A Str O N O M Y D Ep Ar T Ment Steward Observatory
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Manastash Ridge Observatory History by Julie Lutz
Manastash Ridge Observatory History by Julie Lutz MRO Site Survey: Western Washington has a well-deserved reputation for clouds and rainy weather. Hence, the desirability of an observatory for professional astronomers in Washington state was not instantly obvious. However, a drive to the east side of the Cascade mountains yields much better weather. Long time University of Washington (UW) astronomer Theodor Jacobson started thinking about convenient telescope access for faculty and students when the university decided to expand astronomy dramatically in the mid-1960s. When the first UW astronomy department chair George Wallerstein arrived in 1965, he immediately started a campaign to get a research telescope. Wallerstein came to UW from Berkeley where faculty and Ph.D. students had ready access to telescopes, including a productive 20-inch. He felt strongly that a high-quality research telescope in Washington state would help create a high-quality astronomy department. A grant from the National Science Foundation (NSF) provided enough money to purchase automated cameras for a site survey and a 16-inch Boller and Chivens telescope. The eastern side of the Cascade mountains was the obvious region to survey for the best telescope location. The site had to be within reasonable driving distance of the UW Seattle campus and have road access on at least a dirt/gravel track. Founding telescope engineer and jack-of-all-trades Ed Mannery surveyed severall locations during 1965/66. The best site turned out to be Manastash Ridge on US Forest Service land southwest of Ellensberg. However, Rattlesnake Mountain on the Hanford Reservation (owned by the US Department of Energy) outside of Richland had a developed road and readily-available electricity. -
Campus Building & Department Index- Alphabetical
CAMPUS BUILDING & DEPARTMENT INDEX- ALPHABETICAL 2009-2010 A --- Electrical & Computer Nuerology Clinic 522 (F1) Adminstration 66 (D5) Engineering Bldg. 104 (C4) Nugent, Robert L. 40 (C6) Admissions, Office of 40 (C6) Engineering & Mines, College of 72 (C4) Nursing, College of 203 (F2) African American Studies 128 (D4) Engineering Building 20 (C5) O --- Agricultural Sciences 38 (C6) Dennis DeConcini Environment Old Main Building 21 (C5) Agriculture, College of 36 (C6) & Natural Resources Bldg. 120 (B7) Optical Science(Meinel) 94 (F6) A.M.E. Building 119 (D3) Extended University 158 (A5) P --- Apache Hall 50A (D7) F --- Park Ave. Parking Garage 116 (B3) Architecture, College of 75 (C4) Facilities Mgmt., AHSC 206 (E1) Park Student Center 87 (A6) Art Annex, Ceramics 470 (C3) Facilities Mgmt., Annex 460 (E1) Parking and Transportation Services 181 (C7) AZ Coop. Wildlife & Fishery Facilities Mgmt., Renovation 470 (D3) Payroll Department 158 (A5) Research Unit 43 (D6) Facilities Mgmt. Warehouse 215 (E1) Pharmacy, College of 207 (F2) Arizona Hall 84 (A7) Faculty Office Building 220 (E1) PHASE 420 (B3) Arizona Health Sciences Ctr. 201 (F2) Faculty Senate Office 456 (C2) Physics & Atmospheric Science (PAS) 81 (C6) Basic Services 201 (F2) Family & Consumer Res. 33 (B6) Pima Hall 135 (D4) Biomed. Research Lab 209 (E1) Family Practice Unit, AHSC 204 (E2) Pinal Hall 59 (E7) Bookstore 201 (F2) Fine Arts, Faculty of 4 (B4) Plantarium, Flandrau 91 (E5) Cancer Center 222 (F2) Fluid Dynamics Res. Lab 112 (C4) Planetary Sci., Dept. of 92 (E5) Central Heat/Refrig. 205 (E2) Forbes (Agriculture) 36 (C6) Police Department 100 (F4) Cl. Sci. -
Highly Sampled Measurements in a Controlled Atmosphere at the Biosphere 2 Landscape Evolution Observatory
