activity
19972001
collaborators

7 papers

astro-ph2001

Noise estimation in CMB time-streams and fast map-making. Application to the BOOMERanG98 data

S. Prunet, P. A. R. Ade, J. J. Bock +35

We describe here an iterative method for jointly estimating the noise power spectrum from a CMB experiment's time-ordered data, together with the maximum-likelihood map. We test th…

astro-ph2000

From the time-ordered data to the Maximum-Likelihood temperature maps of the Cosmic Microwave Backgorund anisotropy

R. Stompor, A. Balbi, J. Borrill +10

We review selected methods of the Cosmic Microwave Background data analysis appropriate for the analysis of the largest currently available data sets. We focus on techniques of the…

astro-ph2000

Detection of anisotropy in the Cosmic Microwave Background at horizon and sub-horizon scales with the BOOMERanG experiment

P. de Bernardis, P. A. R. Ade, J. J. Bock +35

BOOMERanG has recently resolved structures on the last scattering surface at redshift 1100 with high signal to noise ratio. We review the technical advances which made this…

astro-ph2000

CMB Analysis of Boomerang & Maxima & the Cosmic Parameters {Omega_tot,Omega_b h^2,Omega_cdm h^2,Omega_Lambda,n_s}

J. R. Bond, P. Ade, A. Balbi +40

We show how estimates of parameters characterizing inflation-based theories of structure formation localized over the past year when large scale structure (LSS) information from ga…

astro-ph1998

Evidence for non-Gaussianity in the CMB

J. Magueijo, P. Ferreira, K. Gorski

In a recent Letter we have shown how COBE-DMR maps may be used to disprove Gaussianity at a high confidence level. In this report we digress on a few issues closely related to this…

astro-ph1998

The impact on cosmology of a primordial scaling field

Pedro G. Ferreira

A scalar field with an exponential potential has the particular property that it is attracted into a solution in which its energy scales as the dominant component (radiation or mat…