SALT ANNUAL REPORT 2018 Message from the SAAO Director
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Arxiv:1705.04776V1 [Astro-Ph.HE] 13 May 2017 Aaua M
White Paper on East Asian Vision for mm/submm VLBI: Toward Black Hole Astrophysics down to Angular Resolution of 1 RS Editors Asada, K.1, Kino, M.2,3, Honma, M.3, Hirota, T.3, Lu, R.-S.4,5, Inoue, M.1, Sohn, B.-W.2,6, Shen, Z.-Q.4, and Ho, P. T. P.1,7 Authors Akiyama, K.3,8, Algaba, J-C.2, An, T.4, Bower, G.1, Byun, D-Y.2, Dodson, R.9, Doi, A.10, Edwards, P.G.11, Fujisawa, K.12, Gu, M-F.4, Hada, K.3, Hagiwara, Y.13, Jaroenjittichai, P.15, Jung, T.2,6, Kawashima, T.3, Koyama, S.1,5, Lee, S-S.2, Matsushita, S.1, Nagai, H.3, Nakamura, M.1, Niinuma, K.12, Phillips, C.11, Park, J-H.15, Pu, H-Y.1, Ro, H-W.2,6, Stevens, J.11, Trippe, S.15, Wajima, K.2, Zhao, G-Y.2 1 Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan 2 Korea Astronomy and Space Science Institute, Daedukudae-ro 776, Yuseong-gu, Daejeon 34055, Republic of Korea 3 National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo, 181-8588, Japan 4 Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China 5 Max-Planck-Institut f¨ur Radioastronomie, Auf dem H¨ugel 69, D-53121 Bonn, Germany 6 University of Science and Technology, 217 Gajeong-ro, Yuseong-gu, Daejeon 34113, Republic of Korea 7 East Asian Observatory, 660 N. -
The Bright Galaxies NGC 1068 (M 77), NGC 2146, NGC 3079, NGC 4826 (M 64), and NGC 7469 F
A&A 493, 525–538 (2009) Astronomy DOI: 10.1051/0004-6361:200810655 & c ESO 2009 Astrophysics CI and CO in nearby galaxy centers The bright galaxies NGC 1068 (M 77), NGC 2146, NGC 3079, NGC 4826 (M 64), and NGC 7469 F. P. Israel Sterrewacht Leiden, Leiden University, PO Box 9513, 2300 RA Leiden, The Netherlands e-mail: [email protected] Received 22 July 2008 / Accepted 5 November 2008 ABSTRACT Aims. We study the physical properties and amount of molecular gas in the central regions of galaxies with active nuclei. Methods. Maps and measurements of the J = 1−0, J = 2−1, J = 3−2, J = 4−3 12CO, the J = 1−0, J = 2−1, and J = 3−2 13CO lines in the central arcminute squared of NGC 1068, NGC 2146, NGC 3079, NGC 4826, and NGC 7469, as well as 492 GHz CI maps in three of these are used to model the molecular gas clouds in these galaxies. Results. Bright CO concentrations were detected and mapped in all five objects. In all cases, the observed lines could be fitted with two distinct gas components. The physical condition of the molecular gas is found to differ from galaxy to galaxy. Rather high kinetic temperatures of 125−150 K occur in NGC 2146 and NGC 3079. Very high densities of 0.3−1.0 × 105 cm−3 occur in NGC 2146, NGC 3079, and NGC 7469. The CO to H2 conversion factor X is typically an order of magnitude less than the “standard” value in the solar neighborhood. -
Two Rivers Urban Park Contextual Framework Review and Preliminary Heritage Study
1 TWO RIVERS URBAN PARK CONTEXTUAL FRAMEWORK REVIEW AND PRELIMINARY HERITAGE STUDY Phase One Report Submitted by Melanie Attwell and Associates in association with ARCON Heritage and Design, and ACO Associates on behalf of NM & Associates Planners and Designers [email protected] 2 Caxton Close Oakridge 7806 021 7150330 First submitted: November 2015 Resubmitted: May 2016 2 Table of Contents List of Figures....................................................................................................................................... 3 Executive Summary ........................................................................................................................... 4 List of Acronyms ................................................................................................................................. 5 1. Introduction .................................................................................................................................... 6 1.1 Report Structure ....................................................................................................................... 6 1.2 Brief and Scope of Work ......................................................................................................... 7 2. Limitations ....................................................................................................................................... 7 3. Location ......................................................................................................................................... -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
