3 citations · 3 across the 1 of their papers we have counts for
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Searching for non Gaussian signals in the BOOMERanG 2003 CMB maps
G. De Troia, P. A. R. Ade, J. J. Bock +38
We analyze the BOOMERanG 2003 (B03) 145 GHz temperature map to constrain the amplitude of a non Gaussian, primordial contribution to CMB fluctuations. We perform a pixel space anal…
CMB multipole measurements in the presence of foregrounds
Angelica de Oliveira-Costa, Max Tegmark
Most analysis of Cosmic Microwave Background spherical harmonic coefficients a_lm has focused on estimating the power spectrum C_l=<|a_lm|^2> rather than the coefficients themselve…
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…
How accurately can suborbital experiments measure the CMB?
Angelica de Oliveira-Costa, Max Tegmark, Mark Devlin +4
Great efforts are currently being channeled into ground- and balloon-based CMB experiments, mainly to explore anisotropy on small angular scales and polarization. To optimize instr…
The Cosmic Microwave Background and Its Polarization
Angelica de Oliveira-Costa
The DASI discovery of CMB polarization, confirmed by WMAP, has opened a new chapter in cosmology. Most of the useful information about inflationary gravitational waves and reioniza…
The Quest for Microwave Foreground X
Angelica de Oliveira-Costa, Max Tegmark, R. D. Davies +4
The WMAP team has produced a foreground map that can account for most of the low-frequency Galactic microwave emission in the WMAP maps, tentatively interpreting it as synchrotron…