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Results from Three-Year WMAP Observations PowerPoint PPT Presentation

Results from Three-Year WMAP Observations - Title: Three-Year WMAP Observations: Polarization Analysis Author: Eiichiro Komatsu Last modified by: Eiichiro Komatsu Created Date: 3/30/2006 12:10:25 AM

Title: Three-Year WMAP Observations: Polarization Analysis Author: Eiichiro Komatsu Last modified by: Eiichiro Komatsu Created Date: 3/30/2006 12:10:25 AM

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2. Cosmologia Despues de WMAP PowerPoint PPT Presentation

2. Cosmologia Despues de WMAP - ... is ionized, baryons and photons are coupled via. Thomson scattering: we refer to a 'photon-baryon fluid' ... Increasing the baryon density increases the density ...

... is ionized, baryons and photons are coupled via. Thomson scattering: we refer to a 'photon-baryon fluid' ... Increasing the baryon density increases the density ...

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Three-Year WMAP Observations: Polarization Analysis PowerPoint PPT Presentation

Three-Year WMAP Observations: Polarization Analysis - Three-Year WMAP Observations: Polarization Analysis Eiichiro Komatsu The University of Texas at Austin Irvine, March 23, 2006 Summary of Improvements in the ...

Three-Year WMAP Observations: Polarization Analysis Eiichiro Komatsu The University of Texas at Austin Irvine, March 23, 2006 Summary of Improvements in the ...

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FIRST RESULTS FROM THE WMAP MISSION - FIRST RESULTS FROM THE WMAP MISSION

FIRST RESULTS FROM THE WMAP MISSION

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WMAP CMB Conclusions PowerPoint PPT Presentation

WMAP CMB Conclusions - ... P(k) because of the (assumed) isotropy of the distribution (i.e. scales matter ... By isotropy, only separation r matters, and not the vector r. ...

... P(k) because of the (assumed) isotropy of the distribution (i.e. scales matter ... By isotropy, only separation r matters, and not the vector r. ...

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The Cosmic Microwave Background and the WMAP satellite results PowerPoint PPT Presentation

The Cosmic Microwave Background and the WMAP satellite results - Properties: frequency spectrum, temperature, (an)isotropy ... Properties: isotropy and anisotropies. The CMB radiation is isotropic ...

Properties: frequency spectrum, temperature, (an)isotropy ... Properties: isotropy and anisotropies. The CMB radiation is isotropic ...

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Non-Gaussianity at low and high multipoles from WMAP data PowerPoint PPT Presentation

Non-Gaussianity at low and high multipoles from WMAP data - Non-Gaussianity at low and high multipoles from WMAP data ... Spanish (Vielva, Martinez-Gonzales et al., 2003) wavelet analysis ...

Non-Gaussianity at low and high multipoles from WMAP data ... Spanish (Vielva, Martinez-Gonzales et al., 2003) wavelet analysis ...

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Third Year WMAP Results PowerPoint PPT Presentation

Third Year WMAP Results - Olivier Dore. Mike Nolta. Penn. Licia Verde. UT Austin. Eiichiro Komatsu ... Three times as much data, sqrt(3) smaller errors in maps: more than 50x ...

Olivier Dore. Mike Nolta. Penn. Licia Verde. UT Austin. Eiichiro Komatsu ... Three times as much data, sqrt(3) smaller errors in maps: more than 50x ...

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The WMAP normalization of inflationary cosmologies PowerPoint PPT Presentation

The WMAP normalization of inflationary cosmologies - ... White (1995) used 4-year COBE TT data to create fitting formula for n (tilt) and ... We use 3 year WMAP TT, TE and EE data to do the same thing ...

... White (1995) used 4-year COBE TT data to create fitting formula for n (tilt) and ... We use 3 year WMAP TT, TE and EE data to do the same thing ...

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Wilkinson Microwave Anisotropy Probe WMAP Timeline PowerPoint PPT Presentation

Wilkinson Microwave Anisotropy Probe WMAP Timeline - April 2003: third full sky scan due to be completed ... Radiometer: Differential pseudo-correlation with polarization. Optics: Dual Gregorian, ...

April 2003: third full sky scan due to be completed ... Radiometer: Differential pseudo-correlation with polarization. Optics: Dual Gregorian, ...