Nrf/Saao/Slib/59/2020-21
INVITATION TO BID THE SUPPLY AND DELIVERY OF ANNUAL JOURNAL SUBSCRIPTIONS TO SAAO FOR A 60 MONTH PERIOD Bid Number: NRF/SAAO/SLIB/59/2020-21 Closing date: 6 April 2021 Time: 11H00 Bidder Name: __________________________________________________________ __________________________________________________________ Bid Number: NRF/SAAO/SLIB/59/2020-21 Page 1 of 46 Ver. Standard 2018-6a TABLE OF CONTENTS INTRODUCTION TO THE NRF ......................................................................................................................... PAGE 3 INTRODUCTION TO THE BUSINESS UNIT ..................................................................................................... PAGE 3 CONTEXT OF THIS PROCUREMENT NEED ................................................................................................... PAGE 3 PART A (FIRST ENVELOPE) PRE-QUALIFICATION ELIGIBILITY CRITERIA ................................................................................................ PAGE 4 DETAILED SPECIFICATIONS .......................................................................................................................... PAGE 4 CONTRACT PERIOD ................................................................................................................................ PAGE 11 PERFORMANCE/SERVICE LEVEL CONDITIONS .......................................................................................... PAGE 11 EVALUATION PROCESS ............................................................................................................................... -
Thomas Maclear, Astrologer Royal at the Cape
SYMPOSIUM PROCEEDINGS ThomasMaclear, Astrologer Royal at the Cape Ethleen Lastovica Librarian, South African Astronomical Observatory, PO Box 9, Observatory, 7935 At the 14th Annual General Meeting of the Royal Maclear was convinced that the meridian Astronomical Society in 1834, it was announced observations of sun, moon, planets and princi that: “Mr Maclear, so well known forhis ardour pal stars should form the chief work of the Ob in the cause of astronomy,is gone to take upon servatory of the South. (RAS 1858). His inten himself the care of the Observatory of the Cape tions however, were diverted by the major chal of Good Hope.” In his letter of appointment, lenge of remeasuring Abbe de la Caille’s Arc of Maclear was commanded by the British Admi Meridian at the Cape, and of publishing there ralty to proceed without losstime of to theCape sults.This work occupied almost hisentire work of Good Hope, and there to assume the control ing life. Initial investigations were undertaken in and direction ofHis Majesty’s Observatory from 1836, but the major survey was startedin 1838 the Assistant Astronomer,Lieutenant William and only completed in 1847. Maclear’s magnum Meadows, and to take chargeimmediately of all opus was the 2-volumework, Verification and the instruments, books and other stores left there Extension of La Caille’s Arc of Meridian at the at the departure of his predecessor. Cape of Good Hope thatwas published in 1866 It interests me as librarian at SAAO, to read underthe editorship ofSir George Airy. (Maclear that he was specifically instructed to care for the 1866) books. -
Volume 75 Nos 3 & 4 April 2016 News Note
Volume 75 Nos 3 & 4 April 2016 In this issue: News Note – Galaxy alignment on a cosmic scale News Note – Presentation of EdinburghMedal Port Elizabeth Peoples’ Observatory Updated Biographical Index to MNASSA and JASSA EDITORIAL Mr Case Rijsdijk (Editor, MNASSA ) BOARD Mr Auke Slotegraaf (Editor, Sky Guide Africa South ) Mr Christian Hettlage (Webmaster) Prof M.W. Feast (Member, University of Cape Town) Prof B. Warner (Member, University of Cape Town) MNASSA Mr Case Rijsdijk (Editor, MNASSA ) PRODUCTION Dr Ian Glass (Assistant Editor) Ms Lia Labuschagne (Book Review Editor) Willie Koorts (Consultant) EDITORIAL MNASSA, PO Box 9, Observatory 7935, South Africa ADDRESSES Email: [email protected] Web page: http://mnassa.saao.ac.za MNASSA Download Page: www.mnassa.org.za SUBSCRIPTIONS MNASSA is available for free download on the Internet ADVERTISING Advertisements may be placed in MNASSA at the following rates per insertion: full page R400, half page R200, quarter page R100. Small advertisements R2 per word. Enquiries should be sent to the editor at [email protected] CONTRIBUTIONS MNASSA mainly serves the Southern African astronomical community. Articles may be submitted by members of this community or by those with strong connections. Else they should deal with matters of direct interest to the community . MNASSA is published on the first day of every second month and articles are due one month before the publication date. RECOGNITION Articles from MNASSA appear in the NASA/ADS data system. Cover picture: An image of the deep radio map covering the ELAIS-N1 region, with aligned galaxy jets. The image on the left has white circles around the aligned galaxies; the image on the right is without the circles. -
