927 William Wirt Howe, 1903–1909 Elihu Root, Jr., 1937–1967 Thomas Barbour, 1934–1946 Charles L. Hutchinson, 1902–1904 Julius Rosenwald, 1929–1931 James F. Bell, 1935–1961 Walter A. Jessup, 1938–1944 William M. Roth, 1968–1979 John S. Billings, 1902–1913 Frank B. Jewett, 1933–1949 William W. Rubey, 1962–1974 Robert Woods Bliss, 1936–1962 George F. Jewett, Jr., 1983–1987 Martin A. Ryerson, 1908–1928 Amory H. Bradford, 1959–1972 Antonia Ax:son Johnson, 1980–1994 Howard A. Schneiderman, 1988–1990 Lindsay Bradford, 1940–1958 William F. Kieschnick, 1985–1991 Henry R. Shepley, 1937–1962 Omar N. Bradley, 1948–1969 Samuel P. Langley, 1904–1906 Theobald Smith, 1914–1934 Lewis M. Branscomb, 1973–1990 Kenneth G. Langone, 1993–1994 John C. Spooner, 1902–1907 Robert S. Brookings, 1910–1929 Ernest O. Lawrence, 1944–1958 William Benson Storey, 1924–1939 James E. Burke, 1989–1993 Charles A. Lindbergh, 1934–1939 Richard P. Strong, 1934–1948 Vannevar Bush, 1958–1971 William Lindsay, 1902–1909 Charles P. Taft, 1936–1975 John L. Cadwalader, 1903–1914 Henry Cabot Lodge, 1914–1924 William H. Taft, 1906–1915 William W. Campbell, 1929–1938 Alfred L. Loomis, 1934–1973 William S. Thayer, 1929–1932 John J. Carty, 1916–1932 Robert A. Lovett, 1948–1971 Juan T. Trippe, 1944–1981 Whitefoord R. Cole, 1925–1934 Seth Low, 1902–1916 James W. Wadsworth, 1932–1952 John T. Connor, 1975–1980 Wayne MacVeagh, 1902–1907 Charles D. Walcott, 1902–1927 Frederic A. Delano, 1927–1949 William McChesney Martin, 1967–1983 Frederic C. Walcott, 1931–1948 Cleveland H. Dodge, 1903–1923 Keith S. McHugh, 1950–1974 Henry P. Walcott, 1910–1924 William E. Dodge, 1902–1903 Andrew W. Mellon, 1924–1937 Lewis H. Weed, 1935–1952 James D. Ebert, 1987–2001 John C. Merriam, 1921–1938 William H. Welch, 1906–1934 Gerald M. Edelman, 1980–1987 J. Irwin Miller, 1988–1991 Gunnar Wessman, 1984–1987 Charles P. Fenner, 1914–1924 Margaret Carnegie Miller, 1955–1967 Andrew D. White, 1902–1916 Michael Ference, Jr., 1968–1980 Roswell Miller, 1933–1955 Edward D. White, 1902–1903 Homer L. Ferguson, 1927–1952 Darius O. Mills, 1902–1909 Henry White, 1913–1927 Simon Flexner, 1910–1914 S. Weir Mitchell, 1902–1914 James N. White, 1956–1979 W. Cameron Forbes, 1920–1955 Andrew J. Montague, 1907–1935 George W. Wickersham, 1909–1936 James Forrestal, 1948–1949 Henry S. Morgan, 1936–1978 Robert E. Wilson, 1953–1964 William N. Frew, 1902–1915 William W. Morrow, 1902–1929 Robert S. Woodward, 1905–1924 Lyman J. Gage, 1902–1912 Seeley G. Mudd, 1940–1968 Carroll D. Wright, 1902–1908 T rustees Thomas N. Urban, Chairman William I. M. Turner, Jr., Vice-Chairman David Greenewalt, Secretary Philip H. Abelson Euan Baird Daniel N. Belin William T. Coleman, Jr., Senior Trustee Tom Cori John F. Crawford Edward E. David, Jr., Emeritus John Diebold W. Gary Ernst Sandra M. Faber Bruce W. Ferguson Stephen P. A. Fodor Michael E. Gellert Robert G. Goelet William T. Golden, Senior Trustee Caryl P. Haskins, Emeritus William R. Hearst III Richard E. Heckert, Emeritus Kazuo Inamori Suzanne Nora Johnson Gerald D. Laubach, Senior Trustee John D. Macomber, Senior Trustee Steven L. McKnight Burton J. McMurtry Jaylee Mead Richard A. Meserve Richard S. Perkins, Emeritus Frank Press, Senior Trustee Deborah Rose William J. Rutter Robert C. Seamans, Jr., Emeritus Frank Stanton, Emeritus Christopher T. S. Stone David F. Swensen Charles H. Townes, Emeritus Sidney J.