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Impressions of the WMAP Results PowerPoint PPT Presentation

Impressions of the WMAP Results - Vibrating String: Characteristic frequencies because ends are tied down ... Isotropic radiation field produces no polarization after Compton scattering ...

Vibrating String: Characteristic frequencies because ends are tied down ... Isotropic radiation field produces no polarization after Compton scattering ...

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ThreeYear WMAP Observations PowerPoint PPT Presentation

ThreeYear WMAP Observations - One can decompose it into a divergence-like 'E-mode' and a vorticity-like 'B-mode' ... We can also see that noise is larger on the ecliptic plane. W Band (94 GHz) ...

One can decompose it into a divergence-like 'E-mode' and a vorticity-like 'B-mode' ... We can also see that noise is larger on the ecliptic plane. W Band (94 GHz) ...

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WMAP 3year constraints on the inflationary expansion PowerPoint PPT Presentation

WMAP 3year constraints on the inflationary expansion - Galileo Galilei Institute for Theoretical Physics, Oct. 16, 2006 ... Galileo Galilei Institute for Theoretical Physics, Oct. 16, 2006. The zoo plot in ( 2, 1) plane ...

Galileo Galilei Institute for Theoretical Physics, Oct. 16, 2006 ... Galileo Galilei Institute for Theoretical Physics, Oct. 16, 2006. The zoo plot in ( 2, 1) plane ...

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Natural Inflation after WMAP PowerPoint PPT Presentation

Natural Inflation after WMAP - Emily Dickinson, 1860. Spectrum of Perturbations. Total number of inflation e-foldings Ntot 60 ... TO DO: perturbations (with S. Watson) Rolling Models: ...

Emily Dickinson, 1860. Spectrum of Perturbations. Total number of inflation e-foldings Ntot 60 ... TO DO: perturbations (with S. Watson) Rolling Models: ...

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Limits on nonGaussianities from WMAP data PowerPoint PPT Presentation

Limits on nonGaussianities from WMAP data - Ghost Condensation (N. Arkani-Hamed, H.C. Cheng, M.A.Luty,S. Mukohyama) ... Ghost condensate with. In the past the Cosmology is: Need to ensure stability in the past: ...

Ghost Condensation (N. Arkani-Hamed, H.C. Cheng, M.A.Luty,S. Mukohyama) ... Ghost condensate with. In the past the Cosmology is: Need to ensure stability in the past: ...

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The giant arc statistic in the threeyear WMAP cosmological model PowerPoint PPT Presentation

The giant arc statistic in the threeyear WMAP cosmological model - Giant arcs are background galaxies distorted into long arcs by foreground ... also sensitive to the cosmogony, particularly the power-spectrum normalisation s8 ...

Giant arcs are background galaxies distorted into long arcs by foreground ... also sensitive to the cosmogony, particularly the power-spectrum normalisation s8 ...

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First Year Wilkinson Microwave Anisotropy Probe WMAP Results PowerPoint PPT Presentation

First Year Wilkinson Microwave Anisotropy Probe WMAP Results - Dipole: the motion of the solar system relative to CMB ... fluctuations and thus falsify different theories and set constraints on theories ...

Dipole: the motion of the solar system relative to CMB ... fluctuations and thus falsify different theories and set constraints on theories ...

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The Universe according to WMAP III PowerPoint PPT Presentation

The Universe according to WMAP III - Quadrupole anisotropy : E-mode. Cross-correlated spectrum TE ... Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam ...

Quadrupole anisotropy : E-mode. Cross-correlated spectrum TE ... Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam ...

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Discrepancy between average WMAP observed and ROSAT predicted SunyaevZel'dovich Effect profiles of 3 PowerPoint PPT Presentation

Discrepancy between average WMAP observed and ROSAT predicted SunyaevZel'dovich Effect profiles of 3 - Discrepancy between average WMAP observed and ROSAT predicted Sunyaev-Zel'dovich ... The S-Z effect may be probe of cluster non-thermal processes, not cosmology. ...

Discrepancy between average WMAP observed and ROSAT predicted Sunyaev-Zel'dovich ... The S-Z effect may be probe of cluster non-thermal processes, not cosmology. ...