Hi Ms AH, the Views of This Branch Remain As Stated in Our E-M to You
From: Alvin Cope To: Amy Hill Subject: RE: Stakeholder Comment Period: BAR for the Proposed Redevelopment of the River Club in Observatory - JN 11912 Date: Tuesday, 14 January 2020 11:37:32 Attachments: image002.png image003.jpg Hi Ms AH, The views of this Branch remain as stated in our e-m to you of 8 June 2019. Thanx Regards. A Alvin L Cope WCG 9 Dorp Street P O Box 2603 Cape Town 8000 Road Network Management – Room 3-36 +27 21 483 2009 (Tel) [email protected] cid:[email protected] From: Amy Hill <[email protected]> Sent: Monday, January 13, 2020 4:08 PM To: Amy Hill <[email protected]> Subject: Stakeholder Comment Period: BAR for the Proposed Redevelopment of the River Club in Observatory Dear Stakeholder Notice of Stakeholder Comment Period on Basic Assessment Report and Tabling of Heritage Impact Assessment Supplementary Report at Heritage Western Cape Impact Assessment Committee: Proposed Redevelopment of the River Club in Observatory, Cape Town DEA&DP Reference Number: 16/3/3/6/7/1/A7/17/3217/19 HWC Case Number: 15112504WD1217E DWS Reference Number: WU9026 River Club and 16/2/7/G22/A/11 The Liesbeek Leisure Properties Trust (“the LLPT” or “the proponent”) operates the River Club in Observatory, Cape Town which, together with portions of adjacent properties, is collectively referred to as the site. The River Club is currently operated as a commercial facility, mainly for recreational (golfing) activities and conferencing. The LLPT is proposing to redevelop most of the site for residential, commercial, institutional and associated uses (the project or the development). -
ESO Annual Report 2004 ESO Annual Report 2004 Presented to the Council by the Director General Dr
ESO Annual Report 2004 ESO Annual Report 2004 presented to the Council by the Director General Dr. Catherine Cesarsky View of La Silla from the 3.6-m telescope. ESO is the foremost intergovernmental European Science and Technology organi- sation in the field of ground-based as- trophysics. It is supported by eleven coun- tries: Belgium, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Sweden, Switzerland and the United Kingdom. Created in 1962, ESO provides state-of- the-art research facilities to European astronomers and astrophysicists. In pur- suit of this task, ESO’s activities cover a wide spectrum including the design and construction of world-class ground-based observational facilities for the member- state scientists, large telescope projects, design of innovative scientific instruments, developing new and advanced techno- logies, furthering European co-operation and carrying out European educational programmes. ESO operates at three sites in the Ataca- ma desert region of Chile. The first site The VLT is a most unusual telescope, is at La Silla, a mountain 600 km north of based on the latest technology. It is not Santiago de Chile, at 2 400 m altitude. just one, but an array of 4 telescopes, It is equipped with several optical tele- each with a main mirror of 8.2-m diame- scopes with mirror diameters of up to ter. With one such telescope, images 3.6-metres. The 3.5-m New Technology of celestial objects as faint as magnitude Telescope (NTT) was the first in the 30 have been obtained in a one-hour ex- world to have a computer-controlled main posure. -
Modelling Ionised and Photodissociated Regions
