DOCSLIB.ORG

Quarterly Report, April 1

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Quarterly Report, April 1 NATIONAL RADIO ASTRONOMY OBSERVATORY QUARTERLY REPORT April 1,1996 - June 30,1996 TABLE OF CONTENTS A. TELESCOPE USAGE .............................................................. 1 B. 140 FOOT OBSERVING PROGRAMS ................................................ 1 C. 12 METER TELESCOPE OBSERVING PROGRAMS .................................... 3 D. VERY LARGE ARRAY OBSERVING PROGRAMS ..................................... 7 E. VERY LONG BASELINE ARRAY OBSERVING PROGRAMS ........................... 15 F. SCIENCE HIGHLIGHTS ........................................................... 22 G. PUBLICATIONS ................................................................ 23 H. CHARLOTTESVILLE ELECTRONICS ............................................... 23 I. GREEN BANK ELECTRONICS .................................................... 25 J. TUCSON ELECTRONICS ......................................................... 26 K. SOCORRO ELECTRONICS........................................................ 27 L. COMPUTING AND AIPS.......................................................... 30 M . AIPS++ .................................................... .................... 32 N. GREEN BANK TELESCOPE PROJECT ............................................... 32 O. PERSONNEL .................................................................... 33 APPENDIX A. PREPRINTS A. TELESCOPE USAGE The following telescopes have been scheduled for research and maintenance in the following manner during the second quarter of 1996. 140 Foot 12 Meter VLA VLBA Scheduled Observing (hrs) 1728.75 1751.25 1685.5 1012 Scheduled Maintenance and Equipment Changes 169.50 64.75 239.5 379 Scheduled Tests and Calibration 263.75 335.25 291.0 412 Time Lost 39.50 87.00 48.9 50 Actual Observing 1689.25 1664.25 1636.6 962 B. 140 FOOT OBSERVING PROGRAMS The following continuum programs were conducted during this quarter. N._o. Observer(s) Program D191 de Pater, I. (Calif., Berkeley) Observations of the aftermath of the comet Shoemaker-Levy Heiles, C. (Calif., Berkeley) with Jupiter crash. Maddalena, R. Millan, R. (Calif., Berkeley) Wong, M. (Michigan) The following line programs were conducted during this quarter. No. Observer(s) Prosas B654 Barnbaum, C. Observations of OH masers associated with the extraordinary Morris, M. (UCLA) star, U Equ. Omont, A. (IAP, Paris) B657 Balser, D. Observations of ionized helium in diffuse HII regions. Lockman, F. J. B659 Burton, W. B. (Leiden) 21 cm measurements toward weak shoulders on HI spectra observed near b = 0. B663 Brown, R. Observations at 1.7 and 3 GHz for detections of HI fine Wiseman, J. structure emission at high redshift. Schulman, E. Cox, C. (Virginia) C305 Carilli, C. Redshifted HI 21 cm line observations of red quasars and red Menten, K. (CFA) gravitational lenses. Reid, M. (CFA) Rupen, M. Stocke, J. (Colorado/JILA) No. Observer(s) Pryogam D190 Dickey, J. (Minnesota) A search for OH emission at 18 cm from diffuse molecular Elliot, E. (Minnesota) clouds. H304 Haynes, M. (Cornell) 21 cm spectra ofredshift independent distances to spiral Giovanelli, R. (Cornell) galaxies. L320 Lockman, F. J. 21 cm HI observing and data reduction procedures testing. Murphy, E. (Virginia) M385 Murphy, E. (Virginia) The magnetic field in galactic HI. Lockman, F. J. T348 Thuan, T. (Virginia) 21 cm observations of the influence of local environment on Martin, J-M. (Meudon) the physical properties of dwarf galaxies. Karachentseva, V. (Kiev) The following pulsar programs were conducted during this quarter. No. Observer(s) Pro ram A118Al 18 Arzoumanian, Z. (Cornell) Bi-monthly timing of 63 pulsars at 550, 800, 1420, and Nice, D. 1660 