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Joint analysis of Archeops and WMAP observations of the CMB PowerPoint PPT Presentation

Joint analysis of Archeops and WMAP observations of the CMB - ai,ps(Krj) = (ni/n0)-2. 3 astrophysical components: CMB, thermal SZ, unresolved point sources ... ai,sz(n) is perfectly known. Results: CMB and SZ power ...

ai,ps(Krj) = (ni/n0)-2. 3 astrophysical components: CMB, thermal SZ, unresolved point sources ... ai,sz(n) is perfectly known. Results: CMB and SZ power ...

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Cosmological Parameters from WMAP and SDSS PowerPoint PPT Presentation

Cosmological Parameters from WMAP and SDSS - and then something happened and our universe was 'born' ... Enrico Fermi, Course CXXXII, Varenna, 1995, available from http://www.hep.upenn. ...

and then something happened and our universe was 'born' ... Enrico Fermi, Course CXXXII, Varenna, 1995, available from http://www.hep.upenn. ...

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Finding Extragalactic Point Sources in WMAP Temperature Maps: A CMBindependent Technique PowerPoint PPT Presentation

Finding Extragalactic Point Sources in WMAP Temperature Maps: A CMBindependent Technique - ... and 9.3% of the WMAP three-year cataloged sources are 5 detections at V and W band respectively. ... 291 WMAP cataloged point sources, 75 newly detected sources ...

... and 9.3% of the WMAP three-year cataloged sources are 5 detections at V and W band respectively. ... 291 WMAP cataloged point sources, 75 newly detected sources ...

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GEM Project CrossCorrelations of WMAP5 PowerPoint PPT Presentation

GEM Project CrossCorrelations of WMAP5 - ... similar to above, but uses auto and cross-correlations to use ... sync,dust,ff = syncrotron, dust, and free-free template maps, Vary a/b as above...

... similar to above, but uses auto and cross-correlations to use ... sync,dust,ff = syncrotron, dust, and free-free template maps, Vary a/b as above...

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Constraining hybrid inflation models with WMAP threeyear results PowerPoint PPT Presentation

Constraining hybrid inflation models with WMAP threeyear results - The original hybrid inflation model naturally predicts ns 1 in the false ... In the inverted hybrid model there is no problem obtaining small values for aa. ...

The original hybrid inflation model naturally predicts ns 1 in the false ... In the inverted hybrid model there is no problem obtaining small values for aa. ...

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1Wilkinson Anisotropy Microwave Probe WMAP PowerPoint PPT Presentation

1Wilkinson Anisotropy Microwave Probe WMAP - Wilkinson Anisotropy Microwave Probe (WMAP) is one of the most impressive probes ... The WMAP experiment is based on a satellite which has now spent about 2 years in ...

Wilkinson Anisotropy Microwave Probe (WMAP) is one of the most impressive probes ... The WMAP experiment is based on a satellite which has now spent about 2 years in ...

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WMAP et la mesure des anisotropies du rayonnement de fond cosmologique PowerPoint PPT Presentation

WMAP et la mesure des anisotropies du rayonnement de fond cosmologique - Pr dit par George Gamow en 1948 et par Ralph Alpher et Robert Herman en 1950 ... 419 W; 3.1 m2 GaAs/Ge array, 22.5 off full Sun. 23 A-hr NiH battery; ...

Pr dit par George Gamow en 1948 et par Ralph Alpher et Robert Herman en 1950 ... 419 W; 3.1 m2 GaAs/Ge array, 22.5 off full Sun. 23 A-hr NiH battery; ...

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IIT Kanpur IUCAA PowerPoint PPT Presentation

IIT Kanpur IUCAA - ... universe can be deconvolved from the measured CMB anisotropy spectrum ... WMAP CMB anisotropy map. WMAP Angular power spectrum. Fig: NASA/WMAP science team ...

... universe can be deconvolved from the measured CMB anisotropy spectrum ... WMAP CMB anisotropy map. WMAP Angular power spectrum. Fig: NASA/WMAP science team ...

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MAPping the Universe PowerPoint PPT Presentation

MAPping the Universe - MAPping the Universe Introduction: the birth of a new cosmology The cosmic microwave background Measuring the CMB Results from WMAP The future of cosmology

MAPping the Universe Introduction: the birth of a new cosmology The cosmic microwave background Measuring the CMB Results from WMAP The future of cosmology

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DEK - ( M : reduced Planck-mass , H : Hubble parameter ) Ob=?b/?c. fraction in baryons ... picture of the big bang. Otot=1. WMAP 2006. Polarization. Dark Energy. Om ...

