Citations to Australian Astronomy: 5 and 10 Year Benchmarks
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The Wigglez Dark Energy Survey: Probing the Epoch of Radiation Domination Using Large-Scale Structure
MNRAS 429, 1902–1912 (2013) doi:10.1093/mnras/sts431 The WiggleZ Dark Energy Survey: probing the epoch of radiation domination using large-scale structure Gregory B. Poole,1,2‹ Chris Blake,1 David Parkinson,3 Sarah Brough,4 Matthew Colless,4 Carlos Contreras,1 Warrick Couch,1 Darren J. Croton,1 Scott Croom,5 Tamara Davis,3 Michael J. Drinkwater,3 Karl Forster,6 David Gilbank,7 Mike Gladders,8 Karl Glazebrook,1 Ben Jelliffe,5 Russell J. Jurek,9 I-hui Li,10 Barry Madore,11 D. Christopher Martin,6 Kevin Pimbblet,12 Michael Pracy,1,13 4,13 1,14 15 Rob Sharp, Emily Wisnioski, David Woods, Downloaded from Ted K. Wyder6 and H. K. C. Yee10 1Centre for Astrophysics & Supercomputing, Swinburne University of Technology, PO Box 218, Hawthorn, VIC 3122, Australia 2School of Physics, University of Melbourne, Parksville, VIC 3010, Australia 3School of Mathematics and Physics, University of Queensland, Brisbane, QLD 4072, Australia 4Australian Astronomical Observatory, PO Box 915, North Ryde, NSW 1670, Australia http://mnras.oxfordjournals.org/ 5Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Australia 6California Institute of Technology, MC 278-17, 1200 East California Boulevard, Pasadena, CA 91125, USA 7South African Astronomical Observatory, PO Box 9, 7935 Observatory, Cape Town, South Africa 8Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637, USA 9Australia Telescope National Facility, CSIRO, Epping, NSW 1710, Australia 10Department of Astronomy and Astrophysics, -
The Wigglez Dark Energy Survey
The WiggleZ Dark Energy Survey Chris Blake (Swinburne University) Sarah Brough, Warrick Couch, Karl Glazebrook, Greg Poole (Swinburne University); Tamara Davis, Michael Drinkwater, Russell Jurek, Kevin Pimbblet (Uni. of Queensland); Matthew Colless, Rob Sharp (Anglo-Australian Observatory); Scott Croom (University of Sydney); Michael Pracy (Australian National University); David Woods (University of New South Wales); Barry Madore (OCIW); Chris Martin, Ted Wyder (Caltech) Abstract: The accelerating expansion rate of the Universe, attributed to “dark energy”, has no accepted theoretical explanation. The origin of this phenomenon unambiguously implicates new physics via a novel form of matter exerting neg- ative pressure or an alteration to Einstein’s General Relativity. These profound consequences have inspired a new generation of cosmological surveys which will measure the influence of dark energy using various techniques. One of the forerun- ners is the WiggleZ Survey at the Anglo-Australian Telescope, a new large-scale high-redshift galaxy survey which is now 50% complete and scheduled to finish in 2010. The WiggleZ project is aiming to map the cosmic expansion history using delicate features in the galaxy clustering pattern imprinted 13.7 billion years ago. In this article we outline the survey design and context, and predict the likely science highlights. Figure 1: Caption: The distribution of galaxies currently observed in the three WiggleZ Survey fields located near the Northern Galactic Pole. The observer is situated at the origin of the co-ordinate system. The radial distance of each galaxy from the origin indicates the observed redshift, and the polar angle indicates the galaxy right ascension. The faint patterns of galaxy clustering are visible in each field. -
The H-Index in Australian Astronomy
Addenda: The h-index in Australian Astronomy Kevin A. PimbbletA,B A School of Physics, Monash University, Clayton, VIC 3800, Australia B Email: [email protected] Abstract: Pimbblet (2011) published an evaluation of the Hirsch h-index in the context of the Aus- tralian astronomical community. This addenda adds treatment of changes of surname to the compu- tation of the h-index and presents derivative data on the m-index. Keywords: Errata, Addenda 1 Change of Surname Table 1: Top 10 h-index for Australian Astron- Pimbblet (2011) published a variety of analyses on the omy, excluding overseas professionals with correc- h-index (e.g. Hirsch 2005) in the context of Australian