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Robo-AO: Demo Period Nicholas Law
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The Demo Period 4 weeks on the Palomar 60” Q2 2011
Mission: do lots of great science
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What’s unique to Robo-AO?
Large surveys High efficiency Continual availability Great sky coverage Visible-light & high speed imaging
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Demo Period Goals Variety of science programs Extragalactic Transients
Stars Planets ... Cover all Robo-AO unique capabilities Large surveys High efficiency Visible-light AO High NIR Strehl Resulting in great science... and a large group of papers
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Survey Programs Binarity survey
all spectral types, companions down to brown dwarfs for most cover range of stellar parameter space with one instrument and one coherent survey
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Monitoring Trent Dupuy 2008, 2009
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High availability programs
New Old Subtraction The Palomar Transient Factory finds 1 transient candidate every ~10 minutes Many found near galactic nuclei - how do we separate them?
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High-speed, high-resolution imaging
5/17/2010 Astronomy Tea Talk 2
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How much time is one month?
Overheads 35-40 secs: telescope pointing & settling 20 secs: Centering on target & verification 10 secs: WFS calibration, wait for loop to close Assume: no science in first week 50% uptime 30% weather losses Conservatively ~60 hours, or 1800 targets at 2 mins per target However, we need about 5000 targets for contingency!
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Types of demo programs Large, 1000 targets
Need to be very exciting papers -- only 2-3 possible High-risk if incomplete Medium, targets 10+ projects Lower risk Others eg. transient followup (equiv. to 4m in sensitivity...)
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Demo period capabilities
General AO imaging NIR & Visible [specific NIR camera TBD] Dithering, standard observation sequences, etc. Visible-light high-speed imaging Efficiency will improve throughout run Likely semi-robotic system Probably manual target lists to start with Maybe some simple scheduling by end of demo
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Decision process Projects defined by September
Robo-AO team will collaborate, provide data, and support for data reduction, in exchange for paper authorship Mini-TAC process within Robo-AO team Current science team: C. Baranec, R. Dekany, J. Johnson, M. Kasliwal, M. van Kerkwijk, S. Kulkarni, N. Law, T. Morton, E. Ofek, A. Ramaprakash, R. Riddle, S. Tendulkar
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