( M : reduced Planck-mass , H : Hubble parameter ) Ob=?b/?c. fraction in baryons ... picture of the big bang. Otot=1. WMAP 2006. Polarization. Dark Energy. Om ...

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Wavelets, ridgelets, curvelets on the sphere PowerPoint PPT Presentation

Wavelets, ridgelets, curvelets on the sphere - ... Earth's surface with POLDER. http://polder.cnes.fr. Introduction - Motivations ... imaging the Earth's surface with POLDER - mapping CMB fluctuations with WMAP ...

... Earth's surface with POLDER. http://polder.cnes.fr. Introduction - Motivations ... imaging the Earth's surface with POLDER - mapping CMB fluctuations with WMAP ...

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$The Universe: a sphere, a donut, or a fractal? PowerPoint PPT Presentation$

The Universe: a sphere, a donut, or a fractal? - Stephen Hawking A photographic image of quantum fluctuations blown up to the size of the universe WMAP and spectrum of the cosmic microwave background anisotropy ...

Stephen Hawking A photographic image of quantum fluctuations blown up to the size of the universe WMAP and spectrum of the cosmic microwave background anisotropy ...

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Diapositiva 1 PowerPoint PPT Presentation

Diapositiva 1 - Antena de ondas de radio Segundo sat lite (WMAP) ...

Antena de ondas de radio Segundo sat lite (WMAP) ...

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Inquiring minds want to know ... PowerPoint PPT Presentation

Inquiring minds want to know ... - Fermi National Accelerator Laboratory (near Chicago) CDF. Minos ... WMap data on the temperature fluctuations in the CMB. why structure matters ...

Fermi National Accelerator Laboratory (near Chicago) CDF. Minos ... WMap data on the temperature fluctuations in the CMB. why structure matters ...

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Predictions of the MSO10SM : PowerPoint PPT Presentation

Predictions of the MSO10SM : - Dark Matter & WMAP. Bs - m m- Light Higgs mass - mh. Upper bound on mA ... 6. Direct dark matter detection. by next generation exp'ts. 7. Indirect detection ...

Dark Matter & WMAP. Bs - m m- Light Higgs mass - mh. Upper bound on mA ... 6. Direct dark matter detection. by next generation exp'ts. 7. Indirect detection ...

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Olbers paradox PowerPoint PPT Presentation

Olbers paradox - ... through space causes this dipole (anisotropy with 2 well-defined/opposite points) ... NASA's Wilkinson Microwave Anisotropy Probe (WMAP) ...

... through space causes this dipole (anisotropy with 2 well-defined/opposite points) ... NASA's Wilkinson Microwave Anisotropy Probe (WMAP) ...

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Is there a preferred direction in the Universe PowerPoint PPT Presentation

Is there a preferred direction in the Universe - The Virgo cluster sits at the center of this disc like structure ... Hence WMAP data suggests the existence of a preferred direction (pointing towards Virgo) ...

The Virgo cluster sits at the center of this disc like structure ... Hence WMAP data suggests the existence of a preferred direction (pointing towards Virgo) ...

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Observational constraints and cosmological parameters PowerPoint PPT Presentation

Observational constraints and cosmological parameters - ns 1 (2 sigma) CMB Degeneracies. TT. All. Main WMAP3 parameter results rely on polarization ... ns 1 at 2 sigma. LUQAS. Conclusions ...

ns 1 (2 sigma) CMB Degeneracies. TT. All. Main WMAP3 parameter results rely on polarization ... ns 1 at 2 sigma. LUQAS. Conclusions ...

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In The Beginning PowerPoint PPT Presentation

In The Beginning - anisotropy of CMB: 1 part in 100,000. Temperature Maps. Cosmic Temp Curve. perfect blackbody fit ... WMAP (Wilkinson Microwave Anisotropy Probe) Goals launched 2001 ...

anisotropy of CMB: 1 part in 100,000. Temperature Maps. Cosmic Temp Curve. perfect blackbody fit ... WMAP (Wilkinson Microwave Anisotropy Probe) Goals launched 2001 ...

