Maps of the CMB Temperature Anisotropy: from the Time-Ordered Data to the Maximum-Likelihood Solution

2003 ◽  
pp. 414-420
Author(s):  
Radek Stompor ◽  
Amedeo Balbi ◽  
Julian Borrill ◽  
Pedro Ferreira ◽  
Shaul Hanany ◽  
...  
Keyword(s):  
Maximum Likelihood ◽  
Temperature Anisotropy ◽  
Ordered Data ◽  
Cmb Temperature

CMB temperature anisotropy

Cosmology ◽  
2017 ◽  
pp. 279-308
Author(s):  
Nicola Vittorio
Keyword(s):  
Temperature Anisotropy ◽  
Cmb Temperature

scholarly journals A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG

2006 ◽  
Vol 647 (2) ◽  
pp. 823-832 ◽  
Author(s):  
W. C. Jones ◽  
P. A. R. Ade ◽  
J. J. Bock ◽  
J. R. Bond ◽  
J. Borrill ◽  
...  
Keyword(s):  
Power Spectrum ◽  
Temperature Anisotropy ◽  
Angular Power Spectrum ◽  
Cmb Temperature

Observations and simulations of the CMB temperature anisotropy at very small angular scales

2012 ◽  
Author(s):  
Màrius Josep Fullana i Alfonso ◽  
Josep Vicent Arnau i Córdoba ◽  
Robert J. Thacker ◽  
Hugh M. P. Couchman ◽  
Diego P. Sáez
Keyword(s):  
Temperature Anisotropy ◽  
Cmb Temperature

scholarly journals Cosmological constraints on matter density perturbations amplitude, neutrino mass and number of relativistic species

2018 ◽  
Vol 191 ◽  
pp. 01009
Author(s):  
Rodion Burenin
Keyword(s):  
Neutrino Mass ◽  
Large Scale ◽  
Hubble Constant ◽  
Density Perturbation ◽  
Matter Density ◽  
Temperature Anisotropy ◽  
Perturbation Amplitude ◽  
High Multipoles ◽  
Density Perturbations ◽  
Cmb Temperature

It is shown that Planck CMB temperature anisotropy data at high multipoles, ℓ > 1000, produce the measurement of matter density perturbations amplitude that contradict to all other constraints obtained both from remaining Planck CMB anisotropy data and from other cosmological data, at about 3:7σ significance level. With the exception of Planck CMB temperature anisotropy data at high multipoles, all other measurements of density perturbation amplitude are in good agreement between each other and give the following measurements of linear density perturbation amplitude: σ8 = 0:792 ± 0:006, mean density of the Universe: Ωm = 0:287 ± 0:007, and Hubble constant: H0 = 69:4 ± 0:6 km s-1 Mpc-1. Therefore, in this case the tensions in H0 constraints between Planck+BAO data and direct H0 measurements are weaken, and the tensions in σ8 measurements between Planck CMB data and large scale structure data disappear completely. Taking in account the data on baryon acoustic oscillations and (or) direct measurements of the Hubble constant, one can obtain different constraints on sum of neutrino mass and number of relativistic species.

Sign in / Sign up

Export Citation Format

Share Document