2dfgrs PowerPoint PPT Presentations

All Time
Show:
Recommended
Sort by:
The Galaxy Power Spectrum: 2dFGRS-SDSS Tension PowerPoint PPT Presentation
The Galaxy Power Spectrum: 2dFGRS-SDSS Tension - Shaun Cole. ICC, University of Durham. Main Contributors: ... Completeness and magnitude limit masks from Cole et al 2005 using methods of Norberg et al 2002 ...
Shaun Cole. ICC, University of Durham. Main Contributors: ... Completeness and magnitude limit masks from Cole et al 2005 using methods of Norberg et al 2002 ...
| PowerPoint PPT presentation | free to download
Local LSS after 2dFGRS PowerPoint PPT Presentation
Local LSS after 2dFGRS - Halo mass-to-light ratios. Group luminosity ... The halo model ... Halo M/L to local group level measure efficiency peak ...
Halo mass-to-light ratios. Group luminosity ... The halo model ... Halo M/L to local group level measure efficiency peak ...
| PowerPoint PPT presentation | free to view
Radio sources in the 2dF Galaxy Redshift Survey (2dFGRS) PowerPoint PPT Presentation
Radio sources in the 2dF Galaxy Redshift Survey (2dFGRS) - Title: SUMSS Author: Elaine Sadler Last modified by: astrop10 Created Date: 11/17/1999 10:06:56 AM Document presentation format: Overhead Other titles
Title: SUMSS Author: Elaine Sadler Last modified by: astrop10 Created Date: 11/17/1999 10:06:56 AM Document presentation format: Overhead Other titles
| PowerPoint PPT presentation | free to download
Hierarchical Galaxy Clustering in the 2dFGRS PowerPoint PPT Presentation
Hierarchical Galaxy Clustering in the 2dFGRS - Hierarchical Galaxy Clustering in the 2dFGRS. Peder Norberg (ETHZ) in ... statistical homogeneity and isotropy of the cosmic density field: not true on ...
Hierarchical Galaxy Clustering in the 2dFGRS. Peder Norberg (ETHZ) in ... statistical homogeneity and isotropy of the cosmic density field: not true on ...
| PowerPoint PPT presentation | free to view
Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models PowerPoint PPT Presentation
Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models - The disruption of satellite galaxies that already lost their dark matter halos ... cross-matched galaxies from the 2dFGRS with published clusters catalogues (Abell, ...
The disruption of satellite galaxies that already lost their dark matter halos ... cross-matched galaxies from the 2dFGRS with published clusters catalogues (Abell, ...
| PowerPoint PPT presentation | free to download
Redshift Surveys: New Challenges PowerPoint PPT Presentation
Redshift Surveys: New Challenges - Limits on Neutrino masses. Bimodality in the 2dFGRS. Colour (B-R) Peacock 2003. Blue ... Weighing Neutrinos with 2dFGRS. Free streaming effect: Wn/Wm 0.13 ...
Limits on Neutrino masses. Bimodality in the 2dFGRS. Colour (B-R) Peacock 2003. Blue ... Weighing Neutrinos with 2dFGRS. Free streaming effect: Wn/Wm 0.13 ...
| PowerPoint PPT presentation | free to view
The Galaxy Luminosity Function PowerPoint PPT Presentation
The Galaxy Luminosity Function - 2dFGRS, SDSS, ESP, (APM, SSRS2, LCRS, UKST, NOG, CS) ... Hubble Space Telescope WFPC2 Observations. Abell 0868 (A morphological dissection) ...
2dFGRS, SDSS, ESP, (APM, SSRS2, LCRS, UKST, NOG, CS) ... Hubble Space Telescope WFPC2 Observations. Abell 0868 (A morphological dissection) ...
| PowerPoint PPT presentation | free to view
Wiener Reconstruction of the Galaxy Redshift Surveys PowerPoint PPT Presentation
Wiener Reconstruction of the Galaxy Redshift Surveys - Wiener Reconstruction of the Galaxy Redshift Surveys. Pirin ... Density Field of 2dFGRS in Declination Strips ... (For details see Zaroubi et al 1995, ...
