'Dark energy survey des' diaporamas de présentation

Brenna Flaugher Fermilab

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The Lure of the Dark and Mysterious: Observational cosmology at UIUC

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Particle Astrophysics at Fermilab

Overview and Strategic Plan for the Fermilab Center for Particle Astrophysics. Particle Astrophysics at Fermilab. Craig Hogan, Director, FCPA Dan Bauer, Deputy Director, FCPA Presented to the FNAL PAC November, 2009. DOE/OHEP Mission.

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Observing Dark Energy

Observing Dark Energy. SDSS, DES, WFMOS teams. Understanding Dark Energy. We can make progress on questions: Is DE just a cosmological constant (w(z)=-1)? (Make better observations and push to higher z) Is DE a new form of matter (with negative effective pressure) or a breakdown of GR?

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The Dark Energy Survey (DES)

The Dark Energy Survey (DES). Sarah Bridle, UCL On behalf of the DES Collaboration. The Dark Energy Survey. Blanco 4-meter at CTIO. Study Dark Energy using 4 complementary techniques: I. Cluster Counts II. Weak Lensing III. Baryon Acoustic Oscillations

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Dark Energy and Dark Matter

Dark Energy and Dark Matter. Dark Energy is the dominant constituent of the Universe Dark Matter is next 95% of the Universe is in Dark Energy and Dark matter for which we have no understanding. 1998 and 2003 Science breakthroughs of the year. Probing Dark Energy.

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Fermilab Strategy

Fermilab Strategy. Pier Oddone P5 Meeting on Tevatron 2009 Running June 9, 2007. Programs. The Energy Frontier Tevatron, LHC ILC The neutrino frontier Minos, MiniBooNe, SciBooNe NOvA, Minerva Particle Astrophysics SDSS, Pierre Auger, CDMS II DES, CDMS-25kg, SNAP. P5 Recommendations.

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What is it? Large and deep imaging survey in Southern Hemisphere

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