Load more

Recommended publications
  • 100 Closest Stars Designation R.A
    100 closest stars Designation R.A. Dec. Mag. Common Name 1 Gliese+Jahreis 551 14h30m –62°40’ 11.09 Proxima Centauri Gliese+Jahreis 559 14h40m –60°50’ 0.01, 1.34 Alpha Centauri A,B 2 Gliese+Jahreis 699 17h58m 4°42’ 9.53 Barnard’s Star 3 Gliese+Jahreis 406 10h56m 7°01’ 13.44 Wolf 359 4 Gliese+Jahreis 411 11h03m 35°58’ 7.47 Lalande 21185 5 Gliese+Jahreis 244 6h45m –16°49’ -1.43, 8.44 Sirius A,B 6 Gliese+Jahreis 65 1h39m –17°57’ 12.54, 12.99 BL Ceti, UV Ceti 7 Gliese+Jahreis 729 18h50m –23°50’ 10.43 Ross 154 8 Gliese+Jahreis 905 23h45m 44°11’ 12.29 Ross 248 9 Gliese+Jahreis 144 3h33m –9°28’ 3.73 Epsilon Eridani 10 Gliese+Jahreis 887 23h06m –35°51’ 7.34 Lacaille 9352 11 Gliese+Jahreis 447 11h48m 0°48’ 11.13 Ross 128 12 Gliese+Jahreis 866 22h39m –15°18’ 13.33, 13.27, 14.03 EZ Aquarii A,B,C 13 Gliese+Jahreis 280 7h39m 5°14’ 10.7 Procyon A,B 14 Gliese+Jahreis 820 21h07m 38°45’ 5.21, 6.03 61 Cygni A,B 15 Gliese+Jahreis 725 18h43m 59°38’ 8.90, 9.69 16 Gliese+Jahreis 15 0h18m 44°01’ 8.08, 11.06 GX Andromedae, GQ Andromedae 17 Gliese+Jahreis 845 22h03m –56°47’ 4.69 Epsilon Indi A,B,C 18 Gliese+Jahreis 1111 8h30m 26°47’ 14.78 DX Cancri 19 Gliese+Jahreis 71 1h44m –15°56’ 3.49 Tau Ceti 20 Gliese+Jahreis 1061 3h36m –44°31’ 13.09 21 Gliese+Jahreis 54.1 1h13m –17°00’ 12.02 YZ Ceti 22 Gliese+Jahreis 273 7h27m 5°14’ 9.86 Luyten’s Star 23 SO 0253+1652 2h53m 16°53’ 15.14 24 SCR 1845-6357 18h45m –63°58’ 17.40J 25 Gliese+Jahreis 191 5h12m –45°01’ 8.84 Kapteyn’s Star 26 Gliese+Jahreis 825 21h17m –38°52’ 6.67 AX Microscopii 27 Gliese+Jahreis 860 22h28m 57°42’ 9.79,
    [Show full text]
  • Abstract a Search for Extrasolar Planets Using Echoes Produced in Flare Events
    ABSTRACT A SEARCH FOR EXTRASOLAR PLANETS USING ECHOES PRODUCED IN FLARE EVENTS A detection technique for searching for extrasolar planets using stellar flare events is explored, including a discussion of potential benefits, potential problems, and limitations of the method. The detection technique analyzes the observed time versus intensity profile of a star’s energetic flare to determine possible existence of a nearby planet. When measuring the pulse of light produced by a flare, the detection of an echo may indicate the presence of a nearby reflective surface. The flare, acting much like the pulse in a radar system, would give information about the location and relative size of the planet. This method of detection has the potential to give science a new tool with which to further humankind’s understanding of planetary systems. Randal Eugene Clark May 2009 A SEARCH FOR EXTRASOLAR PLANETS USING ECHOES PRODUCED IN FLARE EVENTS by Randal Eugene Clark A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science in