The AAO: 2005-2015 Matthew Colless 17 December 2004.

Slides:



Advertisements
Similar presentations
The Australian Virtual Observatory (a.k.a. eAstronomy Australia) Ray Norris CSIRO ATNF.
Advertisements

TheEuropean Extremely Large Telescope. The E-ELT 40-m class telescope: largest optical- infrared telescope in the world. Segmented primary mirror. Active.
Extremely Large Telescopes and Surveys Mark Dickinson, NOAO.
RAVE status report Matthias Steinmetz (AIP) June RAVE collaboration meeting - Padova Data collection  325k spectra for 280k stars (Jan.
ESRC Key Priorities & Future Strategy Adrian Alsop 2 nd Feb 2011.
The Search for New “r-process-Enhanced” Metal-Poor Stars Timothy C. Beers Michigan State University.
Planning for the Virtual Observatory Tara Murphy … with input from other Aus-VO members …
1 SONG Exoplanet Searches in the Context of Next Generation Exoplanet Surveys Joe Carson College of Charleston September 17, 2011.
Facilities & Infrastructure Working Groups Meeting UNSW, 17 December 2004 Gemini Warrick Couch, UNSW.
An Echidna-style positioner for DESpec Will Saunders 8 March 2011.
Spectroscopy Techniques and Projects at 1.2-m UK Schmidt Telescope
Providing Access for US Astronomers to the Next Generation of Large Ground Based OIR Telescopes 1.Scientific Potential 2.Current Design Efforts 3.Complementarity.
Wide-Field Science Capabilities at the AAO Stuart Ryder Australian Gemini Office Australian Astronomical Observatory.
Research Impact 19 November 2012 Dr Fiona Cameron Executive Director Australian Research Council.
THE CAASTRO TEAM IS PURSUING THREE INTERLINKED SCIENCE PROGRAMS: THE EVOLVING UNIVERSE When did the first galaxies form, and how have they then evolved?
Keck Observatory and The System: Astro2010 Activities Mike Bolte, Shri Kulkarni, Taft Armandroff Keck Strategic Planning Discussions September 18, 2009.
Enabling a GSMT for the US Community: AURA’s Proposal to the NSF Stephen E. Strom 04 June, 2004 Tucson, AZ National Optical Astronomy Observatory Tucson.
A. McGrath *a,A. Moore b ( a Anglo-Australian Observatory, b Osservatorio Astrofisico di Arcetri) Starbug – enabling the smart focal plane TECHNICAL CHALLENGES.
Comprehend the Historical Benefits of Exploration Comprehend the US Strategic Plan to Explore Space Comprehend the Current Costs of Exploring Space Comprehend.
This page is intentionally blank. A new view of the Universe VIII Fred Watson (and the RAVErs) April 2005 A new view of the Universe VIII Fred Watson.
14-16 January, 2009Subaru User’s Meeting (NAOJ) Possible Collaboration between Seoul National University and Subaru Myungshin Im (CEOU/Astronomy Seoul.
Scottish Universities Physics Alliance SUPA Astronomy & Space Physics Graham Woan University of Glasgow.
AAAC Meeting February, New GSMT Role NSF has asked that AURA/NOAO act as NSF’s "Program Manager" for the GSMT Technology development effort at a.
Observing modes at the AT ATUC Presentations October 2000 Ray Norris CSIRO Australia Telescope National Facility.
Advancing GSMT SWG Recommendations: AURA’s Proposal to the NSF Stephen E. Strom AURA New Initiatives Office Presented to the GSMT SWG 12 February, 2004.
U.S. Department of Energy Office of Science Advanced Scientific Computing Research Program NERSC Users Group Meeting Department of Energy Update September.
European Extremely Large Telescope - Status April ESO.
The SOC Pilot and the ATOA Jessica Chapman CASS Observatory Operations Research Program Leader 28 June 2011.
European small and medium sized telescopes Paul Murdin Particle Physics & Astronomy Research Council.
Multi-slit spectroscopy In sky-noise dominated conditions (most interesting!) the use of slits is essential: eg: Faint object, extra-galactic, surveys:
Exo-Planet Task Force (ExoPTF) Jonathan Lunine (LPL) Stephen Ridgway (NASA)
Report from Subaru Advisory Committee The main issues of the current SAC: ・ Extensive (strategic) program of Subaru telescope ・ International collaborations.
Gemini and the MNRF: An Update Gary Da Costa Chair, Australian Gemini Steering Committee.
WFMOS Status Report Doug Simons Gemini Observatory January 2008.
6dFGS Workshop, Epping 11 July 2003 Fred Watson (and the RAVErs) 6dFGS Workshop, Epping 11 July 2003 Fred Watson (and the RAVErs)
John Peoples for the DES Collaboration BIRP Review August 12, 2004 Tucson1 DES Management  Survey Organization  Survey Deliverables  Proposed funding.
Suggested Subaru-NAOJ/Princeton Consortium: Overview Michael Strauss, Ed Turner, Jim Gunn January 25, 2007.
WFMOS KAOS concept identified via the Gemini Aspen Process and completed a Feasibility Study (Barden et al.) Proposed MOS on Subaru via an international.
MNRF Management and milestone achievements Chris Evans AAO.
The Discovery Channel Telescope: An Investment in Astronomical Science at Boston University.
Australia’s Path to a Giant Telescope Matthew Colless MNRF Symposium 7 June 2003.
The FMOS Facility for the SUBARU telescope Gavin Dalton Oxford/RAL.
A global approach to ELT instrument developments J.-G. Cuby for the French ELT WG.
CELT Science Case. CELT Science Justification Process Put together a Science Working Group –Bolte, Chuck Steidel, Andrea Ghez, Mike Brown, Judy Cohen,
Selected Preliminary Results of the WIYN Survey Survey designed based on UW-Madison strategic planning. Adjusted for WIYN by Eileen Friel (Indiana) Analysis:
The Future of the Hubble Space Telescope Steven Beckwith April 25, 2005 Space Telescope Science Institute.
FELT 1 Study of the capability and configuration of a fixed mirror Extremely Large Telescope (FELT) Low cost path to large telescope Primary concern is.
The ARC — overview and opportunities (Japan) 19 October 2015 Presented by Mr Justin Withers Director, Policy and Integrity The Australian Research Council.
The ARC — overview and opportunities (China) 16 November 2015 Presented by Mr Justin Withers Director, Policy and Integrity The Australian Research Council.
Telescope Access Metrics Presentation to Program Review Panel September 16, 2004.
1 LSST Town Hall 227 th meeting of the AAS 1/7/2016 Pat Eliason, LSSTC Executive Office Pat Osmer, LSSTC Senior Advisor.
Senior Review of NSF Facilities NOAO Users Committee October 4, 2005.
Theme 2 AO for Extremely Large Telescopes Center for Adaptive Optics.
Faculty meeting - 13 Dec 2006 The Hubble Legacy Archive Harald Kuntschner & ST-ECF staff 13 December 2006.
GSMT SWG Meeting November, New GSMT Role NSF has asked that AURA/NOAO act as NSF’s "Program Manager" for the GSMT Technology development effort.
Independent Living Innovation Platform 04/03/15 Hazel Harper ILIP Programme Manager Innovate UK.
The Australian Astronomy MNRF Ray Norris June 2004.
LSST CORPORATION Patricia Eliason LSSTC Executive Officer Belgrade, Serbia 2016.
The Science Case Hubble Space Telescope CELT+AO HDF.
Community Science Updates
Wide-Field Science Capabilities at the AAO
SOAR Observatory Strategic Planning Initial Concept Presentation
EIROforum is a partnership between eight of Europe’s largest intergovernmental scientific organisations Previously.
For more information, visit
Theme 2 AO for Extremely Large Telescopes
For more information, visit
A 10-m Diameter Submillimeter-wave Telescope for the South Pole
Theme 2 AO for Extremely Large Telescopes
Theme 2 AO for Extremely Large Telescopes
Presentation transcript:

The AAO: Matthew Colless 17 December 2004

AAO’s Mission The mission of the Anglo-Australian Observatory (AAO) is to provide world-class optical and infrared observing facilities that enable Australian and British astronomers to carry out excellent science. The AAO is a world leader in astronomical research and in the development of innovative telescope instrumentation. It also takes a leading role in the formulation of long- term plans for astronomy in Australia.

AAO Usage + Users AAO telescopes do observing programs involving astronomers (AU+AAO~40%, UK~40%, other~20%) Time on the AAT is over-subscribed by factor of Of 318 astronomers and students currently at Australian institutions (an over-estimate?), 114 (36%) used the AAO’s telescopes in the past 5 years. AAT over-subscription factors

Publications + Citations About 140 papers/yr from AAO telescopes (most productive in 4m-class according to ESO study in 2000). Of the 300 most-cited papers produced by the international community in the last 3 years (the top 0.5%), 17 (i.e. 6%) used AAO telescopes. Publications from AAT + UKST data and by AAO staff. Publications from AAT data by location of first author.

Science Impact Recent high-impact projects using AAO telescopes include: –The 2dF Galaxy/QSO Redshift Surveys + follow-up 2SLAQ survey –The RAVE Project: stellar velocities over 5 years on UKST –Anglo-Australian Planet Search: 20 exoplanets and counting Other high-impact research from the past few years that used the AAO telescopes includes: –Discovery of ultra-compact dwarfs, first new galaxy type in 70 years –The use of stellar seismology to probe the interiors of stars –The discovery of some of the most distant objects in the universe. –The identification of gamma-ray bursts with exploding stars –Discovery of a satellite galaxy being torn apart by the Milky Way

Innovative Technology The AAO has excelled in astronomical instrumentation. On the AAT and UKST… –AAO pioneered robotic optic-fibre spectrographs and is world leader –2dF and 6dF have proved world-beating instruments - AAOmega will ditto –IRIS2 was winner Australian Engineering Excellence 2002 On other telescopes… –OzPoz for ESO’s VLT (produced 15 VLT nights and 6dF) –FMOS for Subaru (Japanese collaborations, WFMOS-on-Subaru) –WFMOS (major new instrument for Gemini/Subaru, unique 8m capability for outstanding science and value even in ELT era) New technology in the pipeline… –Starbugs - micro-robotics for smart focal planes in very large telescopes –Sky-suppression fibres - a revolution in ground-based near-infrared observations will follow from near-perfect suppression of OH sky lines

New AAT Agreement Key features of the new Agreement are : –UK funding halves in FY , again in FY UK contribution then steady at ~$1M/yr until –Relative AU:UK funding  relative fractions AAT time –While agreement open beyond 2010, expect UK will withdraw all funding from mid-2010 –Once UK withdraws, the AU government assumes full ownership of the AAO.

The Need for the AAT For next ~5 years Australia O/IR astronomers will have access to: –6.2% of Gemini (36nt/yr plus short-term extra 8m nights via MNRF) –50% of AAT now, rising to 80% from mid-2007 (165nt/yr  265nt/yr) –100% of a range of smaller telescopes (2.3-metre, Skymapper, etc.) Supposing very optimistic scenario, in 5 years’ time might have… –10% of Gemini, or equivalent 8m access (~60nt/yr) –100% of PILOT (~2-metre in Antarctica) –share in ELT program (provides no nights in coming decade!) …can Australia do without the AAT in the coming decade? Australia needs the AAT as… –A workhorse O/IR telescope for research by Australian astronomers –An on-shore, classical-observing-mode facility for training students –A test-bed for prototyping and exploiting innovative instrumentation