MHz. Taylor, J. (Princeton) Taylor, H. (Princeton) A128 Arzoumanian, Z. (Cornell) A 1.4 GHz directed search for radio pulsars in the first maps of Cordes, J. (Cornell) the NRAO VLA sky survey. Gregg, M. (LLNL) Becker, R. (Calif., Davis) Nice, D. Sayer, R. (]Princeton) A132 Arzoumanian, Z. (Cornell) Monitoring at 575 MHz of the evolution of the PSR B1957+20 Nice, D. eclipsing binary system. B617 Backer, D. (Calif., Berkeley) Pulsar timing array observations at 800 and 1395 MHz. Sallmen, S. (Calif., Berkeley) Foster, R. (NRL) Matsakis, D. (NRL) F132 Foster, R. (NRL) Timing measurements of two new millisecond pulsars found in Wolszczan, A. (Penn State) the Arecibo high latitude survey. Cadwell, B. (Penn State) Anderson, S. (Penn State) F133 Fruchter, A. (STScI) Timing observations of a new, bright, fast pulsar. Eder, J. (NAIC) No. Observer(s) P0rn L317 Lundgren, S. (NRL) Joint radio and x-ray observations of the fluctuations of the Cordes, J. (Cornell) Crab pulsar. Arzoumanian, Z. (Cornell) Hankins, T. (NMIMT) Moffett, D. (NMIMT) Finley, J. (Purdue) M386 McKinnon, M. A 1.3-1.8 GHz polarization model test and timing of young Fisher, J. R. pulsar PSR B 1823-13. Z139 Zepka, A. (Calif., Berkeley) A 1.4 GHz search for the radio pulsars associated with SNR Backer, D. (Calif., Berkeley) G78.2+2.1. Nice, D. The following very long baseline programs were conducted with Green Bank telescopes this quarter. No. Observer(s) Progra C293 Clark, T. (NASA/GSFC) 140 Foot, 85-3, and 20 meter Green Bank geodetic ties. Ryan, J. (NASA/GSFC) Gordon, D. (Hughes/STX) Himwich, W. (NVI, Inc.) Varney, D. (NVI, Inc.) Vandenberg, N. (NVI, Inc.) VT002 Okayasu, R. (ISAS, Japan) VSOP scheduling test. C. 12 METER TELESCOPE OBSERVING PROGRAMS The following line programs were conducted during this quarter. No. Observer(s) Proram B653 Butner, H. (DTM/Carnegie) Tracing interstellar deuterium fractionation pathways. Charnley, S. (NASA/Ames) Lada, E. (Maryland) B657 Boselli, A. (Paris Obs) CO (1-0) in a complete sample of spiral galaxies in the Coma Gavazzi, G. (Brera Obs) supercluster. Lequeux, J. (Paris Obs) Buat, V. (Marseille) Donas, J. (Marseille) Casoli, F. (Paris Obs) C296 Clancy, R. T. (Colorado/JILA) Mars dust storm observations. Sandor, B. (Colorado/JILA) C300 Combes, F. (Paris Obs) A search for 02 at z = 0.685 at 70 GHz. Wiklind, T. (Chalmers, Onsala) 4 No. Observer(s) Proaa C303 Caselli, P. (CFA) Search for quiescent massive molecular dense cores in Chen, H. (CFA) Orion B. Myers, P. (CFA) CB05 Bower, G. (Calif., Berkeley) Study of a dramatic flare in the extremely flat-spectrum QSO Backer, D. (Calif., Berkeley) NRAO 530. Wright, M. (Calif., Berkeley) CDO3 Doeleman, S. (Haystack) Imaging and evolution of radio galaxy 3C 111. CDO4 Doeleman, S. (Haystack) 3 mm VLBI observations of the galactic center. Rogers, A. (Haystack) Bower, G. (Calif., Berkeley) Backer, D. (Calif., Berkeley) Wright, M. (Calif., Berkeley) CLO2 Lonsdale, C. (Haystack) A large-scale 3 mm VLBI survey. Doeleman, S. (Haystack) Phillips, R. (Haystack) F134 Frayer, D. (Toronto) Study of molecular gas in chemically young IRAS galaxies. Thuan, T. (Virginia) Seaquist, E. (Toronto) G350G Gensheimer, P. (WMPIR, Bonn) Observations of HCO* toward CIT 6. G351 Gensheimer, P. (MPIR, Bonn) Study of H20 toward NGC 7027. Henkel, C. (MPIR, Bonn) H317 Helfer, T. (Maryland) On-the-fly CO mapping of NGC 3628, NGC 4826, and M83. Blitz, L. (Maryland) H318 Holdaway, M. Verification of 3 mm continuum fluxes of bright quasars. 