Physics in the College of Science and Mathematics California State University, Fresno May 2009 © 2009 Randal Eugene Clark APPROVED For the Department of Physics: We, the undersigned, certify that the thesis of the following student meets the required standards of scholarship, format, and style of the university and the student's graduate degree program for the awarding of the master's degree. Randal Eugene Clark Thesis Author Fred Ringwald (Chair) Physics Karl Runde Physics Ray Hall Physics For the University Graduate Committee: Dean, Division of Graduate Studies AUTHORIZATION FOR REPRODUCTION OF MASTER’S THESIS X I grant permission for the reproduction of this thesis in part or in its entirety without further authorization from me, on the condition that the person or agency requesting reproduction absorbs the cost and provides proper acknowledgment of authorship.
    [Show full text]
  • Salubrious Living
    Salubrious Living 00. Salubrious Living - Introduction 01. The Search for Youth 02. The Myth of Medical Progress 03. The Hygienic System 04. The Nature of Disease 05. The Foods of Civilization 06. The Foods of Primitive Man 07. Don't Cook Your Foods 08. The Fruitarian Diet 09. How to Plan Your Meals 10. The Best Sources of Minerals and Vitamins 11. Soil and Food 12. Nature's Supreme Healing Agency 13. The Value of Heliotherapy 14. Building Strength and Health Through Exercise 15. Some Common Ailments 16. Why Lose Your Teeth? 17. Better Vision Without Glasses 18. Building Strong Feet 19. Keep Your Hair 20. The Needs of Infants and Growing Children 21. To Build Beauty You Must Build Health 22. Eugenics and the Survival of the White Race Author: Ben Klassen Format: Paperback Creativity Book Publisher Pub. Date: 1982 Food Chart Copyright © 2003 by World Church of Creativity Salubrious Living - Introduction The term "Salubrious Living" is a nomenclature I have coined as part and parcel of a very important facet of our religious creed and program set forth by the CHURCH OF THE CREATOR. The word "salubrious" comes from the Latin word "salubris" meaning "healthy; wholesome; sound; useful; vigorous". Webster's dictionary defines the English derivative "salubrious" as: 1. favorable to, or promoting health or well being; invigorating; 2. spiritually wholesome; conducive to good results". It is in this context of fully promoting the health and well being of the White Race that we use this term in its true literal meaning. We of the CHURCH OF THE CREATOR want to differentiate this term from "Natural Hygiene popularly used for many decades by health practitioners devoted to this worthy art and science.
    [Show full text]
  • The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
    THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile.