www.nature.com/scientificdata OpEN Highly sampled measurements Data DEscRiptor in a controlled atmosphere at the Biosphere 2 Landscape Evolution Observatory Jorge Arevalo 1,2 ✉ , Xubin Zeng 1,3, Matej Durcik3, Michael Sibayan4, Luke Pangle5, Nate Abramson6, Aaron Bugaj3, Wei-Ren Ng3, Minseok Kim3, Greg Barron-Gaford 3,7, Joost van Haren3,8,9, Guo-Yue Niu 1,3, John Adams3, Joaquin Ruiz3,6 & Peter A. Troch1,3 Land-atmosphere interactions at diferent temporal and spatial scales are important for our understanding of the Earth system and its modeling. The Landscape Evolution Observatory (LEO) at Biosphere 2, managed by the University of Arizona, hosts three nearly identical artifcial bare-soil hillslopes with dimensions of 11 × 30 m2 (1 m depth) in a controlled and highly monitored environment within three large greenhouses. These facilities provide a unique opportunity to explore these interactions. The dataset presented here is a subset of the measurements in each LEO’s hillslopes, from 1 July 2015 to 30 June 2019 every 15 minutes, consisting of temperature, water content and heat fux of the soil (at 5 cm depth) for 12 co-located points; temperature, relative humidity and wind speed above ground at 5 locations and 5 diferent heights ranging from 0.25 m to 9–10 m; 3D wind at 1 location; the four components of radiation at 2 locations; spatially aggregated precipitation rates, total subsurface discharge, and relative water storage; and the measurements from a weather station outside the greenhouses. Background & Summary Te understanding of land-atmosphere interactions is important for improvements in Earth System Modelling1–3 for climate assessment, weather prediction, and subseasonal-to-seasonal forecasts4. -
The 100-Inch Telescope of the Mount Wilson Observatory
The 100-Inch Telescope of the Mount Wilson Observatory An International Historical Mechanical Engineering Landmark The American Society of Mechanical Engineers June 20, 1981 Mount Wilson Observatory Mount Wilson, California BACKGROUND THE MOUNT WILSON OBSERVATORY was founded in 1904 by the CARNEGIE INSTITUTION OF WASH- INGTON, a private foundation for scientific research supported largely from endowments provided by Andrew Carnegie. Within a few years, the Observatory became the world center of research in the new science of astrophysics, which is the application of principles of physics to astronomical objects beyond the earth. These include the sun, the planets of our solar system, the stars in our galaxy, and the system of galaxies that reaches to the limits of the The completed facility. visible universe. SCIENTIFIC ACHIEVEMENTS The Mount Wilson 100-inch reflector dominated dis- coveries in astronomy from its beginning in 1918 until the dedication of the Palomar 200-inch reflector in 1948. (Both telescopes are primarily the result of the lifework of one man — George Ellery Hale.) Many of the foundations of modern astrophysics were set down by work with this telescope. One of the most important results was the discovery that the intrinsic luminosities (total light output) of the stars could be found by inspection of the record made when starlight is dispersed into a spectrum by a prism or a grating. These so-called spectroscopic absolute lumi- nosities, discovered at Mount Wilson and developed for over forty years, opened the way to an understanding of the evolution of the stars and eventually to their ages. Perhaps the most important scientific discovery of the 20th century is that we live in an expanding Universe. -
A Needs Analysis Study of Amateur Astronomers for the National Virtual Observatory : Aaron Price1 Lou Cohen1 Janet Mattei1 Nahide Craig2
A Needs Analysis Study of Amateur Astronomers For the National Virtual Observatory : Aaron Price1 Lou Cohen1 Janet Mattei1 Nahide Craig2 1Clinton B. Ford Astronomical Data & Research Center American Association of Variable Star Observers 25 Birch St, Cambridge MA 02138 2Space Sciences Laboratory University of California, Berkeley 7 Gauss Way Berkeley, CA 94720-7450 Abstract Through a combination of qualitative and quantitative processes, a survey was con- ducted of the amateur astronomy community to identify outstanding needs which the National Virtual Observatory (NVO) could fulfill. This is the final report of that project, which was conducted by The American Association of Variable Star Observers (AAVSO) on behalf of the SEGway Project at the Center for Science Educations @ Space Sci- ences Laboratory, UC Berkeley. Background The American Association of Variable Star Observers (AAVSO) has worked on behalf of the SEGway Project at the Center for Science Educations @ Space Sciences