Stories from Siding Spring Observatory

Total Page:16

File Type:pdf, Size:1020Kb

Stories from Siding Spring Observatory Please return to reception Stories from Siding Spring Observatory PHOTOGRAPHS BY STAFF OF THE AUSTRALIAN ASTRONOMICAL OBSERVATORY Siding Spring Observatory sits on a mountaintop in the Warrumbungle Range, 400 km northwest of Sydney and 25 km west of the town of Coonabarabran. Run by the Australian National University, it is Australia’s most important site for optical astronomy. On 13 January 2013 a bushfire swept through the observatory. Despite damage to some buildings, the telescopes were unharmed and are now back at work. The photos in this exhibition tell stories of life and work on the mountain. They were taken by staff of the Australian Astronomical Observatory (AAO), which operates two telescopes there: the 4-m Anglo- Australian Telescope (AAT) and the UK Schmidt telescope. GROUND FLOOR Room 4 Comet Lovejoy Room 1 by Steven Lee, Sunset at Siding Spring Head Night Assistant by Maritza Lara-López, Comet Lovejoy, discovered ARC Super Science Fellow by Australian amateur A view of the Siding astronomer Terry Lovejoy, was one of the brightest Spring Observatory, looking west from the Anglo- comets of recent years. This photo was taken in Australian Telescope. The observatory is home to the morning twilight on Christmas Day 2011. 11 operating telescopes: not all of them can be seen in this photo. FIRST FLOOR Wide-angle view of the AAT by Ángel López-Sánchez, South Dome Astronomy Fellow The AAT at evening This wide-angle view of the by Sarah Brough, Anglo-Australian Telescope Research Astronomer shows the whole telescope structure, which is Sarah Brough took this photo hard to capture in a single shot. while visiting the Anglo- Australian Telescope in 2008 to observe for In the AAT control room WiggleZ, a project to investigate the properties of by Keith Shortridge, the mysterious ‘dark energy’. Software Engineer Astronomers and engineers North Dome in the control room of the UK Schmidt telescope Anglo-Australian Telescope during testing of a by Nuria Lorente, Software Engineer new instrument, called GNOSIS, in 2011. (Left to Nuria Lorente joined the AAO right) Simon Ellis, Jon Lawrence, Anthony Horton in 2012 after working overseas and Steve Chapman. for 20 years. This photo was her response to seeing the UK Schmidt telescope (far left) for the first time in two decades. Testing an instrument Room 7 by Keith Shortridge, Rainbows at sunrise from the AAT Software Engineer by Amanda Bauer, Instrument scientist Simon ARC Super Science Fellow Ellis works beside the “We’d just finished observing [all Anglo-Australian Telescope during testing of a night]. I walked out and saw this new instrument, called GNOSIS, in 2011. GNOSIS massive double rainbow. I was contained special optical fibres that filter out exhausted and ready to go to bed, unwanted light from Earth’s atmosphere, but when I saw this I ran right back up to the improving the view of the Universe beyond. catwalk.” FIRST FLOOR Lightning to the west (VIA RECEPTION STAIRCASE) by Andy Green, Science Fellow Stairs landing (Room 12) “The storm had multiple layers, with lightning going in many AAT dome and directions.” Andy Green took this photo from the Milky Way catwalk of the Anglo-Australian Telescope in 2012. by James Gilbert, Electronics Engineer Room 9 This image, covering almost 180º, is made from seven photos ‘stitched’ together. James Gilbert Kangaroos outside the door was at the observatory to supervise two students by Maritza Lara-López, in September 2012, when he captured this view ARC Super Science Fellow of the Anglo-Australian Telescope and the Maritza Lara-López took this Milky Way. photo from the Lodge — the astronomers’ accommodation block at Siding The sky over the AAT Spring Observatory. Kangaroos were always by Maritza Lara-López, ARC around, day and night. The Lodge was