    [Show full text]
  • Lick Observatory Records: Photographs UA.036.Ser.07
    http://oac.cdlib.org/findaid/ark:/13030/c81z4932 Online items available Lick Observatory Records: Photographs UA.036.Ser.07 Kate Dundon, Alix Norton, Maureen Carey, Christine Turk, Alex Moore University of California, Santa Cruz 2016 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Lick Observatory Records: UA.036.Ser.07 1 Photographs UA.036.Ser.07 Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Photographs Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.07 Physical Description: 101.62 Linear Feet127 boxes Date (inclusive): circa 1870-2002 Language of Material: English . https://n2t.net/ark:/38305/f19c6wg4 Conditions Governing Access Collection is open for research. Conditions Governing Use Property rights for this collection reside with the University of California. Literary rights, including copyright, are retained by the creators and their heirs. The publication or use of any work protected by copyright beyond that allowed by fair use for research or educational purposes requires written permission from the copyright owner. Responsibility for obtaining permissions, and for any use rests exclusively with the user. Preferred Citation Lick Observatory Records: Photographs. UA36 Ser.7. Special Collections and Archives, University Library, University of California, Santa Cruz. Alternative Format Available Images from this collection are available through UCSC Library Digital Collections. Historical note These photographs were produced or collected by Lick observatory staff and faculty, as well as UCSC Library personnel. Many of the early photographs of the major instruments and Observatory buildings were taken by Henry E. Matthews, who served as secretary to the Lick Trust during the planning and construction of the Observatory.
    [Show full text]
  • South Pole-Aitken Basin
    Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole.
    [Show full text]
  • July 2019 Medicine’S Lunar Legacies • René T
    OslerianaA Medical Humanities Journal-Magazine Volume 1 • July 2019 Medicine’s Lunar Legacies • René T. H. Laennec Walter R. Bett • Leonardo da Vinci OslerianaA Medical Humanities Journal-Magazine Editor-in-Chief Nadeem Toodayan MBBS Associate Editor Zaheer Toodayan MBBS Corrigendum: As indicated in the introductory piece to this journal and in footnotes to their respective articles, both editors are Basic Physician Trainees and therefore registered members of the Royal Australasian College of Physicians (RACP). In the initial printing of this volume (on this inner cover and on page 5) the postnominal of ‘MRACP’ was used to refer to the editors’ membership status. This postnominal was first applied to the Edi- tor-in-Chief in formal correspondence from The Osler Club of London. Subsequent discussions with the RACP have confirmed that the postnominal is not formally endorsed by the College for trainee members and so it has been removed in this digital edition. Osleriana – Volume 1 Published July 2019 © The William Osler Society of Australia & New Zealand (WOSANZ) e-mail: [email protected] All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, digital, print, photocopy, recording or otherwise, without the prior written permission of WOSANZ or the individual author(s). Permission to reproduce any copyrighted images used in this publication must be obtained from the appropriate rightsholder(s). Please contact WOSANZ for further information as required. Privately printed in Brisbane, Queensland, by Clark & Mackay Printers. Journal concept and WOSANZ logo by Nadeem Toodayan. Journal design and layout by Zaheer Toodayan.
    [Show full text]
  • Lasker Interactive Research Nom'18.Indd
