Letizia Stanghellini NOAO 16 June 2008 – Science with Giant Telescopes

Slides:



Advertisements
Similar presentations
NSF Experience with Management of Research Infrastructure
Advertisements

1 AAO AusGO : 29 June 2009 Demystifying the Queue at Gemini Observatory AAO Epping - 29 June 2009 Henry Lee Gemini South, Chile.
Extremely Large Telescopes and Surveys Mark Dickinson, NOAO.
Sinai Observatory A Regional Center of Excellence The Sinai initiative group.
CNTAC SOCHIAS, Santiago 15 Enero 2009 CNTAC -- Background CNTAC=Chilean Telescope Allocation Committee Role: Administer 10% Chilean time on 20 telescopes.
GLAST LAT ProjectISOC CDR, 4 August 2004 Document: LAT-PR-04500Section 4.11 GLAST Large Area Telescope: Instrument Science Operations Center CDR Section.
Telescopes in the world Lison Malo Student CRAQ workshop.
Department of Physics and Astronomy Michigan State University.
Providing Access for US Astronomers to the Next Generation of Large Ground Based OIR Telescopes 1.Scientific Potential 2.Current Design Efforts 3.Complementarity.
Observational Astronomy. Astronomy Primary Goal: Understanding the nature of the universe and its constituents Means: Equipment building, research, teaching.
The KPNO 4m “Mayall” Telescope Arjun Dey (NOAO). National Optical Astronomy Observatory Mission: provide the best ground-based astronomical capabilities.
Keck Observatory and The System: Astro2010 Activities Mike Bolte, Shri Kulkarni, Taft Armandroff Keck Strategic Planning Discussions September 18, 2009.
Hands-on experience on medium-sized telescopes or: The need to train young researchers in observing techniques M. Dennefeld IAP-Paris and University Paris.
SSSC 02/18/2010 P. Marcum Science Utilization Policies SOFIA SCIENCE UTILIZATION POLICIES Pamela M. Marcum SOFIA Project Scientist SSSC Feb 19, 2010.
Users Committee Recommendations How did we do in 2005 ? NOAO Users Committee 5 October 2005.
Type and redshift distributions 65 candidates have been observed between June 2003 and May Redshift is measured by using emission and/or absorption.
Observing modes at the AT ATUC Presentations October 2000 Ray Norris CSIRO Australia Telescope National Facility.
Astronomy Networking Needs 5 December 2001 Jim Kennedy Gemini Observatory Important Contributions by Dick Crutcher, NCSA, UIUC Tom Troyland, UKY Arun Venkataraman,
TSIP (Telescope System Instrumentation Program) proposal February, 2005 Carnegie submission, on behalf of Magellan Consortium: “A Second, More Sensitive.
F. Genova, Berlin 7, Paris, 2 December 2009 The astronomical information network.
1 What we are: Two 8m telescopes, capable of forefront imaging and spectroscopy at optical and IR wavelengths. A young Observatory designed to enable and.
Cycle 1 Planning Process B-G Andersson (SOFIA Science Operations Manager) & Ravi Sankrit (User Support Scientist) SSSC, May 11, 2011 Mountain View.
Report from Subaru Advisory Committee The main issues of the current SAC: ・ Extensive (strategic) program of Subaru telescope ・ International collaborations.
Subaru Advisory Committee Report すばる小委員長 吉田道利 SAC Chair: Michitoshi Yoshida 2014/1/21Subaru UM
The Space Grant Internet Telescope Network: The Beginning Dr. Paul S. Hardersen Director, ND Space Grant Consortium National Space Grant Directors Meeting.
WFMOS Status Report Doug Simons Gemini Observatory January 2008.
John Peoples for the DES Collaboration BIRP Review August 12, 2004 Tucson1 DES Management  Survey Organization  Survey Deliverables  Proposed funding.
1 NOAO – National Optical Astronomy Observatory Overview for the AST Committee of Visitors February 2011 Jeff Pier, Program Officer.
“From the Ground Up: Balancing the NSF Astronomy Program” Senior Review Major Recommendations November 2006 Implications for GSMT.
Managing Under a Six-Nation Partnership Gemini Observatory soon to be Five.
© Crown copyright Met Office Space Weather Mr John Hirst, Permanent Representative of the UK to WMO 17 th May 2011.
American Geophysical Union December 6, 2005 Evolution of a Teacher Professional Development Program that Promotes Teacher and Student Research Evolution.
Australia’s Path to a Giant Telescope Matthew Colless MNRF Symposium 7 June 2003.
Obs. Planning Workshop 22 July 2011 NASA Herschel Science Center - page 1 PACS David R. Ardila NHSC-HSC liaison The OT2 Call.
What the Data Products Program Offers Users Todd Boroson Dick Shaw Presentation to NOAO Users Committee October 23, 2003.
May 17, 2004SSWG - PFIS Shared Risk1 PFIS Commissioning, Shared Risk, and Transition to Operations.
A105 Stars and Galaxies  News Quiz Today  1 st NovaSearch homework due Thursday  First Exam on Thursday, Sept. 28 Today’s APODAPOD.
ALTAIR: Access to Large Telescopes for Instruction and Research Chair: Larry Ramsey (14 members, 8.5L, 2S, 3.5U) Report: Submitted Mar 9, 2009
GSC Report Simon Morris (Durham University, GSC Chair)
College of Public Health and Human Sciences Communicating About Public Health Policy Presenter: Craig Mossbaek Date: August 22, 2013 Public Health Policy.
ALMA’s Roots in Three Scientific Visions Paul Vanden Bout NRAO The Dusty & Molecular Universe – Paris 28/10/04.
Telescope Access Metrics Presentation to Program Review Panel September 16, 2004.
Sino-French Workshop on the Dark Universe, Spectroscopy program of The SuperNovae Legacy Survey Filiol Mélanie 3rd year PhD Supervisors :
VISAS - ODG P74: a first view ESO Faculty meeting, 6 April 2004.
HSC Queue Mode Implementation Plan ~ Stage I, II, III ~ Tae-Soo Pyo Subaru Telescope /01/15.
Berlin Observatory Berlin, Germany. What is it? The Berlin Observatory is a series of observatories and related organizations in and around the city of.
Legacy Proposals for GLAST GI Program? (Aug. 04 AI # 11, Josh and Rita) The GI program for GLAST should allow for Legacy Projects defined as: very large.
Future Blanco Instrumentation and how to get it…
Telescope Access Metrics
Contract Formulation and Administration
JWST Science Policy & Science Parallels
An Overview of the Global Fund and its Architecture
Community Science Updates
Wide-Field Science Capabilities at the AAO
SOAR Observatory Strategic Planning Initial Concept Presentation
JCMT Observation Management Project
S4 will be a “big” Collaboration:
ESO Phase 1 & 2 Procedures Gaitee Hussain
Science Policies and Timeline
Observing with Modern Observatories
User instrument policy
IAWN Update.
The Vision The UK and partner countries, through the Newton Fund, will continue to build on existing science and innovation partnerships to promote the.
Science Operation Report FY2017
Observing with Modern Observatories (the data flow)
S3P Agri-Food Working Committee Meeting
Strategy
Scientific Potential Current Design Efforts Complementarity with JWST
How to get started & What you need to know
Enhancing WMO and CEOS COLLABORATION
Presentation transcript:

Letizia Stanghellini NOAO 16 June 2008 – Science with Giant Telescopes TAC issues Letizia Stanghellini NOAO 16 June 2008 – Science with Giant Telescopes

The NOAO TAC The NOAO TAC system deals with the community access to: The national observatories (KPNO, CTIO) Gemini (international partnership) Public and private partnership observatories NOAO + university partners (e.g., WIYN, SOAR) NOAO public time on Keck, Magellan, MMT, HET via TSIP NOAO TAC science-based; observers request selection of telescopes/instruments offered, based on their science needs TAC Members chosen from the community at large, based on scientific excellence

TAC models Single observatory International partners Multi-partners ESO (one OPC, national partners shares expected to be fulfilled- members selected from member counties) Gemini (national TACs, ITAC to oversee queue/shares/ToO ) Multi-partners Keck, Magellan, WIYN (member TACs, no super-TAC, no general ToO policy except for public access)

TAC models – ground based obs. Partner TACs plus observatory TAC (i.e., super-TAC) Oversight of science policies, control over science time especially ToO Lesser partners are disadvantaged (especially if queue modes are used, since availability of specific weather conditions is limited) Pre-determined shares and partner TACs Limited scientific oversight Partners more likely to get their fair share

Proposal pressure

Distribution of the size of scheduled programs Telescope aperture < 6m (KP, CT, WIYN, SOAR) Telescope aperture > 6m (GEM and TSIP) Note the evolution toward smaller programs

Scheduled programs by team size Over time, the number of large (>5 people) teams is almost invariant for proposals requesting small apertures, while it increases for those requesting large apertures

Joint NASA/NOAO programs