Labo- ratory, UC Berkeley, to conduct a needs analysis study of the amateur astronomy com- munity. The goal of the study is to identify outstanding needs in the amateur community which the National Virtual Observatory (NVO) project can fulfill. The AAVSO is a non-profit, independent organization dedicated to the study of vari- able stars. It was founded in 1911 and currently has a database of over 11 million vari- able star observations, the vast majority of which were made by amateur astronomers. The AAVSO has a rich history and extensive experience working with amateur astrono- mers and specifically in fostering amateur-professional collaboration. AAVSO Director Dr. Janet Mattei headed the team assembled by the AAVSO. -
(Most Recent Update, March 16, 2020, 6 Pm) Stewa
Steward/Astronomy Specific Guidelines for Responding/Adapting to C19 Pandemic (Most Recent Update, March 16, 2020, 6 p.m.) Steward Observatory and the Department of Astronomy are adopting policies that will minimize the risk of transmission of COVID-19 while allowing us to continue to support our educational, outreach, and research missions. Facts and information are being shared with us at a high rate -- and these policies will have to evolve with time. We appreciate your patience and attention to the information below. We have tried to identify by subsection the individuals to whom you should address questions, but please always start with your supervisor/advisor. Our policies are intended to be consistent with those of the University of Arizona and the College of Science. We refer you to their web pages at these links: https://www.arizona.edu/coronavirus-covid-19-information and https://science.arizona.edu/coronavirus This is an evolving situation. We will update this document based on Federal, State and University policies as they become available. Please check the Provost and College pages at least daily, as they are also being updated frequently. Effective Immediately -- These policies are effective March 16, 2020 and will be updated as needed to stay consistent with U Arizona and College of Science Policies Courses and Classes (undergraduate and graduate) - All courses will be 100% online for the remaining of the semester. If you are an instructor and are having trouble moving your course to on-line, please contact Associate Department Head Xiaohui Fan, who will help you find assistance. - No in-person component to any classes. -
LSST Jan2005 3Page.Indd
EMBARGOED FOR RELEASE: 12:30 p.m. PST, January 11, 2005 RELEASE: LSSTC-02 Steward Observatory Mirror Lab Awarded Contract for Large Synoptic Survey Telescope Mirror The LSST Corporation has awarded a $2.3 million contract to the University of Arizona Steward Observatory Mirror Lab to purchase the glass and begin engineering work for the 8.4-meter diameter main mirror for the Large Synoptic Survey Telescope (LSST). This award was announced today in San Diego at the 205th meeting of the American Astronomical Society. Acquiring the LSST primary mirror was made possible by a generous, private donation from Arizona businessman Richard Caris. The UA award covers the first of four phases in an estimated $13.8 million effort to design, cast, polish and integrate the mirror into the LSST mirror support cell. Coupled with substantial support provided by Research Corporation under the leadership of John Schaefer, these private funds boost the LSST off the drawing board and into production. The LSST is a proposed world-class, ground-based telescope that can survey the entire visible sky every three nights. It will generate an awesome 30 terabytes of data per night from a three billion-pixel digital camera, producing a vast database of information on the universe. LSST will take exposures every 10 seconds, opening a movie-like window on objects that change or move on rapid timescales -- exploding supernovae, Earth-approaching asteroids, and The contract for casting of the 8.4-meter primary mirror of the distant Kuiper belt objects. Via the light-bending gravity of dark matter, LSST Large Synoptic Survey Telescope by the University of Arizona will chart the history of the expansion of the universe, yielding a unique probe (UA) Mirror Lab is signed by (L-R) Dr. -