tion applied for surname changes. Astronomy. Alongside that, a discussion of a number Rank Name h of caveats was also made. One further caveat merits =1 KenFREEMAN 77 explicit attention in the interpretation of the h-index: =1 JeremyMOULD 77 changes of surname. In the Pimbblet (2011) analysis, 3 Karl GLAZEBROOK 71 no attempt was made to track surname changes. This 4 Dick MANCHESTER 68 has the effect of depressing the h-index of individuals 5 MichaelDOPITA 64 who have changed their names over the years. Its effect can readily be seen in Table 1 where we re-compute the 6 Warrick COUCH 61 top ten h-index for Australian Astronomy and account 7 Joss BLAND-HAWTHORN 57 for changing surnames: Bland-Hawthorn’s previous h- 8 MatthewCOLLESS 56 index was suppressed by 4 points by not taking this in 9 Brian SCHMIDT 54 to account. We emphasize that the same dataset was 10 MikeBESSELL 53 used for this re-computation as the original paper. -
Evidence for a Non-Zero L and a Low Matter Density from a Combined Analysis of the 2Df Galaxy Redshift Survey and Cosmic Microwa
Mon. Not. R. Astron. Soc. 330, L29–L35 (2002) Evidence for a non-zero L and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and cosmic microwave background anisotropies Downloaded from https://academic.oup.com/mnras/article-abstract/330/2/L29/1085554 by California Institute of Technology user on 20 May 2020 G. Efstathiou,1,2P Stephen Moody,1 John A. Peacock,3 Will J. Percival,3 Carlton Baugh,4 Joss Bland-Hawthorn,5 Terry Bridges,5 Russell Cannon,5 Shaun Cole,4 Matthew Colless,6 Chris Collins,7 Warrick Couch,8 Gavin Dalton,9 Roberto De Propris,8 Simon P. Driver,10 Richard S. Ellis,11 Carlos S. Frenk,4 Karl Glazebrook,12 Carole Jackson,6 Ofer Lahav,1 Ian Lewis,5 Stuart Lumsden,13 Steve Maddox,14 Peder Norberg,4 Bruce A. Peterson,6 Will Sutherland3 and Keith Taylor11 (The 2dFGRS Team) 1Institute of Astronomy, Madingley Road, Cambridge CB3 0HA 2Theoretical Astrophysics, Caltech, Pasadena, CA 91125, USA 3Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ 4Department of Physics, University of Durham, South Road, Durham DH1 3LE 5Anglo-Australian Observatory, PO Box 296, Epping, NSW 2121, Australia 6Research School of Astronomy and Astrophysics, The Australian National University, Weston Creek, ACT 2611, Australia 7Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Birkenhead L14 1LD 8Department of Astrophysics, University of New South Wales, Sydney, NSW 2052, Australia 9Astrophysics, Nuclear and Astrophysics Laboratory, University of Oxford, Keble Road, Oxford OX1 3RH 10School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife KY6 9SS 11Department of Astronomy, Caltech, Pasadena, CA 91125, USA 12Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218-2686, USA 13Department of Physics, University of Leeds, Woodhouse Lane, Leeds LS2 9JT 14School of Physics and Astronomy, University of Nottingham, Nottingham NG7 2RD Accepted 2001 November 26. -
Curriculum Vitae
CURRICULUM VITAE FULL NAME: George Petros EFSTATHIOU NATIONALITY: British DATE OF BIRTH: 2nd Sept 1955 QUALIFICATIONS Dates Academic Institution Degree 10/73 to 7/76 Keble College, Oxford. B.A. in Physics 10/76 to 9/79 Department of Physics, Ph.D. in Astronomy Durham University EMPLOYMENT Dates Academic Institution Position 10/79 to 9/80 Astronomy Department, Postdoctoral Research Assistant University of California, Berkeley, U.S.A. 10/80 to 9/84 Institute of Astronomy, Postdoctoral Research Assistant Cambridge. 10/84 to 9/87 Institute of Astronomy, Senior Assistant in Research Cambridge. 10/87 to 9/88 Institute of Astronomy, Assistant Director of Research Cambridge. 10/88 to 9/97 Department of Physics, Savilian Professor of Astronomy Oxford. 10/88 to 9/94 Department of Physics, Head of Astrophysics Oxford. 10/97 to present Institute of Astronomy, Professor of Astrophysics (1909) Cambridge. 10/04 to 9/08 Institute of Astronomy, Director Cambridge. 10/08 to present Kavli Institute for Cosmology, Director Cambridge. PROFESSIONAL SOCIETIES Fellow of the Royal Society since 1994 Fellow of the Instite of Physics since 1995 Fellow of the Royal Astronomical Society 1983-2010 Member of the International Astronomical Union since 1986 Associate of the Canadian Institute of Advanced Research since 1986 1 AWARDS/Fellowships/Major Lectures 1973 Exhibition Keble College Oxford. 1975 Johnson Memorial Prize University of Oxford. 1977 McGraw-Hill Research Prize University of Durham. 1980 Junior Research Fellowship King’s College, Cambridge. 1984 Senior Research Fellowship King’s College, Cambridge. 1990 Maxwell Medal & Prize Institute of Physics. 1990 Vainu Bappu Prize Astronomical Society of India. -
