nsf program update
DESCRIPTION
NSF Program Update. Astronomy and Astrophysics Advisory Committee May 16, 2005. Status of Decadal Survey Recommendations. Small Initiatives: - PowerPoint PPT PresentationTRANSCRIPT
NSF Program Update
Astronomy and Astrophysics Astronomy and Astrophysics Advisory CommitteeAdvisory Committee
May 16, 2005May 16, 2005
Status of Decadal Survey Recommendations
Small Initiatives:–National Virtual Observatory (NVO) - Framework development funded; discussion with NASA planning long-term support through joint solicitation; Cyber funds in ’06 and beyond?
–Laboratory Astrophysics program - funded in grants program, strongly represented in FY2004 proposals and awards; substantial co-funding with chemistry and physics divisions
–Theory support – MPS Theory Workshop; science opportunities, modes of support, education and training issues - ~30% of grants are for theory, no need for separate theory program in AST
Status of Decadal Survey Recommendations
Small Initiatives:–National Virtual Observatory (NVO) - Framework development funded
–Laboratory Astrophysics program - funded in grants program, examined by AAAC
–Low Frequency Array (LOFAR) - D&D funded–Theory postdoc program - funded through AAPF program–SOLIS expansion
Status of Decadal Survey Recommendations
Moderate Initiatives:–Telescope System Instrument Program (TSIP) - funded–Advanced Technology Solar Telescope (ATST)*–Square Kilometer Array technology development (SKA)*
–Combined Array for Research in Mm-wave Astronomy (CARMA) - funded
–VERITAS - funded–Frequency Agile Solar Radio Telescope (FASR)–South Pole Sub-millimeter Telescope - funded in NSF/OPP
(* = Design/Development)
Status of Decadal Survey Recommendations
Major Initiatives:–Atacama Large Millimeter Array (ALMA) - funded
– Giant Segmented Mirror Telescope (GSMT) - technology development funded under Adaptive Optics Roadmap*
–Expanded Very Large Array (EVLA) - Phase I - funded
– Large Synoptic Survey Telescope (LSST) - development on detector arrays funded*
(* = Design/Development)
Status of Decadal Survey Recommendations
“US Ground-based O/IR facilities should be viewed … as a
single integrated system drawing on both federal and non-
federal funding sources”
- TSIP and Systems Workshops
- AURA/CELT partnership for GSMT
- LSST Corporation
Status of Quarks to Cosmos recommendations
– CMB Polarization measurement - CMB Research Task Force
– LSST - detector development funded
– Underground laboratory - NSF Physics phased approach
– Southern Auger array - funded
– Interagency initiative on Physics of the Universe
Physics of the Universe Interagency Plan
Highest priority, ready
– LSST
– S-Z effect - coordinated NSF/NASA effort - CMB Research Task
Force
– Dark Energy Task Force being formed under AAAC and HEPAP
– Underground facility
– Strengthen numerical relativity research - planned in Physics
– Upgrade of LIGO - approved by NSB for new start
GSMT Planning
National Optical Astronomy Observatory (NOAO) Science Working National Optical Astronomy Observatory (NOAO) Science Working Group has formulated a detailed science caseGroup has formulated a detailed science case. .
Consortium formed to undertake an extensive technology development Consortium formed to undertake an extensive technology development and site characterization effort. and site characterization effort.
Would result in a public-private partnership with private funds Would result in a public-private partnership with private funds supporting approximately 50% of the $70M estimated cost; proposal supporting approximately 50% of the $70M estimated cost; proposal to NSF for the remaining 50%. Public funds would support to NSF for the remaining 50%. Public funds would support community effort in several major groups.community effort in several major groups.
Current estimate is that this effort would take five to seven years.Current estimate is that this effort would take five to seven years. Proposal under review.Proposal under review.
NSF and consortium have met as a group and individually to discuss NSF and consortium have met as a group and individually to discuss timing and continue a constructive dialoguetiming and continue a constructive dialogue
Funds in FY2005 appropriation limited; similar for FY2006; Planned Funds in FY2005 appropriation limited; similar for FY2006; Planned growth awaits outcome of Senior Reviewgrowth awaits outcome of Senior Review
LSST Planning
National Optical Astronomy Observatory (NOAO) Science Working National Optical Astronomy Observatory (NOAO) Science Working Group formulated detailed science case.Group formulated detailed science case.