50 Years of Existence of the European Southern Observatory (ESO) 30 Years of Swiss Membership with the ESO
Federal Department for Economic Affairs, Education and Research EAER State Secretariat for Education, Research and Innovation SERI 50 years of existence of the European Southern Observatory (ESO) 30 years of Swiss membership with the ESO The European Southern Observatory (ESO) was founded in Paris on 5 October 1962. Exactly half a century later, on 5 October 2012, Switzerland organised a com- memoration ceremony at the University of Bern to mark ESO’s 50 years of existence and 30 years of Swiss membership with the ESO. This article provides a brief summary of the history and milestones of Swiss member- ship with the ESO as well as an overview of the most important achievements and challenges. Switzerland’s route to ESO membership Nearly twenty years after the ESO was founded, the time was ripe for Switzerland to apply for membership with the ESO. The driving forces on the academic side included the Universi- ty of Geneva and the University of Basel, which wanted to gain access to the most advanced astronomical research available. In 1980, the Federal Council submitted its Dispatch on Swiss membership with the ESO to the Federal Assembly. In 1981, the Federal Assembly adopted a federal decree endorsing Swiss membership with the ESO. In 1982, the Swiss Confederation filed the official documents for ESO membership in Paris. In 1982, Switzerland paid the initial membership fee and, in 1983, the first year’s member- ship contributions. High points of Swiss participation In 1987, the Federal Council issued a federal decree on Swiss participation in the ESO’s Very Large Telescope (VLT) to be built at the Paranal Observatory in the Chilean Atacama Desert. -
The Southern Arizona Region
This report was prepared for the Southern Arizona’s Regional Steering Committee as an input to the OECD Review of Higher Education in Regional and City Development. It was prepared in response to guidelines provided by the OECD to all participating regions. The guidelines encouraged constructive and critical evaluation of the policies, practices and strategies in HEIs’ regional engagement. The opinions expressed are not necessarily those of the Regional Steering Committee, the OECD or its Member countries. 2 TABLE OF CONTENTS ACKNOWLEDGEMENTS............................................................................................................. iii ACRONYMS..................................................................................................................................... v LIST OF FIGURES, TABLES AND APPENDICES....................................................... ………. vii EXECUTIVE SUMMARY.............................................................................................................. ix CHAPTER 1. OVERVIEW OF THE SOUTHERN ARIZONA REGION................................. 1 1.1 Introduction…………………………………………………………………............................... 1 1.2 The geographical situation............................................................................................................ 1 1.3 History of Southern Arizona…………………………….………………………….................... 3 1.4 The demographic situation………………………………………………………………............ 3 1.5 The regional economy………………………………………………………………………...... 14 1.6 Governance.................................................................................................................................. -
Table of Contents
