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BenasqueBlanchard2008
Cosmo.WebHome clusters and Omega_m = 1 ? Sheth, Mo, Tormen 2001, MNRAS, 323, 1 %$\sigma_8 = fn(A_{TM})$% M T calibration * Ferramacho Blanchard 2007 ...
BenasqueCrittendon2008
Cosmo.WebHome Rob Crittendon IS ArXiv:0801.4380 * a lot from Giannantonio et al. 2008 ArXiv:0801.4380 * about 80% of ISW signal is from z 1 for a standard ...
BenasqueGaztanaga2008
Cosmo.WebHome Enrique Gaztanaga correlation fn of LRGs in the SDSS DR6 * theoretical (analytical simulational) models of xi radial tangential vs observational ...
BenasqueHernandezM2008
Cosmo.WebHome Carlos Hernandez Monteagudo ArXiv:0805.3710 Also: * ISW is at big scales, not at the small scales where there are delta baryon fluctuations ...
BenasqueMiquel2008
Cosmo.WebHome Ramon Miquel BAO PAU Physics of the Accelerating Universe Project to measure BAO Baryonic Acoustic Oscillations and use them as a standard ...
BenasqueMiraldeEscude2008
Cosmo.WebHome Jordi Miralde Escud ArXiv:0710.4488 Self Consistent Models of the AGN and Black Hole Populations: Duty Cycles, Accretion Rates, and the Mean Radiative ...
BenasqueNotes2008
Cosmo.WebHome Benasque (included) informal, personal notes * Mon 28.07.2008 BenasqueStarkman2008 motivations for MOND/TeVeS * 28.07.2008 BenasqueBlanchard2008 ...
BenasqueRebolo2008
Cosmo.WebHome Rebolo polarisation searching for BB modes project QUIJOTE QUIJOTE = Q U I JOdrell bank Tenerife CMB project * 10 30 GHz * in 1 year ...
BenasqueRoukema2008
Cosmo.WebHome Boud Roukema Is the Poincare Dodecahedral Sphere model the explanation of the missing fluctuations about 60 degrees? See ArXiv:0801.0006 and 0807 ...
BenasqueSchwarz2008
0$% * volume averaging affects power spectrum P(k) ! * averaging time is over time cone volume, not comoving volume? * "synchronous coordinates" * can set ...
BenasqueStarkman2008
Cosmo.WebHome motivations for MOND/TeVeS Glenn Starkman 29.07.2008 * C_l's are not independent because %$S_{1/2}$% is low * See e.g. AstroPh:0605135 ...
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Number of topics: 12
 
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