destroyed Super Science Fellow by the bushfire of 13 January 2013 To the left, the Milky Way looms over the dome of the Night and day Anglo-Australian Telescope; it is our own galaxy, by Ángel López-Sánchez, seen from within. The bright fuzzy patches, centre Astronomy Fellow and right, are the Large and Small Magellanic This image was created from Clouds, tiny galaxies that orbit ours. All three are photos taken for a time- prime targets for telescopes in the Southern lapse video of the Anglo-Australian Telescope in Hemisphere. October 2011. The frame on the left was taken during the morning twilight; the frame on the Star-trails above the AAT right, 15 hours earlier, during the day. by Ángel López-Sánchez, Astronomy Fellow SkyMapper and Milky Way This image was created from by James Gilbert, Electronics Engineer more than 1400 exposures, The ANU’s new SkyMapper taken during one night. Each exposure took 30 telescope stands on almost the seconds. As the Earth turns, the stars appear to highest point of Siding Spring rotate around the south celestial pole in the sky Observatory. Here, the centre of our above the Anglo-Australian Telescope. Milky Way galaxy rides in the sky behind it, bright with stars but veiled with dark dust. SkyMapper will record the whole southern sky — more than a billion stars. The fire approaches Astronomers at the AAT by Andy Green, Science Fellow by Amanda Bauer, Andy Green was at the ARC Super Science Fellow Anglo-Australian Telescope It’s hard to study our own to support four visiting galaxy from within. These astronomers, when the bushfire approached astronomers were at the Anglo-Australian Siding Spring Observatory on 13 January 2013. Telescope to search for other galaxies the same Soon after he took this photo, the observatory size and shape as the Milky Way — ones that can was evacuated. be studied from the outside. (Left to right) Mehmet Alpaslan, ICRAR, and Andrew Hopkins, AAO. Survivor by Alex King, Coonabarabran Rural Fire Service pilot by Yuri Kondrat, Alex King took this photo on Mechanical Engineer 13 January 2013. Two Siding Spring Observatory lies observatory buildings were lost to the fire but all 25 km from the small town of the telescopes were saved.“The NSW Rural Fire Coonabarabran. SSO staff live in and around the Service posted this image, and I started to cry.” town, and visiting staff and observers often stay – Amanda Bauer there also. Yuri Kondrat took this photo on a winter morning before going to the observatory. After the fire by Steven Lee, Night assistant ‘at rest’ Head Night Assistant by Amanda Bauer, “It was a dramatic change to a ARC Super Science Fellow familiar scene.” Steven Lee Night assistant Tim Connor took this photo of the Warrumbungle National takes a few minutes’ break. Park from the catwalk of the Anglo-Australian The night assistants at the AAT help visiting Telescope on 31 January 2013, two weeks after fire astronomers make their observations. had swept through the park and observatory. Ready for work Regrowth by Ángel López-Sánchez, by Fred Watson, Astronomer in Astronomy Fellow Charge, AAT This photo shows the Anglo- Seven weeks after the fire, Australian Telescope, with the new shoots are bursting out mirror cover open, ready to start of the trees on and around Siding Spring observing. The ‘top end’ of the Observatory. This photo was taken on 5 March telescope is carrying the 2dF (two-degree field) 2013. instrument, which has optical fibres that capture light reflected upwards by the main mirror. Room 11 Time-lapse videos On top of the dome by Ángel López-Sánchez by Andrew Hopkins, Head of AAT Science • The sky over the Anglo-Australian Telescope Andrew Hopkins has used the • A 6dF night at the UK Schmidt telescope Anglo-Australian Telescope since • A 2dF night at the Anglo-Australian Telescope the mid 1990s, but this was the • The sky over Siding Spring Observatory first time he had climbed