118 Irwin, J. (Virginia) Search for CO in the HI cloud between NGC 4472 and Frayer, D. (Toronto) UGC 7636. Sarazin, C. (Virginia) K353 Kutner, M. (unaffiliated) Study of the molecular content of dwarf spirals. Schombert, J. (NASA/GSFC) Pildas, R. (CFA) L316 Liszt, H. Study of CO8 0 emission around rho Ophiuchus. L321 Liszt, H. Study of galactic CO toward extragalactic sources. Lucas, R. (IRAM) M398 Mauersberger, R. (Arizona) Study of interstellar sulfur isotopes and oxygen burning in Henkel, C. (MPIR, Bonn) stars. Chin, Y. (Bonn U.) Observer(s) Proram No. Mauersberger, R. (Arizona) A search for interstellar Van der Waals complexes. M400 Havenith, M. (IAP, Bonn) Wilson, T. (MPIR, Bonn) P170 Pound, M. (Calif., Berkeley) An investigation of cluster formation in Orion. Lada, E. (Maryland) Mundy, L. (Maryland) Gruendl, R. (Maryland) P180 Papadopoulos, P. (Toronto) Study of CO (2-1) in Markarian 10. R265 Robinson, B. (Northwestern) Search for high density molecular gas at -5 km/s toward OH Yusef-Zadeh, F. (Northwestern) masers surrounding the galactic center SNR G359.1-0.5. S404 Sandor, B. (Colorado/JILA) Microwave spectroscopy of earth's atmosphere. Clancy, T. (Colorado/JILA) S409 Smith, B. (IPAC) CO (1-0) observations of low-luminosity Virgo spiral Madden, S. (NASA/Ames) galaxies. T362 Turner, B. How big can interstellar molecules get in translucent clouds? V86 van Dishoeck, E. (Leiden) Studying the youngest stellar regions: The evolution of Mundy, L. (Maryland) chemical morphologies. McMullin, J. (Arizona) Blake, G. (Caltech) Evans, N. (Texas) Mattingly, B. (Texas) V87 Yun, M. (CFA) Study of the molecular component of Hickson groups. Verdes-Montenegro, L. (IAA, Andalucia) Perea, J. (IAA, Andalucia) del Olmo, A. (IAA, Andalucia) W351 Wootten, H. A. Study of origin of broad formaldehyde line emission in Mangum, J. millimeter-bright, low-mass, star-forming regions. Wilking, B. (Missouri) W353 Williams, J. (Calif., Berkeley) Study of the clump structure in the Rosette molecular cloud. Blitz, L. (Maryland) W357 Womack, M. (Penn State) Study of carbon chemistry in Kuiper disk comets. Stern, A. (SWRI) W367 Wyckoff, S. (Arizona State) A 2 mm spectral-line survey of Comet Hale-Bopp (150- Ziurys, L. (Arizona State) 170 GHz). Kleine, M. (Arizona State) Wehinger, P. (Arizona State) 2 13 W370 Wyckoff, S. (Arizona State) 1 C/ C ratios in molecular clouds from CN: chemical Kleine, M. (Arizona State) processing in
Load more

Recommended publications
  • Bulletin No. 6 Issn 1520-3581
    UNIVERSITY OF HAWAII LIBRARY THE PACIFIC CIRCLE DECEMBER 2000 BULLETIN NO. 6 ISSN 1520-3581 PACIFIC CIRCLE NEW S .............................................................................2 Forthcoming Meetings.................................................. 2 Recent Meetings..........................................................................................3 Publications..................................................................................................6 New Members...............................................................................................6 IUHPS/DHS NEWS ........................................................................................ 8 PACIFIC WATCH....................................................................... 9 CONFERENCE REPORTS............................................................................9 FUTURE CONFERENCES & CALLS FOR PAPERS........................ 11 PRIZES, GRANTS AND FELLOWSHIPS........................... 13 ARCHIVES AND COLLECTIONS...........................................................15 BOOK AND JOURNAL NEWS................................................................ 15 BOOK REVIEWS..........................................................................................17 Roy M. MacLeod, ed., The ‘Boffins' o f Botany Bay: Radar at the University o f Sydney, 1939-1945, and Science and the Pacific War: Science and Survival in the Pacific, 1939-1945.................................. 17 David W. Forbes, ed., Hawaiian National Bibliography: 1780-1900.