Wiener Reconstruction of the Galaxy Redshift Surveys. Pirin ... Density Field of 2dFGRS in Declination Strips ... (For details see Zaroubi et al 1995, ...
| PowerPoint PPT presentation | free to view
Diapositiva 1 PowerPoint PPT Presentation
Diapositiva 1 - cosmology (WMAP 2dFGRS ...) mS = 3mn 0.7 eV (model dependent...) present knowledge ... disfavoured by cosmology. Dm 2atm 0. Dm 2atm 0. next generation bb-0n exp ...
cosmology (WMAP 2dFGRS ...) mS = 3mn 0.7 eV (model dependent...) present knowledge ... disfavoured by cosmology. Dm 2atm 0. Dm 2atm 0. next generation bb-0n exp ...
| PowerPoint PPT presentation | free to view
NG2dF A Next Generation 2degree Field Instrument for the AAT. PowerPoint PPT Presentation
NG2dF A Next Generation 2degree Field Instrument for the AAT. - ... multiplex gain of an order of magnitude over the current 2dF instrument plus ... These are 2.5 magnitudes fainter than the current 2dFGRS limit and they would be ...
... multiplex gain of an order of magnitude over the current 2dF instrument plus ... These are 2.5 magnitudes fainter than the current 2dFGRS limit and they would be ...
| PowerPoint PPT presentation | free to view
Massive Neutrinos and Cosmology PowerPoint PPT Presentation
Massive Neutrinos and Cosmology - n-2004, Paris Massive Neutrinos and Cosmology * Brief history of Hot Dark Matter * Limits on the total Neutrino mass from redshift surveys: Mn
n-2004, Paris Massive Neutrinos and Cosmology * Brief history of Hot Dark Matter * Limits on the total Neutrino mass from redshift surveys: Mn
| PowerPoint PPT presentation | free to download
Short Description of PowerPoint PPT Presentation
Short Description of - pay VERY MUCH attention to time stamps. -)I sometimes gave quality flags to data (bad from logs) not used ... Now: new background subtraction method. Problems ...
pay VERY MUCH attention to time stamps. -)I sometimes gave quality flags to data (bad from logs) not used ... Now: new background subtraction method. Problems ...
| PowerPoint PPT presentation | free to download
Radio galaxies: timescales and triggers Elaine Sadler, University of Sydney PowerPoint PPT Presentation
Radio galaxies: timescales and triggers Elaine Sadler, University of Sydney - Title: SUMSS Author: Elaine Sadler Last modified by: Elaine Sadler Created Date: 11/17/1999 10:06:56 AM Document presentation format: Overhead Other titles
Title: SUMSS Author: Elaine Sadler Last modified by: Elaine Sadler Created Date: 11/17/1999 10:06:56 AM Document presentation format: Overhead Other titles
| PowerPoint PPT presentation | free to download
Cosmic Structures: Challenges for Astro-Statistics PowerPoint PPT Presentation
Cosmic Structures: Challenges for Astro-Statistics - Title: The 2dF Galaxy Redshift Survey Author: Ofer Lahav Last modified by: Ofer Created Date: 4/8/2002 11:55:24 AM Document presentation format: On-screen Show
Title: The 2dF Galaxy Redshift Survey Author: Ofer Lahav Last modified by: Ofer Created Date: 4/8/2002 11:55:24 AM Document presentation format: On-screen Show
| PowerPoint PPT presentation | free to view
Galaxy formation PowerPoint PPT Presentation
Galaxy formation - Distortion due to non-linear evolution, peculiar velocities and galaxy bias ... P(k) / Pref(Wbaryon=0) Also detected in SDSS LRG sample (Eisenstein etal 05) ...
