'Wmap' presentation slideshows

Licia Verde

Licia Verde. University of Pennsylvania. www.physics.upenn.edu/~lverde. Connecting cosmology to fundamental physics. Dark matter (Spergel talk). Neutrinos (Spergel talk). Inflation. Dark energy. Testing fundamental physics by looking up at the sky is not new.

685 views • 59 slides

Cosmic Microwave Background

655 views • 52 slides

Gaussianity, Flatness, Tilt, Running, and Gravity Waves: WMAP and Some Future Prospects

Gaussianity, Flatness, Tilt, Running, and Gravity Waves: WMAP and Some Future Prospects. Eiichiro Komatsu University of Texas at Austin July 11, 2007. Cosmology and Strings: 6 Numbers. Successful early-universe models must produce: The universe that is nearly flat, | ? K |<O(0.02)

554 views • 46 slides

WMAP3 catalog sources Sergei Trushkin [ Bul.SAO, v.55, 90 (2003) + 2006/2007 ]

WMAP3 catalog sources Sergei Trushkin [ Bul.SAO, v.55, 90 (2003) + 2006/2007 ]. WMAP design. WMAP parameters. Radiometers. 1 day = 30% of sky, 6 month = total sky. ???? ?????????? ??? ???????? ?????. MW Synchrotron, f-f emission and dust. Sky at 61 GHz (Q-band) ?.

650 views • 38 slides

WMAP: Recent Results and Dark Energy

WMAP: Recent Results and Dark Energy. L. Page, STScI, May 2008. A 6 parameter model agrees with virtually all cosmological measurements regardless of redshift or method.

417 views • 34 slides

CMB Constraints on the Intracluster Medium

CMB Constraints on the Intracluster Medium. Niayesh Afshordi Institute for Theory and Computation Harvard College Observatory. My Collaborators. Yen-Ting Lin University of Illinois Urbana-Champaign Princeton Alastair Sanderson University of Illinois Urbana-Champaign

325 views • 25 slides

Searching for the Polarizing Influence of Inflation

Searching for the Polarizing Influence of Inflation. Or How I Learned to Stop Worrying and Love B-modes. Suzanne Staggs Princeton University. The Other CMB Power Spectra. The CMB must be polarized. (Martin Rees, 1968)

279 views • 19 slides

Modern cosmology 4: The cosmic microwave background

Modern cosmology 4: The cosmic microwave background. Expectations Experiments: from COBE to Planck COBE ground-based experiments WMAP Planck Analysis Results. Analysis of WMAP data: the power spectrum. Resolution and sky coverage

254 views • 14 slides

Chan-Gyung Park (KIAS)

Foreground Subtraction with an Internal Linear Combination Method: Application to the Wilkinson Microwave Anisotropy Probe Data. Chan-Gyung Park (KIAS). Internal Linear Combination Method.

180 views • 5 slides