Garth D. Illingworth Resume Summary Astronomer/Professor Of
Garth D. Illingworth Resume Summary Astronomer/Professor of Astronomy University of California Observatories/Lick Observatory/ Department of Astronomy and Astrophysics University of California, Santa Cruz, California 95064 Voice: 831.459.2843 Fax: 831.426.3115 [email protected] http://www.ucolick.org/~gdi/ http://firstgalaxies.org Citizenship: U.S. ACADEMIC HISTORY 1965–1968 B.Sc. (Honors) 1st Class (Physics), University of Western Australia, Perth, WA 1969–1973 Ph.D. (Astrophysics) Australian National University, Mount Stromlo and Siding Spring Observatory, Ken Freeman, Supervisor 2010 D.Sc. (h.c.), University of Western Australia, Perth, Western Australia POSITIONS HELD 1974–1975 Postdoctoral Fellow, Kitt Peak National Observatory, Tucson, Arizona 1976–1977 Miller Fellow, Department of Astronomy, University of California, Berkeley 1978–1984 Astronomer, Kitt Peak National Observatory, Tucson, Arizona 1984–1987 Deputy Director, Space Telescope Science Institute, Baltimore, Maryland 1985–1987 Research Professor, Department of Physics and Astronomy, JHU 1988– Astronomer, University of California Observatories/Lick Observatory 1988– Professor, Department of Astronomy and Astrophysics, UCSC MAJOR ACTIVITIES/ACHIEVEMENTS 1. Awarded 2016 American Astronomical Society Lancelot M. Berkeley New York Community Trust Prize for work on The most-distant galaxies viewed with Hubble. Plenary Talk at January 2017 AAS 229 on Exploring for Galaxies in the First Billion Years with Hubble and Spitzer — Pathfinding for JWST 2. Science 1: Garth’s early work was on globular clusters and nearby ellipticals, but then with the advent of the powerful instruments on Hubble he transitioned to working on distant galaxies. Major ongoing programs on galaxy formation and evolution at high redshift from z ~ 2 ~ 10; recent work on galaxy build-up in the reionization epoch – during the first Gyr. -
Nobel Lecture: Measuring the Acceleration of the Cosmic Expansion Using Supernovae*
REVIEWS OF MODERN PHYSICS, VOLUME 84, JULY–SEPTEMBER 2012 Nobel Lecture: Measuring the acceleration of the cosmic expansion using supernovae* Saul Perlmutter University of California at Berkeley and Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA (published 13 August 2012) DOI: 10.1103/RevModPhys.84.1127 The ‘‘discovery of the acceleration of the expansion of the were studying supernovae. They saw that in principle, you Universe’’ does not flow trippingly off the tongue—which is could use a very bright exploding star, a supernova, to fitting, since the work that led to it was comparably long and perhaps answer this question. I will show you why that would tortuous. In this Lecture, I would like to give you a feel for be possible. some of the science issues we were facing over the ten years You could take the brightness of a supernova as an indi- leading up to the discovery. I will primarily use the graphics cator of how far away it is: the fainter it is, the farther away it from the original overhead projector transparencies we were is from us—and hence its light has taken more time to reach using in those years. Although they are not as beautiful as our us. So with the fainter supernovae, you are looking farther and modern-day graphics, I hope they will help give some of the farther back in time. You can also use the colors of the texture of what was going on during that period. spectral features of a supernova: a supernova would look The question that motivated all this work is something you blue if it were seen nearby, but when you see it very, very can imagine that the very first humans might have asked when far away it looks red. -
The K2-HERMES Survey. I. Planet-Candidate Properties from K2 Campaigns 1–3