Distortion due to non-linear evolution, peculiar velocities and galaxy bias ... P(k) / Pref(Wbaryon=0) Also detected in SDSS LRG sample (Eisenstein etal 05) ...
| PowerPoint PPT presentation | free to download
Surveys with OmegaCAM / VST KIDS Koen Kuijken, Leiden PowerPoint PPT Presentation
Surveys with OmegaCAM / VST KIDS Koen Kuijken, Leiden - w' (wiggles) Use scale of power spectrum wiggles as standard candle ... The challenges II. Lensing measurements with shapelets ...
w' (wiggles) Use scale of power spectrum wiggles as standard candle ... The challenges II. Lensing measurements with shapelets ...
| PowerPoint PPT presentation | free to download
Interpreting Large Scale Structure PowerPoint PPT Presentation
Interpreting Large Scale Structure - Model scale-dependent bias as b(k)=(1 Qk2)(1 Ak)-1 ... 1-halo term: galaxy pairs in the same halo. 2-halo term: galaxy pairs in separate halos ...
Model scale-dependent bias as b(k)=(1 Qk2)(1 Ak)-1 ... 1-halo term: galaxy pairs in the same halo. 2-halo term: galaxy pairs in separate halos ...
| PowerPoint PPT presentation | free to download
How to kill a galaxy (A review of galaxy properties as a function of environment) PowerPoint PPT Presentation
How to kill a galaxy (A review of galaxy properties as a function of environment) - Mark I and II imaging of Virgo galaxies. 18 nearby clusters: Solanes et al. 2001 ... this with large fraction of Virgo spirals with unusual Ha distributions? ...
Mark I and II imaging of Virgo galaxies. 18 nearby clusters: Solanes et al. 2001 ... this with large fraction of Virgo spirals with unusual Ha distributions? ...
| PowerPoint PPT presentation | free to view
The Void Probability function and related statistics PowerPoint PPT Presentation
The Void Probability function and related statistics - Count probability PN(V): probability of finding N galaxies in a randomly chosen ... Skewness and kurtosis (2D) for the Deeprange and SDSS. From Szapudi et al. 2002 ...
Count probability PN(V): probability of finding N galaxies in a randomly chosen ... Skewness and kurtosis (2D) for the Deeprange and SDSS. From Szapudi et al. 2002 ...
| PowerPoint PPT presentation | free to download
Testing CPT with CMB PowerPoint PPT Presentation
Testing CPT with CMB - Interacting dark energy induces cosmological CPT violation, ... CPT is conserved The rolling of dark energy scalar field breaks Lorentz covariance It provides a ...
Interacting dark energy induces cosmological CPT violation, ... CPT is conserved The rolling of dark energy scalar field breaks Lorentz covariance It provides a ...
| PowerPoint PPT presentation | free to download
Large Scale Structure in 2MRS PowerPoint PPT Presentation
Large Scale Structure in 2MRS - Large Scale Structure in 2MRS
Large Scale Structure in 2MRS
| PowerPoint PPT presentation | free to view
Probing Dark Energy with Cosmological Observations PowerPoint PPT Presentation
Probing Dark Energy with Cosmological Observations - Outline Introduction Current Status Discussion Future Introduction The development of cosmology is largely driven by observations The accelerating expansion of the ...
Outline Introduction Current Status Discussion Future Introduction The development of cosmology is largely driven by observations The accelerating expansion of the ...
| PowerPoint PPT presentation | free to view
A New Upper Limit on the Total Neutrino Mass from the 2dF Galaxy Redshift Survey PowerPoint PPT Presentation
A New Upper Limit on the Total Neutrino Mass from the 2dF Galaxy Redshift Survey - In Standard Model, assumed that neutrinos have no mass. This is by choice and is not required a priori ' ... From CMB anisotropy [astro-ph/0210306] Dark Matter ...
In Standard Model, assumed that neutrinos have no mass. This is by choice and is not required a priori ' ... From CMB anisotropy [astro-ph/0210306] Dark Matter ...
| PowerPoint PPT presentation | free to view
6dF Data Release 2 The good, the bad and the ugly Will Saunders AAO 270405 PowerPoint PPT Presentation
6dF Data Release 2 The good, the bad and the ugly Will Saunders AAO 270405 - But ergonomics very. poor, and all depends. on a giddy edifice of. flaky hardware and ... VPH gratings used in Littrow exhibit a zeroth order ghost image of ...