AAS Newsletter November/December 2012, Issue 167 - Published for the Members of the American Astronomical Society Table of Contents 2 President’s Column 23 Committee on Employment 3 From the Executive Office 24 Committee on the Status of Women in 4 On the Waterfront: AAS Returns to Long Astronomy Beach 25 Bringing Sustainability into Your Institution 5 2012 Kavli Lecturers 27 Calendar of Events 7 HAD News 28 Announcements 8 JWST Update 29 United Nations Basic Space Science Initiative 12 Candidate Statements (UNBSSI) 1991-2012 21 News from NSF Division of Astronomical Sciences (AST) Back page Washington News 22 News from the Astronomical Society of the Pacific (ASP) A A S American Astronomical Society President's Column AAS Officers David J. Helfand, President David J. Helfand, [email protected] Debra M. Elmegreen, Past President Nicholas B. Suntzeff, Vice-President Edward B. Churchwell, Vice-President Paula Szkody, Vice-President From close-up pictures of water-sculpted pebbles on Hervey (Peter) Stockman, Treasurer G. Fritz Benedict, Secretary Mars, to the detection of galaxies at the boundary of Anne P. Cowley, Publications Board Chair the Dark Ages, discoveries in our field continue to Edward E. Prather, Education Officer advance our understanding of the Universe and to Councilors fascinate legions of the public who support our inquiry. Bruce Balick Nancy S. Brickhouse Unfortunately, we do not see similar progress in the Eileen D. Friel political sphere, even now that the consequences have Edward F. Guinan been spelled out of allowing budget sequestration to hit Todd J. Henry Steven D. Kawaler every government agency in January. -
Exoplanet Community Report
JPL Publication 09‐3 Exoplanet Community Report Edited by: P. R. Lawson, W. A. Traub and S. C. Unwin National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California March 2009 The work described in this publication was performed at a number of organizations, including the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (NASA). Publication was provided by the Jet Propulsion Laboratory. Compiling and publication support was provided by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not constitute or imply its endorsement by the United States Government, or the Jet Propulsion Laboratory, California Institute of Technology. © 2009. All rights reserved. The exoplanet community’s top priority is that a line of probeclass missions for exoplanets be established, leading to a flagship mission at the earliest opportunity. iii Contents 1 EXECUTIVE SUMMARY.................................................................................................................. 1 1.1 INTRODUCTION...............................................................................................................................................1 1.2 EXOPLANET FORUM 2008: THE PROCESS OF CONSENSUS BEGINS.....................................................2 -
HAT-P-39B–HAT-P-41B: THREE HIGHLY INFLATED TRANSITING HOT JUPITERS∗
The Astronomical Journal, 144:139 (18pp), 2012 November doi:10.1088/0004-6256/144/5/139 C 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A. HAT-P-39b–HAT-P-41b: THREE HIGHLY INFLATED TRANSITING HOT JUPITERS∗ J. D. Hartman1,G.A.´ Bakos1,15,B.Beky´ 2, G. Torres2, D. W. Latham2,Z.Csubry1, K. Penev1, A. Shporer3,4, B. J. Fulton3, L. A. Buchhave5,6,J.A.Johnson7, A. W. Howard8, G. W. Marcy8,D.A.Fischer9,G.Kovacs´ 10,11, R. W. Noyes2, G. A. Esquerdo2, M. Everett2, T. Szklenar´ 2,S.N.Quinn2,12, A. Bieryla2,R.P.Knox13,P.Hinz13, D. D. Sasselov2,G.Fur˝ esz´ 2, R. P. Stefanik2,J.Laz´ ar´ 14, I. Papp14,andP.Sari´ 14 1 Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA; [email protected] 2 Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA 3 LCOGT, 6740 Cortona Drive, Santa Barbara, CA, USA 4 Department of Physics, Broida Hall, UC Santa Barbara, CA, USA 5 Niels Bohr Institute, University of Copenhagen, DK-2100, Denmark 6 Centre for Star and Planet Formation, Natural History Museum of Denmark, DK-1350 Copenhagen, Denmark 7 Department of Astrophysics, California Institute of Technology, MC 249-17, Pasadena, CA, USA 8 Department of Astronomy, University of California, Berkeley, CA, USA 9 Astronomy Department, Yale University, New Haven, CT, USA 10 Konkoly Observatory, Budapest, Hungary 11 Department of Physics and Astrophysics, University of North Dakota, Grand Forks, ND, USA 12 Department of Physics and Astronomy, Georgia State University, Atlanta, GA, USA 13 Steward Observatory, University of Arizona, Tucson, AZ, USA 14 Hungarian Astronomical Association, Budapest, Hungary Received 2012 July 13; accepted 2012 August 30; published 2012 October 9 ABSTRACT We report the discovery of three new transiting extrasolar planets orbiting moderately bright (V = 11.1, 11.7, and 12.4) F stars.