LSST Corporation established. LSST Corporation established. Pan-STARRS underway in Hawaii with DoD funding. No operations Pan-STARRS underway in Hawaii with DoD funding. No operations
money at all and insufficient resources for softwaremoney at all and insufficient resources for software NSF provided $1.3M in FY03 for detector development for LSST NSF provided $1.3M in FY03 for detector development for LSST
Camera; NOAO is funding telescope design at roughly $1.7M/year. Camera; NOAO is funding telescope design at roughly $1.7M/year. DOE labs have expressed strong interest in participating in the project DOE labs have expressed strong interest in participating in the project
through provision of the camera. DOE science budget a problem?through provision of the camera. DOE science budget a problem? Technology development program and possible architecture studies Technology development program and possible architecture studies
planned in FY2005, FY2006 (Physics of the Universe)planned in FY2005, FY2006 (Physics of the Universe)
The ATSTProject
The Advanced Technology Solar Telescope
Improvements over current state of the art:• Resolution – ~7X improvement• Light grasp – 10X improvement (solar physics is actually photon starved in some experiments)
Technical Specifications:• 4-m, off-axis Gregorian (all reflective), alt-az mount.• Integrated adaptive optics.• Hybrid enclosure with thermal control and dust mitigation.• Wavelength sensitivity from 0.3-28 microns (near-UV through thermal infrared).• Field of view: 3 arcminutes (5 arcminute goal).• Angular resolution < 0.03 arcsecond.• Polarization accuracy < 0.01%.
ATST will be the world’s flagship facility for ground-based solar physics observation and the first large US solar telescope constructed in the past 30 years.
The Telescope
Marching toward MREFC• ATST team had planned aggressively for an FY06 start of construction. This will not happen.
• Additional funding will be required to pay marching army and produce final design (note that current MREFC rules preclude funding design from MREFC). AST will fund through FY06 (FY07).
• The next steps:
ATST and AST craft development plan for FY05-6. Site selection complete – contract for environmental impact study Preliminary design reviews. Brought to MREFC panel in March 2005; awaiting action In-depth cost review endorsed costing models Attempt to address critical path items – early procurement of primary mirror. Let contracts for final design to design and engineering firms. Complete Project Execution Plan. Final design review in early 2006. Construction begins in fall of 2006/2007.
Planning(Activity Accelerating)
O/IR roadmap team convened by NOAO O/IR roadmap team convened by NOAO well underwaywell underway
Radio/mm/sub-mm convened by AUI Radio/mm/sub-mm convened by AUI underwayunderway
CMB Roadmap CMB Roadmap Dark Energy Task ForceDark Energy Task Force
Near Term Intermediate
Term
Horizon Facilities
Gemini
GSMT
EVLA I
VLA
GBT LOFAR
EVLA Phase II
LSST
SKA
OWL?
LOI?
CHARA
ALMA
CARMA
VLA
GBT LOFAR
LSST
GSMTNAIC
ATST
AST Budget FY2004 - $196.55M
Res & Inst. $71.8M
Facilities $124.75M
ALMA $50.7 M
Astronomy Division Budget - FY2004
Astronomy Division Budget - FY2004
Facilities - $124.75 M
National Optical Astronomy Observatory (NOAO)
National Solar Observatory (NSO)
Gemini Observatory
National Radio Astronomy Observatory (NRAO)
National Astronomy & Ionosphere Center (NAIC)
University Radio Observatories ===================================================================
Atacama Large Millimeter Array (ALMA)
$34.4 M(excludes $4M for TSIP
$3M for AODP)
$14.27 M
$54.98 M (directed)
$10.54 M
$10.56 M _______________
$50.7 M
Astronomy Division Budget - FY2004
Astronomy Research & Instrumentation - $71.8 M
Astronomy & Astrophysics Research Grants (AAG)Particle AstrophysicsEducation & Special Programs (ESP)
CAREER, REU, Postdoctoral fellowships
Advanced Technologies & Instrumentation (ATI)Electromagnetic Spectrum Management (ESM)Science & Technology Centers (STC)
Center for Adaptive Optics (CfAO)
NSF/MPS Priorities and programs e.g. ITR, Math Sciences, Biocomplexity in the Environment
• FY2005 AST request level - $204.35M (increase of 4% over FY2004)
• “Final” AST number $195.1M (< FY2004 - $196.6M)
• FY2006 Request $198.64M (FY2005 + 1.81%)
• Planning level budgets for next ? years
• Closer coupling between NSF and NASA budgets in difficult years?
