ESO 50Th Anniversary Gala Dinner
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ESO to Build World's Biggest Eye on the Sky 11 June 2012
ESO to build world's biggest eye on the sky 11 June 2012 36/) and Switzerland voted in favour of the start of the E-ELT programme. Four further countries voted in favour ad referendum: Belgium, Finland, Italy, and the United Kingdom. The remaining four Member States are actively working towards joining the programme in the near future. Following the resolution, spending on elements of the project other than the initial civil works will not commence until the contributions pledged by the Member States, as agreed in the funding principles Artist's impression of the European Extremely Large approved by Council in late 2011, exceed 90% of Telescope (E-ELT) in its enclosure on Cerro Armazones, the 1083 million euro cost-to-completion (at 2012 a 3060-metre mountaintop in Chile's Atacama Desert. The 39.3-meter E-ELT will be the largest optical/infrared prices). telescope in the world -- the world's biggest eye on the sky. Operations are planned to start early in the next On the current schedule the first large E-ELT decade, and the E-ELT will tackle some of the biggest industrial contracts would have to be approved and scientific challenges of our time. Credit: ESO/L. Calçada major funding committed within the next year. This is expected to provide sufficient time for the conditions to be satisfied: the confirmations of the votes from Belgium, Finland, Italy, and the United ESO's governing body, the Council, met today, at Kingdom; other Member States to join the project; the ESO Headquarters in Garching, Germany. -
Libro Resumen Sea2016v55 0.Pdf
2 ...................................................................................................................................... 4 .................................................................................................. 4 ........................................................................................................... 4 PATROCINADORES .................................................................................................................... 5 RESUMEN PROGRAMA GENERAL ............................................................................................ 7 PLANO BIZKAIA ARETOA .......................................................................................................... 8 .......................................................................................... 9 CONFERENCIAS PLENARIAS ................................................................................................... 14 ............................................................................................. 19 ................................................................................................ 21 ............... 23 CIENCIAS PLANETARIAS ......................................................................................................... 25 - tarde ....................................................................................................... 25 - ............................................................................................ 28 - tarde ................................................................................................ -
ASTRONET IR Final Word Doc for Printing with Logo
ASTRONET: Infrastructure Roadmap Update Ian Robson The ASTRONET Science Vision and Infrastructure Roadmap were published in 2007 and 2008 respectively and presented a strategic plan for the development of European Astronomy. A requirement was to have a light-touch update of these midway through the term. The Science Vision was updated in 2013 and the conclusions were fed into the Roadmap update. This was completed following the outcome of the ESA decisions on the latest missions. The community has been involved through a variety of processes and the final version of the update has been endorsed by the ASTRONET Executive. ASTRONET was created by a group of European funding agencies in order to establish a strategic planning mechanism for all of European astronomy . It covers the whole astronomical domain, from the Sun and Solar System to the limits of the observable Universe, and from radioastronomy to gamma-rays and particles, on the ground as well as in space; but also theory and computing, outreach, training and recruitment of the vital human resources. And, importantly, ASTRONET aims to engage all astronomical communities and relevant funding agencies on the new map of Europe. http://www.astronet-eu.org/ ASTRONET has been supported by the EC since 2005 as an ERA-NET . Despite the formidable challenges of establishing such a comprehensive plan, ASTRONET reached that goal with the publication of its Infrastructure Roadmap in November 2008. Building on this remarkable achievement, the present project will proceed to the implementation stage, a very significant new step towards the coordination and integration of European resources in the field. -
Recent Results from the SAURON Galaxy Survey Tim De Zeeuw