to the Running time: 12 minutes top of the dome. Andrew took the photo during a group visit by AAO staff in December 2012. (Left to right) Simon Ellis, Doug Gray, Simon O’Toole, Tony Farrell, Andy Sheinis, Anthony Horton and Nuria Lorente. Please return to reception THE AUSTRALIAN ASTRONOMICAL OBSERVATORY The Australian Astronomical Observatory, a division of the Department of Industry, Innovation, Climate Change, Science, Research and Tertiary Education, operates the Anglo-Australian and UK Schmidt telescopes on behalf of the Australian astronomical community. The AAO exists to provide world-class optical and infrared observing facilities that enable Australian astronomers to do excellent science. It is a world leader in astronomical research and in the development of innovative telescope instrumentation, and also plays an active role in the formulation of long-term plans for Australian astronomy. The telescopes of the AAO are located in the Warrumbungle mountains near Coonabarabran in northern New South Wales. Harley Wood, NSW Government Astronomer at Sydney Observatory from 1943 to 1974, suggested this location, among others, during site-selection visits he made throughout the state. The site is now recognised as one of the darkest astronomical observing sites in the world. This exhibition was developed by the Australian Astronomical Observatory, with support from Sydney Observatory and the Powerhouse Museum. TOILETS (outside) 5 EMERGENCY WHEELCHAIR/GROUP EXIT ENTRY Lecture room GROUND FLOOR 4 EMERGENCY EXIT ENTRY/EXIT 3 Planetarium 1 (occasional sessions) 2 EMERGENCY EXIT North Dome Balcony 10 Videos 11 FIRST FLOOR 6 Russell room 12 9 Stairs landing South Dome 7 8 Sydney Observatory, part of the Powerhouse Museum, is a NSW government cultural institution. Brochure design © Trustees of the Powerhouse Museum. Text and images © Australian Astronomical Observatory.
Recommended publications
  • 2004-2005 Annual Report
    Anglo-Australian Observatory Annual Report of the Anglo-Australian Telescope Board 1 July 2004 to 30 June 2005 Anglo-Australian Observatory 167 Vimiera Road Eastwood NSW 2122 Australia Postal Address: PO Box 296 Epping NSW 1710 Australia Telephone: (02) 9372 4800 (international) + 61 2 9372 4800 Facsimile: (02) 9372 4880 (international) + 61 2 9372 4880 e-mail: [email protected] Website: http://www.aao.gov.au/ Annual Report Website: http://www.aao.gov.au/annual/ Anglo-Australian Telescope Board Address as above Telephone: (02) 9372 4813 (international) + 61 2 9372 4813 e-mail: [email protected] ABN: 71871323905 © Anglo-Australian Telescope Board 2005 ISSN 1443-8550 Cover: Dome of the UK Schmidt Telescope. Photo courtesy Shaun Amy. Combined H-alpha and Red colour mosaic image of the Vela Supernova remnant taken from several AAO/UK Schmidt Telescope H- alpha survey fields. Image produced by Mike Read and Quentin Parker Cover Design: TTR Print Management Computer Typeset: Anglo-Australian Observatory Picture Credits: The editors would like to thank for their photographs and images throughout this publication Shaun Amy, Stuart Bebb (Physics Photo- graphic Unit, Oxford), Jurek Brzeski, Chris Evans, Kristin Fiegert, David James, Urs Klauser, David Malin, Chris McCowage and Andrew McGrath ii AAO Annual Report 2004–2005 The Honourable Dr Brendan Nelson, MP, Minister for Education, Science and Training Government of the Commonwealth of Australia The Right Honourable Alan Johnson, MP, Secretary of State for Trade and Industry, Government of the United Kingdom of Great Britain and Northern Ireland In accordance with Article 8 of the Agreement between the Australian Government and the Government of the United Kingdom to provide for the establishment and operation of an optical telescope at Siding Spring Mountain in the state of New South Wales, I present herewith a report by the Anglo-Australian Telescope Board for the year from 1 July 2004 to 30 June 2005.