    [Show full text]
  • California Institute of Technology Catalog 1957-8
    Bulletin of the California Institute of Technology Catalog 1957-8 PAS ADEN A, CALIFORNIA BULLETIN OF THE CALIFORNIA INSTITUTE OF TECHNOLOGY VOLUME 66 NUMBER 3 The California Institute of Technology Bulletin is published quarterly Entered as Second Class Matter at the Post Office at Pasadena, California, under the Act of August 24, 1912 CALIFORNIA INSTITUTE OF TECHNOLOGY A College, Graduate School, and Institute of Research in Science, Engineering, and the Humanities CATALOG 1957 -1958 PUBLISHED BY THE INSTITUTE SEPTEMBER, 1957 PASADENA, CALIFORNIA CONTENTS PART ONE. GENERAL INFORMATION PAGE Academic Calendar .............................. __ ...... _.. _._._. __ . __ . __ . __ .. _____ 11 Board of Trustees ..................... _...................... _... __ ....... _.. ______ .. 15 Trustee Committees ......................... _..... __ ._ .. _____ .. _........... _... __ .. 16 Administrative Officers of the Institute ..... ___ ........... _.. _.. _.... 18 Faculty Officers and Committees, 1957-58 ... __ .. __ ._ .. _... _......... _.... 19 Staff of Instruction and Research-Summary ._._ .. ___ ... ___ ._. 21 Staff of Instruction and Research .... _. __ .. __ .... _____ ._ .. __ .... _ 38 Fellows, Scholars and Assistants _.. _: __ ... _..._ ...... __ . __ .. _ 66 California Institute Associates .... _... _ ... _._ .. _... __ ... ._ .. __ .. _.. 79 Historical Sketch .................... _..... __ ........... __ .. __ ... _.... _... _.. ____ . 83 Educational Policies ...... _.. __ .... __ . 88 Industrial Associates ........_. __ 91 Industrial
    [Show full text]
  • Newly Opened Correspondence Illuminates Einstein's Personal Life
    CENTER FOR HISTORY OF PHYSICS NEWSLETTER Vol. XXXVIII, Number 2 Fall 2006 One Physics Ellipse, College Park, MD 20740-3843, Tel. 301-209-3165 Newly Opened Correspondence Illuminates Einstein’s Personal Life By David C. Cassidy, Hofstra University, with special thanks to Diana Kormos Buchwald, Einstein Papers Project he Albert Einstein Archives at the Hebrew University of T Jerusalem recently opened a large collection of Einstein’s personal correspondence from the period 1912 until his death in 1955. The collection consists of nearly 1,400 items. Among them are about 300 letters and cards written by Einstein, pri- marily to his second wife Elsa Einstein, and some 130 letters Einstein received from his closest family members. The col- lection had been in the possession of Einstein’s step-daughter, Margot Einstein, who deposited it with the Hebrew University of Jerusalem with the stipulation that it remain closed for twen- ty years following her death, which occurred on July 8, 1986. The Archives released the materials to public viewing on July 10, 2006. On the same day Princeton University Press released volume 10 of The Collected Papers of Albert Einstein, con- taining 148 items from the collection through December 1920, along with other newly available correspondence. Later items will appear in future volumes. “These letters”, write the Ein- stein editors, “provide the reader with substantial new source material for the study of Einstein’s personal life and the rela- tionships with his closest family members and friends.” H. Richard Gustafson playing with a guitar to pass the time while monitoring the control room at a Fermilab experiment.