But ergonomics very. poor, and all depends. on a giddy edifice of. flaky hardware and ... VPH gratings used in Littrow exhibit a zeroth order ghost image of ...
| PowerPoint PPT presentation | free to download
Prospects for Infrared AGN Surveys PowerPoint PPT Presentation
Prospects for Infrared AGN Surveys - What are the key scientific questions? ... Spectroscopy from HYDRA & WYFFOS. Reddening. The time domain.? Largely unexplored regime. ...
What are the key scientific questions? ... Spectroscopy from HYDRA & WYFFOS. Reddening. The time domain.? Largely unexplored regime. ...
| PowerPoint PPT presentation | free to download
Why Study Nothing Voids and void galaxies in the Universe PowerPoint PPT Presentation
Why Study Nothing Voids and void galaxies in the Universe - The Void Finder Algorithm. Based on El-Ad and Piran algorithm some differences ... No free parameters except density threshold ...
The Void Finder Algorithm. Based on El-Ad and Piran algorithm some differences ... No free parameters except density threshold ...
| PowerPoint PPT presentation | free to view
Cosmological Structure Formation A Short Course PowerPoint PPT Presentation
Cosmological Structure Formation A Short Course - Cosmological Structure Formation A Short Course III. Structure Formation in the Non-Linear Regime Chris Power
Cosmological Structure Formation A Short Course III. Structure Formation in the Non-Linear Regime Chris Power
| PowerPoint PPT presentation | free to download
wz via 2dF QSO Galaxy Redshift Surveys PowerPoint PPT Presentation
wz via 2dF QSO Galaxy Redshift Surveys - Tom Shanks, Phil Outram, Jose Cruz da Angela, Bill Frith and Nic Ross. University of Durham ... 2QZ SDSS-2dF QSO Redshift Surveys. 2QZ P(k) vs SDSS DR2 LRG P(k) ...
Tom Shanks, Phil Outram, Jose Cruz da Angela, Bill Frith and Nic Ross. University of Durham ... 2QZ SDSS-2dF QSO Redshift Surveys. 2QZ P(k) vs SDSS DR2 LRG P(k) ...
| PowerPoint PPT presentation | free to view
Surveys of high-z galaxies and galaxy clusters with Herschel and SCUBA-2 PowerPoint PPT Presentation
Surveys of high-z galaxies and galaxy clusters with Herschel and SCUBA-2 - H1K fields (white blocks) superimposed on the IRAS 100 micron maps ... A blank field (850 micron @ JCMT) Add a (proto-)cluster at z=2.5 ...
H1K fields (white blocks) superimposed on the IRAS 100 micron maps ... A blank field (850 micron @ JCMT) Add a (proto-)cluster at z=2.5 ...
| PowerPoint PPT presentation | free to download
Cosmology and Dark Matter III: The Formation of Galaxies PowerPoint PPT Presentation
Cosmology and Dark Matter III: The Formation of Galaxies - Cosmology and Dark Matter III: The Formation of Galaxies Jerry Sellwood The story so far Four serious problems with the hot big bang model were solved in one ...
Cosmology and Dark Matter III: The Formation of Galaxies Jerry Sellwood The story so far Four serious problems with the hot big bang model were solved in one ...
| PowerPoint PPT presentation | free to view
STUDIO DI PowerPoint PPT Presentation
STUDIO DI - STUDIO DI STAR FORMATION HISTORY DA SPETTRI COSMICI Martinelli Federica Seminario finale per il corso di COSMOLOGIA OSSERVATIVA Prof. Guido Chincarini
STUDIO DI STAR FORMATION HISTORY DA SPETTRI COSMICI Martinelli Federica Seminario finale per il corso di COSMOLOGIA OSSERVATIVA Prof. Guido Chincarini
| PowerPoint PPT presentation | free to view
Ofer%20Lahav PowerPoint PPT Presentation
Ofer%20Lahav - Neutrino Masses from LSS Neutrino Masses from the CMB (III) The Dark Energy Survey Ofer Lahav University College London
Neutrino Masses from LSS Neutrino Masses from the CMB (III) The Dark Energy Survey Ofer Lahav University College London
| PowerPoint PPT presentation | free to download
Geometry and Topology PowerPoint PPT Presentation
Geometry and Topology - Superclusters in LCDM simulation (VIRGO consortium) by SURFGEN ... Web has both characteristics: filamentary network and bubble structure ...
