'Science goals' diaporamas de présentation

Task and Charge

Task and Charge. Negotiated by NRC with Agencies

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The Final (?) Frontier of Star and Planet Formation: Piled Deeper and Wider Michael R. Meyer

The Final (?) Frontier of Star and Planet Formation: Piled Deeper and Wider Michael R. Meyer Institute for Astronomy, ETH, Zurich, Switzerland 8 June 2011, Frontier Science Opportunities with the James Webb Space Telescope. Context for JWST in Kourou:. COROT/Kepler as well as

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THE NEED FOR A SQUARE KILOMETER ARRAY

THE NEED FOR A SQUARE KILOMETER ARRAY. What is the SKA? Why build the SKA? Science Goals & Payoffs Configurations, Modes and Sites Development Plan (International, US). For the US SKA Consortium Jim Cordes, Cornell University CfA talk, 3 April 2001. The SKA Concept.

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Science Goals and AO for the TMT

Science Goals and AO for the TMT. Jerry Nelson University of California at Santa Cruz Adaptive Optics for Extremely Large Telescopes Paris, 2009June23. Outline. Project Introduction Telescope overview Science-based metrics TMT key features Major science goals Science Instruments.

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test

test. Next Generation Sky Surveys:. Astronomical Opportunities. and Computational Challenges. Bob Mann Wide-Field Astronomy Unit School of Physics & Astronomy University of Edinburgh. Outline. Survey Astronomy 101 Next Generation Sky Surveys Astronomical Opportunities

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Decrypting the Universe with LOFAR

Decrypting the Universe with LOFAR. Philip Best Institute for Astronomy, Edinburgh. Overview. Introduction to LOFAR Instrument description & status European LOFAR LOFAR science Brief overview of the science case Epoch of Reionisation with LOFAR LOFAR extragalactic surveys

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Mission to Mars

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Technologies for Future Far-IR Telescopes and Interferometers

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STAR Experiment

STAR Experiment: Status & Future - Spin Structure of Proton - Properties of QCD Matter at Extreme Conditions - QCD Phase Structure Nu Xu Nuclear Science Division Lawrence Berkeley National Laboratory Berkeley, CA 94720, USA. STAR Experiment. STAR Experiment at RHIC

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Student Led Conferences March 2013

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DIXIE High School ROTC March 16, 2010 WATER ON THE MOON AT NASA Andy Christensen

DIXIE High School ROTC March 16, 2010 WATER ON THE MOON AT NASA Andy Christensen. What is NASA?. An agency of the US government Annual Budget ~ $18 B Name: National Aeronautics and Space Administration. NASA STRATEGIC GOALS 2006.

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The Analysis of Binary Inspiral Signals in LIGO Data

The Analysis of Binary Inspiral Signals in LIGO Data. Jun-Qi Guo Sept.25, 2007 Department of Physics and Astronomy The University of Mississippi LIGO Scientific Collaboration. Outline. Background of Compact Binary coalescence (CBC) work Matched filtering

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Philip Diamond Radio Net Coordinator University of Manchester Jodrell Bank Observatory, UK

Philip Diamond Radio Net Coordinator University of Manchester Jodrell Bank Observatory, UK. Leonid Gurvits Radio Net Project Scientist Joint Institute for VLBI in Europe Dwingeloo, The Netherlands. OPTICON FP7 Strategy meeting Edinburgh, 23 June 2006. FP6 Radio Net at a glance.

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Welcome to the 2003 PanAm PI Workshop

Welcome to the 2003 PanAm PI Workshop. David Gutzler US CLIVAR PanAm panel co-chair. special thanks to: our hosts at NCAR David Legler, US CLIVAR Office Jill Reisdorf, UCAR JOSS. Workshop goals. Bring extended PanAm research community together to exchange ideas and results

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Outline

Outline. Science goals, mission name (bonus for acronym and logo!!) Define telescope and instrument Choose orbit Calculate data volume, rate and downlink Calculate pointing requirements Select spacecraft bus Determine launch mass Select launch vehicle Describe major risks

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X-ray Solar Science For Solar-C Plan A

X-ray Solar Science For Solar-C Plan A. Kelly Korreck SAO kkorreck@cfa.harvard.edu. X-ray/EUV Science for Plan A. Taken from the presentation on Monday- Goals of Plan A “Understanding solar magnetic cycle” To look at the poles during a magnetic field reversal Solar wind at the poles

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DOE/NSF Review of DES

DOE/NSF Review of DES. 2 Science (SC1) Andy Albrecht (UC Davis) & Nicholas Suntzeff (Texas A&M) 2.2 Findings and Comments

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The FASR Reference Instrument

The FASR Reference Instrument Tim Bastian (tbastian@nrao.edu) 1 , Dale E. Gary(dgary@njit.edu) 2 , Steven M. Gross (smgross@umich.edu) 4 , Gordon J. Hurford(ghurford@ssl.berkeley.edu) 3 ,

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The ALMA Level One Science Goals

Al Wootten NRAO; ALMA/NA Project Scientist. A galaxy Spectral Energy Distribution similar to that of the Milky Way at a redshift of z=2 is shown. The 5 ? signal levels in a one hour integration are shown for various instruments.

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