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Ollongren 1962 PowerPoint PPT Presentation

Ollongren 1962 - Ollongren (1962) 'Quite unexpectedly, all these orbits behaved as if they had ... SOHO. WMAP. Planck. JWST. Trojan asteroids. a(Jupiter)=5.2 AU ...

Ollongren (1962) 'Quite unexpectedly, all these orbits behaved as if they had ... SOHO. WMAP. Planck. JWST. Trojan asteroids. a(Jupiter)=5.2 AU ...

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Lensing of the CMB PowerPoint PPT Presentation

Lensing of the CMB - Temperature anisotropy data: WMAP 3-year smaller scales. BOOMERANG. Hinshaw et al ... source of confusion for anisotropy lensing signal ...

Temperature anisotropy data: WMAP 3-year smaller scales. BOOMERANG. Hinshaw et al ... source of confusion for anisotropy lensing signal ...

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A COSMIC JOURNEY WITH BIKASH SINHA PowerPoint PPT Presentation

A COSMIC JOURNEY WITH BIKASH SINHA - (Wilkinson Microwave Anisotropy Probe) First Year WMAP Observations. Universe is 13.7 billion years old ... 1. Shibaji Banerjee (St. Xaviers College, Kolkata) ...

(Wilkinson Microwave Anisotropy Probe) First Year WMAP Observations. Universe is 13.7 billion years old ... 1. Shibaji Banerjee (St. Xaviers College, Kolkata) ...

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Cosmological implications of the first year PowerPoint PPT Presentation

Cosmological implications of the first year - Cosmological implications of the first year. WILKINSON MICROWAVE ... (Most of) WMAP Science Team, August 2002. Launched from cape Canaveral on June 30 2001 ...

Cosmological implications of the first year. WILKINSON MICROWAVE ... (Most of) WMAP Science Team, August 2002. Launched from cape Canaveral on June 30 2001 ...

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www.dark-cosmology.dk/~pela PowerPoint PPT Presentation

www.dark-cosmology.dk/~pela - ... (2004) Probing the Epoch of Reionization * Probing the Epoch of Reionization WMAP: zre = 11.0 1.4 Thomson scattering optical depth: ...

... (2004) Probing the Epoch of Reionization * Probing the Epoch of Reionization WMAP: zre = 11.0 1.4 Thomson scattering optical depth: ...

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Lecture 3 - Formation of Galaxies PowerPoint PPT Presentation

Lecture 3 - Formation of Galaxies - The Hydra cluster. CMB from WMAP ~10-5. Lecture 3 - Formation of Galaxies. What processes lead from the tiny fluctuations which we see on the surface of ...

The Hydra cluster. CMB from WMAP ~10-5. Lecture 3 - Formation of Galaxies. What processes lead from the tiny fluctuations which we see on the surface of ...

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A Linear Perturbation Theory of Inhomogeneous Reionization PowerPoint PPT Presentation

A Linear Perturbation Theory of Inhomogeneous Reionization - A Linear Perturbation Theory of Inhomogeneous Reionization. Jun Zhang (UC Berkeley) ... High redshift quasar spectra. Credit: WMAP team & SDSS team. Introduction ...

A Linear Perturbation Theory of Inhomogeneous Reionization. Jun Zhang (UC Berkeley) ... High redshift quasar spectra. Credit: WMAP team & SDSS team. Introduction ...

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Michele Liguori PowerPoint PPT Presentation

Michele Liguori - Predictions for the detectability of a NG signal in the CMB with WMAP and Planck ... 3. Convolve with the radiation transfer functions ...

Predictions for the detectability of a NG signal in the CMB with WMAP and Planck ... 3. Convolve with the radiation transfer functions ...

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cosmology pioneer: David Wilkinson PowerPoint PPT Presentation

cosmology pioneer: David Wilkinson - The Bell Labs horn antenna. All-sky map of the CMBR. The spectrum of the Cosmic Microwave ... All-sky map of the CMBR. A detailed all-sky map of the CMBR (WMAP 2003) ...

The Bell Labs horn antenna. All-sky map of the CMBR. The spectrum of the Cosmic Microwave ... All-sky map of the CMBR. A detailed all-sky map of the CMBR (WMAP 2003) ...