Superclusters in LCDM simulation (VIRGO consortium) by SURFGEN ... Web has both characteristics: filamentary network and bubble structure ...
| PowerPoint PPT presentation | free to download
The 6dF Galaxy Redshift Survey: Status Report and Data Release 2 PowerPoint PPT Presentation
The 6dF Galaxy Redshift Survey: Status Report and Data Release 2 - The 6dF Galaxy Redshift Survey: Status Report and Data Release 2. Heath ... Galaxy ... SuperCosmos galaxy catalogs. ROSAT All-Sky Survey (RASS) HI Parkes Sky ...
The 6dF Galaxy Redshift Survey: Status Report and Data Release 2. Heath ... Galaxy ... SuperCosmos galaxy catalogs. ROSAT All-Sky Survey (RASS) HI Parkes Sky ...
| PowerPoint PPT presentation | free to view
The largescale structure of the universe 2 PowerPoint PPT Presentation
The largescale structure of the universe 2 - The correlation function and power spectrum. Gaussianity and topology. ... small scales, there is a slight meatball' shift w.r.t. Gaussian g(n), as ...
The correlation function and power spectrum. Gaussianity and topology. ... small scales, there is a slight meatball' shift w.r.t. Gaussian g(n), as ...
| PowerPoint PPT presentation | free to view
Cosmic%20Voids,%20Void%20Galaxies,%20and%20Void%20AGN PowerPoint PPT Presentation
Cosmic%20Voids,%20Void%20Galaxies,%20and%20Void%20AGN - KNAW colloquium 'Cosmic Voids' December 12-15, 2006 ... I. Void Finding in Nearby Redshift Surveys. Fiona Hoyle, Danny Pan ... Anca Constantin, Fiona Hoyle ...
KNAW colloquium 'Cosmic Voids' December 12-15, 2006 ... I. Void Finding in Nearby Redshift Surveys. Fiona Hoyle, Danny Pan ... Anca Constantin, Fiona Hoyle ...
| PowerPoint PPT presentation | free to download
Data%20mirrors:%20Techniques%20and%20Issues PowerPoint PPT Presentation
Data%20mirrors:%20Techniques%20and%20Issues - Techniques of Mirroring. Replication is one way to solve ... High Availability - ADS mirrors. Multilingual replication - www.debian.org ... Mirrors ...
Techniques of Mirroring. Replication is one way to solve ... High Availability - ADS mirrors. Multilingual replication - www.debian.org ... Mirrors ...
| PowerPoint PPT presentation | free to download
Weighing%20neutrinos%20with%20Cosmology PowerPoint PPT Presentation
Weighing%20neutrinos%20with%20Cosmology - is called the neutrino free-streaming. scale and roughly corresponds to the ... On scales much larger than the free streaming scale, on the other hand, ...
is called the neutrino free-streaming. scale and roughly corresponds to the ... On scales much larger than the free streaming scale, on the other hand, ...
| PowerPoint PPT presentation | free to download
FMOS Workshop, Jan. 2004 PowerPoint PPT Presentation
FMOS Workshop, Jan. 2004 - ... Jan. 2004. The Decline in Cosmic Star Formation: is Environment to ... Mapping the interaction of galaxies with their environment as a function of cosmic time. ...
... Jan. 2004. The Decline in Cosmic Star Formation: is Environment to ... Mapping the interaction of galaxies with their environment as a function of cosmic time. ...
| PowerPoint PPT presentation | free to download
First-Epoch VVDS data: The Redshift Evolution of the Non-Linear Bias between Matter and Galaxies PowerPoint PPT Presentation
First-Epoch VVDS data: The Redshift Evolution of the Non-Linear Bias between Matter and Galaxies - Title: First-Epoch VVDS data: The Redshift Evolution of the Non-Linear Bias between Matter and Galaxies Author: alain mazure Last modified by
Title: First-Epoch VVDS data: The Redshift Evolution of the Non-Linear Bias between Matter and Galaxies Author: alain mazure Last modified by
| PowerPoint PPT presentation | free to download
THE DARK MATTER PROBLEM PowerPoint PPT Presentation
THE DARK MATTER PROBLEM - More baryons. Potential. Density photons plasma ... baryon/photon ratio enhances peaks 1,3,5,... Strong measurement of baryon density ...
