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 ...
Cosmo.WebHome Enrique Gaztanaga correlation fn of LRGs in the SDSS DR6 * theoretical (analytical simulational) models of xi radial tangential vs observational ...
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 ...
Cosmo.WebHome Ramon Miquel BAO PAU Physics of the Accelerating Universe Project to measure BAO Baryonic Acoustic Oscillations and use them as a standard ...
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 ...
Cosmo.WebHome for inclusion in BenasqueNotes2008 etc main page: BenasqueNotes2008 These are just rough notes feel free to correct them, add links, etc. from ...
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 ...
0$% * volume averaging affects power spectrum P(k) ! * averaging time is over time cone volume, not comoving volume? * "synchronous coordinates" * can set ...
Cosmo.WebHome motivations for MOND/TeVeS Glenn Starkman 29.07.2008 * C_l's are not independent because %$S_{1/2}$% is low * See e.g. AstroPh:0605135 ...
*This page is incomplete and out of date. Feel free to help update it.* new * Inhomogeneous Cosmologies IV https://cosmo.torun.pl/CosmoTorun19 (announcements ...
Toruń Cosmology Group (CA UMK CAMK) (en) Welcome to the home of Foswiki.Cosmo. This is a web based collaboration area for cosmology research and education. (pl) ...