    [Show full text]
  • Surveys with Small Optical Telescopes
    SMALL-TELESCOPE SURVEYS Surveys with small optical telescopes Downloaded from https://academic.oup.com/astrogeo/article-abstract/60/6/6.14/5625003 by Institute of Child Health/University College London user on 04 March 2020 Tony Lynas-Gray reviews the odern astrophysics owes its exist- 1976) detectors, surveys were extended into history of surveys with small ence to small-telescope surveys the near-infrared. Moreover, images and Mdating back to the 18th century, spectra obtained using CCDs and digitized telescopes and explains why they for example Flamsteed (1725). In the 19th photographic plates are in a machine-read- are still vital to support the work century, Argelander’s survey based on able form and amenable to processing with of much larger telescopes. visual observations with small telescopes modern numerical methods. and meridian circles culminated in the 1859 In this article I summarize some of the publication of the Bonner Durchmusterung more important surveys – and results – (BD), a catalogue of northern hemisphere carried out so far with small telescopes stars brighter than ninth magnitude, with (having an aperture of no more than 2 m). accompanying charts (Batten 1991). The BD Modern networks of small tele scopes catalogue was later extended to the south- operated robotically are expected to ern hemisphere by the Córdoba Durch- continue survey work for the foreseeable musterung (CD; 1892 onwards) prepared future: small telescopes in general need to using Argelander’s method, and the Cape be retained for follow-up observations of Photographic Durchmusterung (CPD; 1885 brighter targets of interest discovered in onwards) based on photographic plates.
    [Show full text]
  • WG 3.2 National-Scale Facilities
    National Facilities A report to the National Committee for Astronomy for the Australian Astronomy Decadal Plan 2006-2015 By Working Group 3.2 September 2005 Executive Summary Australia’s national facilities for observational astronomy are the Anglo-Australian Observatory (AAO) and the Australia Telescope National Facility (ATNF). In the period covered by this Decadal Plan the United Kingdom will substantially reduce its contribution to the operations budget of the AAO. In consequence, a major issue for this WG to consider is the future funding of the AAO. In addition to the AAO and ATNF, several Australian universities operate observing facilities that have a significant role at a national level: either by offering observing time to outside users or by providing infrastructure as in the case of the ANU’s Siding Spring Observatory (SSO). Rather than duplicate the detailed discussions of these facilities, the three Facilities WG chairs agreed to assign facilities like SSO into one or the other WGs: this was for practical reasons and does not imply any judgement about the status of the respective university facilities. Our discussions at this stage of the Decadal Plan process were independent of the scientific priorities from the science WGs, so are based mainly on strategic issues informed by the submissions we received and our own experience as users (and senior staff) of national facilities. The lack of a detailed science case at this stage of the process makes it hard to assign relative ranks to all the facilities discussed. However we have identified the top and bottom items: • In all our discussions there was unqualified support for the AAO and ATNF as our two national facilities.
    [Show full text]
  • The 6Df Galaxy Survey Is a Very Effective Means of Determining the True Mass Distribution in the Local Universe
    **TITLE** ASP Conference Series, Vol. **VOLUME***, **YEAR OF PUBLICATION** **NAMES OF EDITORS** The 6dF Galaxy Survey Ken-ichi Wakamatsu Faculty of Engineering, Gifu University, Gifu 501-1192, Japan Matthew Colless Mount Stromlo & Siding Spring Observatories, ACT 2611, Australia Tom Jarrett IPAC, Caltech, MS 100-22, Pasadena, CA 91125, USA Quentin Parker Macquarie University, Sydney 2109, Australia William Saunders Anglo-Australian Observatory, Epping NSW 2121, Australia Fred Watson Anglo-Australian Observatory, Coonabarabran NSW 2357, Australia Abstract. The 6dF Galaxy Survey (6dFGS) 1 is a spectroscopic sur- vey of the entire southern sky with |b| > 10◦, based on the 2MASS near infrared galaxy catalog. It is conducted with the 6dF multi-fiber spec- trograph attached to the 1.2-m UK Schmidt Telescope. The survey will produce redshifts for some 170,000 galaxies, and peculiar velocities for about 15,000 and is expected to be complete by June 2005. arXiv:astro-ph/0306104v1 5 Jun 2003 1. Introduction In order to reveal large-scale structures at intermediate and large distances, ex- tensive galaxy redshift surveys have been carried out, e.g. the 2dFGRS and SDSS, and the Hubble- and Subaru-deep field surveys. There is now an ur- gent need to study the large-scale structure of the Local Universe that can be compared with the above deeper surveys. However to do this required hemi- 1Member of Science Advisory Group: M. Colless (Chair; ANU, Australia), J. Huchra (CfA, USA), T. Jarrett (IPAC, USA), O. Lahav (Cambridge, UK), J. Lucey (Dahram, UK), G. Mamon (IAP, France), Q. Parker (Maquarie Univ. Australia), D. Proust (Meudon, France), E.