Recent Results from the SAURON Galaxy Survey Tim de Zeeuw European Southern Observatory Abstract Much world-wide effort is devoted to the study of the formation and evolution of galaxies, ranging from observations of the most distant objects in the early Universe to detailed analysis of the motions of individual stars in the Milky Way, combined with theoretical work and numerical simulations. Integral field spectroscopy makes it possible to measure the motions en physical properties of stellar populations in nearby galaxies, and to determine the properties of the supermassive black holes in their centres. A representative survey of nearby early-type galaxies and spiral bulges with SAURON, a panoramic integral-field spectrograph custom-built for the UK/NL/E 4.2m William Herschel Telescope on La Palma, reveals a fascinating diversity of properties. The stellar and gaseous kinematics and the line-strength distributions provide the intrinsic shape of the galaxies, their orbital structure, the mass-to-light ratio as a function of radius, the frequency and structure of kinematically decoupled cores, the masses of nuclear black holes, and the relation between orbital structure and the age and metallicity of the stellar populations. This 'fossil record' gives key insight into the galaxy formation process. The talk will summarize recent results of the SAURON survey, and briefly discuss the next steps. Resume Tim de Zeeuw received his PhD degree from Leiden University. He worked at the Institute for Advanced Study and Caltech before returning to Leiden as professor of astronomy. His research focuses on the formation, structure and dynamics of galaxies. He directed the Netherlands Research School for Astronomy and Leiden Observatory, and served on oversight committees for AURA, ESA, ESO and NASA. -
ESO@50 — the First 50 Years of ESO Held at ESO Headquarters, Garching, Germany, 3–7 September 2012
Astronomical News Report on the Workshop ESO@50 — The First 50 Years of ESO held at ESO Headquarters, Garching, Germany, 3–7 September 2012 Jeremy Walsh1 Young stars and planets Transients Eric Emsellem1 Michael West1 ESO’s next major milestone, the Atacama Steven Smartt (Belfast) summarised Large Millimeter/submillimeter Array detection and follow-up surveys for bright (ALMA) featured strongly in the first few transients which have recently begun at 1 ESO talks. Some of the first Cycle 0 results La Silla Observatory. The La Silla–QUEST in young stars and star-forming regions survey (see Baltay et al., p. 34) produces were presented by Leonardo Testi (ESO) transient alerts within days and these In recognition of the 50th anniversary where the high spatial resolution and sen- are followed up spectroscopically by the of the signing of the ESO Convention, a sitivity of ALMA will bring many ad vances. Public ESO Survey of Transient Objects special science workshop was held at The field of astrochemistry was covered (PESSTO) with EFOSC on the New Tech- ESO Headquarters in Garching to focus by Ewine van Dishoeck (Leiden), con- nology Telescope (NTT). on the main scientific topics where centrating on very high spectral resolution, ESO has made important contributions, including some ALMA spectra from pro- The Very Large Telescope (VLT) was very from Solar System astronomy to funda toplanetary discs, demonstrating the well timed for the beginning of the era mental physics, and to provide a per potential for finding new species (up to of observations of gamma-ray burst after- spective for future scientific challenges. -
Cosmic Vision: Space Science for Europe 2015-2025 Contents
COVER5 11/3/05 3:56 PM Page 1 BR-247 Cosmic Vision Space Science for Science Space 2015-2025 Europe Contact: ESA Publications Division c/o ESTEC, PO Box 299, 2200 AG Noordwijk, The Netherlands Tel. (31) 71 565 3400 - Fax (31) 71 565 5433 LAYOUT3 11/3/05 4:32 PM Page 1 BR-247 October 2005 Cosmic Vision Space Science for Europe 2015-2025 LAYOUT3 11/3/05 4:32 PM Page 2 Cover A fresco painted 1509-1511 by Raphael (1483-1520) in the Vatican (Stanza della Segnatura, Palazzi Pontifici) perhaps depicts the embodiment of Astronomy. (Copyright Photo SCALA, Florence) Replacing the original astronomical globe is Mars viewed by the High Resolution Stereo Camera (ESA/DLR/FU Berlin, G. Neukum) carried by the ESA Mars Express spacecraft, merging into an image (G. Hasinger, Astrophysikalisches Institute, Potsdam) of X-ray sources in the Lockman Hole made using the Newton X-ray Observatory spacecraft. Chapter divider Artist's impression of a quasar located in a primieval galaxy a few hundred million years after the Big Bang. (ESA/W. Freudling, ST-ECF/ESO) BR-247 ‘Cosmic Vision’ Prepared by: Giovanni Bignami, Peter Cargill, Bernard Schutz and Catherine Turon on behalf of the Science advisory structure of ESA, and by the Executive of the Science Directorate, supported by Nigel Calder Published by: ESA Publications Division, ESTEC, PO Box 299, 2200 AG Noordwijk,The Netherlands Editor/Design: Andrew Wilson Layout: Jules Perel Copyright: © 2005 European Space Agency ISSN: 0250-1589 ISBN: 92-9092-489-6 Price: EUR 10 Printed in The Netherlands LAYOUT3 11/3/05 4:32 PM Page 3 Cosmic Vision: Space Science for Europe 2015-2025 Contents Foreword 4 Executive Summary 6 Introduction:Why Space Science Needs Long-Term Planning 10 1. -
The Messenger