The Astronomical Journal, 155:84 (10pp), 2018 February https://doi.org/10.3847/1538-3881/aaa3e4 © 2018. The American Astronomical Society. All rights reserved. The K2-HERMES Survey. I. Planet-candidate Properties from K2 Campaigns 1–3 Robert A. Wittenmyer1,2 , Sanjib Sharma3 , Dennis Stello3,4,5 , Sven Buder6,23, Janez Kos3, Martin Asplund7 , Ly Duong7, Jane Lin7,KarinLind6,8, Melissa Ness6, Tomaz Zwitter9 , Jonathan Horner1 ,JakeClark1, Stephen R. Kane10 , Daniel Huber3,11,12,13, Joss Bland-Hawthorn3 , Andrew R. Casey14,GayandhiM.DeSilva3,15,ValentinaD’Orazi16,KenFreeman7 , Sarah Martell4 , Jeffrey D. Simpson15,DanielB.Zucker15,17,18 , Borja Anguiano17,19, Luca Casagrande20 , James Esdaile4, Marc Hon4, Michael Ireland20 ,PrajwalR.Kafle21 , Shourya Khanna3,J.P.Marshall22,MohdHafiz Mohd Saddon4, Gregor Traven9 , and Duncan Wright4,15 1 University of Southern Queensland, Computational Engineering and Science Research Centre, Toowoomba, Queensland 4350, Australia; [email protected] 2 Australian Centre for Astrobiology, University of New South Wales, Sydney, NSW 2052, Australia 3 Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006, Australia 4 School of Physics, University of New South Wales, Sydney, NSW 2052, Australia 5 Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark 6 Max Planck Institute for Astronomy (MPIA), Koenigstuhl 17, D-69117 Heidelberg, Germany 7 Research School of Astronomy & Astrophysics, Australian National University, ACT 2611, Australia -
Annual Report Astronomy Australia Limited
2012 / 13 Annual Report Astronomy Australia Limited Vision Astronomers in Australia will have access to the best astronomical research infrastructure. Mission AAL will achieve its vision by: 1. Engaging with Australian astronomers to advance the national research infrastructure priorities of the Australian astronomy decadal plan. 2. Advising the Australian Government on future investments in national astronomical research infrastructure. 3. Managing investments in national astronomical research infrastructure as required. Principles 1. Access to major astronomical research infrastructure should be available to any Australian-based astronomer purely on scientific merit. 2. The concept of national astronomical research infrastructure includes Australian participation in international facilities. 3. The AAO and CSIRO are empowered by the Australian Government to provide a component of the national astronomical research infrastructure and there is no need for AAL to directly manage investments to upgrade or operate the AAT and ATNF. About AAL Astronomy Australia Limited (AAL) is a not-for-profit company whose members are all the Australian universities and research organisations with a significant astronomical research capability. AAL works with Australia’s National Observa- tories, astronomers and the Australian Government to advance the infrastructure goals in the 2006-2015 Decadal Plan for Australian Astronomy. Since its incorporation in 2007, AAL has coordinated the Australian astronomy response to, and managed the funding for, a number of national schemes and projects, including the Australian Government’s investments in astronomy infra- structure through the National Collaborative Research Infrastructure Strategy (NCRIS), the Education Investment Fund (EIF) and the Collaborative Research Infrastructure Scheme (CRIS). Background image 5x2-minute snapshot of the Galactic centre taken using 121 tiles of the Murchison Widefield Array at 150MHz, mosaicked together in the im- age domain. -
In Search of Dark Matter Ken Freeman and Geoff Mcnamara in Search of Dark Matter
In Search of Dark Matter Ken Freeman and Geoff McNamara In Search of Dark Matter Published in association with Praxis Publishing Chichester, UK Professor Ken Freeman Mr Geoff McNamara Research School of Astronomy & Astrophysics Science Teacher The Australian National University Evatt Mount Stromlo Observatory ACT ACT Australia Australia SPRINGER±PRAXIS BOOKS IN POPULAR ASTRONOMY SUBJECT ADVISORY EDITOR: John Mason B.Sc., M.Sc., Ph.D. ISBN 10: 0-387-27616-5 Springer Berlin Heidelberg New York ISBN 13: 978-0-387-27616-8 Springer is a part of Springer Science + Business Media (springeronline.com) Library of Congress Control Number: 2005931115 Apart