    [Show full text]
  • Hr17903book Review
    CSIRO PUBLISHING Historical Records of Australian Science, 2017, 28, 194–200 https://doi.org/10.1071/HR17903 Book Reviews Compiled by Peter Hobbins Department of History, The University of Sydney, NSW 2006, Australia. Email: [email protected] Neil Chambers (ed): Essays by scholars and curators including editor Neil Cham- Endeavouring Banks: Exploring bers, John Gascoigne, Jeremy Coote, Philip Hatfield and Anna Collections from the Agnarsdóttir—editor of Banks’ Iceland correspondence—take the Endeavour Voyage 1768–1771. text of the book into some surprising areas. Indeed, they lift it NewSouth Publishing: Sydney, from a catalogue to a substantial history. Collectively, they delve 2016. 304 pp., illus., into myriad thoughts and events associated with the voyage, from ISBN: 9781742235004 (HB), advice by the Admiralty regarding the transit of Venus to instruc- $69.99. tions regarding mapping, commerce and the possession of territory. But rather than telling a coherent story there is frequent repetition, The cover of Endeavouring Banks excessive detail, or superfluous information concerning intrigue and indicates the wide array of mate- minor characters. The contributors are deeply absorbed in their rial this book considers, includ- subject and the history of British exploration, sometimes at the ing subject matter only marginally expense of the general reader. related to its subtitle. In fact, the Items pictured include a model of the Endeavour, plans and 1773 satirical cartoon in which sketches, a nautical almanac, a Gregorian telescope, a quadrant, Joseph Banks appears as The Fly- a clock, a chart of the South Pacific, a hummingbird’s nest, shells, catching Macaroni—‘an amateur collector and dandy’—belies the botanical specimens, breadfruit, drums, canoes, spears, fish, belts, intense detail and seriousness with which the book deals with the pendants and instruments.
    [Show full text]
  • From Radar to Radio Astronomy
    John Bolton and the Nature of Discrete Radio Sources Thesis submitted by Peter Robertson BSc (Hons) Melbourne, MSc Melbourne 2015 for the degree of Doctor of Philosophy in the School of Agricultural, Computational and Environmental Sciences University of Southern Queensland ii Peter Robertson: ‘John Bolton and the Nature of Discrete Radio Sources’ Abstract John Bolton is regarded by many to be the pre-eminent Australian astronomer of his generation. In the late 1940s he and his colleagues discovered the first discrete sources of radio emission. Born in Sheffield in 1922 and educated at Cambridge University, in 1946 Bolton joined the Radiophysics Laboratory in Sydney, part of Australia’s Council for Scientific and Industrial Research. Radio astronomy was then in its infancy. Radio waves from space had been discovered by the American physicist Karl Jansky in 1932, followed by Grote Reber who mapped the emission strength across the sky, but very little was known about the origin or properties of the emission. This thesis will examine how the next major step forward was made by Bolton and colleagues Gordon Stanley and Bruce Slee. In June 1947, observing at the Dover Heights field station, they were able to show that strong radio emission from the Cygnus constellation came from a compact point-like source. By the end of 1947 the group had discovered a further five of these discrete radio sources, or ‘radio stars’ as they were known, revealing a new class of previously-unknown astronomical objects. By early 1949 the Dover Heights group had measured celestial positions for the sources accurately enough to identify three of them with known optical objects.
