[PDF] Top 20 Cosmological parameters from velocities, cosmic microwave background and supernovae

... values obtained without this additional term. This and other ways of correcting for non-linear effects have been found recently to provide consistent and more reliable results, based on improved mock catalogues drawn ... See full document

... a cosmological constant, gen- eral relativity predicts that there will be ...2003), from an observational point of view one should not rule out the possibility in ...constraints from x-ray and type ... See full document

... Robertson-Walker cosmological model, these parameters are linked in our ...standard cosmological models where no such prediction is ...the cosmic seed re- main today in the form of temperature ... See full document

... of cosmological parameters; (2) cosmic microwave background (CMB) radia- tion maps; (3) channel data maps (temperature anisotropy and polarization); (4) foregrounds maps; (5) secondary ... See full document

... the cosmic fluid in the early universe includes a dominant contribution from the evolution of a scalar ...deduced from the Klein-Gordon Equation ρ(φ) = φ ˙ 2 2 + ∇ 2 φ + ... See full document

... of background galaxies and through radio emis- sion from the halos and relics of the clusters (Govoni & Feretti 2004; Ferrari et ...range from a few to several ...ments from low-density ... See full document

... The design of Bicep2 /Keck Array, which are derivative of the Bicep1 instrument [85], is contrary to the usual design of most science quality telescopes in operation today, which boast very large mirrors and very fine ... See full document

... events from relativistic heavy ion collisions using methods commonly em- ployed in the analysis of the photons from the Cosmic Microwave Background ...arizing from collective flow ... See full document

... Out of the four modern theories of universe two are obsolete now, Static Theory and Steady State Theory, because we have very strong evidences which prove them wrong. Intergalactic redshift, Radio sources count, ... See full document

... these cosmological distances neutrinos travel toward the observer almost freely, except for the adiabatic energy losses and flavour oscillations, the opacity of the universe to neutrinos being relevant only at ... See full document

... A Bayesian approach to this problem was discussed in [11], where an entropic prior was proposed for the sources. Such a prior regularizes the separation such that the most plausible (highest entropy) sources are obtained ... See full document

... The multiplexing (or “MUX”) architecture of the electronics readout results in a variety of different cross-talk mechanisms between detectors. These coupling mechanisms are described and charac- terized in detail in de ... See full document

... microwaves from all-sky images taken at different ...the cosmic microwave background (CMB) signal from the other ...samples from the posterior ...extracted from the ... See full document

... obtained from BOSS rather than from ...obtained from the SDSS Legacy Survey and other targeted surveys within SDSS, many of which had much brighter limiting mag- ...demonstrated from hosts ... See full document

... in cosmic microwave background experiments throughout the paper, although the method we present is totally general and can be used in many other fields of data ...in microwave experiments—on a ... See full document

... the cosmic microwave background ...free parameters, for the deviation of the microwave background anisotropy that can be compared with the data [32, 33, ... See full document

... A Measurement of the Angular Power Spectrum of the Cosmic Microwave Background with a Long Duration Balloon-borne Receiver Thesis by Brendan P.. In Partial Ful..[r] ... See full document

... the microwave and millimeter-wave range, the dominant ra- diations are the cosmic microwave background, the galactic dust, the free-free emission and the synchrotron (see ...comes from ... See full document

... in cosmic his- ...the cosmic mi- crowave background (CMB) and galaxy clustering statistics, have been found to independently require late epoch cosmic acceleration in the FLRW ... See full document

... objects from all ...other from the impinging corpuscles, resulting in a net imbalance in the pressure exerted by the impact of corpuscles on the bodies, tending to drive the bodies ... See full document