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Axion and axino contribution to dark matter PowerPoint PPT Presentation

Axion and axino contribution to dark matter - It is accepted now that dark matter is observed(SN1,WMAP). There are several particle physics ... compared to X-ray images(red) Gravitational lensing ...

It is accepted now that dark matter is observed(SN1,WMAP). There are several particle physics ... compared to X-ray images(red) Gravitational lensing ...

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The CMB TE Cross Correlation and Primordial Gravitational Waves PowerPoint PPT Presentation

The CMB TE Cross Correlation and Primordial Gravitational Waves - Polnarev, Miller, Keating 'The CMB TE Cross Correlation and PGWs I: ... 3% of sky, ~1 degree beam FWHM. r=0.3. WMAP Errors. Taken from published WMAP data. r=0.3 ...

Polnarev, Miller, Keating 'The CMB TE Cross Correlation and PGWs I: ... 3% of sky, ~1 degree beam FWHM. r=0.3. WMAP Errors. Taken from published WMAP data. r=0.3 ...

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Dust and Gravitational Waves PowerPoint PPT Presentation

Dust and Gravitational Waves - Amplitude gotten from comparison of FDS Dust in Bicep region and WMAP region ... Dust physics: interesting in its own right and useful to inform BICEP II. ...

Amplitude gotten from comparison of FDS Dust in Bicep region and WMAP region ... Dust physics: interesting in its own right and useful to inform BICEP II. ...

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The universe: dark matter and dark energy PowerPoint PPT Presentation

The universe: dark matter and dark energy - Results from spacecraft WMAP, released on ... will we confirm its existence in a laboratory? ... is the ultimate Copernican viewpoint; not only are ...

Results from spacecraft WMAP, released on ... will we confirm its existence in a laboratory? ... is the ultimate Copernican viewpoint; not only are ...

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A MultiMission Model for Spacecraft Flight Software Sustaining Engineering PowerPoint PPT Presentation

A MultiMission Model for Spacecraft Flight Software Sustaining Engineering - At least two engineers in the group are able to maintain the FSW for each mission ... Wilkinson Microwave Anisotropy Probe (WMAP) Sustaining Engineering History. ...

At least two engineers in the group are able to maintain the FSW for each mission ... Wilkinson Microwave Anisotropy Probe (WMAP) Sustaining Engineering History. ...

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Microwaves - Each one shares tips with neighboring cavities. Oscillate alternately. Cycle: ... The new WMAP observations favor specific inflation scenarios over other long ...

Each one shares tips with neighboring cavities. Oscillate alternately. Cycle: ... The new WMAP observations favor specific inflation scenarios over other long ...

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What do we know about Dark Matter and Dark Energy PowerPoint PPT Presentation

What do we know about Dark Matter and Dark Energy - Maybe pigeons? Proposed error: pigeon crap in antenna. Real reason: a signal from the Big Bang ... Pigeon trap. Horn antenna. Latest Results: WMAP (Wilkinson ...

Maybe pigeons? Proposed error: pigeon crap in antenna. Real reason: a signal from the Big Bang ... Pigeon trap. Horn antenna. Latest Results: WMAP (Wilkinson ...

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Introduction to variable selection I PowerPoint PPT Presentation

Introduction to variable selection I - To predict the output of a test point x, the average of fw(x) over the posterior ... wMAP is the vector of parameters called the Maximum a Posteriori (MAP), i.e. 19 ...

To predict the output of a test point x, the average of fw(x) over the posterior ... wMAP is the vector of parameters called the Maximum a Posteriori (MAP), i.e. 19 ...

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Observation Constraints of the End of Reionization PowerPoint PPT Presentation

Observation Constraints of the End of Reionization - Gemini Keck. From Avi Loeb. reionization. Two Key Constraints: WMAP 3-yr: zreion=10 /-3 ... 0.6 (2-sigma) by fitting both DLA and IGM profiles. Damping wing? ...

Gemini Keck. From Avi Loeb. reionization. Two Key Constraints: WMAP 3-yr: zreion=10 /-3 ... 0.6 (2-sigma) by fitting both DLA and IGM profiles. Damping wing? ...

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Wmap PowerPoint PPT Presentations