ESO 50th anniversary celebrations The Messenger Allocation of observing programmes La Silla–QUEST Survey b Pictoris and RS Puppis No. 150 – December 2012 – 150 No. ESO 50th Anniversary A Milestone for The Messenger in ESO’s 50th Anniversary Year Tim de Zeeuw1 nent launch of the construction of the trated book by Govert Schilling and Lars 39.3-metre diameter European Extremely Christensen (Europe to the Stars), many Large Telescope on Cerro Armazones additional images on the ESO website, 1 ESO with a projected start of operations in exhibitions and competitions, one of the about ten years’ time. Meanwhile, the latter with, as a prize, the opportunity number of Member States has increased to observe at Paranal, and a gala event In May 1974, Adriaan Blaauw launched to 14, with Brazil poised to join as the for representatives of the Member States The Messenger. He stated the goal first from outside Europe as soon as the and key contributors to ESO’s develop- explicitly: “To promote the participation Accession Agreement is ratified. ment, past and present (see the report of ESO staff in what goes on in the on p. 7, with copies of the speeches). In Organisation, especially at places of duty ESO’s mission is to design, construct and this special issue, four former Directors other than our own. Moreover, The operate powerful ground-based observ- General also contribute their reflections Messenger may serve to give the world ing facilities which enable astronomers on the significance of the 50th anniver- outside some impression of what hap to make important scientific discoveries sary: Lodewijk Woltjer (1975–1987), pens inside ESO.” Today The Messenger and to play a leading role in promoting Harry van der Laan (1988–1992), Riccardo is known the world over, and has reached and organising cooperation in astronomi- Giacconi (1993–1999) and Catherine a major milestone with the publication cal research. -
ESO and the International Year of Astronomy 2009 Opening Ceremony
Astronomical News that LPs make use of an expensive The workshop overall was very success- complement the current arsenal of pro- resource and that they have to provide ful and clarified the need for, and the gramme types undertaken with ESO additional benefits for the community. competitive edge of, Large Programmes facilities at the upper end. It is planned to This has led to the requirement that at ESO facilities. The increased demand monitor their success in another work- reduced data from LPs, once published, for the 3.6-metre telescope after the shop in a few years time. should be returned to the ESO Archive time limit for LPs was raised to four years so that they can be used by other astron- speaks for itself. There are some very omers, possibly for different purposes. substantial programmes in progress, References The large investment by the community which will keep this telescope busy for Wagner, S. & Leibundgut, B. 2004, The Messenger, into LPs should justify this modest return. years to come. 115, 41 There was a lively discussion on how this return should be achieved and Beyond the Large Programmes, the Pub- whether it would put astronomers using lic Surveys with VISTA and VST will Notes ESO facilities at a disadvantage com- start during this year and next year. These 1 http://www.eso.org/sci/meetings/LP2008/program. pared to users of private observatories. will be truly massive projects, which html ESO and the International Year of Astronomy 2009 Opening Ceremony Pedro Russo1 2 Figure 1. Catherine Cesarky, IAU President, Lars Lindberg Christensen1 addressing the audience during the IYA2009 Opening Ceremony Douglas Pierce-Price1 Yours to Discover”. -
ESO Annual Report 2018 Posals to ALMA Every Year
ESO European Organisation for Astronomical Research in the Southern Hemisphere Annual Report 2018 ESO European Organisation for Astronomical Research in the Southern Hemisphere Annual Report 2018 Presented to the Council by the Director General Xavier Barcons The European Southern Observatory ESO, the European Southern Observa tory, is the foremost intergovernmental astronomy organisation in Europe. It ESO/M. Claro has 16 Member States: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the Host State of Chile, and with Australia as a Strategic Partner. Several other countries have expressed an interest in membership. Created in 1962, ESO carries out an ambi tious programme focused on the design, construction and operation of powerful groundbased observing facilities, ena bling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three worldclass observ The VLT at the Paranal Observatory at sunset. this interferometric mode, the telescope’s ing sites in the Atacama Desert region vision is as sharp as that of a telescope of Chile: La Silla, Paranal and Chajnantor. The VLT is a unique facility and arguably as large as the separation between La Silla, located 2400 metres above sea the world’s most advanced optical instru the most distant mirrors. For the VLTI, level and 600 kilometres north of Santiago ment. It is not just one telescope but an this can be up to 200 metres. de Chile, was ESO’s first observatory. -
European Extremely Large Telescope Site Chosen 26 April 2010