Can the AAT compete? Is the AAT a worthwhile facility in the 8-metre era? (Note that the ELT era begins in the decade after next!) It has competed successfully for last 5 years in the 8m era! Keys to success were innovative instrumentation and bulk access to observing time… –AAOmega will be the world’s most powerful instrument for survey spectroscopy in 2006 and for several years thereafter –Modest upgrades to IRIS2 (e.g. starbug IFUs) and UCLES (e.g. multi-fibre feed) would make those instruments highly competitive for a range of interesting applications –Bulk access to AAT time makes possible ambitious observing programs impossible on 8m telescopes (given limited access)

Need for instrument program The AAO’s instrumentation program is valuable because… –It provides innovative instrumentation for the AAT, keeping it ahead of the technology cycle & doing high-impact research –It provides Australia with leverage in determining the science agenda on Gemini (e.g. success of the WFMOS concept) –It connects to observatories around the world, providing access to powerful facilities (e.g. OzPoz on VLT, FMOS on Subaru) –It earns external income that allows the AAO to undertake new instruments with direct benefits for Australian astronomers (e.g. 6dF was the OzPoz prototype, WFMOS benefits from FMOS) –It is a highly-rated research program in its own right, with a long history (and bright future) of seminal contributions to astronomical technology and instrumentation

Need for AAO as institution The AAO is valuable to Australian astronomers as an institution, since… –It provides independent services and facilities for all Australian astronomers; independent in that it is not a university and so is not competing with universities in any way (esp. for ARC funding). –It is focussed on delivering facilities for O/IR astronomy, a field in which Australia is historically strong, which involves a large fraction of the research community, and which has a very exciting future. –The AAO has a separate funding stream through DEST that is independent of the universities, of the ARC, and of CSIRO. Diversity of funding sources provides robustness to astronomy. –The AAO can provide a natural home for all O/IR national facilities. At present this means just the AAT and UKST, but in future it might include the Gemini National Project Office and the national support facilities for Australian access to an ELT or an Antarctic telescope.

Recommendations? Based on the above arguments, the Decadal Plan might include recommendations as follows… 1.The AAO should be the national organization that supports all of Australia’s major optical/infrared astronomy facilities. 2.The AAT is required as a major facility for Australian astronomers throughout the decade A major new optical/infrared facility is required by about The AAO could wind down AAT operations and transfer effort to supporting operation of the new facility. 4.The AAO instrumentation program is a world leader and benefits Australian astronomers. It should continue to be supported at least at its current level.

The National Observatory The AAO should be the organization supporting all of Australia’s national optical/infrared astronomy facilities. The AAO (as the Anglo-Australian Observatory up to 2010, and perhaps as the “Australian Astronomical Observatory” thereafter) should not only operate the AAT and UKST, but also be the support organization for Gemini and other major new optical/infrared facilities in which Australia gains a share (e.g. an ELT or an Antarctic telescope).

AAT needed The AAT is required as a major observational facility for Australian astronomers throughout the decade This means Australia needs not only to maintain the new Agreement for the first five years ( ), but also be ready and able to take sole responsibility for running the telescope after the end of the Agreement.

A Graceful Transition A major new optical/infrared facility is required by about The AAO would wind down AAT operations in order to support this new facility. Australia should be aiming to obtain access to an operating ELT, Antarctic 8m, or other equivalent major new optical/infrared facility by around The AAO could re-direct the operations cost of the AAT to operating/supporting this new facility. This may mean operating the AAT in full-cost-recovery mode, converting it to other purposes, or closing it down. A plan for a graceful transition is required.

Instrument Program The AAO instrumentation program is a world leader and benefits Australian astronomers. It should continue to be supported at least at its current level. Australian O/IR astronomy benefits from the AAO’s instrumentation program and should be prepared to invest in it. The AAO can then remain a source of innovative technology that gives Australian astronomers access to the best instruments on the best telescopes. There may be opportunities for partnerships with RSAA, ATNF, CIP, etc.