    [Show full text]
  • The Discovery of Quasars and Its Aftermath
    Journal of Astronomical History and Heritage, 17(3), 267–282 (2014). THE DISCOVERY OF QUASARS AND ITS AFTERMATH K.I. Kellermann National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22901, USA. Email: [email protected] Abstract: Although the extragalactic nature of quasars was discussed as early as 1960 by John Bolton and others it was rejected largely because of preconceived ideas about what appeared to be an unrealistically-high radio and optical luminosity. Following the 1962 observation of the occultations of the strong radio source 3C 273 with the Parkes Radio Telescope and the subsequent identification by Maarten Schmidt of an apparent stellar object, Schmidt recognized that the simple hydrogen line Balmer series spectrum implied a redshift of 0.16. Successive radio and optical measurements quickly led to the identification of other quasars with increasingly-large redshifts and the general, although for some decades not universal, acceptance of quasars as being by far the most distant and the most luminous objects in the Universe. However, due to an error in the calculation of the radio position, it appears that the occultation position played no direct role in the identification of 3C 273, although it was the existence of a claimed accurate occultation position that motivated Schmidt‘s 200-in Palomar telescope investi- gation and his determination of the redshift. Curiously, 3C 273, which is one of the strongest extragalactic sources in the sky, was first catalogued in 1959, and the 13th magnitude optical counterpart was observed at least as early as 1887. Since 1960, much fainter optical counterparts were being routinely identified, using accurate radio interferometer positions which were measured primarily at the Caltech Owens Valley Radio Observatory.
    [Show full text]
  • 50 Character Selection
    £50 character selection Between the launch and closure of the character selection process for the £50 note announced by the Governor on 2 November, we have received a total of 227,299 nominations from members of the public. This is the list of 989 eligible names that were suggested within the nomination period. This is only the preliminary stage of identifying eligible names for consideration: At this stage, a nomination has been deemed eligible simply if the character is real, deceased and has contributed to the field of science in the UK in any way. These names have not yet been considered by our Banknote Character Advisory Committee. We plan to announce the character for the new £50 banknote in Summer 2019. Aaron Klug Alister Hardy Augustus De Morgan Abraham Bennet Allen Coombs Austin Bradford Hill Abraham Darby Allen McClay Barbara Ansell Abraham Manie Adelstein Alliott Verdon Roe Barbara Clayton Ada Lovelace Alma Howard Barnes Neville Wallis Adam Sedgwick Andrew Crosse Baron Charles Percy Snow Aderlard of Bath Andrew Fielding Huxley Bawa Kartar Singh Adrian Hardy Haworth Angela Hartley Brodie Beatrice "Tilly" Shilling Agnes Arber Angela Helen Clayton Beatrice Tinsley Alan Archibald Campbell‐Swinton Anita Harding Benjamin Gompertz Alan Arnold Griffiths Ann Bishop Benjamin Huntsman Alan Baker Anna Atkins Benjamin Thompson Alan Blumlein Anna Bidder Bernard Katz Alan Carrington Anna Freud Bernard Spilsbury Alan Cottrell Anna MacGillivray Macleod Bertha Swirles Alan Lloyd Hodgkin Anne McLaren Bertram Hopkinson Alan MacMasters Anne Warner
    [Show full text]
  • John Bolton — Astronomer Extraordinary
    J. Astrophys. Astr. (1993) 14, 115–120 Obituary JOHN BOLTON – Astronomer Extraordinary Astronomers all over the world would have been saddened to hear of the death of John Bolton in July this year. Not only was he one of the great pioneers who created whole new branches of the subject, but, for those who knew him personally, a friend of truly remarkable individuality. With his unlimited courage and penetrating intuition, and physically indefatigable when in intense pursuit of whatever he was after, John Bolton was a phenomenon that had to be experienced to be believed. So different was he from other scientists of his eminence that it was almost as if he did not belong with them. Before World War II all information about the Cosmos had been obtained through the roughly half an octave window of the visible part of the electromagnetic spectrum. The half a century since then can truly be called the Golden Age of Astronomy when the field underwent a total transformation. The limits of the observable universe were pushed back beyond all reasonable expectations, and it was shown to be populated with surprisingly energetic galaxies radiating powerfully at wavelengths ranging over as many as fourteen orders of magnitude. As summed up by Paul Wild,1 Bolton’s distinguished colleague and contemporary, “... it all began in 1948 when a 26 year old Yorkshireman named John Bolton with two colleagues discovered that three distant objects known from optical observations were extremely powerful emitters of radio waves. One, which Bolton called Taurus A’ was located in our own galaxy: the Crab Nebula.
