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Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG
S Masi, P Ade, J Bock +41
We present the BOOMERanG-03 experiment and maps of the Stokes parameters I, Q, U of the microwave sky obtained during a 14 day balloon flight in 2003. Three regions of the southern…
Maps of the millimetre sky from the BOOMERanG experiment
P. de Bernardis, P. A. R. Ade, A. Balbi +38
In the 1998-99 flight, BOOMERanG has produced maps of of the sky at high Galactic latitudes, at frequencies of 90, 150, 240 and 410 GHz, with resolution $\simgt 10'$. Th…
Measuring CMB Polarization with BOOMERANG
T. Montroy, P. A. R. Ade, A. Balbi +38
BOOMERANG is a balloon-borne telescope designed for long duration (LDB) flights around Antarctica. The second LDB Flight of BOOMERANG took place in January 2003. The primary goal o…
Observations of Galactic and Extra-galactic Sources From the BOOMERANG and SEST Telescopes
K. Coble, P. A. R. Ade, J. J. Bock +32
We present millimeter-wave observations of three extra-galactic and six Galactic sources in the Southern sky. Observations were made at 90, 150, 240 and 400 GHz with resolutions of…
Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the CMB from Two New Analyses of BOOMERANG Observations
J. E. Ruhl, P. A. R. Ade, J. J. Bock +27
We report the most complete analysis to date of observations of the Cosmic Microwave Background (CMB) obtained during the 1998 flight of BOOMERANG. We use two quite different metho…
BOOMERANG: A Balloon-borne Millimeter Wave Telescope and Total Power Receiver for Mapping Anisotropy in the Cosmic Microwave Background
B. P. Crill, P. A. R. Ade, D. R. Artusa +34
We describe BOOMERANG; a balloon-borne microwave telescope designed to map the Cosmic Microwave Background (CMB) at a resolution of 10' from the Long Duration Balloon (LDB) platfor…
The BOOMERanG experiment and the curvature of the Universe
S. Masi, P. A. R. Ade, J. J. Bock +35
We describe the BOOMERanG experiment and its main result, i.e. the measurement of the large scale curvature of the Universe. BOOMERanG is a balloon-borne microwave telescope with s…
Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology
P. de Bernardis, P. A. R. Ade, J. J. Bock +32
Three peaks and two dips have been detected in the power spectrum of the cosmic microwave background from the BOOMERANG experiment, at and $\ell \sim 420,…
The BOOMERANG North America Instrument: a balloon-borne bolometric radiometer optimized for measurements of cosmic background radiation anisotropies from 0.3 to 4 degrees
F. Piacentini, P. A. R. Ade, R. Bathia +24
We describe the BOOMERANG North America (BNA) instrument, a balloon-borne bolometric radiometer designed to map the Cosmic Microwave Background (CMB) radiation with 0.3 deg resolut…
A measurement by BOOMERANG of multiple peaks in the angular power spectrum of the cosmic microwave background
C. B. Netterfield, P. A. R. Ade, J. J. Bock +30
This paper presents a measurement of the angular power spectrum of the Cosmic Microwave Background from l=75 to l=1025 (~10' to 5 degrees) from a combined analysis of four 150 GHz…
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…
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…
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…
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…
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…
First Estimations of Cosmological Parameters From BOOMERANG
A. E. Lange, P. A. R. Ade, J. J. Bock +29
The anisotropy of the cosmic microwave background radiation contains information about the contents and history of the universe. We report new limits on cosmological parameters der…
A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
P. de Bernardis, P. A. R. Ade, J. J. Bock +33
The blackbody radiation left over from the Big Bang has been transformed by the expansion of the Universe into the nearly isotropic 2.73K Cosmic Microwave Background. Tiny inhomoge…
BOOMERanG: a scanning telescope for 10 arcminutes resolution CMB maps
S. Masi, P. A. R. Ade, R. Artusa +24
The BOOMERanG experiment is a stratospheric balloon telescope intended to measure the Cosmic Microwave Background anisotropy at angular scales between a few degrees and ten arcminu…
Mapping the CMB Sky: The BOOMERANG experiment
P. de Bernardis, P. A. R. Ade, R. Artusa +23
We describe the BOOMERanG experiment, a stratospheric balloon telescope intended to measure the Cosmic Microwave Background anisotropy at angular scales between a few degrees and t…
Measurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American test flight of BOOMERANG
P. D. Mauskopf, P. A. R. Ade, P. de Bernardis +31
We describe a measurement of the angular power spectrum of anisotropies in the Cosmic Microwave Background (CMB) from 0.3 degrees to ~10 degrees from the North American test flight…