    THE 2018 LASKER MEDICAL RESEARCH AWARDS Nomination Packet albert and mary lasker foundation November 1, 2017 Greetings: On behalf of the Albert and Mary Lasker Foundation, I invite you to submit a nomination for the 2018 Lasker Medical Research Awards. Since 1945, the Lasker Awards have recognized the contributions of scientists, physicians, and public citizens who have made major advances in the understanding, diagnosis, treatment, cure, and prevention of disease. The Medical Research Awards will be offered in three categories in 2018: Basic Research, Clinical Research, and Special Achievement. The Lasker Foundation seeks nominations of outstanding scientists; nominations of women and minorities are encouraged. Nominations that have been made in previous years are not automatically reconsidered. Please see the Nomination Requirements section of this booklet for instructions on updating and resubmitting a nomination. The Foundation accepts electronic submissions. For information on submitting an electronic nomination, please visit www.laskerfoundation.org. Lasker Awards often presage future recognition of the Nobel committee, and they have become known popularly as “America’s Nobels.” Eighty-seven Lasker laureates have received the Nobel Prize, including 40 in the last three decades. Additional information on the Awards Program and on Lasker laureates can be found on our website, www.laskerfoundation.org. A distinguished panel of jurors will select the scientists to be honored with Lasker Medical Research Awards. The 2018 Awards will
    [Show full text]
  • Index to JRASC Volumes 61-90 (PDF)
    THE ROYAL ASTRONOMICAL SOCIETY OF CANADA GENERAL INDEX to the JOURNAL 1967–1996 Volumes 61 to 90 inclusive (including the NATIONAL NEWSLETTER, NATIONAL NEWSLETTER/BULLETIN, and BULLETIN) Compiled by Beverly Miskolczi and David Turner* * Editor of the Journal 1994–2000 Layout and Production by David Lane Published by and Copyright 2002 by The Royal Astronomical Society of Canada 136 Dupont Street Toronto, Ontario, M5R 1V2 Canada www.rasc.ca — [email protected] Table of Contents Preface ....................................................................................2 Volume Number Reference ...................................................3 Subject Index Reference ........................................................4 Subject Index ..........................................................................7 Author Index ..................................................................... 121 Abstracts of Papers Presented at Annual Meetings of the National Committee for Canada of the I.A.U. (1967–1970) and Canadian Astronomical Society (1971–1996) .......................................................................168 Abstracts of Papers Presented at the Annual General Assembly of the Royal Astronomical Society of Canada (1969–1996) ...........................................................207 JRASC Index (1967-1996) Page 1 PREFACE The last cumulative Index to the Journal, published in 1971, was compiled by Ruth J. Northcott and assembled for publication by Helen Sawyer Hogg. It included all articles published in the Journal during the interval 1932–1966, Volumes 26–60. In the intervening years the Journal has undergone a variety of changes. In 1970 the National Newsletter was published along with the Journal, being bound with the regular pages of the Journal. In 1978 the National Newsletter was physically separated but still included with the Journal, and in 1989 it became simply the Newsletter/Bulletin and in 1991 the Bulletin. That continued until the eventual merger of the two publications into the new Journal in 1997.
    [Show full text]
  • Map Showing the Clusters That Can Be Reached Using One
    Castor cluster HYG 542 6.3 7.2 Map of nearby space 2320AD HD 145 3.8 Beta Tucanae cluster HYG 664 HD 2749 6.6 13 Cas Based on information in 2320AD by Colin Dunn, Near Star 6.3 5.8 5.7 List II by Andy Brick and the HYG database by David Nash. Bet1TucBet2Tuc HD 164181 7.3 6.76.7 5.8 HD 2785 7.1 HD 2712 Boxes represent connected clusters of more than10 stars that HD 2779 3.8 4.8 HD 2665155 HD 417 7.2 HD 183 HD 2784 7.2 7.2 HD 336 can be reached by stutterwarp tug from normally reachable HD 375 HYG 716 2.8 7.27.1 5.2 HD 442 7.1 HD 446 7.5 stars. Striped lines denote tug-links. 7.2 6.0 HD 135 5.6 5.9 7.3 HD 2589 6.6 HD 2762 6.9 HD 2766 6.7 HD 383 2.0 3.3 7.3 HD 457 HD 277 6.9 7.2 HD 434 6.6 HD 429 5.5 HD 319 6.3 HD 208 7.0 HD 2829 HD 162 4.3 HD 2804 5.5 5.5 6.9 4.8 5.5 HD 2815 HD 236 HD 458 5.6 5.8 HD 216 HDHD 2711 290 2.6 3.2 4.0 HD 279 7.5 6.8 HYG 587 14Lam CasHD 2882 5.7 HD 441 7.1 1.5 3.6 4.6 7.1 7.0 6.7 HYG 2433 HD 233 4.8 3.3 5.7 5.1 7.3 7.4 HD 425 6.4 7.2 HD 406 7.6 HYG 2495 7.0 7.4 HDHD 2663 299 7.1 6.6 HD 483 HD 334 6.9 2.2 HD 2893 6.7 7.3 7.6 HD 449 HD 512 3.1 4.2 HD 2839 HD 464 11.3 5.4 HD 313 6.5 HYG 762 5.8 6.3 Gl 6 9.1 0.5 HD 28367.5 9.1 HD 2871 10.4 5.8 7.5 6.6 5.1 3.4 6.7 7.7 7.7 5.1 HYGHD 5212538 HD 422 HD 2775 6.8 4.4 7.6 6.8 10.1 8.7 5.8 HYG 739 6.4 6.2 3.4 9.3 6.6 7.6 HD 2837 HYGHD 4522493 6.4 HD 403 6.1 6.8 9.1 9.5 HD 2833 HYG 751 6.7 4.2 3.1 3.9 6.6 HD 505 5.8 6.6 HD 225 10.2 3.8 8.0 0.5 11.5 HD 2873 HD 2826 HD 28232798 4.9 HD 2806 HD 2702 6.1 HD 404 HD 538 7.6 4.5 HD 2824 61 Virginis cluster HYG 778 3.7 4.6 2.5 HD 2773