• Changes in appropriations committee structure
FY2005 Budget and Outlook
AST Budget FY1992-2004
AST Budget FY1992-2004
$0
$50,000
$100,000
$150,000
$200,000
$250,000
1992 1993 1994 1995 1996 1997 1998 1999 2000 2001 2002 2003 2004
Fiscal Year
$ (
Th
ou
san
ds)
Total Facilities Res & Instr.
How can we afford it?
Proposals and studies Proposals and studies will sharpen costwill sharpen cost
Planning will provide Planning will provide phasing, decision phasing, decision points, down-selectspoints, down-selects
Overall plan must Overall plan must meet fiscal realitymeet fiscal reality
How?How?
NSF Budget Authority Projection
$4.40
$4.60
$4.80
$5.00
$5.20
$5.40
$5.60
$5.80
$6.00
2002 2003 2004 2005 2006 2007 2008 2009
Fiscal Year
Bil
lio
ns
of
Do
llar
s
“Senior Review”
Responds to:Responds to: Decade Survey recommendation re: facilitiesDecade Survey recommendation re: facilities Calls for examination of balance in AST Calls for examination of balance in AST
portfolio (Committee of Visitors, Feb)portfolio (Committee of Visitors, Feb) Made imperative by:Made imperative by:
Budget outlookBudget outlook Ambitions of the communityAmbitions of the community AST budget growthAST budget growth
“Senior Review” AST retreatAST retreat
Established understanding of need and goalsEstablished understanding of need and goals Self-examination of balanceSelf-examination of balance Identified issues that NSF and community must addressIdentified issues that NSF and community must address First time this has been undertaken by ASTFirst time this has been undertaken by AST
AST retreat “conclusions”AST retreat “conclusions” IF significant progress is to be made on development of major recommendations, ~~$30M of IF significant progress is to be made on development of major recommendations, ~~$30M of
free energy in AST budget must be identified.free energy in AST budget must be identified. Implications for program may be profound Implications for program may be profound Balance: grants program (AAG) must be held sacrosanctBalance: grants program (AAG) must be held sacrosanct Free energy will come from non-AAG portion of AST portfolioFree energy will come from non-AAG portion of AST portfolio
Next StepsNext Steps Letter sent to facilities – component costs and metrics due 7/31Letter sent to facilities – component costs and metrics due 7/31 AST exploring implications of all issues identifiedAST exploring implications of all issues identified Will frame options along with best understanding of consequences, positive and negativeWill frame options along with best understanding of consequences, positive and negative Will convene community representatives (Sept/October) to advise on best option(s) (or Will convene community representatives (Sept/October) to advise on best option(s) (or
identify others).identify others).
Senior Review Parameters
The primary goal of the review and the The primary goal of the review and the resultant adjustment of balance that will resultant adjustment of balance that will result is to enable progress on the result is to enable progress on the recommendations of the Decade Survey, recommendations of the Decade Survey, including such things as operations funds including such things as operations funds for ALMA, and other priorities. At the same for ALMA, and other priorities. At the same time we must preserve, indeed grow, a time we must preserve, indeed grow, a healthy core program of astronomical healthy core program of astronomical researchresearch
Boundary ConditionsThe assumption is that the AST budget will grow no faster than inflationary The assumption is that the AST budget will grow no faster than inflationary increases for the remainder of the decadeincreases for the remainder of the decade
In concert with the advice of every community advisory body that we have In concert with the advice of every community advisory body that we have asked (and in keeping with our own evaluation of balance and need), we will asked (and in keeping with our own evaluation of balance and need), we will not use resources from the unrestricted grants programs (AAG) to address the not use resources from the unrestricted grants programs (AAG) to address the challenges of facility operations or the design and development costs for new challenges of facility operations or the design and development costs for new facilities of the scale of LSST, GSMT, SKA, etc.facilities of the scale of LSST, GSMT, SKA, etc.
The process and the adjustments in balance that may result must be realistic and The process and the adjustments in balance that may result must be realistic and
realizablerealizable Recommendations should be based on well-understood criteriaRecommendations should be based on well-understood criteria
There should be ample opportunity for community input at all stages.There should be ample opportunity for community input at all stages.