from any fair dealing for the purposes of research or private study, or criticism or review, as permitted under the Copyright, Designs and Patents Act 1988, this publication may only be reproduced, stored or transmitted, in any form or by any means, with the prior permission in writing of the publishers, or in the case of reprographic reproduction in accordance with the terms of licences issued by the Copyright Licensing Agency. Enquiries concerning reproduction outside those terms should be sent to the publishers. # Copyright, 2006 Praxis Publishing Ltd. The use of general descriptive names, registered names, trademarks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. Cover design: Jim Wilkie Copy editing and graphics processing: R. A. Marriott -
Astronomers Count the Cost of Thinking
news Astronomers count the cost of thinking big Carina Dennis,Sydney Optical astronomy is now dominated by the word ‘large’,which is posing a sizeable prob- lem for many countries that want to remain at its cutting edge. Increasingly, ground-based projects are centred on big, expensive endeavours as exemplified by several proposals currently being circulated for an extremely large tele- scope (ELT). But medium-sized countries such as Australia face an uphill struggle to achieve meaningful participation in these D. OBSERVATORY MALIN/ANGLO-AUSTRALIAN large,internationally funded projects. Australian astronomers are keenly aware of the dilemma,and a task force set up in May by the National Committee for Astronomy (NCA) is seeking a way for the country to establish a prominent role in an ELT project. “We need to be part of a large telescope programme to survive,” says Ken Freeman, an astronomer based at the Australian National University (ANU) in Canberra. “There is an urgent need for Australia to decide what it wants to do, how it does it and with whom,” says Matthew Colless, who is chairing the task force. The panel aims to help prepare a case that could convince a sceptical government to fork out upwards of A$100 million (US$65 million) for partici- The Anglo-Australian Observatory, which recorded these star trails, has had to redefine its priorities. pation in an ELT project. The NCA,part of the Australian Academy projects. Local telescopes are being upgraded says Penny Sackett, director of the ANU’s of Science, is preparing its decadal review of to carry out surveys of the entire southern sky, Mount Stromlo Observatory,which is build- astronomy priorities, which it will deliver to including the Radial Velocity Experiment and ing two instruments for Gemini. -
HERMES Shipped
OBSERVERTHE AUSTRALIAN ASTRONOMICAL OBSERVATORY NEWSLETTER NUMBER 124 AUGUST 2013 HERMES shipped New AAO Director | Wambelong Fire: Before and After | Growth of BCGs DIRECTOR’S MESSAGE Director’s message Warrick Couch Having been associated with the AAO where there are many areas the AAO Director’s cottage adjacent to the AAT. for more than 30 years as both one of its and ANU can both benefit by working The Warrumbungles seem to have taken employees and a user of its telescopes, closely together (e.g. on instrumentation on a whole new character and appearance, I feel very honoured to now being projects and SSO operations). with rocky outcrops and other geological making this appearance on page 3 of features that had never been seen before As readers will be well aware from the the newsletter, with the responsibility now rendered visible, and the ghostly last issue of the AAO Observer, the of providing the Director’s message. appearance of hectare upon hectare of time between this most recent change Moreover, I realize I have a very hard act gum trees stripped bare of their leaves, but of directors was a very eventful and to follow, given the outstanding calibre their pale bark left intact. That none of the challenging period for the AAO. Just days of my immediate predecessor, Matthew telescopes on Siding Spring Mountain were after I had accepted the job, I wondered Colless, as well as his predecessors (Brian seriously damaged would seem a miracle, if there would be any telescopes left for Boyle, Russell Cannon, Don Morton, and and the fact that the AAT was back in me to direct, with a massive bushfire Joe Wampler).