Publications (19)
Radio Sources Toward Galaxy Clusters at 30 GHz
K. Coble, M. Bonamente, J. E. Carlstrom +7
Extra-galactic radio sources are a significant contaminant in cosmic microwave background and Sunyaev-Zel'dovich effect experiments. Deep interferometric observations with the BIMA…
The Quintessential CMB, Past & Future
J. R. Bond, D. Pogosyan, S. Prunet +42
The past, present and future of cosmic microwave background (CMB) anisotropy research is discussed, with emphasis on the Boomerang and Maxima balloon experiments. These data are co…
Anisotropy in the Cosmic Microwave Background at Degree Angular Scales: Python V Results
K. Coble, M. Dragovan, J. Kovac +12
Observations of the microwave sky using the Python telescope in its fifth season of operation at the Amundsen-Scott South Pole Station in Antarctica are presented. The system consi…
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…
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…
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…