    [Show full text]
  • Not Yet Imagined: a Study of Hubble Space Telescope Operations
    NOT YET IMAGINED A STUDY OF HUBBLE SPACE TELESCOPE OPERATIONS CHRISTOPHER GAINOR NOT YET IMAGINED NOT YET IMAGINED A STUDY OF HUBBLE SPACE TELESCOPE OPERATIONS CHRISTOPHER GAINOR National Aeronautics and Space Administration Office of Communications NASA History Division Washington, DC 20546 NASA SP-2020-4237 Library of Congress Cataloging-in-Publication Data Names: Gainor, Christopher, author. | United States. NASA History Program Office, publisher. Title: Not Yet Imagined : A study of Hubble Space Telescope Operations / Christopher Gainor. Description: Washington, DC: National Aeronautics and Space Administration, Office of Communications, NASA History Division, [2020] | Series: NASA history series ; sp-2020-4237 | Includes bibliographical references and index. | Summary: “Dr. Christopher Gainor’s Not Yet Imagined documents the history of NASA’s Hubble Space Telescope (HST) from launch in 1990 through 2020. This is considered a follow-on book to Robert W. Smith’s The Space Telescope: A Study of NASA, Science, Technology, and Politics, which recorded the development history of HST. Dr. Gainor’s book will be suitable for a general audience, while also being scholarly. Highly visible interactions among the general public, astronomers, engineers, govern- ment officials, and members of Congress about HST’s servicing missions by Space Shuttle crews is a central theme of this history book. Beyond the glare of public attention, the evolution of HST becoming a model of supranational cooperation amongst scientists is a second central theme. Third, the decision-making behind the changes in Hubble’s instrument packages on servicing missions is chronicled, along with HST’s contributions to our knowledge about our solar system, our galaxy, and our universe.
    [Show full text]
  • Astronomy in Australia
    The Organisation DOI: 10.18727/0722-6691/5047 Astronomy in Australia Fred Watson1 Aboriginal peoples, is the Emu, whose position as engineer and surveyor to Warrick Couch1 head, neck and body are the Coalsack the new settlement, Dawes was also a Nebula and the dust clouds of Circinus, botanist and a keen astronomer who Norma and Scorpius. built a small observatory at what is now 1 Australian Astronomical Observatory, called Dawes Point, close to the southern Sydney, Australia Conventional “join-the-dots” constella- pylon of the Sydney Harbour Bridge. He tions also abound, but vary widely from is also notable as the first compiler of an one Aboriginal culture to another. Orion, Aboriginal language dictionary through Australians have watched the sky for for example, is seen as Njiru (the hunter) his association with Petyegarang (Grey tens of thousands of years. The nine- in the Central Desert Region, but the Kangaroo), a woman of the Eora Nation. teenth century saw the foundation of Yolngu people of Northern Australia see government observatories in capital the constellation as a canoe, with three Of more lasting significance to astronomy cities such as Sydney and Melbourne. brothers sitting abreast in the centre is a piece of Australian-Scottish heritage While early twentieth-century astron- ( Orion’s Belt) and a forbidden fish in the centring around Sir Thomas Makdougall omy focused largely on solar physics, canoe represented by the Orion Nebula. Brisbane (1773–1860), a conservation- the advent of radio astronomy at the Virtually all Dreamtime stories character- minded soldier, statesman and scientist. end of the Second World War enabled ise the Moon as male and the Sun as Brisbane was the sixth governor of New Australia to take a leading role in the female, with a tacit understanding that South Wales (NSW), and an examination new science, with particular emphasis the covering of the Sun by the Moon dur- of his career prior to this suggests that on low-frequency studies.