European Extremely Large Telescope site chosen 26 April 2010 and may, eventually, revolutionise our perception of the Universe, much as Galileo's telescope did 400 years ago. The final go-ahead for construction is expected at the end of 2010, with the start of operations planned for 2018. The decision on the E-ELT site was taken by the ESO Council, which is the governing body of the This night-time panorama shows Cerro Armazones in Organisation composed of representatives of the Chilean desert, near ESO's Paranal Observatory, ESO's fourteen Member States, and is based on an site of the Very Large Telescope. Cerro Armazones was extensive comparative meteorological investigation, chosen as the site for the planned European Extremely which lasted several years. The majority of the data Large Telescope, which, with its 42-meter diameter collected during the site selection campaigns will be mirror, will be the world’s biggest eye on the sky. Credit: ESO/S. Brunier made public in the course of the year 2010. Various factors needed to be considered in the site selection process. Obviously the "astronomical On April 26, 2010, the ESO Council selected Cerro quality" of the atmosphere, for instance, the number Armazones as the baseline site for the planned of clear nights, the amount of water vapour, and the 42-meter European Extremely Large Telescope (E- "stability" of the atmosphere (also known as seeing) ELT). Cerro Armazones is a mountain at an played a crucial role. But other parameters had to altitude of 3060 meters in the central part of Chile's be taken into account as well, such as the costs of Atacama Desert, some 130 kilometers south of the construction and operations, and the operational town of Antofagasta and about 20 kilometers from and scientific synergy with other major facilities Cerro Paranal, home of ESO's Very Large (VLT/VLTI, VISTA, VST, ALMA and SKA etc). -
Science with the E-Elt in the Northern Hemisphere
SCIENCE WITH THE E-ELT IN THE NORTHERN HEMISPHERE Report on a workshop organised by the Red de Infraestructuras de Astronomía Madrid, April 16 th - 17 th 2009 June 2009 Foreword The workshop " Science with the E-ELT in the Northern Hemisphere ” was held on the premises of the CSIC headquarters in Madrid on the 16 th and 17 th of April 2009. This meeting, organized by the Spanish Astronomy Infrastructures Network (RIA) was attended by a very significant number of scientists from all of the Spanish astronomical research centres and university departments. This document summarizes the conclusions of that meeting. The main goals of the meeting were: • Motivate the Spanish scientific community to collaborate in the scientific definition of the E-ELT, in the light of the Design Reference Science Programme being assembled by the E-ELT Project Office at ESO. Promote the preparation of scientific cases that would need observations of Northern Hemisphere targets with the E-ELT. Analyze the sensitivity of the E-ELT proposed scientific cases to celestial Hemispheres. The meeting was very successful in fostering a very strong scientific interest from the whole of the Spanish astronomical community in the E-ELT as a key research infrastructure for the future. The 59 participants came from 18 Institutes and University Departments, mostly from Spain. It was especially pleasant to see the high attendance from young researchers, who will ultimately be leading the scientific exploitation of the E-ELT when it comes operation within a decade. Hemisphere issues came up as a secondary theme in the discussions. -
Annual Report 2011 Facts and Figures of 2011
Annual report 2011 Facts and figures of 2011 3 Awards or grants 112 refereed articles 157 employees 9 press releases Funding: € 30.446.230 Expenditure: € 30.482.073 Balance: € -35.843 Contents Director’s report 3 ASTRON in brief 5 Performance indicators 9 Astronomy Group 13 Radio Observatory 21 R&D Laboratory 27 Connected legal entities 33 NOVA Optical/ Infrared Instrumentation Group 35 JIVE 39 Outreach and Education 43 Appendix 1: Financial summary 53 Appendix 2: Personnel highlights 54 Appendix 3: Board, Committees and Staff 56 Appendix 4: Publications 58 Appendix 5: Earning capacity 76 Appendix 6: Abbreviations 78 Cover photo: impression of the dense aperture arrays for the Square Kilometre Array (SKA). Credits: Swinburne Astronomy Productions. 2 ASTRON Annual report 2011 Report 2011 was another great year for ASTRON. The highlight was undoubtedly the evaluation of the institute by a panel of international experts, chaired by Prof. Catherine Cesarsky. The panel judged ASTRON to be excellent in all possible categories - at the overall institute level and in each of our departments - Astronomy Group, Radio Observatory and Research &Development. Director’s In this year, the output in astronomy continued its enviable track-record in doubling research continued to grow - not only in the base budget received from NWO through terms of publications and impact, but also competitive grants and contracts - maintaining in connecting ASTRON to the outside world, this approach will be key to ASTRON’s future and in particular NOVA and the university success, especially in the coming years. Outwith groups in the Netherlands. LOFAR began ASTRON, the SKA project made progress with to produce its first scientific results and leaps and bounds.