    [Show full text]
  • The National Radio Astronomy Observatory and Its Impact on US Radio Astronomy Historical & Cultural Astronomy
    Historical & Cultural Astronomy Series Editors: W. Orchiston · M. Rothenberg · C. Cunningham Kenneth I. Kellermann Ellen N. Bouton Sierra S. Brandt Open Skies The National Radio Astronomy Observatory and Its Impact on US Radio Astronomy Historical & Cultural Astronomy Series Editors: WAYNE ORCHISTON, Adjunct Professor, Astrophysics Group, University of Southern Queensland, Toowoomba, QLD, Australia MARC ROTHENBERG, Smithsonian Institution (retired), Rockville, MD, USA CLIFFORD CUNNINGHAM, University of Southern Queensland, Toowoomba, QLD, Australia Editorial Board: JAMES EVANS, University of Puget Sound, USA MILLER GOSS, National Radio Astronomy Observatory, USA DUANE HAMACHER, Monash University, Australia JAMES LEQUEUX, Observatoire de Paris, France SIMON MITTON, St. Edmund’s College Cambridge University, UK CLIVE RUGGLES, University of Leicester, UK VIRGINIA TRIMBLE, University of California Irvine, USA GUDRUN WOLFSCHMIDT, Institute for History of Science and Technology, Germany TRUDY BELL, Sky & Telescope, USA The Historical & Cultural Astronomy series includes high-level monographs and edited volumes covering a broad range of subjects in the history of astron- omy, including interdisciplinary contributions from historians, sociologists, horologists, archaeologists, and other humanities fields. The authors are distin- guished specialists in their fields of expertise. Each title is carefully supervised and aims to provide an in-depth understanding by offering detailed research. Rather than focusing on the scientific findings alone, these volumes explain the context of astronomical and space science progress from the pre-modern world to the future. The interdisciplinary Historical & Cultural Astronomy series offers a home for books addressing astronomical progress from a humanities perspective, encompassing the influence of religion, politics, social movements, and more on the growth of astronomical knowledge over the centuries.
    [Show full text]
  • The History of Early Low Frequency Radio Astronomy in Australia. 3: Ellis, Reber and the Cambridge Field Station Near Hobart
    Journal of Astronomical History and Heritage, 18(2), 177–189 (2015). THE HISTORY OF EARLY LOW FREQUENCY RADIO ASTRONOMY IN AUSTRALIA. 3: ELLIS, REBER AND THE CAMBRIDGE FIELD STATION NEAR HOBART Martin George, Wayne Orchiston National Astronomical Research Institute of Thailand, 191 Huay Kaew Road, Suthep District, Muang, Chiang Mai 50200, Thailand, and University of Southern Queensland, Toowoomba, Queensland, Australia. Emails: [email protected]; [email protected] Bruce Slee CSIRO Astronomy and Space Sciences, Sydney, Australia. Email: [email protected] and Richard Wielebinski Max-Planck-Institut für Radioastronomie, Bonn, Germany, and University of Southern Queensland, Toowoomba, Queensland, Australia. Email: [email protected] Abstract: Low frequency radio astronomy in Tasmania began with the arrival of Grote Reber to the State in 1954.1 After analysing ionospheric data from around the world, he concluded that Tasmania would be a very suitable place to carry out low frequency observations. Communications with Graeme Ellis in Tasmania, who had spent several years studying the ionosphere, led to a collaboration between the two in 1955 during which year they made observations at Cambridge, near Hobart. Their observations took place at four frequencies between 2.13 MHz and 0.52 MHz inclusive, with the results at the higher frequencies revealing a clear celestial component. Keywords: Australian low frequency radio astronomy, Tasmania, Grote Reber, Graeme Ellis, Cambridge. 1 INTRODUCTION galactic objects (see Bolton et al., 1949; Robert- son et al., 2014). The science of what would later be termed radio astronomy began in 1931 with the discovery by Reber‘s interest turned increasingly to low the American physicist Karl Jansky (1905–1950) frequency radio astronomy (Reber, 1977), but of radio-frequency radiation of celestial origin.