    [Show full text]
  • TAIPAN Instrument Fibre Positioner and Starbug Robots: Engineering Overview Nicholas F
    TAIPAN Instrument Fibre Positioner and Starbug Robots: Engineering Overview Nicholas F. Staszak*, Jon Lawrence, David M. Brown, Rebecca Brown, Ross Zhelem, Michael Goodwin, Kyler Kuehn, Nuria P. F. Lorente, Vijay Nichani, Lew Waller, Scott Case, Robert Content, Andrew M. Hopkins, Urs Klauser, Naveen Pai, Rolf Mueller, Slavko Mali, Minh V. Vuong Australian Astronomical Observatory, 105 Delhi Rd., North Ryde, NSW 2113, Australia. ABSTRACT TAIPAN will conduct a stellar and galaxy survey of the Southern sky. The TAIPAN positioner is being developed as a prototype for the MANIFEST instrument on the GMT. The design for TAIPAN incorporates 150 optical fibres (with an upgrade path to 300) situated within independently controlled robotic positioners known as Starbugs. Starbugs allow precise parallel positioning of individual fibres, thus significantly reducing instrument configuration time and increasing the amount of observing time. Presented is an engineering overview of the UKST upgrade of the completely new Instrument Spider Assembly utilized to support the Starbug Fibre Positioning Robot and current status of the Starbug itself. Keywords: fibre positioning systems, Starbugs, MANIFEST, TAIPAN, UKST, GMT 1. INTRODUCTION TAIPAN, currently nearing completion, is a multi-object parallel-positioning fibre-optic spectrograph designed for the UK Schmidt Telescope at Siding Spring Observatory in northern New South Wales, Australia. The instrument will be used to perform galaxy and stellar surveys across the whole Southern hemisphere sky, over a 5 year period. The fibre positioning portion of TAIPAN consists of a complete refurbishment of the UKST interior spider which replaces the 6DF serial positioning instrument used for the RAVE and 6dfG surveys. The TAIPAN Instrument Structure provides a stiff, low deflection, spider to interface the necessary support infrastructure to allow the Starbug Positioning Robots to operate, while maintaining a minimum obscuration of the incoming beam.
    [Show full text]
  • Know Thy Star, Know Thy Planet: Chemo-Kinematically Characterizing TESS Targets
    MNRAS 000, 1{19 (2019) Preprint 19 November 2019 Compiled using MNRAS LATEX style file v3.0 Know thy star, know thy planet: Chemo-kinematically characterizing TESS targets Andreia Carrillo1;2?, Keith Hawkins1, Brendan P. Bowler1, William Cochran1, and Andrew Vanderburg1 1Department of Astronomy, University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712-1205, USA 2Large Synoptic Survey Telescope Corporation Data Science Fellow Accepted XXX. Received YYY; in original form ZZZ ABSTRACT The Transiting Exoplanet Survey Satellite (TESS) has already begun to discover what will ultimately be thousands of exoplanets around nearby cool bright stars. These potential host stars must be well-understood to accurately characterize exoplanets at the individual and population levels. We present a catalogue of the chemo-kinematic properties of 2,218,434 stars in the TESS Candidate Target List using survey data from Gaia DR2, APOGEE, GALAH, RAVE, LAMOST, and photometrically-derived stellar properties from SkyMapper. We compute kinematic thin disc, thick disc, and halo membership probabilities for these stars and find that though the majority of TESS targets are in the thin disc, 4% of them reside in the thick disc and <1% of them are in the halo. The TESS Objects of Interest in our sample also display similar contributions from the thin disc, thick disc, and halo with a majority of them being in the thin disc. We also explore metallicity and [α/Fe] distributions for each Galactic component and show that each cross-matched survey exhibits metallicity and [α/Fe] distribution functions that peak from higher to lower metallicity and lower to higher [α/Fe] from the thin disc to the halo.