More baryons. Potential. Density photons plasma ... baryon/photon ratio enhances peaks 1,3,5,... Strong measurement of baryon density ...
| PowerPoint PPT presentation | free to download
Clustering%20of%20Luminous%20Red%20Galaxies%20and%20Applications%20to%20Cosmology PowerPoint PPT Presentation
Clustering%20of%20Luminous%20Red%20Galaxies%20and%20Applications%20to%20Cosmology - The 2dF-SDSS LRG And QSO (2SLAQ) Survey. Clustering techniques ... `Bump' in the 2 Point Correlation Function at ~100 h-1 Mpc. Due to ``baryon acoustic oscillations' ...
The 2dF-SDSS LRG And QSO (2SLAQ) Survey. Clustering techniques ... `Bump' in the 2 Point Correlation Function at ~100 h-1 Mpc. Due to ``baryon acoustic oscillations' ...
| PowerPoint PPT presentation | free to download
University of Pennsylvania PowerPoint PPT Presentation
University of Pennsylvania - The cosmic connection: the big picture. The cosmic connection: the details: an example. ... Relict from. the big bang. per m. 3. Cosmic rays. reactors. accelerators ...
The cosmic connection: the big picture. The cosmic connection: the details: an example. ... Relict from. the big bang. per m. 3. Cosmic rays. reactors. accelerators ...
| PowerPoint PPT presentation | free to view
NEUTRINO MASS BOUNDS FROM COSMOLOGICAL OBSERVABLES PowerPoint PPT Presentation
NEUTRINO MASS BOUNDS FROM COSMOLOGICAL OBSERVABLES - NEUTRINO MASS BOUNDS FROM COSMOLOGICAL OBSERVABLES. Sergio Pastor (IFIC) ?. XIth International Workshop on Neutrino Telescopes, Venice Feb 2005. Current bounds and ...
NEUTRINO MASS BOUNDS FROM COSMOLOGICAL OBSERVABLES. Sergio Pastor (IFIC) ?. XIth International Workshop on Neutrino Telescopes, Venice Feb 2005. Current bounds and ...
| PowerPoint PPT presentation | free to download
The Theory/Observation connection lecture 4 dark energy: linking with observations PowerPoint PPT Presentation
The Theory/Observation connection lecture 4 dark energy: linking with observations - SNe in passive galaxies: seem more powerful probes, but substantially rarer (esp. ... Also effects from the transition from mass to galaxies ...
SNe in passive galaxies: seem more powerful probes, but substantially rarer (esp. ... Also effects from the transition from mass to galaxies ...
| PowerPoint PPT presentation | free to download
Superclusters%20as%20future%20 PowerPoint PPT Presentation
Superclusters%20as%20future%20 - Future of structure in CDM cosmology. Spherical collapse, gravitational binding ... Cosmology. Initially matter-dominated: hierarchical growth of structure ...
Future of structure in CDM cosmology. Spherical collapse, gravitational binding ... Cosmology. Initially matter-dominated: hierarchical growth of structure ...
| PowerPoint PPT presentation | free to download
??????: SU(3) C PowerPoint PPT Presentation
??????: SU(3) C - Title: Author: M.C. Li Last modified by: xmzhang Created Date: 11/15/2003 3:19:33 PM Document presentation format:
Title: Author: M.C. Li Last modified by: xmzhang Created Date: 11/15/2003 3:19:33 PM Document presentation format:
| PowerPoint PPT presentation | free to download
Piggyback redshift surveys of radio galaxies at z0'3 PowerPoint PPT Presentation
Piggyback redshift surveys of radio galaxies at z0'3 - `Piggyback' redshift surveys of radio galaxies at z 0.3 ... Needs new large-area (50-100 deg2) sub-mJy radio survey. ... the local radio-source population is ...