    [Show full text]
  • Project Icarus: Astronomical Considerations Relating to the Choice of Target Star
    Project Icarus: Astronomical Considerations Relating to the Choice of Target Star I. A. Crawford Department of Earth and Planetary Sciences, Birkbeck College London, Malet Street, London, WC1E 7HX Abstract In this paper we outline the considerations required in order to select a target star system for the Icarus interstellar mission. It is considered that the maximum likely range for the Icarus vehicle will be 15 light‐years, and a list is provided of all known stars within this distance range. As the scientific objectives of Icarus are weighted towards planetary science and astrobiology, a final choice of target star(s) cannot be made until we have a clearer understanding of the prevalence of planetary systems within 15 light‐ years of the Sun, and we summarize what is currently known regarding planetary systems within this volume. We stress that by the time an interstellar mission such as Icarus is actually undertaken, astronomical observations from the solar system will have provided this information. Finally, given the high proportion of multiple star systems within 15 light‐years (including the closest of all stars to the Sun in the α Centauri system), we stress that a flexible mission architecture, able to visit stars and accompanying planets within multiple systems, is desirable. This paper is a submission of the Project Icarus Study Group. Keywords: Interstellar travel; nearby stars; extrasolar planets; astrobiology 1. Introduction The Icarus study is tasked with designing an interstellar space vehicle capable of making in situ scientific investigations of a nearby star and accompanying planetary system [1,2]. This paper outlines the considerations which will feed into the choice of the target star, the choice of which will be constrained by a number of factors.
    [Show full text]
  • May 2007 ASCB Newsletter
    ASCB M A Y 2 0 0 7 NEWSLETTER VOLUME 30, NUMBER 5 Annual Senate Approves Stem Cell Bills Meeting Once again, the United States Senate has ap- The current federal policy limits federally Program proved a bill that would expand the exist- funded research to research using human Page 8 ing federal human embryon- embryonic stem cell lines ic stem cell policy. The bill, derived before August 9, 2001. S.5, the Stem Cell Research “[N]aturally dead Despite U.S. President Bush’s NIH Enhancement Act of 2007, initial claim that as many as Proponents passed the Senate by a vote of is a scientifi cally 78 stem cell lines would be 63–34. Three Senators who meaningless available to researchers, only 21 Rally Support support stem cell research did lines are actually available. idea. To our not vote. Only two of the nine S.5, the pro-research bill, in Congress new Senators —Sens. Bob knowledge, there would expand the current policy Page 13 Corker (R-TN) and Bob Casey is no scientifi cally to allow investigators to receive (D-PA)—opposed the bill. federal funds for research using A Network of The Senate also passed a credible way to human embryonic stem cells bill that would limit federally determine this derived from IVF clinic excess Our Own funded research to research embryos that would otherwise using human embryonic stem [for embryos].” be destroyed. S.5 combines Page 18 cells derived from “naturally the bill that was passed by the dead” embryos. That bill, House and Senate last year S.30, the Hope Offered through Principled and (H.R.810) but vetoed by President Bush, along Inside Ethical Stem Cell Research Act, was approved with the main components of a second bill 70–28.
    [Show full text]