    [Show full text]
  • Galaxy Populations in Galaxy Clusters Selected by the Sunyaev-Zeldovich Effect
    Galaxy Populations in Galaxy Clusters Selected by the Sunyaev-Zeldovich Effect Alfredo Andr´esZenteno Vivanco Galaxy Populations in Galaxy Clusters Selected by the Sunyaev-Zeldovich Effect Alfredo Andr´esZenteno Vivanco Dissertation an der Fakult¨at f¨urPhysik Dissertation at the Faculty of Physics der Ludwig-Maximilians-Universit¨atM¨unchen of the Ludwig Maximilian University of Munich f¨urden Grad des for the degree of Doctor rerum naturalium vorgelegt von Alfredo Andr´esZenteno Vivanco presented by Alfredo Andr´esZenteno Vivanco aus Concepci´on,Chile from Concepci´on,Chile M¨unchen,den 09.12.2013 1st Evaluator: Prof. Dr. Joseph Mohr 2nd Evaluator: Prof. Dr. Andreas Burkert Date of the oral exam: 24.02.2014 vii To the memory of Crystal Marie Brasseur viii Zusammenfassung Wir pr¨asentieren eine Studie ¨uber die Galaxienpopulation in massereichen Galaxienhaufen, ausgew¨ahltaufgrund ihrer Signatur im Sunyaev{Zel'dovich Effekt (SZE). Die Auswahl mit- tels des SZE ist ann¨aherndmassenlimitiert, d.h. das untere detektierbare Massenlimit variiert nur geringf¨ugigmit der Rotverschiebung, wodurch der SZE eine ideale Auswahlmethode f¨ur ein Studium der Entwicklung von Galaxien innerhalb einer Haufenumgebung ist. Wir be- ginnen diese Arbeit mit einer Einf¨uhrungin den SZE, einer Vorstellung des S¨udpolteleskops (SPT) mittels dessen der SZE gemessen werden kann, sowie des Forschungsprojekts, inner- halb dessen diese Arbeit entstanden ist. Im Folgenden pr¨asentieren wir dann die Studien zur Galaxienpopulation, die der Kern dieser Doktorarbeit sind. In Kapitel 3 pr¨asentieren wir die erste großskalige Folgestudie eines mittels des SZE aus- gew¨ahltenGalaxienhaufen{Samples. Von 224 Galaxienhaufen{Kandidaten des Samples wer- den 158 Haufen durch Beobachtungen im Optischen best¨atigtund deren photometrische Rotverschiebungen bestimmt.
    [Show full text]
  • Spectroscopy Techniques and Projects at 1.2-M UK Schmidt Telescope
    Spectroscopy Techniques and Projects at 1.2-m UK Schmidt Telescope PrimoˇzCigler Mentor: prof. dr. TomaˇzZwitter Seminar Leader: prof. dr. Peter Kriˇzan March, 2012 Abstract Spectroscopy is one of the most important techniques for obtaining information from the celestial objects. At Australian Astronomical Observatory in New South Wales, Australia, the most advanced method for obtaining multiple spectra has been developed in the last decade. This seminar will present the spectroscopy techniques developed and recent projects on 1.2-m UK Schmidt Telescope equipped with optical fibers to obtain up to 150 spectra of stars or galaxies simultaneously. 1 Contents 1 Introduction 3 2 Spectroscopy 3 2.1 Prisms and Gratings . 3 2.2 Application of Optical Fibers . 4 3 UK Schmidt Telescope at AAO 6 3.1 Australian Astronomical Observatory . 6 3.2 1.2-m UK Schmidt Telescope . 6 4 6dF and Multi{Object Spectroscopy 9 4.1 6-degree Field . 9 4.2 Spectrograph . 10 4.3 RAVE . 11 4.4 Why Multi-Object Spectroscopy? . 12 5 Acknowledgements 12 2 1 Introduction This script is a product of the subject seminar, which is mandatory in the third grade of study on Fakulteta za matematiko in fiziko, Univerza v Ljubljani. I am a student of astronomy direction, so I decided to prepare a seminar about the astronomical topic. Since I had a plan to go to the holidays in Australia after the winter semester of study year 2011/12, my mentor, prof. dr. TomaˇzZwitter, suggested me to visit the Australian Astronomical Observatory in New South Wales, Australia and prepare a seminar based on the visit and their work at the observatory.