Modelling ionised and photodissociated regions Magda Vasta Thesis submitted for the Degree of Doctor of Philosophy of University College London Department of Physics & Astronomy UNIVERSITY COLLEGE LONDON March 2010 I, Magda Vasta, confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. To my parents, my brother and my husband, who always supported and encouraged me no matter what. I tell people I am too stupid to know what is impossible. I have ridiculously large dreams, and half the time they come true. — Thomas D. ACKNOWLEDGEMENTS Some people come into our lives and quickly go. Some stay for a while and leave footprints on our hearts. And we are never, ever the same. I made it, I still cannot believe it, but I finally made it. However, it would have been almost impossible to reach this target without the constant scientific support from some people. My first big THANKS go to my supervisor Serena Viti. Thanks for being the supportive person you are, for giving me the possibility to be independent in my research, but being always present when I needed you. Thanks for all the times that you did not talk to me in Italian, for encouraging me to not give up and for being the lovely person you are. Thanks to Mike Barlow for the amazing scientific suggestions and for tolerating ALL my silly questions (most of them grammatically incorrect!). Thanks to Barbara Ercolano for her patience when answering my emails “HELP, PLEASE!!” about MOCASSIN. -
Bulletin Issue 29 Spring 2018 New Series by Paul Haley Begins in This Issue: 19Th Century Observatories 2018 Sha Spring Conference
BULLETIN ISSUE 29 SPRING 2018 NEW SERIES BY PAUL HALEY BEGINS IN THIS ISSUE: 19TH CENTURY OBSERVATORIES 2018 SHA SPRING CONFERENCE The first talk is at 1015 and the Saturday 21st April 2018 The conference registraon is morning session ends at 1215 Instute of Astronomy, between 0930 and 1000 at which for lunch. The lunch break is University of Cambridge me refreshments are available unl 1330. An on-site lunch Madingley Road, Cambridge in the lecture theatre. The will be available (£5.00) BUT CB3 0HA conference starts at 1000 with a MUST BE PRE-ORDERED. There welcome by the SHA Chairman are no nearby eang places. Bob Bower introduces the There is a break for refreshments Aer the break there is the aernoon session at 1330 then from 1530 to 1600 when Tea/ final talk. The aernoon there are two one-hour talks. Coffee and biscuits will be session will end at 5 p.m. and provided. the conference will then close. 10 00 - 1015 10 15 - 1115 1115 - 1215 SHA Chairman Bob Bower Carolyn Kennett and Brian Sheen Kevin Kilburn Welcomes delegates to Ancient Skies and the Megaliths Forgotten Star Atlas the Instute of of Cornwall Astronomy for the SHA 2018 Archeoastronomy in Cornwall The 18th Century unpublished Spring Conference Past and Present Uranographia Britannica by Dr John Bevis 13 30 - 1430 14 30 - 1530 16 00 – 17 00 Nik Szymanek Kenelm England Jonathan Maxwell The Road to Modern Berkshire Astronomers 5000 BC Some lesser known aspects Astrophotography to AD 2018 regarding the evolution of The pioneering days of Some topics on astronomers and refracting telescopes: from early astrophotographers, observations made from Lippershey's spectacle lens to the up to modern times Berkshire since pre-historic Apochromats times until last week An insight into the development of 2 the refracting telescope In this Issue BOOK SALE AT THE 2017 AGM Digital Bulletin The Digital Bulletin provides extra content and links when viewing the 4 Bulletin as a PDF. -
CI and CO in Nearby Galaxy Centers
Astronomy & Astrophysics manuscript no. brightgal c ESO 2018 October 22, 2018 CI and CO in nearby galaxy centers The bright galaxies NGC 1068 (M 77), NGC 2146, NGC 3079, NGC 4826 (M 64), and NGC 7469 F.P. Israel1 Sterrewacht Leiden, Leiden University, P.O. Box 9513, 2300 RA Leiden, The Netherlands Received ????; accepted ???? ABSTRACT Aims. We study the physical properties and amount of molecular gas in the central regions of galaxies with active nuclei. Methods. Maps and measurements of the J=1–0, J=2–1, J=3–2, J=4–3 12CO, the J=1–0, J=2–1, and J=3–2 13CO lines in the central arcminute squared of NGC 1068, NGC 2146, NGC 3079, NGC 4826, and NGC 7469, as well as 492 GHz CI maps in three of these are used to model the molecular gas clouds in these galaxies. Results. Bright CO concentrations were detected and mapped in all five objects. In all cases, the observed lines could be fitted with two distinct gas components. The physical condition of the molecular gas is found to differ from galaxy to galaxy. Rather high kinetic temperatures of 125-150 K occur in NGC 2146 and NGC 3079. Very high densities of 5 −3 0.3−1.0 × 10 cm occur in NGC 2146, NGC 3079, and NGC 7469. The CO to H2 conversion factor X is typically an order of magnitude less than the ‘standard’ value in the Solar Neighborhood. The molecular gas is constrained within 8 radii between 0.9 and 1.5 kpc from the nuclei.