`Piggyback' redshift surveys of radio galaxies at z 0.3 ... Needs new large-area (50-100 deg2) sub-mJy radio survey. ... the local radio-source population is ...
| PowerPoint PPT presentation | free to view
Diapositive 1 PowerPoint PPT Presentation
Diapositive 1 - Galaxies are observed in redshift space (z) and not physical space (d) ... 3D Voronoi Representation of a group with 10 galaxies ...
Galaxies are observed in redshift space (z) and not physical space (d) ... 3D Voronoi Representation of a group with 10 galaxies ...
| PowerPoint PPT presentation | free to download
Rotation of Cosmic Voids (Lee PowerPoint PPT Presentation
Rotation of Cosmic Voids (Lee - Rotation of Cosmic Voids (Lee & Park 2006, ApJ in press, ... LCDM Cosmogony. 8964936 galaxies at z=0. The Void-Finder by Hoyle & Vogeley (2002, ApJ, 566, 641) ...
Rotation of Cosmic Voids (Lee & Park 2006, ApJ in press, ... LCDM Cosmogony. 8964936 galaxies at z=0. The Void-Finder by Hoyle & Vogeley (2002, ApJ, 566, 641) ...
| PowerPoint PPT presentation | free to download
CREATION THEORY and the demonstration of biotic patterns in quantum and cosmological time series PowerPoint PPT Presentation
CREATION THEORY and the demonstration of biotic patterns in quantum and cosmological time series - Title: PowerPoint Presentation Author: Hector Sabelli Last modified by: Hector Sabelli Created Date: 5/5/2005 8:53:25 PM Document presentation format
Title: PowerPoint Presentation Author: Hector Sabelli Last modified by: Hector Sabelli Created Date: 5/5/2005 8:53:25 PM Document presentation format
| PowerPoint PPT presentation | free to view
Observing Dark Energy PowerPoint PPT Presentation
Observing Dark Energy - No compelling theory, must be observational driven. We can make ... Blake et al. 2006, Padmanabhan et al. 2006. Cosmological Constraints. Sullivan et al. (2003) ...
No compelling theory, must be observational driven. We can make ... Blake et al. 2006, Padmanabhan et al. 2006. Cosmological Constraints. Sullivan et al. (2003) ...
| PowerPoint PPT presentation | free to download
The 6dF Galaxy Survey PowerPoint PPT Presentation
The 6dF Galaxy Survey - redshifts (z) of 150,000 galaxies. peculiar velocities (v) of 15,000 galaxies ... 3D positions and radial velocity give kinematics of galaxies, clusters, superclusters ...
redshifts (z) of 150,000 galaxies. peculiar velocities (v) of 15,000 galaxies ... 3D positions and radial velocity give kinematics of galaxies, clusters, superclusters ...
| PowerPoint PPT presentation | free to view
Observational Cosmology PowerPoint PPT Presentation
Observational Cosmology - Observational Cosmology
Observational Cosmology
| PowerPoint PPT presentation | free to download
An Experimentalists Perspective on Testing Field Theories with the CMB. PowerPoint PPT Presentation
An Experimentalists Perspective on Testing Field Theories with the CMB. - Approx EE/BB foreground. Gravitational Waves. B modes from lensing of E modes (not primordial) ... EE/BB model at 60 GHz. r=0.3. Since reionization is late we ...
Approx EE/BB foreground. Gravitational Waves. B modes from lensing of E modes (not primordial) ... EE/BB model at 60 GHz. r=0.3. Since reionization is late we ...
| PowerPoint PPT presentation | free to view
Neutrino masses from double beta decay PowerPoint PPT Presentation
Neutrino masses from double beta decay - Neutrino masses from double beta decay Kai Zuber University of Sussex
Neutrino masses from double beta decay Kai Zuber University of Sussex
| PowerPoint PPT presentation | free to view


Home About Us Terms and Conditions Privacy Policy Contact Us
Copyright 2024 CrystalGraphics, Inc. — All rights Reserved. PowerShow.com is a trademark of CrystalGraphics, Inc.
2dfgrs — Search results on PowerShow.com