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19942024
most citedA Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation

2.5k citations · 12.1k across the 93 of their papers we have counts for

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9 papers · 1 filter

astro-ph2000

Foregrounds in the BOOMERANG-LDB data: a preliminary rms analysis

S. Masi, P. A. R. Ade, J. Bock +18

We present a preliminary analysis of the BOOMERanG LDB maps, focused on foregrounds. BOOMERanG detects dust emission at moderately low galactic latitudes () in bands cen…

astro-ph2000★ 6 cited

First results from the BOOMERanG experiment

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

We report the first results from the BOOMERanG experiment, which mapped at 90, 150, 240 and 410 GHz a wide (3%) region of the microwave sky with minimal local contamination. From t…

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-ph2000★ 518 cited

Cosmology from Maxima-1, Boomerang and COBE/DMR CMB Observations

A. H. Jaffe, P. A. R. Ade, A. Balbi +39

Recent results from BOOMERANG-98 and MAXIMA-1, taken together with COBE-DMR, provide consistent and high signal-to-noise measurements of the CMB power spectrum at spherical harmoni…

astro-ph2000★ 53 cited

Constraints on Cosmological Parameters from MAXIMA-1

A. Balbi, P. Ade, J. Bock +16

We set new constraints on a seven-dimensional space of cosmological parameters within the class of inflationary adiabatic models. We use the angular power spectrum of the cosmic mi…