    [Show full text]
  • Pdf (1960-1961)
    CATALOG 1960-1961 CALIFORNIA INSTITUTE OF TECHNOLOGY PASADENA' CALIFORNIA SEPTEMBER 1960 CONTENTS SECTION I. OFFICERS AND F ACUL TY PAGE Academic Calendar 4 Board of Trustees 9 Trustee Committees 10 Administrative Officers of the Institute 12 Faculty Officers and Committees, 1960-61 13 Staff of Instruction and Research 15 Fellows, Scholars, and Assistants 63 California Institute Associates 84 Industrial Associates 88 SECTION II. GENERAL INFORMATION Educational Policies 90 Historical Sketch 92 Industrial Relations Section 98 Buildings and Facilities 100 Study and Research at the California Institute 1. The Sciences 104 Astronomy 104 Biological Sciences 106 Chemistry and Chemical Engineering 108 Geological Sciences 110 Mathematics 113 Physics 115 2. Engineering 118 Aeronautics 120 Civil Engineering 122 Electrical Engineering 123 Engineering Science 125 Mechanical Engineering 125 Guggenheim Jet Propulsion Center 127 Hydrodynamics 127 3. The Humanities 130 Student Life 132 Air Force Reserve Officers Training Corps 138 2 SECTION III. INFORMATION AND REGULATIONS FOR THE GUIDANCE OF UNDERGRADUATE STUDENTS Requirements for Admission to Undergraduate Standing 139 Admission to Freshman Class 139 Admission to Upper Class by Transfer 146 The 3-2 Plan 149 Registration Regulations 150 Scholastic Grading and Requirements 152 Student Health and Physical Education 157 Expenses 160 Scholarships, Student Aid, and Prizes 164 SECTION IV. INFORMATION AND REGULATIONS FOR THE GUIDANCE OF GRADUATE STUDENTS General Regulations 176 Regulations Concerning Work for the Degree of Master of Science 178 Regulations Concerning Work for the Engineer's Degree 180 Regulations Concerning Work for the Degree of Doctor of Philosophy 182 Opportunities for Graduate and Scientific Work at the Institute 200 Graduate Fellowships, Scholarships, and Assistantships 201 Post-Doctoral Fellowships 203 Institute Guests 204 SECTION V.
    [Show full text]
  • History of Astronomy in Australia: Big-Impact Astronomy from World War II Until the Lunar Landing (1945–1969)
    galaxies Article History of Astronomy in Australia: Big-Impact Astronomy from World War II until the Lunar Landing (1945–1969) Alister W. Graham 1,* , Katherine H. Kenyon 1,†, Lochlan J. Bull 2,‡ , Visura C. Lokuge Don 3,§ and Kazuki Kuhlmann 4,k 1 Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122, Australia 2 Horsham College, PO Box 508, Horsham, VIC 3402, Australia 3 Glen Waverley Secondary College, 39 O’Sullivan Rd, Glen Waverley, VIC 3150, Australia 4 Marcellin College, 160 Bulleen Road, Bulleen, VIC 3105, Australia * Correspondence: [email protected] † Current address: Central Clinical School, The Alfred Centre, Monash University, Melbourne, VIC 3004, Australia. ‡ Current address: Department of Economics, Faculty of Business and Economics, University of Melbourne, Carlton, VIC 3053, Australia. § Current address: Department of Civil Engineering, Faculty of Engineering, Monash University, Clayton, VIC 3800, Australia. k Current address: School of Engineering, RMIT, GPO Box 2476, Melbourne, VIC 3001, Australia. Abstract: Radio astronomy commenced in earnest after World War II, with Australia keenly en- gaged through the Council for Scientific and Industrial Research. At this juncture, Australia’s Citation: Graham, A.W.; Kenyon, K.H.; Bull, L.J.; Lokuge Don, V.C.; Commonwealth Solar Observatory expanded its portfolio from primarily studying solar phenomena Kuhlmann, K. History of Astronomy to conducting stellar and extragalactic research. Subsequently, in the 1950s and 1960s, astronomy in Australia: Big-Impact Astronomy gradually became taught and researched in Australian universities. However, most scientific publica- from World War II until the Lunar tions from this era of growth and discovery have no country of affiliation in their header information, Landing (1945–1969).
    [Show full text]