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Astronomy & Astrophysics in Antarctic 2012 AAAC 11 May 2012 Scott Borg Division of Antarctic Sciences Office of Polar Programs National Science Foundation
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IceCube ANT and PHY partnership, with international partners Observatory Complete, M&O and Science are underway Detector functioning better than anticipated GRB's are not the neutrino engines of existing models Support thru FY14 - major review in a year South Pole Telescope Initial 5 year SZE survey completed - many discoveries CMB constraints on re-ionization Exciting discoveries of structure of the early Universe Support thru FY13 - proposal for new work expected BiCEP, BiCEP2 and SPUD Significant constraint on Inflation First meaningful constraint on inflationary gravitational wave background from B-mode polarization Current support thru FY13, renewal proposal in review
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HEAT at Ridge A TeraHertz, robotic telescope at the Dome A summit Site is 200-km south of Chinese station Kunlun Successful testing; now into THz winter observations US and Australia Support thru FY14 Antarctic Long Duration Ballooning NASA-NSF partnership since 1990; 47 flights Pioneering astrophysics and space physics payloads Agreement thru FY14 (2 more seasons) Anticipate continued interest from NASA
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NRC Review of the USAP OMB requested a high level review Plan developed and implemented by OSTP and NSF Part 1: NAS/NRC Review of Science Drivers. Report issued December 2011. Part 2: Blue Ribbon Panel examining infrastructure: Is USAP structured appropriately to address the science drivers anticipated in the NRC report. Report anticipated July 2012. Includes consideration of international and interagency partnerships.
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Challenges Many opportunities - too many? Stagnant budgets and increasing costs. Better integration/partnerships and priority setting with other national investments in astronomy? SPT after current project - what next? - Transition to multi-user telescope? IceCube M&O recompetition in FY15 – what next?
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Questions? Aurora behind the 10m South Pole Telescope Photo Credit: Dana Hrubes, SP Station Science Leader, 2010
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Questions?
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