Goal
The specific goal of the review is to examine the The specific goal of the review is to examine the impact and the gains we might experience by impact and the gains we might experience by redistributing $30M of annual spending from redistributing $30M of annual spending from Division funds. These funds would be obtained by Division funds. These funds would be obtained by selective reductions in the operations of existing selective reductions in the operations of existing facilities. The near-term needs for new investment facilities. The near-term needs for new investment have lead us to conclude that we must try to have lead us to conclude that we must try to generate the $30M in annual redistributed funding generate the $30M in annual redistributed funding by the end of FY2011. Even with this, there will be by the end of FY2011. Even with this, there will be challenges to be met to satisfy projected need in challenges to be met to satisfy projected need in FY2007-2008. FY2007-2008.
Zero-based Approach
In order to treat each of NRAO, NOAO, NSO, and Gemini on an In order to treat each of NRAO, NOAO, NSO, and Gemini on an equal footing and to obtain an in-depth understanding of the equal footing and to obtain an in-depth understanding of the contributions that each of our facilities makes, component by contributions that each of our facilities makes, component by component, we are adopting a “zero-base” approach. Under this component, we are adopting a “zero-base” approach. Under this approach, we ask that AUI consider and document:approach, we ask that AUI consider and document:
The case for, and priority of, each component of NRAO (VLA, The case for, and priority of, each component of NRAO (VLA, VLBA, GBT, ALMA operations, etc.), along with a defensible cost VLBA, GBT, ALMA operations, etc.), along with a defensible cost for each.for each.
In doing so, build the case for a forward-looking observatory In doing so, build the case for a forward-looking observatory operation, the highest priority components of which would exist in operation, the highest priority components of which would exist in 20112011
Provide as realistic an estimate as possible of the cost and timescale Provide as realistic an estimate as possible of the cost and timescale that would be associated with divestiture of each component that would be associated with divestiture of each component
ExpectationsWe expect that your deliberations will:We expect that your deliberations will: Be based on extensive consultation with your user communityBe based on extensive consultation with your user community Involve evaluation of component facilities and capabilities using well-defined and Involve evaluation of component facilities and capabilities using well-defined and
carefully documented metrics to define productivity, cost effectiveness, and future carefully documented metrics to define productivity, cost effectiveness, and future utility. We will work with all facilities managers to arrive at a common set of utility. We will work with all facilities managers to arrive at a common set of metrics so various components can be compared.metrics so various components can be compared.
Take into consideration systemic issues such as complementing observations at Take into consideration systemic issues such as complementing observations at
other wavelengths, filling critical niches in the overall U.S. system, role in training other wavelengths, filling critical niches in the overall U.S. system, role in training and technical innovation.and technical innovation.
Explore opportunities to deliver scientific knowledge at reduced cost or increased Explore opportunities to deliver scientific knowledge at reduced cost or increased
efficiency through new operating modesefficiency through new operating modes
AST Action
With this information in hand from all of the facilities With this information in hand from all of the facilities
that we support, and with our best understanding of the that we support, and with our best understanding of the needs for development and future programs, we will needs for development and future programs, we will then present a number of scenarios to the senior review then present a number of scenarios to the senior review committee for their comment and advice. These committee for their comment and advice. These scenarios will necessarily trade progress on the various scenarios will necessarily trade progress on the various recommendations before us against preservation of recommendations before us against preservation of existing capability. The challenge will be to strike an existing capability. The challenge will be to strike an acceptable balance.acceptable balance.
The Question
We recognize that this will be a difficult task and that We recognize that this will be a difficult task and that the end result may well be that some facilities are the end result may well be that some facilities are judged to be no longer viable under the circumstances. judged to be no longer viable under the circumstances. We also recognize that the landscape of U.S. We also recognize that the landscape of U.S. astronomy could almost certainly change dramatically astronomy could almost certainly change dramatically as a result of some these actions. The question for all as a result of some these actions. The question for all of us is to judge whether these changes are viable and of us is to judge whether these changes are viable and lead to a vital and sustainable future, or whether the lead to a vital and sustainable future, or whether the pace and scope of change necessary to realize the pace and scope of change necessary to realize the cumulative aspirations of the community under cumulative aspirations of the community under severely constrained budgets are too drasticseverely constrained budgets are too drastic