    [Show full text]
  • The Sixth Data Release of the Radial Velocity Experiment (RAVE)
    The Sixth Data Release of the Radial Velocity Experiment (RAVE). I. Survey Description, Spectra, and Radial Velocities Matthias Steinmetz, Gal Matijevič, Harry Enke, Tomaž Zwitter, Guillaume Guiglion, Paul Mcmillan, Georges Kordopatis, Marica Valentini, Cristina Chiappini, Luca Casagrande, et al. To cite this version: Matthias Steinmetz, Gal Matijevič, Harry Enke, Tomaž Zwitter, Guillaume Guiglion, et al.. The Sixth Data Release of the Radial Velocity Experiment (RAVE). I. Survey Description, Spectra, and Radial Velocities. Astronomical Journal, American Astronomical Society, 2020, 160 (2), pp.82. 10.3847/1538-3881/ab9ab9. hal-02985019 HAL Id: hal-02985019 https://hal.archives-ouvertes.fr/hal-02985019 Submitted on 1 Nov 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Draft version June 11, 2020 Typeset using LATEX preprint style in AASTeX62 The Sixth Data Release of the Radial Velocity Experiment (Rave) { I: Survey Description, Spectra and Radial Velocities Matthias Steinmetz,1 Gal Matijevicˇ,1 Harry Enke,1 Tomaˇz Zwitter,2 Guillaume Guiglion,1 Paul J. McMillan,3 Georges Kordopatis,4 Marica Valentini,1 Cristina Chiappini,1 Luca Casagrande,5 Jennifer Wojno,6 Borja Anguiano,7 Olivier Bienayme´,8 Albert Bijaoui,4 James Binney,9 Donna Burton,10, 11 Paul Cass,10 Patrick de Laverny,4 Kristin Fiegert,10 Kenneth Freeman,5 Jon P.
    [Show full text]
  • The RAVE Survey: the Galactic Escape Speed and the Mass of the Milky Way
    A&A 562, A91 (2014) Astronomy DOI: 10.1051/0004-6361/201322531 & c ESO 2014 Astrophysics The RAVE survey: the Galactic escape speed and the mass of the Milky Way T. Piffl1,2, C. Scannapieco1, J. Binney2, M. Steinmetz1, R.-D. Scholz1, M. E. K. Williams1,R.S.deJong1, G. Kordopatis3, G. Matijevicˇ4, O. Bienaymé5, J. Bland-Hawthorn6,C.Boeche7, K. Freeman8,B.Gibson9, G. Gilmore3,E.K.Grebel7,A.Helmi10, U. Munari11,J.F.Navarro12,Q.Parker13,14,15,W.A.Reid13,14, G. Seabroke16, F. Watson17,R.F.G.Wyse18, and T. Zwitter19,20 1 Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany e-mail: [email protected] 2 Rudolf Peierls Centre for Theoretical Physics, 1 Keble Road, Oxford OX1 3NP, UK 3 Institute for Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK 4 Dept. of Astronomy and Astrophysics, Villanova University, 800 E Lancaster Ave, Villanova, PA 19085, USA 5 Observatoire astronomique de Strasbourg, Université de Strasbourg, CNRS, UMR 7550, 11 rue de l’Université, 67000 Strasbourg, France 6 Sydney Institute for Astronomy, University of Sydney, School of Physics A28, NSW 2088, Australia 7 Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12–14, 69120 Heidelberg, Germany 8 Research School of Astronomy and Astrophysics, Australian National University, Cotter Rd., ACT 2611 Weston, Australia 9 Jeremiah Horrocks Institute, University of Central Lancashire, Preston, PR1 2HE, UK 10 Kapteyn Astronomical Institute, University of Groningen, PO
    [Show full text]